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		<title>Electronics Obstacle Course</title>
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		<summary type="html">&lt;p&gt;Wikiuser: /* Transistors */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;br /&gt;
== Permanent Materials (located in the electronics area): ==&lt;br /&gt;
[[File:Electronic_station.jpg|right|500px]]&lt;br /&gt;
- power supplies  &amp;lt;br&amp;gt;&lt;br /&gt;
- [[Media:DG1022.pdf|function generators]] &amp;lt;br&amp;gt;&lt;br /&gt;
- [[Media:DS1102E.pdf|oscilloscopes ]]&amp;lt;br&amp;gt;&lt;br /&gt;
- [[Media:Fluke_179.pdf| Fluke 179 multimeter (MM)]] &amp;lt;br&amp;gt;&lt;br /&gt;
- [[Media:CX-920A.pdf| capacitance meter]] &amp;lt;br&amp;gt;&lt;br /&gt;
- [[Media:PB-505.pdf|electronic proto-boards]]&amp;lt;br&amp;gt;&lt;br /&gt;
- wire, resistors, capacitors, inductors, diodes, Op-Amps, other ICs&amp;lt;br&amp;gt;&lt;br /&gt;
- photodiodes (PDs), light-emitting diodes (LEDs), laser diodes (LDs)&amp;lt;br&amp;gt;&lt;br /&gt;
- soldering equipment and supplies&lt;br /&gt;
&lt;br /&gt;
=== Materials to borrow when necessary ===&lt;br /&gt;
- LTSpice circuit simulation software (on computers in lab)&amp;lt;br&amp;gt;&lt;br /&gt;
- lab copy of ''The Art of Electronics'', Horowitz &amp;amp; Hill&amp;lt;br&amp;gt;&lt;br /&gt;
- inductance meter&amp;lt;br&amp;gt;&lt;br /&gt;
- Keithley voltage supply&lt;br /&gt;
- Red LD module&lt;br /&gt;
- Optical power meter&lt;br /&gt;
- Spectrometer&lt;br /&gt;
&lt;br /&gt;
[[File:Symbols.png|frame|right|Electronic Component Symbols|200px]]&lt;br /&gt;
&lt;br /&gt;
=== Activities ===&lt;br /&gt;
&lt;br /&gt;
* If you have zero electronic training or experience read chapters 1-6 of Keith Brindley's eBook ''Starting Electronics''.&lt;br /&gt;
* If you have some small experience with electronics proceed and consult ''Starting Electronics'' or ''The Art of Electronics'' as needed.&amp;lt;br&amp;gt;&lt;br /&gt;
* '''CLEAN UP THE OBSTACLE COURSE SETUP AFTER USE - PUT BACK ELECTRONIC COMPONENTS IN APPROPRIATE PLACES AFTER EACH ACTIVITY''' &lt;br /&gt;
* Keep a journal of your activities, results and answers to any questions asked in the activities below. You will use this for your write-up. &lt;br /&gt;
&lt;br /&gt;
==== Resistor &amp;amp; Capacitor Basics ====&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Fluke_179.jpg|right|100px| thumb| multimeter]]&lt;br /&gt;
# With a MM measure the resistance of five 100 Ohm resistors. Do they fall within the specified tolerance?&lt;br /&gt;
## What is resistance? Can you provide an analogy based on water flowing through pipes?&lt;br /&gt;
## Describe physically a resistor.&lt;br /&gt;
## Is energy stored in a resistor or dissipated as heat? Can you provide an explanation of the basic physical processes?&lt;br /&gt;
## What is the resistance of two 100 Ohm resistors in series? How do resistors in series add?&lt;br /&gt;
## What is the resistance of two 100 Ohm resistors in parallel? How do resistors in parallel add?&lt;br /&gt;
## How does the MM measure the resistance? &lt;br /&gt;
## What can you say about the &amp;quot;internal&amp;quot; resistance of the MM in resistance measurement mode?[[File:Pb-505.jpg|right|100px|thumb|proto-board]]&lt;br /&gt;
## Using a proto-board and one of the 100 Ohm resistors put 2.5VDC '''across''' the resistor. Calculate the current. Use the MM in ammeter mode to measure the current. Are the calculated and measured values close? Does the power applied to the resistor fall within the power rating of the resistor? What is power? What could happen if you applied too much power to the resistor?&lt;br /&gt;
## What is current?&lt;br /&gt;
## How does the MM measure current?&lt;br /&gt;
## What can you say about the &amp;quot;internal&amp;quot; resistance of the ammeter used in the measurement of the current?&lt;br /&gt;
## How do the MM wire leads effect these measurements?&lt;br /&gt;
## Could you measure the resistance of a 1cm length of copper wire with the MM? Why?&lt;br /&gt;
# Put 150mA of DC current '''through''' a 10 Ohm resistor. &lt;br /&gt;
## What power is being applied to the resistor? Calculate the voltage '''across''' the resistor. With the MM measure the voltage across the resistor. Are these values close?&lt;br /&gt;
##What is voltage?&lt;br /&gt;
## How does the MM measure a voltage?&lt;br /&gt;
## What can you say about the MM's &amp;quot;internal&amp;quot; resistance when it measures a voltage?&lt;br /&gt;
# With a function generator put a 2.5VAC (peak-to-peak) sinusoidal voltage at frequencies of 50, 500 and 1000Hz '''across''' a 100 Ohm resistor.&lt;br /&gt;
## Using the MM in voltage mode measure the AC voltage. Does it vary with frequency?&lt;br /&gt;
## Using the MM in current mode measure the AC current. Does it vary with frequency?&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
# Measure the capacitance of five 0.1 &amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;f unpolarized capacitors. Do they fall within the specified tolerance?&lt;br /&gt;
## What is capacitance? Describe physically a very simple capacitor.&lt;br /&gt;
## How is energy stored in a capacitor?&lt;br /&gt;
## What is the difference between unpolarized and polarized capacitors?&lt;br /&gt;
## What is the capacitance of two 0.1 &amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;f capacitors in series? How do capacitors in series add?&lt;br /&gt;
## What is the capacitance of two 0.1 &amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;f capacitors in parallel? How do capacitors in parallel add?&lt;br /&gt;
## How does the capacitance meter measure the capacitance?&lt;br /&gt;
## Using a proto-board apply 2.5VDC '''across''' an 0.1 &amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;f capacitor and 100 Ohm resistor in series. Using a MM measure the voltage '''across''' the entire capacitor + resistor series network. Measure the voltage across the capacitor only. Measure the voltage across the resistor only. Explain the measured voltage across the resistor.&lt;br /&gt;
## Now apply a 2.5VAC sinusoidal voltage '''across''' the capacitor + resistor network at 50, 500 and 1000 Hz.&lt;br /&gt;
## What's the voltage across the resistor for 50, 500 and 1000Hz?&lt;br /&gt;
## What's the voltage across the capacitor for 50, 500 and 1000Hz?&lt;br /&gt;
## How does the voltage across the capacitor as a function of frequency compare to the voltage across a resistor as a function of frequency?&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt; [[File:Voltagedivider.gif|right|100px]]&lt;br /&gt;
# Build a network of two (possibly different valued) resistors that takes an input voltage of 5VDC and produces an output voltage at 2.5VDC.&lt;br /&gt;
# Build a network of two (possibly different valued) resistors that takes an input voltage of 5VDC and produces an output voltage at 1.25VDC.&lt;br /&gt;
# Build a network of an &amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;f capacitor and a 100 Ohm resistor in series.&lt;br /&gt;
## Apply a 1VAC sinusoidal (input) signal to the capacitor at 100, 1000, 5000, 10000, 15000, 20000, 25000 and 50000 Hz and measure the (output) voltage between the capacitor and the resistor for each frequency.&lt;br /&gt;
## Plot as a function of frequency. What can you say about the frequency dependence of the ratio of output to input voltage?&lt;br /&gt;
## You've just built three very useful circuits called voltage dividers. Would a voltage divider containing only resistors work for AC voltages? If you're unsure, try it. Would a voltage divider containing at least one capacitor work for DC voltages? Again, if you're unsure, try it.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
# Now, apply a 1V 10Hz square pulse to a 500 Ohm resistor and an 470 &amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;f capacitor in parallel.&lt;br /&gt;
## Using an oscilloscope measure the voltage across the capacitor + resistor parallel network. (You'll need to use the oscilloscope's front-panel controls to get the waveform on the screen and get the triggering to work)&lt;br /&gt;
## Are the leading and trailing edges of the pulse similar? Why?&lt;br /&gt;
## What is the &amp;quot;rise time&amp;quot; of the leading edge (10% to 90%)?&lt;br /&gt;
## What is the &amp;quot;fall time&amp;quot; of the trailing edge (10% to 90%)?&lt;br /&gt;
## What is the time it takes for the trailing edge to fall to 1/e of its initial value?&lt;br /&gt;
## What is the value of the resistance multiplied by the capacitance?&lt;br /&gt;
## Repeat the above measurements with a 100 &amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;f capacitor instead of the 470 &amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;f capacitor.&lt;br /&gt;
## Are the rise and fall times faster or slower?&lt;br /&gt;
## What can you say about the rise time as a function of capacitance?&lt;br /&gt;
# Next let's use resistors and a capacitors to build one frequency-low-pass circuit and one frequency-high-pass circuit.[[File:LPF.png|right|75px]]&lt;br /&gt;
## Use what you've learned about the AC and DC responses of capacitors and resistors to put together a resistor + capacitor network that blocks DC current, strongly attenuates low frequencies but passes high frequencies (hint: recall the voltage divider  of 7 above).[[File:HPF.png|right|75px]]&lt;br /&gt;
## Determine the circuit's 3dB point.&lt;br /&gt;
## Put together a resistor + capacitor network that passes DC current and low frequencies but strongly attenuates high frequencies.&lt;br /&gt;
## Determine the circuit's 3dB point.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== Inductor Basics ====&lt;br /&gt;
[[File:Inductor_symbol.png|thumb|100px|right|Inductor Symbol- L]]&lt;br /&gt;
# Measure the inductance of five 1mH inductors. Estimate their tolerance (5%, 10%, 15% or 20%).&lt;br /&gt;
## What is inductance? Describe physically a very simple inductor.&lt;br /&gt;
## How is energy stored in an inductor?&lt;br /&gt;
## What is the inductance of two 1mH inductors in series? How do inductors add in series?&lt;br /&gt;
## What is the inductance of two 1mH inductors in parallel? How do inductors add in parallel?&lt;br /&gt;
## Do inductors add like resistors or capacitors?&lt;br /&gt;
## How does the inductance meter measure inductance?&amp;lt;br&amp;gt;&lt;br /&gt;
# Using a proto-board apply 1VDC '''across''' a 1mH inductor and 500 Ohm resistor in series. Using a MM measure the voltage '''across''' the entire inductor + resistor series network. What is the inductors &amp;quot;resistance&amp;quot; in this situation?&lt;br /&gt;
# Put a 1VAC sinusoidal signal across the inductor + resistor network at 50, 500, 2kHz, 5kHz and 10kHz, 25kHz, 50000, 250kHz and 1Mhz.&lt;br /&gt;
## At each frequency measure the voltage across the inductor only. Measure the voltage across the resistor only. Explain the measured voltage across the resistor in terms of how the inductor behaves with frequency.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
==== Resonant circuits ====&lt;br /&gt;
[[File:LR_Bandpass_filter.jpg|thumb|right|LC resonant circuit - bandpass filter|150px]]&lt;br /&gt;
# Construct the circuit shown at the right using a 100 Ohm resistor, 1mH inductor and a 10uf capacitor.&lt;br /&gt;
## Apply a 1VAC sinusoidal input voltage at frequencies between 10 and 3000Hz and plot the output voltage as a function of frequency.&lt;br /&gt;
## At what frequency is the response of the circuit maximum?&lt;br /&gt;
## Explain the response of this circuit based on what you've learned about capacitors and inductors.&lt;br /&gt;
## When would a circuit with a response like this be useful?&lt;br /&gt;
##Can you think of an optical-cavity analogy?&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
==== Impedance and Reactance ====&lt;br /&gt;
Impedance is resistance generalized. A resistor resists (dissipates power) but does not change the waveform (square wave in square wave out). Capacitors and inductors (since they store energy) can react and cause changes in the waveform (see section 8 above). &lt;br /&gt;
&lt;br /&gt;
The concept of impedance includes resistance and reactance effects. That is, '''Impedance = Resistance + Reactance'''. All the frequency dependence is contained within the reactance. For ideal capacitors and inductors their resistance is zero (not the case in real life). An ideal resistor is a purely resistive component and has no reactance (again, not the case in real life). &lt;br /&gt;
&lt;br /&gt;
We can use the word &amp;quot;impedance&amp;quot; in general. When we say something like, &amp;quot;What's the resistor's impedance&amp;quot;, we are referring to the resistance term of the resistor's impedance equation. When we say something like, &amp;quot;What's the impedance of the capacitor&amp;quot;, we are referring to the reactance term of the capacitor's impedance equation. &lt;br /&gt;
# Think back to the previous exercises. &lt;br /&gt;
## What is the frequency dependence of a capacitor's impedance?&lt;br /&gt;
## What is the frequency dependance of an inductors impedance?&lt;br /&gt;
&lt;br /&gt;
==== Diodes ====&lt;br /&gt;
For the electronic components considered above (resistor, capacitor, inductor) it doesn't matter which way you put them into a circuit - they are non-directional. That is, you can flip their leads and the circuit will behave the same. For diodes this is not the case. Diodes are directional and it matters which way they are oriented in a circuit. Diodes are physically more complicated than the components treated above so we won't go into an explanation of just what a diode is now. We'll only consider how diodes behave.&lt;br /&gt;
[[File:Diodecathan.png|thumb|Diode]]&lt;br /&gt;
# Put a [[Media:P6KE6.8.pdf| P6KE6.8]] diode in series with a MM in ammeter mode and ground the anode. &lt;br /&gt;
## Apply 0.7VDC to the cathode and measure the current through the diode.&lt;br /&gt;
## Now ground the cathode and apply 0.7VDC to the anode and measure the current through the diode.&lt;br /&gt;
## Are the currents the same? &lt;br /&gt;
# With the cathode grounded apply voltages from 0-1.5 VDC to the anode in 0.1 V increments and plot the result. This is the forward I-V curve for the diode. The diode is said to be &amp;quot;forward biased&amp;quot; in this situation.&lt;br /&gt;
## There should be a &amp;quot;knee&amp;quot; in this curve where the diode &amp;quot;turns on&amp;quot; or conducts. About what voltage is this?&lt;br /&gt;
# Using the (current limited) Keithley voltage supply, apply voltages from 0-100VDC to the anode grounded diode and plot the result. This is the reverse I-V curve for the diode. The diode is said to be &amp;quot;reverse biased&amp;quot; in this situation. &lt;br /&gt;
## There should be a &amp;quot;knee&amp;quot; in this curve too where the diode starts to conduct in the reverse direction. About what voltage is this?&lt;br /&gt;
## Are the forward and reverse &amp;quot;turn on&amp;quot; voltages symmetric about 0V?&lt;br /&gt;
# Construct the diode clamp circuit shown at the right.[[File:Diode_clamp.jpg|thumb| Diode Clamp|100px]]&lt;br /&gt;
## Apply input voltages from 0-10VDC and plot the output voltage vs. input voltage.&lt;br /&gt;
## Does the diode clamp earn its name?&lt;br /&gt;
## Can you explain the maximum output voltage?&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
# Employ an AC voltage divider with a resistor and the P6KE6.8 to measure the diode's capacitance as a function of bias voltage. [[File:Voltage_Divider.png|100px|right]]This diode capacitance issue will play a role later on when we encounter optoelectronic devices. In the AC voltage divider shown at the right the C indicates the capacitance of the diode. That is, don't put a capacitor where &amp;quot;C&amp;quot; is but the P6KE6.8 diode with its cathode grounded. Apply a 20mV AC sinusoidal signal with varying (positive to the anode) DC offsets (larger than 20mV) to the input. The DC offset is the diode's bias voltage. Look for amplitude changes to the AC signal at the output. With the voltage divider formula and the formula for the impedance of a capacitor you should be able to plot the diodes capacitance Cd as a function of bias voltage (the DC offset).&lt;br /&gt;
## Does the diode's capacitance decrease of increase with positive bias voltages?&lt;br /&gt;
## Is there a limiting behaviour? If so, can you explain it?&lt;br /&gt;
## Now measure the diode's capacitance for reverse biases from 0 to 25VDC (positive to the cathode).&lt;br /&gt;
## Does the diode's capacitance change much for reverse bias voltages?&lt;br /&gt;
&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
==== Transistors ====&lt;br /&gt;
[[File:Bipolar-junction-transistors.jpg|thumb|right| Transistors|100px]]&lt;br /&gt;
All the components (even diodes) examined above are considered &amp;quot;passive&amp;quot; components. That is, they can't supply energy. Transistors are considered &amp;quot;active&amp;quot; in the sense that they can supply energy (or amplify). Like diodes, transistors are physically more complicated than resistors, capacitors and inductors and we won't go into detail about just what they are. Instead we'll focus on how transistors behave. The collector C must be biased more positive than the emitter E. The current through the collector IC is roughly proportional to the current into the base IB (usually anywhere from 50 to 250 times IB). So there you have it. In a first approximation the transistor is a current amplifier. A small current flowing into the base controls a much larger current flowing into the collector.&lt;br /&gt;
[[File:Transcurrentamp.png|right|200px]]&lt;br /&gt;
# Ground the emitter of a [[Media:TIP31C.pdf |TIP31C]] npn transistor. Put a 22 Ohm resistor in parallel with a MM in ammeter mode between the collector and a +2.5VDC supply. Put a 1kOhm resistor in series with an ammeter between the base and the +2.5VDC supply.&lt;br /&gt;
## Measure the collector current and the base current for supply voltages VS between 1.3 to 3VDC.&lt;br /&gt;
## Plot IC/IB vs. VS. &lt;br /&gt;
## What is the proportionality factor between IC and IB at VS = 1.3VDC? &lt;br /&gt;
## Is the proportionality factor independent of VS ?&lt;br /&gt;
## Does the transistor amplify current?&lt;br /&gt;
&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== Operational Amplifiers (OpAmps) ====&lt;br /&gt;
OpAmps are integrated circuits (ICs) that contain within them many transistors, resistors, capacitors and possibly diodes miniaturized into a single IC component (see chapter 9 of the eBook ''Starting Electronics''). [[File:Op-Amp.jpg|thumb|What an OpAmp actually looks like|100px]] OpAmps are very high gain dc-coupled differential amplifiers with single-ended outputs and are usually employed with feedback.&lt;br /&gt;
The OpAmp we will be using is National semiconductor's general purpose [[Media:LM741.pdf| LM741]]. OpAmp behaviour can may be simplified into two simple rules.&lt;br /&gt;
* The output attempts to do whatever is necessary to make the voltage difference between the inputs zero.&lt;br /&gt;
* The inputs draw no (very little anyway) current.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[File:Opamp.jpg|thumb|right|150px|OpAmp circuit symbol]]&lt;br /&gt;
# Use an LM741, a 1kOhm and a 500Ohm resistor to construct the non-inverting amplifier shown at the right (power to OpAmp not shown).[[File:Noninverting.png|thumb|Non-inverting amplifier]]&lt;br /&gt;
## Power the OpAmp at +10VDC and -10VDC.&lt;br /&gt;
## Apply a +1VDC signal to the input and measure the output voltage.&lt;br /&gt;
## Can you explain the OpAmps behaviour in terms of the first rule above?&lt;br /&gt;
## What is the gain of your amplifier (Vout/Vin)?&lt;br /&gt;
## What is the value of 1 + Rf/Rg?&lt;br /&gt;
## Are these last two values the same?&lt;br /&gt;
## Replace Rf with Rg and Rg with Rf.&lt;br /&gt;
## Apply a +1VDC signal to the input and measure the output voltage.&lt;br /&gt;
## What is the gain of your amplifier (Vout/Vin)? &lt;br /&gt;
## What is the value of 1 + Rf/Rg (remember you switched the values of Rf and Rg)?&lt;br /&gt;
## What is the general formula for the gain of a non-inverting amplifier?&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
# Reconfigure the LM741, the 1kOhm and 500Ohm resistors for an inverting amplifier (see diagram at right).[[File:Inverting_Amplifier.png|thumb|Inverting amplifier|200px]]&lt;br /&gt;
# Apply a +1VDC input and measure the output.&lt;br /&gt;
## Can you explain the OpAmps behaviour in terms of the first rule above?&lt;br /&gt;
## What is the gain of your amplifier (Vout/Vin)?&lt;br /&gt;
## What is the value of -Rf/Rin&lt;br /&gt;
## Are these last two values the same?&lt;br /&gt;
## Switch Rf and Rin.&lt;br /&gt;
## Apply a -1VDC signal to the input and measure the output voltage.&lt;br /&gt;
## What is the gain of your amplifier (Vout/Vin)? &lt;br /&gt;
## What is the value of -Rf/Rin (remember you switched the values of Rf and Rin)?&lt;br /&gt;
## What is the general formula for the gain of an inverting amplifier?&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
==== Instrumentation and Loading ====&lt;br /&gt;
Since electronic instruments (MMs, oscilloscopes, function generators, even Opamps, etc.) are composed of resistors, capacitors, inductors, diodes, transistors, OpAmps, etc., they have characteristic net input and output impedances.&lt;br /&gt;
&lt;br /&gt;
Consider the simple voltage divider circuit shown at the right.[[File:Voltagedivider.gif|100px|right]]&lt;br /&gt;
Let Vin be 10VDC and R1 = R2 = 10MOhm. Based on your experience in section 5 above what do you think Vout should be?&lt;br /&gt;
# Construct the voltage divider.&lt;br /&gt;
## Let R1 = R2 = 1kOhms. Measure Vout. Is Vout what you expected?&lt;br /&gt;
## Change both resistors to 10kOhm. Measure Vout. Is Vout what you expected?&lt;br /&gt;
## Change both resistors to 500kOhm. Measure Vout. Is Vout what you expected?&lt;br /&gt;
## Change both resistors to 1MOhm. Measure Vout. Is Vout what you expected?&lt;br /&gt;
## Change both resistors to 10MOhm. Measure Vout. Is Vout what you expected?&lt;br /&gt;
## Plot Vout vs. R2.&lt;br /&gt;
## What do you think is going on? Remember how the MM measures voltage. &lt;br /&gt;
&lt;br /&gt;
This voltage sagging effect is the result of circuit loading. The MM bleeds off a small bit of the current and runs it through a very precise calibrated large value resistor (usually between 1MOhm and 10MOhms). When R2 is 1kOhm the MM bleeds off a very small fraction of the current that should have flowed through R2. Consequently, the measured voltage at Vout sags minimally. However, as R2 increases to values approaching the MM's &amp;quot;internal&amp;quot; resistance (or input impedance) the MM draws off larger and larger fractions of the current that should have run through R2. Consequently, the measured voltage at Vout sags substantially. &lt;br /&gt;
&lt;br /&gt;
The voltage divider and MM can be thought of as a two stage electrical device. The first stage does something and then &amp;quot;hands off&amp;quot; the result to the second stage which also does something.&lt;br /&gt;
&lt;br /&gt;
What can you say about the output impedance of a first-stage electronic device in relation to the input impedance of a second-stage electronic device?&lt;br /&gt;
&lt;br /&gt;
==== Unity Gain Non-Inverting Amplifier: The Follower or Buffer ====&lt;br /&gt;
The above consideration on instrumentation and loading naturally lead to a very useful OpAmp device. A follower (pictured at right) [[File:Follower.png|thumb|200px| The follower]] is a unity gain non-inverting amplifier. Why would anyone want this? It just reproduces what you've already got. &lt;br /&gt;
&lt;br /&gt;
Well let's consider the follower's input and output impedances. From the second simple rule for OpAmps (see above) the input impedance (looking into the (+) OpAmp input) is &amp;quot;infinite&amp;quot; (well, very high anyway as it draws little to no current). The OpAmp's output impedance (looking from Vout to the (-) OpAmp input) is zero (or very nearly).&lt;br /&gt;
&lt;br /&gt;
So the follower has the useful properties that it's input impedance is &amp;quot;infinite&amp;quot; and it's output impedance is &amp;quot;zero&amp;quot;. This would have been a wonderful thing to have between the voltage divider stage and the MM stage in the previous section.&lt;br /&gt;
&lt;br /&gt;
# Redo the measurements of the previous section with the follower (or in this case it's maybe better to call it a buffer) in between the stages.&lt;br /&gt;
## Plot the new Vout vs. R2.&lt;br /&gt;
## Does Vout still sag with increasing R2?&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==== Optoelectronics ====&lt;br /&gt;
The electronic components considered above lie completely in the realm of &amp;quot;pure&amp;quot; electronics. In addition to these &amp;quot;pure&amp;quot; electronic components there exists hybrid components that blend the characteristics of electronics and optics. These are called optoelectronic (OE) components and include photodiodes (PDs), light-emitting diodes (LEDs) and laser diodes (LDs). We won't go into detail of what these OE components are but just look at how they behave. Suffice it to say, at this point, that the PD, LED and LD are all diodes and if you understand what a diode is you'll go a long way towards understanding these OE devices.&lt;br /&gt;
&lt;br /&gt;
'''The Photodiode or photodetector:''' Photodiodes are very much like the diodes you encountered above with the exception that currents can be induced not only by biasing voltages but also by light (called the photo-current).[[File:PDsymbol.png|thumb|200px| Photodiode symbol]]&lt;br /&gt;
# Measure the &amp;quot;dark&amp;quot; forward I-V curve of Optek's [[Media:OP950.PDF| OP950]] PD. That is, shield the PD from ambient room light while doing the measurement. &lt;br /&gt;
## Plot the dark forward I-V curve.&lt;br /&gt;
## How does it look compared to the &amp;quot;pure&amp;quot; electronic diode's forward I-V curve?&lt;br /&gt;
## At what voltage does the PD &amp;quot;turn on&amp;quot;. How does this compare with the &amp;quot;pure&amp;quot; diode's turn-on voltage?&lt;br /&gt;
## Now open up the PD to ambient room light and look at the forward I-V curve again. Has it changed?&lt;br /&gt;
## Get a red LD module and shine laser light on the PD. Observe the forward I-V curve again. Has it changed?&lt;br /&gt;
## What can you say about the PD's I-V curve as a function of incident light power?&lt;br /&gt;
## Measure the dark reverse I-V curve of the PD between 0 and -25VDC.&lt;br /&gt;
## Open the PD to ambient light and redo the previous measurement.&lt;br /&gt;
## Shine the red laser light on the PD and repeat the measurement again.&lt;br /&gt;
## What can you say about the reverse I-V curve of the PD vs. incident light power?&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
'''The Light Emitting Diode:''' [[File:Led.jpg|thumb|100px| [[File:LED_Symbol.png|thumb|100px| LED symbol]]Typical LED]]The PD above is a device that when light is incident on it a photocurrent is produced. The LED, on the other hand, is a device that when a (suitable) current is induced through it light is produced.&lt;br /&gt;
# Forward bias (positive voltages applied to the Anode) ANDOptoelectronic's [[Media:AND114-R.pdf| AND114-R]] LED between 0 and 2VDC.&lt;br /&gt;
## What happens as the voltage is increased?&lt;br /&gt;
## With a power meter measure the optical power as a function of forward current and plot.&lt;br /&gt;
## Are there distinct regimes of optical output?&lt;br /&gt;
## With a spectrometer measure the optical power as a function of wavelength.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
'''The Laser diode:''' Laser diodes are similar to LEDs but in addition have optical feedback. Without going into detail, this [[File:LD.jpg|thumb|Typical LD|right|100px]]feedback greatly improves the optical characteristics of the LD (think of the difference between a flashlight and a laser pointer). &lt;br /&gt;
&lt;br /&gt;
LEDs are fairly robust devices. You can mistreat them, within reason, and they'll still function (at least to some degree). LDs, on the other hand, are easily destroyed or damaged. &amp;lt;br&amp;gt;&lt;br /&gt;
* Static Electricity: The static electricity generated by walking across a carpet can (and usually does) destroy them. &lt;br /&gt;
* Reverse Bias Voltages: LDs (and LEDs too) are meant to operate in forward bias only. As such, they can be destroyed by applying too high a reverse bias to them (this reverse bias damage value is usually spec'd). &lt;br /&gt;
* Rapid Current Changes: Abruptly cutting off (or turning on) a LD driving current can (and usually does) destroy the LD.&lt;br /&gt;
* Putting too much current through the LD (again, this usually does destroy the LD).&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
For all these reasons LD are usually operated within a protective circuit (see right).[[File:CCcircuit.png|thumb|400px|LD Constant Current (CC) Circuit]]&lt;br /&gt;
&lt;br /&gt;
There are two components you haven't seen yet. The [[Media:LM317.pdf|LM317 ]] and the square blue component (the pot) connected to the middle pin of the LM317. A pot or potentiometer is a variable resistor. It's got a knob or screw that can be turned to adjust its resistance.&lt;br /&gt;
&lt;br /&gt;
Let's discuss the parts of this circuit and what they do to help protect and operate the LD. The LM317 is a voltage regulator. The pot allows for adjusting the LD current and the resistors act to limit the maximum current. The &amp;quot;pure&amp;quot; electronic diode clamps any reverse biases (accidentally applied) to ~ 0.6V (which is below the reverse bias damage value). The capacitor suppresses static discharges or voltage transients and slows the LD turn-on/turn-off behaviour.&lt;br /&gt;
&lt;br /&gt;
In addition to the LD protection circuit always wear an [[Media:Antistaticwb.jpg|antistatic wrist band ]] when handling LDs. &lt;br /&gt;
&lt;br /&gt;
Also, it's always best to test your CC circuit with an LED first (LED is more robust - and cheaper) before trying it with the LD. &amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The LD we'll use is LiteOn's [[Media:LTLD505T.pdf| LTLD505T]]. It has a center wavelength around 650nm, 5mW optical power, turn-on (or threshold) current around 35mA, operating current 45mA, operating voltage around 2.4V, max operating voltage 2.6V and max reverse voltage of  &lt;br /&gt;
2V.&lt;br /&gt;
&lt;br /&gt;
# Put together this LD CC circuit with V(-) at ground, V(+) at 7VDC, a 1K pot, , R = 30Ohms, C = 10&amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt;f and a  P6KE6.8 diode (oriented the correct way).&lt;br /&gt;
## Test the CC circuit with an LED (cathode grounded).&lt;br /&gt;
## Does the circuit light up the LED? If yes, proceed. If not, troubleshoot the circuit.&lt;br /&gt;
## Replace the LED with the LD (remember to wear the antistatic wrist band).&lt;br /&gt;
## Does the circuit light up the LD? Is yes, proceed. If not, troubleshoot.&lt;br /&gt;
## With the power meter measure the optical power vs. LD current. What's the turn-on current? Is it close to the LD's spec'd threshold current?&lt;br /&gt;
## What is the optical power at the operating current?&lt;br /&gt;
## Are there distinct optical regimes?&lt;br /&gt;
## How does the LD's threshold current relate to these regimes?&lt;br /&gt;
## With a spectrometer measure and plot the optical power vs. wavelength for currents just below threshold and well above threshold.&lt;br /&gt;
## Are these plots similar? Explain.&amp;lt;BR&amp;gt;&amp;lt;BR&amp;gt;&amp;lt;BR&amp;gt;&lt;br /&gt;
* Submit a write-up outlining your activities, results and the answers to all the questions asked above.&amp;lt;br&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
&lt;br /&gt;
* '''CLEAN UP THE OBSTACLE COURSE SETUP AFTER USE'''&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Robotics&amp;diff=2823</id>
		<title>Robotics</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Robotics&amp;diff=2823"/>
		<updated>2017-01-18T01:51:38Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: Created page with &amp;quot;Let's keep this page tidy. That is, let's create links to subpages (that contain possibly further subpages) that contain the various robotics projects and related topics.&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Let's keep this page tidy. That is, let's create links to subpages (that contain possibly further subpages) that contain the various robotics projects and related topics.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Advanced_Projects&amp;diff=2822</id>
		<title>Advanced Projects</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Advanced_Projects&amp;diff=2822"/>
		<updated>2017-01-13T20:55:15Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: /* Computational Projects */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Optics Projects ==&lt;br /&gt;
&lt;br /&gt;
* [[Spontaneous Parametric Downconversion]]&lt;br /&gt;
&lt;br /&gt;
* [[Sonoluminescence]]&lt;br /&gt;
&lt;br /&gt;
* [[Optical Tweezers]]&lt;br /&gt;
&lt;br /&gt;
* [[Optical Tweezers for Biology]]&lt;br /&gt;
&lt;br /&gt;
* [[External-Cavity Tuneable Diode Laser]]&lt;br /&gt;
&lt;br /&gt;
* [[Optics Modeling with Optica]]&lt;br /&gt;
&lt;br /&gt;
* [[Schlieren Flow Visualization]]&lt;br /&gt;
&lt;br /&gt;
== Fiber-Optic Projects ==&lt;br /&gt;
* [[Modelocked Fiberlaser]]&lt;br /&gt;
&lt;br /&gt;
* [[Sagnac Fiber-Optic Gyroscope]]&lt;br /&gt;
&lt;br /&gt;
* [[Erbium-Doped Fiber Amplifier &amp;amp; CW Laser]]&lt;br /&gt;
&lt;br /&gt;
* [[Mode-locked Erbium-Ytterbium Doped Fiber Laser]]&lt;br /&gt;
&lt;br /&gt;
* [[Master Oscillator Power Amplifier Pulsed Laser]]&lt;br /&gt;
&lt;br /&gt;
*[[Graphene as Saturable Absorber]]&lt;br /&gt;
&lt;br /&gt;
* [[Fiber Simulations with RP Fiber Power]]&lt;br /&gt;
&lt;br /&gt;
*[[Optical Chaos with External Feedback Mirror]]&lt;br /&gt;
&lt;br /&gt;
== Solid State Projects ==&lt;br /&gt;
&lt;br /&gt;
* [[Atomic Force Microscope]]&lt;br /&gt;
&lt;br /&gt;
* [[OAM &amp;amp; Surface Plasmon Resonance]]&lt;br /&gt;
&lt;br /&gt;
* [[Superconductivity]]&lt;br /&gt;
&lt;br /&gt;
* [[Physics of Semiconductor Devices]]&lt;br /&gt;
&lt;br /&gt;
* [[Physical Adsorption]]&lt;br /&gt;
&lt;br /&gt;
==Thermodynamics==&lt;br /&gt;
&lt;br /&gt;
* [[Heat Content Asymptotics]]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Computational Projects ==&lt;br /&gt;
&lt;br /&gt;
* [[MEEP]]&lt;br /&gt;
&lt;br /&gt;
* [[Parallel Programming on the APL Cluster]]&lt;br /&gt;
&lt;br /&gt;
* [[Data Mining]]&lt;br /&gt;
&lt;br /&gt;
* [[Robotics]]&lt;br /&gt;
&lt;br /&gt;
== Astronomical Projects ==&lt;br /&gt;
&lt;br /&gt;
* [[Observational Astronomy]]&lt;br /&gt;
&lt;br /&gt;
== Useful Info==&lt;br /&gt;
&lt;br /&gt;
[[Media:How_To_Make_A_Cable.pdf | How To Make a Multi-Strand Shielded Cable]]&lt;br /&gt;
&lt;br /&gt;
[[Media:How_To_Connectorize_BNC_Cables.pdf | How To Make a BNC Cable]]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2777</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2777"/>
		<updated>2016-05-28T01:22:32Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
== Simplified Circuit ==&lt;br /&gt;
&lt;br /&gt;
Lock-in amplifiers are important and powerful devices, but their circuits are not particularly complicated.  The block diagram consists of five parts and is shown below:&lt;br /&gt;
&lt;br /&gt;
1. AC amplifier, called the signal amplifier;&lt;br /&gt;
&lt;br /&gt;
2. Voltage controlled oscillator (VCO);&lt;br /&gt;
&lt;br /&gt;
3. Multiplier, called the phase sensitive detector (PSD);&lt;br /&gt;
&lt;br /&gt;
4. Low-pass filter; and&lt;br /&gt;
&lt;br /&gt;
5. DC amplifier. &lt;br /&gt;
&lt;br /&gt;
[[File:Circuite.jpg]]&lt;br /&gt;
&lt;br /&gt;
The '''AC amplifier''' is simply a voltage amplifier combined with variable filters. Some&lt;br /&gt;
lock-in amplifiers let you change the filters as you wish, others do not. Some lock-in&lt;br /&gt;
amplifiers have the output of the AC amplifier stage available at the signal monitor&lt;br /&gt;
output. Many do not.&lt;br /&gt;
&lt;br /&gt;
The '''voltage controlled oscillator''' is just an oscillator, except that it can synchronize with&lt;br /&gt;
an external reference signal (i.e., trigger) both in phase and frequency. Some lock-in&lt;br /&gt;
amplifiers contain a complete oscillator and need no external reference. In this case they&lt;br /&gt;
operate at the frequency and amplitude that you set, and you must use their oscillator&lt;br /&gt;
output in your experiment to derive the signal that you ultimately wish to measure.&lt;br /&gt;
Virtually all lock-in amplifiers are able to synchronize with an external reference signal.&lt;br /&gt;
The VCO also contains a phase-shifting circuit that allows the user to shift its signal from&lt;br /&gt;
0-360 degrees with respect to the reference.&lt;br /&gt;
&lt;br /&gt;
The '''phase sensitive detector''' is a circuit which takes in two voltages as inputs V1 and V2&lt;br /&gt;
and produces an output which is the product V1*V2. That is, the PSD is just a multiplier&lt;br /&gt;
circuit.&lt;br /&gt;
&lt;br /&gt;
The '''low pass filter''' is an RC filter whose time constant may be selected. In many cases&lt;br /&gt;
you may choose to have one RC filter stage (single pole filter) or two RC filter stages in&lt;br /&gt;
series (2-pole filter). In newer lock-in amplifiers, this might be a digital filter with the&lt;br /&gt;
attenuation of a &amp;quot;many pole&amp;quot; filter.&lt;br /&gt;
&lt;br /&gt;
The '''DC amplifier''' is just a low-frequency amplifier similar to those frequently assembled&lt;br /&gt;
with op-amps. It differs from the AC amplifier in that it works all the way down to zero&lt;br /&gt;
frequency (DC) and is not intended to work well at very high frequencies, say above 10&lt;br /&gt;
KHz.&lt;br /&gt;
&lt;br /&gt;
This block diagram comes from Useful Link number 3, below.&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2776</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2776"/>
		<updated>2016-05-28T01:19:39Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
== Simplified Circuit ==&lt;br /&gt;
&lt;br /&gt;
Lock-in amplifiers are important and powerful devices, but their circuits are not particularly complicated.  The block diagram consists of five parts and is shown below:&lt;br /&gt;
&lt;br /&gt;
1. AC amplifier, called the signal amplifier;&lt;br /&gt;
&lt;br /&gt;
2. Voltage controlled oscillator (VCO);&lt;br /&gt;
&lt;br /&gt;
3. Multiplier, called the phase sensitive detector (PSD);&lt;br /&gt;
&lt;br /&gt;
4. Low-pass filter; and&lt;br /&gt;
&lt;br /&gt;
5. DC amplifier. &lt;br /&gt;
&lt;br /&gt;
[[File:Circuite.jpg]]&lt;br /&gt;
&lt;br /&gt;
The '''AC amplifier''' is simply a voltage amplifier combined with variable filters. Some&lt;br /&gt;
lock-in amplifiers let you change the filters as you wish, others do not. Some lock-in&lt;br /&gt;
amplifiers have the output of the AC amplifier stage available at the signal monitor&lt;br /&gt;
output. Many do not.&lt;br /&gt;
&lt;br /&gt;
The '''voltage controlled oscillator''' is just an oscillator, except that it can synchronize with&lt;br /&gt;
an external reference signal (i.e., trigger) both in phase and frequency. Some lock-in&lt;br /&gt;
amplifiers contain a complete oscillator and need no external reference. In this case they&lt;br /&gt;
operate at the frequency and amplitude that you set, and you must use their oscillator&lt;br /&gt;
output in your experiment to derive the signal that you ultimately wish to measure.&lt;br /&gt;
Virtually all lock-in amplifiers are able to synchronize with an external reference signal.&lt;br /&gt;
The VCO also contains a phase-shifting circuit that allows the user to shift its signal from&lt;br /&gt;
0-360 degrees with respect to the reference.&lt;br /&gt;
&lt;br /&gt;
The '''phase sensitive detector''' is a circuit which takes in two voltages as inputs V1 and V2&lt;br /&gt;
and produces an output which is the product V1*V2. That is, the PSD is just a multiplier&lt;br /&gt;
circuit.&lt;br /&gt;
&lt;br /&gt;
The '''low pass filter''' is an RC filter whose time constant may be selected. In many cases&lt;br /&gt;
you may choose to have one RC filter stage (single pole filter) or two RC filter stages in&lt;br /&gt;
series (2-pole filter). In newer lock-in amplifiers, this might be a digital filter with the&lt;br /&gt;
attenuation of a &amp;quot;many pole&amp;quot; filter.&lt;br /&gt;
&lt;br /&gt;
The '''DC amplifier''' is just a low-frequency amplifier similar to those frequently assembled&lt;br /&gt;
with op-amps. It differs from the AC amplifier in that it works all the way down to zero&lt;br /&gt;
frequency (DC) and is not intended to work well at very high frequencies, say above 10&lt;br /&gt;
KHz.&lt;br /&gt;
&lt;br /&gt;
This circuit diagram comes from useful link number 3, below.&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2775</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2775"/>
		<updated>2016-05-28T01:18:08Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
== Simplified Circuit ==&lt;br /&gt;
&lt;br /&gt;
Lock-in amplifiers are important and powerful devices, but their circuits are not particularly complicated.  The block diagram consists of five parts and is shown below:&lt;br /&gt;
&lt;br /&gt;
1. AC amplifier, called the signal amplifier;&lt;br /&gt;
&lt;br /&gt;
2. Voltage controlled oscillator (VCO);&lt;br /&gt;
&lt;br /&gt;
3. Multiplier, called the phase sensitive detector (PSD);&lt;br /&gt;
&lt;br /&gt;
4. Low-pass filter; and&lt;br /&gt;
&lt;br /&gt;
5. DC amplifier. &lt;br /&gt;
&lt;br /&gt;
[[File:Circuite.jpg]]&lt;br /&gt;
&lt;br /&gt;
The AC amplifier is simply a voltage amplifier combined with variable filters. Some&lt;br /&gt;
lock-in amplifiers let you change the filters as you wish, others do not. Some lock-in&lt;br /&gt;
amplifiers have the output of the AC amplifier stage available at the signal monitor&lt;br /&gt;
output. Many do not.&lt;br /&gt;
&lt;br /&gt;
The voltage controlled oscillator is just an oscillator, except that it can synchronize with&lt;br /&gt;
an external reference signal (i.e., trigger) both in phase and frequency. Some lock-in&lt;br /&gt;
amplifiers contain a complete oscillator and need no external reference. In this case they&lt;br /&gt;
operate at the frequency and amplitude that you set, and you must use their oscillator&lt;br /&gt;
output in your experiment to derive the signal that you ultimately wish to measure.&lt;br /&gt;
Virtually all lock-in amplifiers are able to synchronize with an external reference signal.&lt;br /&gt;
The VCO also contains a phase-shifting circuit that allows the user to shift its signal from&lt;br /&gt;
0-360 degrees with respect to the reference.&lt;br /&gt;
&lt;br /&gt;
The phase sensitive detector is a circuit which takes in two voltages as inputs V1 and V2&lt;br /&gt;
and produces an output which is the product V1*V2. That is, the PSD is just a multiplier&lt;br /&gt;
circuit.&lt;br /&gt;
&lt;br /&gt;
The low pass filter is an RC filter whose time constant may be selected. In many cases&lt;br /&gt;
you may choose to have one RC filter stage (single pole filter) or two RC filter stages in&lt;br /&gt;
series (2-pole filter). In newer lock-in amplifiers, this might be a digital filter with the&lt;br /&gt;
attenuation of a &amp;quot;many pole&amp;quot; filter.&lt;br /&gt;
&lt;br /&gt;
The DC amplifier is just a low-frequency amplifier similar to those frequently assembled&lt;br /&gt;
with op-amps. It differs from the AC amplifier in that it works all the way down to zero&lt;br /&gt;
frequency (DC) and is not intended to work well at very high frequencies, say above 10&lt;br /&gt;
KHz. &lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2774</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2774"/>
		<updated>2016-05-28T01:16:48Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
== Simplified Circuit ==&lt;br /&gt;
&lt;br /&gt;
Lock-in amplifiers are important and powerful devices, but their circuits are not particularly complicated.  The block diagram consists of five parts and is shown below:&lt;br /&gt;
&lt;br /&gt;
1. AC amplifier, called the signal amplifier;&lt;br /&gt;
&lt;br /&gt;
2. Voltage controlled oscillator (VCO);&lt;br /&gt;
&lt;br /&gt;
3. Multiplier, called the phase sensitive detector (PSD);&lt;br /&gt;
&lt;br /&gt;
4. Low-pass filter; and&lt;br /&gt;
&lt;br /&gt;
5. DC amplifier. &lt;br /&gt;
&lt;br /&gt;
[[File:Circuite.jpg]]&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2773</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2773"/>
		<updated>2016-05-28T01:16:23Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
== Simplified Circuit ==&lt;br /&gt;
&lt;br /&gt;
Lock-in amplifiers are important and powerful devices, but their circuits are not particularly complicated.  The block diagram consists of five parts and is shown below:&lt;br /&gt;
&lt;br /&gt;
1. AC amplifier, called the signal amplifier;&lt;br /&gt;
2. Voltage controlled oscillator (VCO);&lt;br /&gt;
3. Multiplier, called the phase sensitive detector (PSD);&lt;br /&gt;
4. Low-pass filter; and&lt;br /&gt;
5. DC amplifier. &lt;br /&gt;
&lt;br /&gt;
[[File:Circuite.jpg]]&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=File:Circuite.jpg&amp;diff=2772</id>
		<title>File:Circuite.jpg</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=File:Circuite.jpg&amp;diff=2772"/>
		<updated>2016-05-28T01:15:24Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2771</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2771"/>
		<updated>2016-05-28T01:15:09Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
== Simplified Circuit ==&lt;br /&gt;
&lt;br /&gt;
Lock-in amplifiers are important and powerful devices, but their circuits are not particularly complicated.  The block diagram consists of five parts and is shown below:&lt;br /&gt;
&lt;br /&gt;
[[File:Circuite.jpg]]&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=File:Circuit.JPG&amp;diff=2770</id>
		<title>File:Circuit.JPG</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=File:Circuit.JPG&amp;diff=2770"/>
		<updated>2016-05-28T01:13:59Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2769</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2769"/>
		<updated>2016-05-28T01:13:26Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
== Simplified Circuit ==&lt;br /&gt;
&lt;br /&gt;
Lock-in amplifiers are important and powerful devices, but their circuits are not particularly complicated.  The block diagram consists of five parts and is shown below:&lt;br /&gt;
&lt;br /&gt;
[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2768</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2768"/>
		<updated>2016-05-28T01:12:31Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Simplified Circuit ==&lt;br /&gt;
&lt;br /&gt;
Lock-in amplifiers are important and powerful devices, but their circuits are not particularly complicated.  The block diagram consists of five parts and is shown below:&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2767</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2767"/>
		<updated>2016-05-28T01:10:54Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Simplified Circuit ==&lt;br /&gt;
&lt;br /&gt;
Testing&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2763</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2763"/>
		<updated>2016-04-25T19:00:51Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
The Model 5202 is an advanced lock-in amplifier and it has two outputs, one labeled 'in-phase' and the other labeled 'quadrature'.  This lock-in actually does the entire calculation twice, the second time with a 90 degree phase shift between input and reference.  These two output quantities represent the signal as a vector relative to the lock-in reference oscillator. By computing the magnitude of the signal vector (adding the 'in-phase' and 'quadrature' values in quadrature), the phase dependency is removed.&lt;br /&gt;
&lt;br /&gt;
So far the results of our lock-in amplifier are less than exciting.  We are inputting a sine wave and the lock-in tells us its strength.  The real use of a lock-in is of course to pull a quiet signal out of a noisy environment.&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2762</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2762"/>
		<updated>2016-04-25T18:53:50Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;br /&gt;
&lt;br /&gt;
[http://www.lehigh.edu/~jph7/website/Physics262/LockInAmplifierAndApplications.pdf Another Paper on Lock-in Amplifiers]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2761</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2761"/>
		<updated>2016-04-25T18:41:09Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier (if it has one) is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  If you change the frequency of the reference or input signals the output of the lock-in should drop off as well.&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2757</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2757"/>
		<updated>2016-04-20T23:35:53Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  The lock-in's output should be connected to the oscilloscope though.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
Hopefully the &amp;quot;Unlock&amp;quot; light on the lock-in amplifier is currently lit up, signifying that there is no reference signal locked.  Now we should plug in our reference output from the function generator into the reference input of the lock-in.  After plugging in the BNC and making sure that the function generator output is active we should see the &amp;quot;Unlock&amp;quot; light turn off.  That means the lock-in is locked to the reference frequency.  Now we can plug in our input signal from the function generator to the lock-in.  After doing so we should see an output voltage showing up on the oscilloscope (and also on the front of the Model 5202).  The lock-in amplifier is now locked in on the reference frequency and displaying the strength of that signal.  If you change the signal strength of the input signal then you should see the output change accordingly.  &lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2756</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2756"/>
		<updated>2016-04-20T23:24:43Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  All devices must of course be powered but for now the lock-in doesn't have to be connected to the function generator.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  Something like 1 MHz should work.&lt;br /&gt;
&lt;br /&gt;
The amplitudes of each signal are once again up to you, but the Model 5202 lock-in has a maximum input voltage of 5 Vrms, so make sure the amplitude of that signal is below that.  Something like 5 mVpp should work.  The reference signal on the other hand should be slightly larger.  Something like 1 Vpp, for example.&lt;br /&gt;
&lt;br /&gt;
There are various settings on the front of the lock-in, some of which should be looked at.  The first dial on the left (Model 5202) represents a sensitivity, and for now can be set to something like 25 mV.  This can be changed later to make our equipment more sensitive.  There is also a setting for the reference phase (0 deg, 90 deg, 180 deg, etc.).  This is the phase difference applied to the reference signal when compared to the input signal.  For now it can be left to 0 degrees.  There may also be a setting for what waveform the reference will be.  We would want that set to a standard sinusoidal waveform.  The Model 5202 has some other Output settings as well, most of which can be left at the default.  The time constant can be left at the lowest value (ex. 10 ms).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2755</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2755"/>
		<updated>2016-04-20T23:06:17Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment: Lock-In Amplifier, Function Generator (two outputs), Oscilloscope, BNC Cables&lt;br /&gt;
&lt;br /&gt;
There are multiple lock-in amplifiers in the lab, so the choice of which to use is yours.  There is one Model 5104 from Princeton Applied Research that may not be working properly, so you may want to avoid that device.  The Model 5202 from Princeton Applied Research was tested and seems to be working as it should.  Each lock-in amplifier has slightly different menus/controls, but the basics are all similar.&lt;br /&gt;
&lt;br /&gt;
Now that we have our equipment and a space in the lab to work we can set up our instruments.  Hopefully the function generator that you're using has two outputs, if it doesn't then another function generator might have to be used.  One of these outputs will be the reference signal and the other will be the lock-in's input signal.  Both signals should be sine waves for now and the frequencies of each can be set to whatever you desire, but if you're using the Model 5202 for example, then there is a corresponding setting on the lock-in for the reference signal frequency.  So you should make sure that dial is set to the right setting for whatever reference frequency you're using.  For now the reference signal and the input signal &lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2754</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2754"/>
		<updated>2016-04-20T22:48:07Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
Required Equipment:&lt;br /&gt;
&lt;br /&gt;
Lock-In Amplifier&lt;br /&gt;
&lt;br /&gt;
Function Generator&lt;br /&gt;
&lt;br /&gt;
Oscilloscope &lt;br /&gt;
&lt;br /&gt;
BNC Cables&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2753</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2753"/>
		<updated>2016-04-18T18:35:08Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2752</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2752"/>
		<updated>2016-04-18T18:34:57Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Informational PDF from Stanford Research Systems]&lt;br /&gt;
[http://www.phys.utk.edu/labs/modphys/lock-in%20amplifier%20experiment.pdf Paper on Phase Sensitive Detection]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2751</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2751"/>
		<updated>2016-04-18T18:33:16Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.thinksrs.com/downloads/PDFs/ApplicationNotes/AboutLIAs.pdf Information PDF from Stanford Research Systems]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2750</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2750"/>
		<updated>2016-04-18T18:30:36Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2749</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2749"/>
		<updated>2016-04-18T18:28:15Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Try it in the Lab ==&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2748</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2748"/>
		<updated>2016-04-18T18:26:46Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Try it out in the Lab ==&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2747</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2747"/>
		<updated>2016-04-18T18:25:56Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The out of phase component of the signal that has the same frequency as the reference signal is also attenuated (sine functions are orthogonal to cosine functions of the same frequency), making lock-in amplifiers phase sensitive detectors.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by an adjustable low pass filter.  Traditional lock-in amplifiers used analog frequency mixers and RC filters for the demodulation, but modern devices are typically digital and use fast digital signal processing.  Sine and cosine demodulation is usually performed simultaneously (dual phase demodulation).&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2746</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2746"/>
		<updated>2016-04-18T18:15:58Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by a low-pass filter.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=File:Example.jpg&amp;diff=2745</id>
		<title>File:Example.jpg</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=File:Example.jpg&amp;diff=2745"/>
		<updated>2016-04-18T18:15:26Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: Wikiuser uploaded a new version of &amp;amp;quot;File:Example.jpg&amp;amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=File:Example.jpg&amp;diff=2744</id>
		<title>File:Example.jpg</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=File:Example.jpg&amp;diff=2744"/>
		<updated>2016-04-18T18:12:47Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: Wikiuser uploaded a new version of &amp;amp;quot;File:Example.jpg&amp;amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=File:Example.jpg&amp;diff=2743</id>
		<title>File:Example.jpg</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=File:Example.jpg&amp;diff=2743"/>
		<updated>2016-04-18T18:08:20Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2742</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2742"/>
		<updated>2016-04-18T18:07:43Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;In Progress&lt;br /&gt;
&lt;br /&gt;
[[File:Example.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by a low-pass filter.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2741</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2741"/>
		<updated>2016-04-18T18:04:54Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;In Progress&lt;br /&gt;
&lt;br /&gt;
[[File:http://www.thinksrs.com/assets/instr/SR810830/SR830_FPlg.jpg]]&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by a low-pass filter.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2740</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2740"/>
		<updated>2016-04-18T18:01:55Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;In Progress&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  The output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by a low-pass filter.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Setting_up_the_cluster&amp;diff=2737</id>
		<title>Setting up the cluster</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Setting_up_the_cluster&amp;diff=2737"/>
		<updated>2016-04-13T02:18:44Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&amp;lt;h1&amp;gt;Building a Beowulf Cluster (MPICH2)&amp;lt;/h1&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Prerequisites&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Have computers&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Have computers on the same network connected by ethernet. &amp;amp;nbsp;I can't explain that too much because I don't know much about it, but I assume you can just get any sort of server console and hook them up via that.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Be ok with wiping the computers. &amp;amp;nbsp;I installed clean versions of Ubuntu onto the cluster I made.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Also, if you want to look at other sources, these are two sources that were very helpful to me&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;https://www-users.cs.york.ac.uk/~mjf/pi_cluster/src/Building_a_simple_Beowulf_cluster.html&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;https://help.ubuntu.com/community/MpichCluster&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Let's Go&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;ol&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Get a copy of Ubuntu 14.04 &amp;lt;b&amp;gt;Server&amp;lt;/b&amp;gt;. &amp;amp;nbsp;If you really want to, you can install a gui interface onto it later, like unity.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ol&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;1? Install Ubuntu&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;This in itself can be a process, and is slow. &amp;amp;nbsp;At least on my computers it was.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Make the bootable USB.&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;At the time of writing this, you can download Ubuntu 14.04 Server here.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;http://www.ubuntu.com/download/server&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;I'm sure that if a newer version comes out, it should work as well, although I tried initially with 15.10 (Desktop) and had some trouble with that.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;&amp;lt;strong&amp;gt;&amp;lt;/strong&amp;gt;Choose a master node&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;People recommend that the master node be the most powerful. &amp;amp;nbsp;Of course if you are using identical computers just choose whichever. &amp;amp;nbsp;In my case, I had 1 computer with 4 cores, whereas the rest had 2.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Plop the usb into the master node and get to the install screen.&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;If you're not booting from the usb it may be because it is not the top priority in the boot sequence. &amp;amp;nbsp;To change this you'll need to go to the bios setup screen.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;While the computer is booting up press f2 or the Delete key. &amp;amp;nbsp;(It could be either or, some manufacturers choose different keys, but that's what it usually is)&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Find the settings for something along the lines of &amp;quot;Boot Sequence&amp;quot;.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Identify the usb and move it to the top. &amp;amp;nbsp;Save and Reboot.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Once you got that all working we can start installing Ubuntu!&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;1. Installing Ubuntu For Reals&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;The installation is mostly straightforward but just follow along to make sure we're on the same page. &amp;amp;nbsp;There are a few things that need to be done during this process - like not encrypting the home directory.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ol&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Do not detect keyboard layout - Choose EN - US (or whichever you'd prefer) manually&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Why? &amp;amp;nbsp;I'm actually not sure, it was just what I was directed to do. &amp;amp;nbsp;Follow directions and stop asking questions. &amp;amp;nbsp;These were directions for installing 12.04, so maybe there was a bug in the autodetect feature.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Set host name to ub&amp;amp;lt;x&amp;amp;gt;, where x is the node number.&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;For example, the master node should be ub0.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Set the name of the new user to &amp;quot;new-user&amp;quot;.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Set the account name to &amp;quot;new-user&amp;quot;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;This might not be an option for you. &amp;amp;nbsp;I don't think I was given this option.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Do not encrypt the home directory.&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;If you do, setting up a shared folder with nfs will be rather difficult.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Partition Method: Guided Use Entire Disk&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Remove existing logical volume data&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Basically just allow it to overwrite whatever it wants.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Leave HTTP proxy information blank&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;No Automatic Updates&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Choose software to install. &amp;amp;nbsp;Just select OpenSSH&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Note that you actually have to press the spacebar to select the option. &amp;amp;nbsp;If you press enter it will just go on without installing. &amp;amp;nbsp;If you do this, it's ok. &amp;amp;nbsp;You can install it later with sudo apt-get later.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Install GRUB&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Hooray!&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Repeat this process for your other nodes. &amp;amp;nbsp;You can of course do some now and some later (I did), though it may be easier to just do them all at once.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ol&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;2. Setting up your hosts file&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;You'll want to do this so that you don't have to type in an entire ip address everytime you want to communicate with another node. &amp;amp;nbsp;Write a list of each ip address and which node it corresponds to.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Set this up on&amp;amp;nbsp;&amp;lt;em&amp;gt;every&amp;amp;nbsp;&amp;lt;/em&amp;gt;node. &amp;amp;nbsp;Go edit the hosts file like so.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;allnodes: sudo nano /etc/hosts/&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Write to the file so it looks like this&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;pre&amp;gt;127.0.0.1	localhost&lt;br /&gt;
192.168.1.6	ub0&lt;br /&gt;
192.168.1.7	ub1&lt;br /&gt;
192.168.1.8	ub2&lt;br /&gt;
192.168.1.9	ub3&amp;lt;/pre&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;amp;nbsp;Be sure that each name is only used once, and replace the ip addresses with yours. &amp;amp;nbsp;You can find the ip address of each node by using&amp;amp;nbsp;&amp;lt;code&amp;gt;ifconfig&amp;lt;/code&amp;gt;in the terminal.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;3. Adding the Cluster User&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Now we'll make a new user that will be our cluster user. &amp;amp;nbsp;This user will have the same name and password on every node. &amp;amp;nbsp;I will call my user &amp;quot;beo&amp;quot;, for beowulf. &amp;amp;nbsp;We also need to clarify a user id. &amp;amp;nbsp;Make the id be a number between 900 and 999. &amp;amp;nbsp;That makes it so it is a user that doesn't show up in the usual gui interface.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Take note that I will write which node the command needs to be run on, followed by a colon, before writing the actual command.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;allnodes: sudo adduser beo --uid 999&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;4. Sharing Your Home Directory With NFS&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Now we need to set up nfs on the master node so that you can share a folder for programs and whatnot. &amp;amp;nbsp;This is so you don't have to install a lot of things on every single node, or put a script on every single computer. &amp;amp;nbsp;As you can imagine that would be quite tedious, especially if you have many nodes.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Install nfs-kernel-server on the master node&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;masternode: sudo apt-get install nfs-kernel-server&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;And on the children nodes install nfs-common&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;span color=&amp;quot;#c7254e&amp;quot;&amp;gt;&amp;lt;span&amp;gt;childnode: sudo apt-get install nfs-common&amp;lt;/span&amp;gt;&amp;lt;/span&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;We will need to indicate which folder we want to share in our exports file. &amp;amp;nbsp;Edit it with nano&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;masternode: sudo nano /etc/exports&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;pre&amp;gt;/home/beo *(rw, sync, no_subtree_check)&amp;lt;/pre&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Add the above line to the bottom of /etc/exports and restart the server&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;masternode: sudo service nfs-kernel-server restart&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Now here, the york article discusses running a sudo ufw allow from &amp;amp;lt;ipaddress&amp;amp;gt;, but I didn't have to do this. &amp;amp;nbsp;If after you run the next few steps you find that your specified folder is not being shared to your other nodes, you may need to check out the york article I posted near the beginning of this post.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Now we need to edit our &amp;lt;code&amp;gt;/etc/fstab&amp;lt;/code&amp;gt;&amp;amp;nbsp;file and install nfs-common on the child nodes. &amp;amp;nbsp;This will tell us where to copy the incoming shared folder from the master node.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;childnode: sudo apt-get install nfs-common&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;childnode: sudo nano /etc/fstab&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Add this line to the file.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;pre&amp;gt;ub0:/home/beo /home/beo nfs&amp;lt;/pre&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Now, when the computer boots it should automatically mount the home directory from the master node, to the child nodes' home directories. &amp;amp;nbsp;Check to see with&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;childnode: ls /home/beo/&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;This should mirror what is on the master node&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;5. Passwordless SSH&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;To get communication working smoothly between the nodes, we're going to want to set up passwordless ssh.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Get on master node&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Change into your cluster user (beo)&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;masternode: su beo&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;masternode:&amp;amp;nbsp;ssh-keygen&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;When asked for a keyphrase, do not enter one. &amp;amp;nbsp;Just leave the field blank, so that it will be &amp;quot;passwordless&amp;quot;.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Once that finishes, run the command&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;masternode: ssh-copy-id localhost&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Now you should be able to quickly log into the other nodes in your cluster through ssh.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;masternode: ssh ub1&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;If you want to change the default port that is used for ssh, we have to make some changes to config files. &amp;amp;nbsp;Unfortunately we have to do this in all nodes.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;allnodes: sudo nano /etc/ssh/ssh_config&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;pre&amp;gt;Port xxxxx&amp;lt;/pre&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;allnodes: sudo nano /etc/ssh/sshd_config&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;pre&amp;gt;Port xxxxx&lt;br /&gt;
PermitRootLogin no&amp;lt;/pre&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Note that there is already a line that says &amp;quot;PermitRootLogin&amp;quot;. &amp;amp;nbsp;Replace that line with the above.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;6. MPICH&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;So there are two main options for setting up a message passing interface on your cluster as far as I can tell. &amp;amp;nbsp;MPICH, and OpenMPI. &amp;amp;nbsp;I am using MPICH. &amp;amp;nbsp;Right before installing mpich2, we might want to install some other software.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;&amp;lt;span&amp;gt;beo@ub0:~$ &amp;lt;/span&amp;gt;sudo apt-get install build-essential gfortran gfortran-multilib autoconf&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Install MPICH2. &amp;amp;nbsp;Now. &amp;amp;nbsp;There are two ways to do this. &amp;amp;nbsp;The easy way, and the way that worked for me. &amp;amp;nbsp;Here's the easy way.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;&amp;lt;span&amp;gt;beo@ub0:~$ &amp;lt;/span&amp;gt;sudo apt-get install mpich2&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;If this works for you, then great! &amp;amp;nbsp;If not, then you're going to have to do the way that worked for me. &amp;amp;nbsp;I had to install the package manually. &amp;amp;nbsp;See&amp;amp;nbsp;&amp;lt;a href=&amp;quot;http://www.mpich.org/static/downloads/3.1.3/mpich-3.1.3-installguide.pdf&amp;quot;&amp;gt;this guide&amp;lt;/a&amp;gt;&amp;amp;nbsp;for how to install it. &amp;amp;nbsp;Make sure to install it in your shared directory, otherwise you're going to have to install it on every node.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;You will need a link to the mpich download. &amp;amp;nbsp;At this time, the download is available at&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;http://www.mpich.org/static/downloads/3.2/mpich-3.2.tar.gz&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Use the&amp;amp;nbsp;&amp;lt;code&amp;gt;wget &amp;amp;lt;link&amp;amp;gt;&amp;lt;/code&amp;gt; command to download the file and then follow the instructions on the guide.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;7. Process Manager&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Once mpich2 is installed we need to set up the machine file so that mpich2 knows how many processes to use in each node. &amp;amp;nbsp;We can make this file somewhere in the shared directory.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;beo@ub0:~$ sudo nano /home/beo/machinefile&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;pre&amp;gt;ub0:4&lt;br /&gt;
ub1:2&lt;br /&gt;
ub2:2&lt;br /&gt;
ub3:4&amp;lt;/pre&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Where we write the node name and how many processes we want to use separated by a colon.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Great! &amp;amp;nbsp;Now everything is set up and should be working, theoretically. Try to test it with this helloworld program from https://help.ubuntu.com/community/MpichCluster&amp;lt;/a&amp;gt;. &amp;amp;nbsp;Place the script in your home directory as &amp;quot;mpi_hello.c&amp;quot;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;pre&amp;gt;#include &amp;amp;lt;stdio.h&amp;amp;gt;&lt;br /&gt;
#include &amp;amp;lt;mpi.h&amp;amp;gt;&lt;br /&gt;
&lt;br /&gt;
int main(int argc, char** argv) {&lt;br /&gt;
    int myrank, nprocs;&lt;br /&gt;
&lt;br /&gt;
    MPI_Init(&amp;amp;amp;argc, &amp;amp;amp;argv);&lt;br /&gt;
    MPI_Comm_size(MPI_COMM_WORLD, &amp;amp;amp;nprocs);&lt;br /&gt;
    MPI_Comm_rank(MPI_COMM_WORLD, &amp;amp;amp;myrank);&lt;br /&gt;
&lt;br /&gt;
    printf(&amp;quot;Hello from processor %d of %d\n&amp;quot;, myrank, nprocs);&lt;br /&gt;
&lt;br /&gt;
    MPI_Finalize();&lt;br /&gt;
    return 0;&lt;br /&gt;
}&amp;lt;/pre&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;You need to compile it and then run it with...&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;&amp;lt;span&amp;gt;beo@ub0:~$ mpicc mpi_hello.c -o mpi_hello&amp;lt;/span&amp;gt;&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;&amp;lt;span&amp;gt;beo@ub0:~$ &amp;lt;/span&amp;gt; mpiexec -n 8 -f /home/beo/machinefile /home/beo/mpi_hello&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;Where -n is the flag for how many processors to use, and -f is the flag for the path to the machinefile.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Installing mpi4py&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;If you're like me and you really like using python, you might want to install mpi4py onto your cluster. &amp;amp;nbsp;This was easy enough for me. &amp;amp;nbsp;I just used pip to install the module. &amp;amp;nbsp;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Don't use sudo apt-get to install mpi4py. &amp;amp;nbsp;Apparently that has given people problems when being used with mpich2.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;&amp;lt;code&amp;gt;&amp;lt;span color=&amp;quot;#c7254e&amp;quot;&amp;gt;&amp;lt;span&amp;gt;&amp;lt;span&amp;gt;beo@ub0:~$ &amp;lt;/span&amp;gt;sudo pip install mpi4py --user&amp;lt;/span&amp;gt;&amp;lt;/span&amp;gt;&amp;lt;/code&amp;gt;&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Notice that I added a --user flag in my pip install. &amp;amp;nbsp;This is because if you do not do this, pip will install the module somewhere in the /usr/ folder, but we want it installed in the shared directory.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;h3&amp;gt;Troubleshooting Errors&amp;lt;/h3&amp;gt;&lt;br /&gt;
&amp;lt;p&amp;gt;During this process I had quite a few errors. &amp;amp;nbsp;I'll try to go through the things that happened to me and tell you how I fixed them.&amp;lt;/p&amp;gt;&lt;br /&gt;
&amp;lt;h4&amp;gt;Installing&amp;amp;nbsp;Ubuntu&amp;lt;/h4&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Got an error right off the bat. &amp;amp;nbsp;&amp;quot;Error loading cdrom&amp;quot;.&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Moved usb to a new port and hit &amp;quot;retry&amp;quot; and it detected everything fine. &amp;amp;nbsp;Strange Error.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;h4&amp;gt;Installing mpich&amp;lt;/h4&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Like I said before, I had problems with using the apt-get install method to install mpich2.&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Installed manually. &amp;amp;nbsp;Use the guide I posted.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;http://www.mpich.org/static/downloads/3.1.3/mpich-3.1.3-installguide.pdf&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;&amp;quot;cannot find hydraproxy file&amp;quot;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;This file is installed when you install mpich2. &amp;amp;nbsp;What I had to do is add its location to my path variable&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;When all was said and done, my .bashrc file had these lines added to it&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;&amp;lt;code&amp;gt;sudo nano ~/.bashrc&amp;lt;/code&amp;gt;&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;&lt;br /&gt;
&amp;lt;pre&amp;gt;export PATH=/home/beo/mpich-install/bin:/home/beo/mpich-install/lib:$PATH&lt;br /&gt;
export LD_LIBRARY_PATH=/usr/lib:/home/beo/mpich-install/lib:$LD_LIBRARY_PATH&lt;br /&gt;
export LD_LIBRARY_PATH=/home/beo/.local/python2.7/site-packages:$LD_LIBRARY_PATH&lt;br /&gt;
export LD_LIBRARY_PATH=/usr/lib/x86_64-linux-gnu:$LD_LIBRARY_PATH&lt;br /&gt;
export HYDRA_HOST_FILE=/home/beo/machinefile&lt;br /&gt;
export PYTHONPATH=/home/beo/.local/python2.7/site-packages:$PYTHONPATH&lt;br /&gt;
export PYTHONPATH=/home/beo/mpich-install/lib:$PYTHONPATH&amp;lt;/pre&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;The HYDRA_HOST_FILE variable didn't actually do what I was hoping it would do, so that line may be unecessary.&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Some error about not being able to find libmpich.so files&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;&amp;lt;code&amp;gt;sudo apt-get install libcr-dev&amp;lt;/code&amp;gt;&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;I actually ran that on each node&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Problems with getting nodes to communicate&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;This was a strange error, but when I was running python programs on the cluster and trying to get the nodes to exchange information, it just refused to work because it couldn't find libmpich.so.10&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;For this I actually physically moved the file to somewhere on the path variable. &amp;amp;nbsp;Also, I couldn't find a file called libmpich.so.10, but I had one called libmpich.so.10.4. &amp;amp;nbsp;So here's what I did&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Move libmpich.so.10.4 from&amp;amp;nbsp;&amp;lt;code&amp;gt;/usr/lib/x86_64-linux-gnu&amp;lt;/code&amp;gt; to &amp;lt;code&amp;gt;/home/beo/mpich-install/lib&amp;lt;/code&amp;gt; then&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Create a symbolic link while in the mpich-install/lib directory&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;&amp;lt;code&amp;gt;sudo ln -s libmpich.so.10.0.4 libmpich.so.10&amp;lt;/code&amp;gt;&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;h4&amp;gt;Python Packages &amp;quot;not installed&amp;quot;&amp;lt;/h4&amp;gt;&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Errors where after installing a python package via &amp;lt;code&amp;gt;pip install &amp;amp;lt;package&amp;amp;gt; --user&amp;lt;/code&amp;gt;, other nodes could not import the module.&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;Saw that the nodes did not have read/write permissions in the shared python package folder. &amp;amp;nbsp;Changed permissions with&lt;br /&gt;
&amp;lt;ul&amp;gt;&lt;br /&gt;
&amp;lt;li&amp;gt;&amp;lt;code&amp;gt;sudo chown -r 755&amp;amp;nbsp;/home/beo/.local/&amp;lt;/code&amp;gt;&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;br /&gt;
&amp;lt;/li&amp;gt;&lt;br /&gt;
&amp;lt;/ul&amp;gt;&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2736</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2736"/>
		<updated>2016-04-11T20:39:07Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;In Progress&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  This means the output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a [https://en.wikipedia.org/wiki/Homodyne_detection homodyne detector] followed by a low-pass filter.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2735</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2735"/>
		<updated>2016-04-11T20:33:48Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;In Progress&lt;br /&gt;
&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  This means the output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a homodyne detector followed by a low-pass filter.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2734</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2734"/>
		<updated>2016-04-11T20:25:54Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and the product is integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  This means the output is a DC signal showing the strength of the original input signal at the reference frequency.&lt;br /&gt;
&lt;br /&gt;
From a circuits standpoint, a lock-in amplifier consists of a homodyne detector followed by a low-pass filter.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2733</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2733"/>
		<updated>2016-04-11T20:04:56Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and then integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  This is the before-mentioned orthogonality of sinusoidal functions.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  This means the output is a DC signal showing the strength of the original signal at the reference frequency.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2732</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2732"/>
		<updated>2016-04-11T20:02:56Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.  High quality lock-in amplifiers can extract signals up to a million times quieter than the surrounding noise.  The output of a lock-in amplifier is a DC signal showing the strength of the signal to be extracted.&lt;br /&gt;
&lt;br /&gt;
== How Does a Lock-In Amplifier Work? ==&lt;br /&gt;
&lt;br /&gt;
Conceptually, a lock-in amplifier works by exploiting the orthogonality of sinusoidal functions.  Use of a lock-in amplifier requires a clear reference signal at the frequency of the signal to be extracted.  This reference signal is multiplied by the noisy input signal and then integrated over a set time.  When sinusoidal functions are multiplied together and integrated over a significant amount of time, the result will be zero unless the two sinusoidal functions have the same frequency.  For the output of a lock-in, this means that the contributions of all signals not at the reference frequency will be attenuated very close to zero.  This is the before-mentioned orthogonality of sinusoidal functions.  This means the output is a DC signal showing the strength of the original signal at the reference frequency.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2731</id>
		<title>Lock-in Amplifier</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=Lock-in_Amplifier&amp;diff=2731"/>
		<updated>2016-04-11T19:29:50Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: Created page with &amp;quot; == What is a Lock-In Amplifier? ==  A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;br /&gt;
== What is a Lock-In Amplifier? ==&lt;br /&gt;
&lt;br /&gt;
A lock-in amplifier is a type of amplifier used to extract quiet signals out of noisy data.&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2730</id>
		<title>LabVIEW Primer</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2730"/>
		<updated>2016-04-03T20:54:54Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Textbook for this Primer ==&lt;br /&gt;
&lt;br /&gt;
This LabVIEW primer is based off of the book [https://books.google.com/books?id=ytwiMTLct48C &amp;quot;Hands-On Introduction to LabVIEW for Scientists and Engineers&amp;quot;] by John Essick.  Two copies of the book can be found in the lab to the right of the computer setup.&lt;br /&gt;
&lt;br /&gt;
== Accessing LabVIEW on Our Computers ==&lt;br /&gt;
&lt;br /&gt;
Currently LabVIEW is installed on one machine in the lab.  When looking at the desktop computers straight on, the rightmost computer closest to the books contains an installation of LabVIEW.  This computer runs Linux but has Windows 7 installed as a virtual machine.  Our version of LabVIEW is installed on Windows, so the Windows virtual machine must be ran before LabVIEW can be accessed.  Running Windows is simple; there is a shortcut on the Linux desktop called &amp;quot;Hankwin&amp;quot; which can be clicked to open.  Once Windows is running, LabVIEW can be found in the Programs menu.&lt;br /&gt;
&lt;br /&gt;
== What is LabVIEW? ==&lt;br /&gt;
&lt;br /&gt;
LabVIEW (Laboratory Virtual Instrument Engineering Workbench) is a development environment and system-design platform for a visual programming language called &amp;quot;G&amp;quot;. LabVIEW is commonly used by scientists and engineers for the purposes of data acquisition, instrument control, and industrial automation.  It is developed and maintained by National Instruments.&lt;br /&gt;
&lt;br /&gt;
LabVIEW is made for engineering and experimental science.  It is a programming language and underneath the hood it does most things similarly to other text-based programming languages, but all of this information is presented to the user very differently.  LabVIEW is a visual and graphical programming language.  Instead of pages of text, LabVIEW source code appears as a graphical block-diagram.  These graphical block-diagrams contain function-nodes (analogous to functions in Python for example) that the user draws virtual wires between.  These virtual wires between different function nodes allow the transfer of variables.  This style of programming is called dataflow programming.&lt;br /&gt;
&lt;br /&gt;
LabVIEW also includes extensive hardware support for interfacing with cameras, sensors, and other devices.  Users can interface to hardware by either writing direct bus commands (USB, GPIB, Serial) or using high-level, device-specific, drivers that provide native LabVIEW function nodes for controlling the device.  LabVIEW's ability to interact with and control different devices is essential to experimental physics and lab work in general.&lt;br /&gt;
&lt;br /&gt;
== Learning from the Text ==&lt;br /&gt;
&lt;br /&gt;
The first four chapters of the text are considered to be essential for understanding the basics of LabVIEW.  They are also meant to be completed sequentially as each section builds on previous sections.  Chapters after number 4 are meant to be more like independent modules that can be completed in any desired order.  The content of chapters is summarized below:&lt;br /&gt;
&lt;br /&gt;
Chapters 1-3: Fundamentals of the LabVIEW Graphical Programming Language.  Central features of LabVIEW including its control loop structures, graphing modes, mathematical functions, and text-based MathScript commands are learned in the course of writing digitized waveform simulation programs.&lt;br /&gt;
&lt;br /&gt;
Chapter 4: Basic Data Acquisition.  Concepts of digitized data such as resolution, sampling frequency, and aliasing are covered.  Then, using LabVIEW's high-level Express VIs, programs are written that execute analog-to-digital, digital-to-analog, and digital input/output tasks on a National Instruments DAQ device.  Computer-based instruments constructed included a DC voltmeter, digital oscilloscope, DC voltage source, waveform generator, and blinking LED array.&lt;br /&gt;
&lt;br /&gt;
Chapters 5-8: More LabVIEW Programming Fundamentals.  Implementation of data file input/output, local memory, and conditional branching in LabVIEW is investigated while writing several useful programs (e.g., spreadsheet data storage, numerical integration, and differentiation).  Additionally, LabVIEW's control flow approach to computer programming is studied.&lt;br /&gt;
&lt;br /&gt;
Chapters 9 and 10: Data Analysis.  Proper use of LabVIEW's curve fitting and fast Fourier transform function is investigated.  Using Express VIs to control a DAQ device, two computer-based instruments (a digitized thermometer and a spectrum analyzer) are constructed.&lt;br /&gt;
&lt;br /&gt;
Chapter 11: Intermediate-Level Data Acquisition.  Programs are written to carry to carry out analog-to-digital, digital-to-analog, and digital counter tasks on a DAQ device using the conventions of DAQmx.  This lower-level approach (in comparison to the high-level Express VIs) allows utilization of the full available range of DAQ device features.  A DC voltmeter, DC voltage source, waveform generator, and frequency meter are constructed, as well as a sophisticated digital oscilloscope based on the state machine architecture.&lt;br /&gt;
&lt;br /&gt;
Chapter 12: Temperature Control Project.  A wide range of the LabVIEW skills acquired throughout the book are used to construct a Proportional-Integral-Derivative (PID) temperature control system.  Appendix I gives a design for the hardware required for this project.&lt;br /&gt;
&lt;br /&gt;
Chapter 13: Control of Stand-Alone Instruments.  Using LabVIEW's VISA communication driver, control of the stand-alone instrument over the General Purpose Interface Bus (GPIB) as well a the Universal Serial Bus (USB) is studied.  An Agilent 34410A Multimeter is used to demonstrate the central concepts of interface bus communication between a PC and stand-alone instrument.&lt;br /&gt;
&lt;br /&gt;
== Chapters from the Text ==&lt;br /&gt;
&lt;br /&gt;
Chapter 1 - The While Loop and Waveform Chart&lt;br /&gt;
&lt;br /&gt;
Chapter 2 - The For Loop and Waveform Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 3 - The Mathscript Node and XY Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 4 - Data Acquisition Using DAQ Assistant&lt;br /&gt;
&lt;br /&gt;
Chapter 5 - Data Files and Character Strings&lt;br /&gt;
&lt;br /&gt;
Chapter 6 - Shift Registers&lt;br /&gt;
&lt;br /&gt;
Chapter 7 - The Case Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 8 - Data Dependency and the Sequence Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 9 - Analysis VIs: Curve Fitting&lt;br /&gt;
&lt;br /&gt;
Chapter 10 - Analysis VIs: Fast Fourier Transform&lt;br /&gt;
&lt;br /&gt;
Chapter 11 - Data Acquisition and Generation Using DAQmx VIs&lt;br /&gt;
&lt;br /&gt;
Chapter 12 - PID Temperature Control Project&lt;br /&gt;
&lt;br /&gt;
Chapter 13 - Control of Stand-Alone Instruments&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.ni.com/f/students/12/7052/en/ Official National Instruments Video Tutorials]&lt;br /&gt;
&lt;br /&gt;
[http://home.hit.no/~hansha/documents/labview/training/Introduction%20to%20LabVIEW/Introduction%20to%20LabVIEW.pdf This LabVIEW tutorial is entirely contained within 1 PDF file, making it easy to download and view as desired.]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2729</id>
		<title>LabVIEW Primer</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2729"/>
		<updated>2016-04-03T20:24:45Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Textbook for this Primer ==&lt;br /&gt;
&lt;br /&gt;
This LabVIEW primer is based off of the book [https://books.google.com/books?id=ytwiMTLct48C &amp;quot;Hands-On Introduction to LabVIEW for Scientists and Engineers&amp;quot;] by John Essick.  Two copies of the book can be found in the lab to the right of the computer setup.&lt;br /&gt;
&lt;br /&gt;
== Accessing LabVIEW on Our Computers ==&lt;br /&gt;
&lt;br /&gt;
Currently LabVIEW is installed on one machine in the lab.  When looking at the desktop computers straight on, the rightmost computer closest to the books contains an installation of LabVIEW.  This computer runs Linux but has Windows 7 installed as a virtual machine.  Our version of LabVIEW is installed on Windows, so the Windows virtual machine must be ran before LabVIEW can be accessed.  Running Windows is simple; there is a shortcut on the Linux desktop called &amp;quot;Hankwin&amp;quot; which can be clicked to open.  Once Windows is running, LabVIEW can be found in the Programs menu.&lt;br /&gt;
&lt;br /&gt;
== What is LabVIEW? ==&lt;br /&gt;
&lt;br /&gt;
LabVIEW (Laboratory Virtual Instrument Engineering Workbench) is a development environment and system-design platform for a visual programming language called &amp;quot;G&amp;quot;. LabVIEW is commonly used by scientists and engineers for the purposes of data acquisition, instrument control, and industrial automation.  It is developed and maintained by National Instruments.&lt;br /&gt;
&lt;br /&gt;
LabVIEW is made for engineering and experimental science.  It is a programming language and underneath the hood it does most things similarly to other text-based programming languages, but all of this information is presented to the user very differently.  LabVIEW is a visual and graphical programming language.  Instead of pages of text, LabVIEW source code appears as a graphical block-diagram.  These graphical block-diagrams contain function-nodes (analogous to functions in Python for example) that the user draws virtual wires between.  These virtual wires between different function nodes allow the transfer of variables.  This style of programming is called dataflow programming.&lt;br /&gt;
&lt;br /&gt;
LabVIEW also includes extensive hardware support for interfacing with cameras, sensors, and other devices.  Users can interface to hardware by either writing direct bus commands (USB, GPIB, Serial) or using high-level, device-specific, drivers that provide native LabVIEW function nodes for controlling the device.  LabVIEW's ability to interact with and control different devices is essential to experimental physics and lab work in general.&lt;br /&gt;
&lt;br /&gt;
== Learning from the Text ==&lt;br /&gt;
&lt;br /&gt;
The first four chapters of the text are considered to be essential for understanding the basics of LabVIEW.  They are also meant to be completed sequentially as each section builds on previous sections.  Chapters after number 4 are meant to be more like independent modules that can be completed in any desired order.  The content of chapters is summarized below:&lt;br /&gt;
&lt;br /&gt;
Chapters 1-3: Fundamentals of the LabVIEW Graphical Programming Language.  Central features of LabVIEW including its control loop structures, graphing modes, mathematical functions, and text-based MathScript commands are learned in the course of writing digitized waveform simulation programs.&lt;br /&gt;
&lt;br /&gt;
Chapter 4: Basic Data Acquisition.  Concepts of digitized data such as resolution, sampling frequency, and aliasing are covered.  Then, using LabVIEW's high-level Express VIs, programs are written that execute analog-to-digital, digital-to-analog, and digital input/output tasks on a National Instruments DAQ device.  Computer-based instruments constructed included a DC voltmeter, digital oscilloscope, DC voltage source, waveform generator, and blinking LED array.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Chapters from the Text ==&lt;br /&gt;
&lt;br /&gt;
Chapter 1 - The While Loop and Waveform Chart&lt;br /&gt;
&lt;br /&gt;
Chapter 2 - The For Loop and Waveform Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 3 - The Mathscript Node and XY Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 4 - Data Acquisition Using DAQ Assistant&lt;br /&gt;
&lt;br /&gt;
Chapter 5 - Data Files and Character Strings&lt;br /&gt;
&lt;br /&gt;
Chapter 6 - Shift Registers&lt;br /&gt;
&lt;br /&gt;
Chapter 7 - The Case Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 8 - Data Dependency and the Sequence Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 9 - Analysis VIs: Curve Fitting&lt;br /&gt;
&lt;br /&gt;
Chapter 10 - Analysis VIs: Fast Fourier Transform&lt;br /&gt;
&lt;br /&gt;
Chapter 11 - Data Acquisition and Generation Using DAQmx VIs&lt;br /&gt;
&lt;br /&gt;
Chapter 12 - PID Temperature Control Project&lt;br /&gt;
&lt;br /&gt;
Chapter 13 - Control of Stand-Alone Instruments&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.ni.com/f/students/12/7052/en/ Official National Instruments Video Tutorials]&lt;br /&gt;
&lt;br /&gt;
[http://home.hit.no/~hansha/documents/labview/training/Introduction%20to%20LabVIEW/Introduction%20to%20LabVIEW.pdf This LabVIEW tutorial is entirely contained within 1 PDF file, making it easy to download and view as desired.]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2728</id>
		<title>LabVIEW Primer</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2728"/>
		<updated>2016-04-03T20:08:45Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Textbook for this Primer ==&lt;br /&gt;
&lt;br /&gt;
This LabVIEW primer is based off of the book [https://books.google.com/books?id=ytwiMTLct48C &amp;quot;Hands-On Introduction to LabVIEW for Scientists and Engineers&amp;quot;] by John Essick.  Two copies of the book can be found in the lab to the right of the computer setup.&lt;br /&gt;
&lt;br /&gt;
== Accessing LabVIEW on Our Computers ==&lt;br /&gt;
&lt;br /&gt;
Currently LabVIEW is installed on one machine in the lab.  When looking at the desktop computers straight on, the rightmost computer closest to the books contains an installation of LabVIEW.  This computer runs Linux but has Windows 7 installed as a virtual machine.  Our version of LabVIEW is installed on Windows, so the Windows virtual machine must be ran before LabVIEW can be accessed.  Running Windows is simple; there is a shortcut on the Linux desktop called &amp;quot;Hankwin&amp;quot; which can be clicked to open.  Once Windows is running, LabVIEW can be found in the Programs menu.&lt;br /&gt;
&lt;br /&gt;
== What is LabVIEW? ==&lt;br /&gt;
&lt;br /&gt;
LabVIEW (Laboratory Virtual Instrument Engineering Workbench) is a development environment and system-design platform for a visual programming language called &amp;quot;G&amp;quot;. LabVIEW is commonly used by scientists and engineers for the purposes of data acquisition, instrument control, and industrial automation.  It is developed and maintained by National Instruments.&lt;br /&gt;
&lt;br /&gt;
LabVIEW is made for engineering and experimental science.  It is a programming language and underneath the hood it does most things similarly to other text-based programming languages, but all of this information is presented to the user very differently.  LabVIEW is a visual and graphical programming language.  Instead of pages of text, LabVIEW source code appears as a graphical block-diagram.  These graphical block-diagrams contain function-nodes (analogous to functions in Python for example) that the user draws virtual wires between.  These virtual wires between different function nodes allow the transfer of variables.  This style of programming is called dataflow programming.&lt;br /&gt;
&lt;br /&gt;
LabVIEW also includes extensive hardware support for interfacing with cameras, sensors, and other devices.  Users can interface to hardware by either writing direct bus commands (USB, GPIB, Serial) or using high-level, device-specific, drivers that provide native LabVIEW function nodes for controlling the device.  LabVIEW's ability to interact with and control different devices is essential to experimental physics and lab work in general.&lt;br /&gt;
&lt;br /&gt;
== Learning from the Text ==&lt;br /&gt;
&lt;br /&gt;
The first four chapters of the text are considered to be essential for understanding the basics of LabVIEW.  They are also meant to be completed sequentially as each section builds on previous sections.  Chapters after number 4 are meant to be more like independent modules that can be completed in any desired order.&lt;br /&gt;
&lt;br /&gt;
== Chapters from the Text ==&lt;br /&gt;
&lt;br /&gt;
Chapter 1 - The While Loop and Waveform Chart&lt;br /&gt;
&lt;br /&gt;
Chapter 2 - The For Loop and Waveform Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 3 - The Mathscript Node and XY Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 4 - Data Acquisition Using DAQ Assistant&lt;br /&gt;
&lt;br /&gt;
Chapter 5 - Data Files and Character Strings&lt;br /&gt;
&lt;br /&gt;
Chapter 6 - Shift Registers&lt;br /&gt;
&lt;br /&gt;
Chapter 7 - The Case Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 8 - Data Dependency and the Sequence Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 9 - Analysis VIs: Curve Fitting&lt;br /&gt;
&lt;br /&gt;
Chapter 10 - Analysis VIs: Fast Fourier Transform&lt;br /&gt;
&lt;br /&gt;
Chapter 11 - Data Acquisition and Generation Using DAQmx VIs&lt;br /&gt;
&lt;br /&gt;
Chapter 12 - PID Temperature Control Project&lt;br /&gt;
&lt;br /&gt;
Chapter 13 - Control of Stand-Alone Instruments&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.ni.com/f/students/12/7052/en/ Official National Instruments Video Tutorials]&lt;br /&gt;
&lt;br /&gt;
[http://home.hit.no/~hansha/documents/labview/training/Introduction%20to%20LabVIEW/Introduction%20to%20LabVIEW.pdf This LabVIEW tutorial is entirely contained within 1 PDF file, making it easy to download and view as desired.]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2727</id>
		<title>LabVIEW Primer</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2727"/>
		<updated>2016-04-03T19:32:53Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Textbook for this Primer ==&lt;br /&gt;
&lt;br /&gt;
This LabVIEW primer is based off of the book [https://books.google.com/books?id=ytwiMTLct48C &amp;quot;Hands-On Introduction to LabVIEW for Scientists and Engineers&amp;quot;] by John Essick.  Two copies of the book can be found in the lab to the right of the computer setup.&lt;br /&gt;
&lt;br /&gt;
== Accessing LabVIEW on Our Computers ==&lt;br /&gt;
&lt;br /&gt;
Currently LabVIEW is installed on one machine in the lab.  When looking at the desktop computers straight on, the rightmost computer closest to the books contains an installation of LabVIEW.  This computer runs Linux but has Windows 7 installed as a virtual machine.  Our version of LabVIEW is installed on Windows, so the Windows virtual machine must be ran before LabVIEW can be accessed.  Running Windows is simple; there is a shortcut on the Linux desktop called &amp;quot;Hankwin&amp;quot; which can be clicked to open.  Once Windows is running, LabVIEW can be found in the Programs menu.&lt;br /&gt;
&lt;br /&gt;
== What is LabVIEW? ==&lt;br /&gt;
&lt;br /&gt;
LabVIEW (Laboratory Virtual Instrument Engineering Workbench) is a development environment and system-design platform for a visual programming language called &amp;quot;G&amp;quot;. LabVIEW is commonly used by scientists and engineers for the purposes of data acquisition, instrument control, and industrial automation.  It is developed and maintained by National Instruments.&lt;br /&gt;
&lt;br /&gt;
LabVIEW is made for engineering and experimental science.  It is a programming language and underneath the hood it does most things similarly to other text-based programming languages, but all of this information is presented to the user very differently.  LabVIEW is a visual and graphical programming language.  Instead of pages of text, LabVIEW source code appears as a graphical block-diagram.  These graphical block-diagrams contain function-nodes (analogous to functions in Python for example) that the user draws virtual wires between.  These virtual wires between different function nodes allow the transfer of variables.  This style of programming is called dataflow programming.&lt;br /&gt;
&lt;br /&gt;
LabVIEW also includes extensive hardware support for interfacing with cameras, sensors, and other devices.  Users can interface to hardware by either writing direct bus commands (USB, GPIB, Serial) or using high-level, device-specific, drivers that provide native LabVIEW function nodes for controlling the device.  LabVIEW's ability to interact with and control different devices is essential to experimental physics and lab work in general.&lt;br /&gt;
&lt;br /&gt;
== Chapters from the Text ==&lt;br /&gt;
&lt;br /&gt;
Chapter 1 - The While Loop and Waveform Chart&lt;br /&gt;
&lt;br /&gt;
Chapter 2 - The For Loop and Waveform Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 3 - The Mathscript Node and XY Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 4 - Data Acquisition Using DAQ Assistant&lt;br /&gt;
&lt;br /&gt;
Chapter 5 - Data Files and Character Strings&lt;br /&gt;
&lt;br /&gt;
Chapter 6 - Shift Registers&lt;br /&gt;
&lt;br /&gt;
Chapter 7 - The Case Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 8 - Data Dependency and the Sequence Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 9 - Analysis VIs: Curve Fitting&lt;br /&gt;
&lt;br /&gt;
Chapter 10 - Analysis VIs: Fast Fourier Transform&lt;br /&gt;
&lt;br /&gt;
Chapter 11 - Data Acquisition and Generation Using DAQmx VIs&lt;br /&gt;
&lt;br /&gt;
Chapter 12 - PID Temperature Control Project&lt;br /&gt;
&lt;br /&gt;
Chapter 13 - Control of Stand-Alone Instruments&lt;br /&gt;
&lt;br /&gt;
== Useful Links ==&lt;br /&gt;
&lt;br /&gt;
[http://www.ni.com/f/students/12/7052/en/ Official National Instruments Video Tutorials]&lt;br /&gt;
&lt;br /&gt;
[http://home.hit.no/~hansha/documents/labview/training/Introduction%20to%20LabVIEW/Introduction%20to%20LabVIEW.pdf This LabVIEW tutorial is entirely contained within 1 PDF file, making it easy to download and view as desired.]&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2726</id>
		<title>LabVIEW Primer</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2726"/>
		<updated>2016-04-03T19:27:02Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Textbook for this Primer ==&lt;br /&gt;
&lt;br /&gt;
This LabVIEW primer is based off of the book [https://books.google.com/books?id=ytwiMTLct48C &amp;quot;Hands-On Introduction to LabVIEW for Scientists and Engineers&amp;quot;] by John Essick.  Two copies of the book can be found in the lab to the right of the computer setup.&lt;br /&gt;
&lt;br /&gt;
== Accessing LabVIEW on Our Computers ==&lt;br /&gt;
&lt;br /&gt;
Currently LabVIEW is installed on one machine in the lab.  When looking at the desktop computers straight on, the rightmost computer closest to the books contains an installation of LabVIEW.  This computer runs Linux but has Windows 7 installed as a virtual machine.  Our version of LabVIEW is installed on Windows, so the Windows virtual machine must be ran before LabVIEW can be accessed.  Running Windows is simple; there is a shortcut on the Linux desktop called &amp;quot;Hankwin&amp;quot; which can be clicked to open.  Once Windows is running, LabVIEW can be found in the Programs menu.&lt;br /&gt;
&lt;br /&gt;
== What is LabVIEW? ==&lt;br /&gt;
&lt;br /&gt;
LabVIEW (Laboratory Virtual Instrument Engineering Workbench) is a development environment and system-design platform for a visual programming language called &amp;quot;G&amp;quot;. LabVIEW is commonly used by scientists and engineers for the purposes of data acquisition, instrument control, and industrial automation.  It is developed and maintained by National Instruments.&lt;br /&gt;
&lt;br /&gt;
LabVIEW is made for engineering and experimental science.  It is a programming language and underneath the hood it does most things similarly to other text-based programming languages, but all of this information is presented to the user very differently.  LabVIEW is a visual and graphical programming language.  Instead of pages of text, LabVIEW source code appears as a graphical block-diagram.  These graphical block-diagrams contain function-nodes (analogous to functions in Python for example) that the user draws virtual wires between.  These virtual wires between different function nodes allow the transfer of variables.  This style of programming is called dataflow programming.&lt;br /&gt;
&lt;br /&gt;
LabVIEW also includes extensive hardware support for interfacing with cameras, sensors, and other devices.  Users can interface to hardware by either writing direct bus commands (USB, GPIB, Serial) or using high-level, device-specific, drivers that provide native LabVIEW function nodes for controlling the device.  LabVIEW's ability to interact with and control different devices is essential to experimental physics and lab work in general.&lt;br /&gt;
&lt;br /&gt;
== Chapters from the Text ==&lt;br /&gt;
&lt;br /&gt;
Chapter 1 - The While Loop and Waveform Chart&lt;br /&gt;
&lt;br /&gt;
Chapter 2 - The For Loop and Waveform Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 3 - The Mathscript Node and XY Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 4 - Data Acquisition Using DAQ Assistant&lt;br /&gt;
&lt;br /&gt;
Chapter 5 - Data Files and Character Strings&lt;br /&gt;
&lt;br /&gt;
Chapter 6 - Shift Registers&lt;br /&gt;
&lt;br /&gt;
Chapter 7 - The Case Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 8 - Data Dependency and the Sequence Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 9 - Analysis VIs: Curve Fitting&lt;br /&gt;
&lt;br /&gt;
Chapter 10 - Analysis VIs: Fast Fourier Transform&lt;br /&gt;
&lt;br /&gt;
Chapter 11 - Data Acquisition and Generation Using DAQmx VIs&lt;br /&gt;
&lt;br /&gt;
Chapter 12 - PID Temperature Control Project&lt;br /&gt;
&lt;br /&gt;
Chapter 13 - Control of Stand-Alone Instruments&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2725</id>
		<title>LabVIEW Primer</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2725"/>
		<updated>2016-04-03T19:25:43Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Textbook for this Primer ==&lt;br /&gt;
&lt;br /&gt;
This LabVIEW primer is based off of the book [https://books.google.com/books?id=ytwiMTLct48C &amp;quot;Hands-On Introduction to LabVIEW for Scientists and Engineers&amp;quot;] by John Essick.  Two copies of the book can be found in the lab to the right of the computer setup.&lt;br /&gt;
&lt;br /&gt;
== Accessing LabVIEW ==&lt;br /&gt;
&lt;br /&gt;
Currently LabVIEW is installed on one machine in the lab.  When looking at the desktop computers straight on, the rightmost computer closest to the books contains an installation of LabVIEW.  This computer runs Linux but has Windows 7 installed as a virtual machine.  Our version of LabVIEW is installed on Windows, so the Windows virtual machine must be ran before LabVIEW can be accessed.  Running Windows is simple; there is a shortcut on the Linux desktop called &amp;quot;Hankwin&amp;quot; which can be clicked to open.  Once Windows is running, LabVIEW can be found in the Programs menu.&lt;br /&gt;
&lt;br /&gt;
== What is LabVIEW? ==&lt;br /&gt;
&lt;br /&gt;
LabVIEW (Laboratory Virtual Instrument Engineering Workbench) is a development environment and system-design platform for a visual programming language called &amp;quot;G&amp;quot;. LabVIEW is commonly used by scientists and engineers for the purposes of data acquisition, instrument control, and industrial automation.  It is developed and maintained by National Instruments.&lt;br /&gt;
&lt;br /&gt;
LabVIEW is made for engineering and experimental science.  It is a programming language and underneath the hood it does most things similarly to other text-based programming languages, but all of this information is presented to the user very differently.  LabVIEW is a visual and graphical programming language.  Instead of pages of text, LabVIEW source code appears as a graphical block-diagram.  These graphical block-diagrams contain function-nodes (analogous to functions in Python for example) that the user draws virtual wires between.  These virtual wires between different function nodes allow the transfer of variables.  This style of programming is called dataflow programming.&lt;br /&gt;
&lt;br /&gt;
LabVIEW also includes extensive hardware support for interfacing with cameras, sensors, and other devices.  Users can interface to hardware by either writing direct bus commands (USB, GPIB, Serial) or using high-level, device-specific, drivers that provide native LabVIEW function nodes for controlling the device.  LabVIEW's ability to interact with and control different devices is essential to experimental physics and lab work in general.&lt;br /&gt;
&lt;br /&gt;
== Chapters from the Text ==&lt;br /&gt;
&lt;br /&gt;
Chapter 1 - The While Loop and Waveform Chart&lt;br /&gt;
&lt;br /&gt;
Chapter 2 - The For Loop and Waveform Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 3 - The Mathscript Node and XY Graph&lt;br /&gt;
&lt;br /&gt;
Chapter 4 - Data Acquisition Using DAQ Assistant&lt;br /&gt;
&lt;br /&gt;
Chapter 5 - Data Files and Character Strings&lt;br /&gt;
&lt;br /&gt;
Chapter 6 - Shift Registers&lt;br /&gt;
&lt;br /&gt;
Chapter 7 - The Case Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 8 - Data Dependency and the Sequence Structure&lt;br /&gt;
&lt;br /&gt;
Chapter 9 - Analysis VIs: Curve Fitting&lt;br /&gt;
&lt;br /&gt;
Chapter 10 - Analysis VIs: Fast Fourier Transform&lt;br /&gt;
&lt;br /&gt;
Chapter 11 - Data Acquisition and Generation Using DAQmx VIs&lt;br /&gt;
&lt;br /&gt;
Chapter 12 - PID Temperature Control Project&lt;br /&gt;
&lt;br /&gt;
Chapter 13 - Control of Stand-Alone Instruments&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2724</id>
		<title>LabVIEW Primer</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2724"/>
		<updated>2016-04-03T19:25:18Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Textbook for this Primer ==&lt;br /&gt;
&lt;br /&gt;
This LabVIEW primer is based off of the book [https://books.google.com/books?id=ytwiMTLct48C &amp;quot;Hands-On Introduction to LabVIEW for Scientists and Engineers&amp;quot;] by John Essick.  Two copies of the book can be found in the lab to the right of the computer setup.&lt;br /&gt;
&lt;br /&gt;
== Accessing LabVIEW ==&lt;br /&gt;
&lt;br /&gt;
Currently LabVIEW is installed on one machine in the lab.  When looking at the desktop computers straight on, the rightmost computer closest to the books contains an installation of LabVIEW.  This computer runs Linux but has Windows 7 installed as a virtual machine.  Our version of LabVIEW is installed on Windows, so the Windows virtual machine must be ran before LabVIEW can be accessed.  Running Windows is simple; there is a shortcut on the Linux desktop called &amp;quot;Hankwin&amp;quot; which can be clicked to open.  Once Windows is running, LabVIEW can be found in the Programs menu.&lt;br /&gt;
&lt;br /&gt;
== What is LabVIEW? ==&lt;br /&gt;
&lt;br /&gt;
LabVIEW (Laboratory Virtual Instrument Engineering Workbench) is a development environment and system-design platform for a visual programming language called &amp;quot;G&amp;quot;. LabVIEW is commonly used by scientists and engineers for the purposes of data acquisition, instrument control, and industrial automation.  It is developed and maintained by National Instruments.&lt;br /&gt;
&lt;br /&gt;
LabVIEW is made for engineering and experimental science.  It is a programming language and underneath the hood it does most things similarly to other text-based programming languages, but all of this information is presented to the user very differently.  LabVIEW is a visual and graphical programming language.  Instead of pages of text, LabVIEW source code appears as a graphical block-diagram.  These graphical block-diagrams contain function-nodes (analogous to functions in Python for example) that the user draws virtual wires between.  These virtual wires between different function nodes allow the transfer of variables.  This style of programming is called dataflow programming.&lt;br /&gt;
&lt;br /&gt;
LabVIEW also includes extensive hardware support for interfacing with cameras, sensors, and other devices.  Users can interface to hardware by either writing direct bus commands (USB, GPIB, Serial) or using high-level, device-specific, drivers that provide native LabVIEW function nodes for controlling the device.  LabVIEW's ability to interact with and control different devices is essential to experimental physics and lab work in general.&lt;br /&gt;
&lt;br /&gt;
== Chapters from the Text ==&lt;br /&gt;
&lt;br /&gt;
Chapter 1 - The While Loop and Waveform Chart&lt;br /&gt;
&lt;br /&gt;
Chapter 2 - The For Loop and Waveform Graph&lt;br /&gt;
Chapter 3 - The Mathscript Node and XY Graph&lt;br /&gt;
Chapter 4 - Data Acquisition Using DAQ Assistant&lt;br /&gt;
Chapter 5 - Data Files and Character Strings&lt;br /&gt;
Chapter 6 - Shift Registers&lt;br /&gt;
Chapter 7 - The Case Structure&lt;br /&gt;
Chapter 8 - Data Dependency and the Sequence Structure&lt;br /&gt;
Chapter 9 - Analysis VIs: Curve Fitting&lt;br /&gt;
Chapter 10 - Analysis VIs: Fast Fourier Transform&lt;br /&gt;
Chapter 11 - Data Acquisition and Generation Using DAQmx VIs&lt;br /&gt;
Chapter 12 - PID Temperature Control Project&lt;br /&gt;
Chapter 13 - Control of Stand-Alone Instruments&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
	<entry>
		<id>https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2723</id>
		<title>LabVIEW Primer</title>
		<link rel="alternate" type="text/html" href="https://june.uoregon.edu/mediawiki/index.php?title=LabVIEW_Primer&amp;diff=2723"/>
		<updated>2016-04-03T19:24:51Z</updated>

		<summary type="html">&lt;p&gt;Wikiuser: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Textbook for this Primer ==&lt;br /&gt;
&lt;br /&gt;
This LabVIEW primer is based off of the book [https://books.google.com/books?id=ytwiMTLct48C &amp;quot;Hands-On Introduction to LabVIEW for Scientists and Engineers&amp;quot;] by John Essick.  Two copies of the book can be found in the lab to the right of the computer setup.&lt;br /&gt;
&lt;br /&gt;
== Accessing LabVIEW ==&lt;br /&gt;
&lt;br /&gt;
Currently LabVIEW is installed on one machine in the lab.  When looking at the desktop computers straight on, the rightmost computer closest to the books contains an installation of LabVIEW.  This computer runs Linux but has Windows 7 installed as a virtual machine.  Our version of LabVIEW is installed on Windows, so the Windows virtual machine must be ran before LabVIEW can be accessed.  Running Windows is simple; there is a shortcut on the Linux desktop called &amp;quot;Hankwin&amp;quot; which can be clicked to open.  Once Windows is running, LabVIEW can be found in the Programs menu.&lt;br /&gt;
&lt;br /&gt;
== What is LabVIEW? ==&lt;br /&gt;
&lt;br /&gt;
LabVIEW (Laboratory Virtual Instrument Engineering Workbench) is a development environment and system-design platform for a visual programming language called &amp;quot;G&amp;quot;. LabVIEW is commonly used by scientists and engineers for the purposes of data acquisition, instrument control, and industrial automation.  It is developed and maintained by National Instruments.&lt;br /&gt;
&lt;br /&gt;
LabVIEW is made for engineering and experimental science.  It is a programming language and underneath the hood it does most things similarly to other text-based programming languages, but all of this information is presented to the user very differently.  LabVIEW is a visual and graphical programming language.  Instead of pages of text, LabVIEW source code appears as a graphical block-diagram.  These graphical block-diagrams contain function-nodes (analogous to functions in Python for example) that the user draws virtual wires between.  These virtual wires between different function nodes allow the transfer of variables.  This style of programming is called dataflow programming.&lt;br /&gt;
&lt;br /&gt;
LabVIEW also includes extensive hardware support for interfacing with cameras, sensors, and other devices.  Users can interface to hardware by either writing direct bus commands (USB, GPIB, Serial) or using high-level, device-specific, drivers that provide native LabVIEW function nodes for controlling the device.  LabVIEW's ability to interact with and control different devices is essential to experimental physics and lab work in general.&lt;br /&gt;
&lt;br /&gt;
== Chapters from the Text ==&lt;br /&gt;
&lt;br /&gt;
Chapter 1 - The While Loop and Waveform Chart&lt;br /&gt;
Chapter 2 - The For Loop and Waveform Graph&lt;br /&gt;
Chapter 3 - The Mathscript Node and XY Graph&lt;br /&gt;
Chapter 4 - Data Acquisition Using DAQ Assistant&lt;br /&gt;
Chapter 5 - Data Files and Character Strings&lt;br /&gt;
Chapter 6 - Shift Registers&lt;br /&gt;
Chapter 7 - The Case Structure&lt;br /&gt;
Chapter 8 - Data Dependency and the Sequence Structure&lt;br /&gt;
Chapter 9 - Analysis VIs: Curve Fitting&lt;br /&gt;
Chapter 10 - Analysis VIs: Fast Fourier Transform&lt;br /&gt;
Chapter 11 - Data Acquisition and Generation Using DAQmx VIs&lt;br /&gt;
Chapter 12 - PID Temperature Control Project&lt;br /&gt;
Chapter 13 - Control of Stand-Alone Instruments&lt;/div&gt;</summary>
		<author><name>Wikiuser</name></author>
		
	</entry>
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