Noise and Interference, the Lock-In Amplifier, (and the IV-meetkast) ( )

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Noise and Interference, the Lock-In Amplifier, (and the IV-meetkast) ( ) Caspar van der Wal FND group talk, modified to web-tutorial - 4 November 2004

Why look into this? You measure much faster if you use the lock-in amplifier and the IV-meetkast options in the optimal way. It takes very little time to do a critical evaluation of actual noise levels that show up. It is more subtle than we like to admit, but worth spending some time on.

Outline Nature of unwanted contributions to measured signals. Why use a lock-in amplifier? Concepts and guidelines for optimal use of lock-in amplifiers. Evaluation of observed noise levels.

Unwanted contributions to measured signals Noise, drift: Setup-made, intrinsic Often non-periodic Shielding and isolation does not help Interference: Environment-made Often periodic Shielding and isolation helps.distinction sometimes artificial.

World with some reality Ideal world Johnson-Nyquist noise R I bias intrinsic noise, drifting offset G Volt meter

V time

Spectrum of amplifier noise Taken from data sheet OPA627 (part of IV-meetkast)

For amplifiers in practice, this gives: V out Stable gain 0 0 Drifting offset V in

World with some more reality Ideal world Q R I bias Φ G Volt meter

V time

Sprectrum of interference from environment

What to do about V? time Simple averaging = low-pass filtering works!.but is inefficient and not always effective because of the 1/f character of the unwanted signals.

So, what about measuring at higher frequencies, and then band-pass filtering? Filter transmission 1 0

Good idea, but.. In practice it is not possible to realize ultra-narrow band-pass filters that are -stable -flexible (this can work in software though lock-in amplifier)

What does work real-time: A lock-in amplifier Idea: Control or bias at some high frequency. Amplify the measured signal (full spectrum) up to a level where noise does not hurt it anymore. Mix (multiply) it with a high-level reference signal at exactly the same frequency as the wanted signal. Low-pass filter the mixed signal (can be realized ultra narrow).

control Oscillator Lock-in amplifyer V R Experiment signal G AC V S V M LPF DC output mix V R = A R sin(ω R t) V S (ω S ) = A S (ω S ) sin( ω S t + θ(ω S ) ) V M = V S V R = ½A R A S cos( (ω S -ω R )+θ ) - ½A R A S cos( (ω S +ω R )+θ ) After LPF, only for ω S = ω R V DCX = ½A R A S cos(θ), also V DCY = ½A R A S sin(θ)

What you should NOT conclude now: If you use lock-in detection, there is little need to worry about interference and shielding etc. Because: Heating of a sample results from the (total current through the sample) 2. V max = I peak-peak *R sets ev energy scale in device. If you study non-linear behavior, you get higher harmonics of unwanted signals (as noise or apparent signal) in your desired signal. If you study variations in non-linear behavior, you get a varying amount of higher harmonics of unwanted signals in your desired signal.

V I bias Non-linearities

Some hints for optimal use of lock-in amplifiers

Time constant and repetition time

Slope of LPF filter

Low-pass filtering: frequency domain 0 db A LPF -120 db 0 Hz f -3dB 50 Hz

Low-pass filtering: time domain Here data taken with T Rep <<T C Signal Sampled output of lock-in Behavior of sample T C time For T Rep <<T C successive sampled data points are not independent, no new information.

Filter slope ENBW T Rep-1% (db/oct) 6 1/(4 T C ) 5 T C 12 1/(8 T C ) 7 T C 18 3/(32 T C ) 9 T C 24 5/(64 T C ) 10 T C For 6 db case, LPF is simple RC filter. T C = RC-time = RC (always defined for single filter!) f -3dB = 1/(2πRC) ENBW = 1/(4RC) (for white Gaussian noise!)

Example 6 db vs 24 db filter slope Say f REF = 1 khz Assume narrow-band noise contribution at 1.05 khz Assume noise = 10 4 times the signal (80 db) Like to see signal 1% accurate (-40 db) Need to LPF 50 Hz by 120 db A LPF 0 db Slope f -3dB T C T Rep 6dB 50 µhz 3000 s 15000 s 24 db 1.6 Hz 100 ms 1 s -120 db 0 Hz f -3dB 50 Hz 24 db case is 15000 times faster than 6 db! Q; How does this work out for white noise?

LINE and SYNC filters Look it up. In general, use it below 200 Hz!

Dynamic reserve

control Oscillator Lock-in amplifyer V R Experiment signal G AC V S V M LPF DC output mix Dynamic reserve: ratio between peak-peak voltage of total signal and peak-peak of wanted signal. Dynamic range: ratio between peak-peak voltage of total signal and resolution of wanted signal.

V S Use Low noise (0-124 db) V S Use Normal (0-154 db) V S Use High reserve (0-174 db) time Note: Lock-in people use x10 = 20 db

Offset and Expand Use OFFSET and EXPAND (x10 or x100) if you have a small signal on top of a constant background.

Without OFFSET and EXPAND you see the AD conversion. 58.2 V (mv) 58.1 B (mt)

Evaluating noise levels (measurement efficiency) Are you at the noise level that is intrinsic to the setup? (can only be improved by averaging longer ) Do measurement vs time, all control fixed. Result from lock-in at certain T C, I bias, etc. V DCX time

Observed Gaussian white noise with f REF = 20 Hz V DCX V RMS V P-P /6 ENBW=1/4T C time Specified amplifier noise Observed V NSD at sample: V V NSD = RMS V4T C Gain Note units: V DCX,V RMS,V P-P ENBW V Hz Gain 1 V NSD V/ VHz

What if you find 100 instead of 10 nv/vhz? a) Try to fix the problem b) Just average longer V RMS = Gain V NSD V4T C 4 days instead of 1 hour for some sweep!

Conclusions The Lock-in is an effective averaging tool to beat 1/f part of the unwanted components in measured signals. Improving your signal:noise ratio (in terms of amplitudes) x 10, means 100 times faster data taking: The difference between results and no results.

IV-meetkast Next time: Why use the IV-meetkast? Shielding Ground loops Clean ground Inductive interference Capacitive interference