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Lecture 21, 22: Noise

Profile picture of Samson ZhangSamson Zhang
Nov 14, 2023Last updated Nov 20, 20233 min read

There are two kinds of noise: thermal and quantization.



Thermal noise is Gaussian and white.



Thermodynamics yields the following equation for noise power (variance in power from thermal noise):

P_n = \sigma_P^2 = kT \Delta f
Pn=σP2=kTΔfP_n = \sigma_P^2 = kT \Delta f

And for voltage and current variance:

v_n^2 = \sigma_v^2 = 4kTR \Delta f \\ \\ i_n^2 = \sigma_i^2 = 4kT\Delta f/R
vn2=σv2=4kTRΔfin2=σi2=4kTΔf/Rv_n^2 = \sigma_v^2 = 4kTR \Delta f \\ \\ i_n^2 = \sigma_i^2 = 4kT\Delta f/R

Thus "noise temperature" is given by:

T_n = \frac{P_n}{k \Delta f}
Tn=PnkΔfT_n = \frac{P_n}{k \Delta f}

Here's a big table of symbols:



Noise variances add. They are also affected by the square gain of the transfer function (which makes sense because voltage => power). So

4kTR 4kTR 4kTR
of voltage noise variance density before would become
4A^2 k TR 4A2kTR 4A^2 k TR
of noise after an amplifier with gain A. If the amplifier has -20dB/dec dropoff somewhere, the noise will have -40dB/dec dropoff.

A greater bandwidth will result in a greater amount of noise, as the noise density for thermal noise is even across frequencies (white noise).



Thus:

\sigma_v^2 = \bar{\sigma_v^2} BW = 4A^2 kTR \cdot BW
σv2=σv2ˉBW=4A2kTRBW\sigma_v^2 = \bar{\sigma_v^2} BW = 4A^2 kTR \cdot BW

and:

T_n = A^2 T
Tn=A2TT_n = A^2 T

Temperature of lossy 2-port passive

The temperature of a lossy 2-port passive is:

T_p = \bigg(\frac{1}{L} - 1\bigg)T
Tp=(1L1)TT_p = \bigg(\frac{1}{L} - 1\bigg)T

where L is the linear power gain, e.g. the insertion loss of a filter or other passive component.



The noise temperature of an antenna is determined through a spherical integral over all the radiation incident on it.



Signal to noise ratio

Signal to noise ratio, SNR, is defined as

SNR = \frac{P_\text{signal}}{P_\text{in}} SNR=PsignalPin SNR = \frac{P_\text{signal}}{P_\text{in}}


For an amplifier with some input noise

T_{in} Tin T_{in}
and added noise
T_a Ta T_a
and power gain
G G G
,

SNR_{in} = \frac{P_{in}}{kT_{in}B} \\ \: \\ SNR_{out} = \frac{P_{in}}{k(T_{in}+T_A)B}
SNRin=PinkTinBSNRout=Pink(Tin+TA)BSNR_{in} = \frac{P_{in}}{kT_{in}B} \\ \: \\ SNR_{out} = \frac{P_{in}}{k(T_{in}+T_A)B}

We also define noise factor:

nf = \frac{SNR_{in}}{SNR_{out}} = 1 + \frac{T_A}{T_{in}}, NF = 10 \log nf
nf=SNRinSNRout=1+TATin,NF=10lognfnf = \frac{SNR_{in}}{SNR_{out}} = 1 + \frac{T_A}{T_{in}}, NF = 10 \log nf

So amps add noise with temperature:

T_A = (nf - 1)T
TA=(nf1)TT_A = (nf - 1)T


Quantization noise

Analog digital converters add random noise with voltage noise variance:

\sigma_q^2 = LSB^2 / 12
σq2=LSB2/12\sigma_q^2 = LSB^2 / 12

where LSB is the "least significant bit."



Cascading amplifiers

In a cascade of amplifiers, the noise of the first amplifier dominates over the noise of the later stages because it gets amplified.

There's a tradeoff -- more amplification reduces the relative effect of quantization noise.



There are a few helpful formulas:

nf_{total} = nf_1 + \frac{nf_2 - 1}{G_1} + \frac{nf_3 - 1}{G_1 G_2} + ...
nftotal=nf1+nf21G1+nf31G1G2+...nf_{total} = nf_1 + \frac{nf_2 - 1}{G_1} + \frac{nf_3 - 1}{G_1 G_2} + ...

and, similarly:

T_{sys} = T_1 + \frac{T_2}{G_1} + \frac{T_3}{G_1 G_2}
Tsys=T1+T2G1+T3G1G2T_{sys} = T_1 + \frac{T_2}{G_1} + \frac{T_3}{G_1 G_2}

thus, for high gain:

SNR \approx \frac{P_{in}}{k(T_{in} + T_{sys})B}
SNRPink(Tin+Tsys)BSNR \approx \frac{P_{in}}{k(T_{in} + T_{sys})B}


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