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Lecture 8,9:
Thermal noise
Aliazam Abbasfar
Outline
Thermal noise
Noise in circuits
Noise figure
Gaussian process
If {X(t1), …, X(tN)} are jointly Gaussian
Properties :
mX(t) and RX(t1,t2) gives complete model
If X(t) passed through an LTI system, the
output signal is Gaussian process as well
If WSS, then strictly stationary and ergodic
White process
If X(t) has flat power spectral density
GX(f) = c
RX(t) = c d(t)
X(t1) and X(t2) are uncorrelated if t1 ≠ t2
Total power =
Limited power when goes through a filter
Thermal noise
Random movements of free electrons in a
resistor
Gaussian process
Zero mean and finite power
2 f
R
f
exp(
) 1
kT
T: temperature [K]
k: Boltzmann constant (1.38×10-23 joule/K)
h: Planck constant (6.625×10-34 joule-sec)
G n (f)
2( kT) 2
E[n (t)]
R
3
f
V2
2kTR 1
Hz
2kT
2
Almost flat PSD ( up to 1012 Hz)
Practically a white process
Gn(f) = 2kTR
Noise power in band-limited systems : 4kTB R
V2
AWGN
Additive white Gaussian noise
Gn(f) = N0/2 and Rn(t) = N0/2 d(t)
SNR = SD/ND
Noise can be modeled as voltage source
Best power delivery when matched
Gn(f) = kT/2
W/Hz
Independent of R
N0 = kT (T = 290 K) is -174 dBm
Filtered noise
Reduce noise power by filtering
Gno(f) = Gn(f) |H(f)|2
Ideal filter with bandwidth B
|H(f)| = rect( f/2B)
Gno(f) = N0/2 rect( f/2B)
Rno(t) = N0 B sinc (2Bt)
Pno = N0 B
Colored noise
Uncorrelated for t1-t2 = n/2B
Noise equivalent bandwidth
Noise power in practical filters
Assume an ideal filter with gain : g= |H(f)|2max
Pno = g N0 BN (noise equivalent bandwidth )
1
2
BN H(f) df
g0
BN is usually greater than 3dB bandwidth
RC filter
g = 1
BN = 1/4RC
Pno = kT/C
Effective noise temperature
Output power of any white noise source
Pno = k Teff B
Noise in two-port networks
Pno = kTgBNg + Pni = k(Tg+Te)BNg
Pni : internal noise
Te : Effective noise temperature
Pno /Pni = (1 + Te/Tg)
Te = Input referred noise temperature
A passive network with loss = L
Te = (L-1)T
Noise figure
Noise enhancement factor (T0 = 290 K)
nf = Pno /Pni = (1 + Te/T0)
nf = (Si/Ni)/ (So/No)
A passive network with loss = L (at T0)
nf = L
Cascade of amplifiers
Te = Te1 + Te2/g1 + Te3/g1 g2 + …
nf = nf1 + (nf2-1)/g1 + (nf3-1)/g1 g2 + …
First stage should have high gain
Noise figure - example
Receiver working at T=250 K
Antenna : Tg = 50 K
Cable : L = 1 dB
Amplifier : Te = 150 K, g = 20 dB
Mixer : L =3 dB, Nf = 3 dB
Amp : Te = 700 K , g = 30 dB
Te1
Te2
Te3
Te4
=
=
=
=
(L-1)T = (100.1 -1) 250; g1= 10-0.1
150; g2 = 102
(100.3-1)x290; g3 = 10-0.3
700; g4 = 103
Te = Te1 + Te2/g1 + Te3/g1g2 + Te4/g1g2g3
Pno = k (Tg + Te) B g
Sample circuits
Circuit
Te (K)
Nf (dB)
Ideal
LNA (VG)
LNA (G)
0
10
100
0
0.2
1.3
LNA (M)
Amplifier
300
500
3
4.5
Reading
Carlson Ch. 9.3, 9.4
Proakis & Salehi 5.5