amplifier noise
TRANSCRIPT
-
8/14/2019 Amplier Noise
1/19
-
8/14/2019 Amplier Noise
2/19
Objectives Estimate expected amount of output noise
Determine minimum usable signal level
Gain insight into possible improvements
-
8/14/2019 Amplier Noise
3/19
-
8/14/2019 Amplier Noise
4/19
RMS value over averaging interval T:
Xn2
is themean square value of noise x represents current ior voltagee
We will deal with multiple sources of noise
Different noise sources are added as vectors
Xn =1
T
T
0
x2n(t)dt
Xn =
X
2
n1+X
2
n2
-
8/14/2019 Amplier Noise
5/19
Frequency Domain
Noise RMS: computed in the frequencydomain
Thenoise power density is normally specified
From the power density the rms value is found
replaceXwithIfor current, Vfor voltage
x2n
(f) =dX2
n
df
Xn =
fH
fL
x2n(f)df
-
8/14/2019 Amplier Noise
6/19
White &1/fNoise
White: uniform spectral density
white-noise power is proportional to BW
1/f noise: varies with reciprocal off
1/f - noise power is proportional to # ofdecades or octaves
Xn = xnwfH fL
xn = K/f Xn = K
ln (f
H
/fL)
-
8/14/2019 Amplier Noise
7/19
-
8/14/2019 Amplier Noise
8/19
Normally noise is described by specifyingenw
andfce(voltage) or inw andfci(current)
Source of noise appear in different places, andequivalent input noise sources are found
Input sources are filtered by amplifier toproduce output noise
To simplify calculations, actual magnituderesponse is replaced by aBrick-wall equivalent
-
8/14/2019 Amplier Noise
9/19
fo
(log)
f
gain
1/21/2
1.57fo
Brick-wall
equivalent
For single-pole system
Noise-equivalent bandwidth: 1.57f0 for above case
-
8/14/2019 Amplier Noise
10/19
Example 7.3 Piece-wise noise integration
20
eni
nV/Hz1/2
10
102
103104
105106
107
10
102
103104
105106
10710
102
103104
105106
107
10
|A|V/V
20
eno
nV/Hz1/2
10
102
103104
105106
107|A|
200
2
1
200
1 Hz to 1kHz:
En = enw
fceln(fH/fL) + fH fLwith
enw = 20nV /Hzfce = 100Hz fL = 1Hz
andfH = 1kH z
The result is Eno1 = 0.822V.
-
8/14/2019 Amplier Noise
11/19
20
eno
nV/Hz1/2
10
102
103104
105106
107|A|
200
From 1kHz to 10kHz,eno increases with f at a rate of
1dec/dec.So let
no(f) =
20nV/Hz
(f/103) = 21011f
nd
no2 = 21011104
103f2df = 11.5V
-
8/14/2019 Amplier Noise
12/19
-
8/14/2019 Amplier Noise
13/19
-
8/14/2019 Amplier Noise
14/19
Sources of noise
R
e
2
R=4kTR
i2R=4kT/R
R
(noiseless)
(noiseless)
!
+
VO
Vn
Vp
inn
inp
e
noiseless
-
8/14/2019 Amplier Noise
15/19
Example 7.7
!
+
R1
R2
R3
Eno
!
+
VO
Vn
Vp
inn
inp
en
noiseless
R1
R2
R3
iR1
iR2
iR3
-
8/14/2019 Amplier Noise
16/19
Use superposition to obtain:
e2
ni = e2
n + i2
npR2
3+ i2R3R
2
3+i2
nn + i2
R1+ i2R2
(R1 R2)
2
Using i2R =4kTR
,
e2
ni = e2
n + i2
npR2
3+ 4kTR3 +
i2
nn +4kTR1
+ 4kTR2
(R1 R2)
2
= e2n + i2
npR2
3+ 4kTR3 + i
2
nn (R1 R2)2 +
4kT
R1 R2(R1 R2)
2
=e2
n +i2
npR
2
3 + 4kTR3
+i2
nn (R1
R2
)
2
+ 4kT
(R1
R2
)= e2n + i
2
npR2
3+ i2nn (R1 R2)
2 + 4kT (R3 + R1||R2)
-
8/14/2019 Amplier Noise
17/19
For inp = inn = in,
e2
ni = e2
n + i2
nR2
s2 + 4kTRs
where Rs = R3 + R1||R2, R2
s2 = R2
3+ (R1||R2)
2.
Setting R3 = 0 reduces noise.
en dominates for low values ofRs: it is called the short-circuitnoise.
For Rs , eni i2
nR
2
s2: in is called the open-circuit noise.
-
8/14/2019 Amplier Noise
18/19
Noise is amplified by:
Av =1 + R2
R11 + (f/fA)
2=
A0
1 + (f/fA)
2
The total output rms noise is
Eno = A0
E21
+ E22
+ E23
+ E24
where
E21
= e2nw
fceln
fAfL
+ 1.57fA fL
E22
= R23i2npw
fcipln
fAfL
+ 1.57fA fL
E23
= (R1||R2)2i2nnw
fcinln
fAfL
+ 1.57fA fL
andE2
4= 4kT(R3 + R1||R2)(1.57fA fL)
-
8/14/2019 Amplier Noise
19/19
Book says: fLis 1/Tobs where Tobs is the averaging time used tomeasure the output.
TI Application note says: take fH/fL = NEB.For low-noise designs, use op amps with low enw and low corner
frequencies fci and fcn.The total rms input noise can be obtained by dividing by the
signal dc gain As0
Eni =Eno|As0|
and the signal-to-noise ratio from
SNR = 20log10Vi(rms)Eni