6.776 High Speed Communication Circuits Lecture 11 Noise Figure, Impact of Amplifier Nonlinearities

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6.776
High Speed Communication Circuits
Lecture 11
Noise Figure, Impact of Amplifier Nonlinearities
Michael Perrott
Massachusetts Institute of Technology
March 10, 2005
Copyright © 2005 by Michael H. Perrott
Noise Factor and Noise Figure (From Lec 10)
Rs
Equivalent output
referred current noise
(assumed to be independent
of Zout and ZL)
enRs
vin
vx
Zin
Linear,Time Invariant
Circuit
(Noiseless)
ƒ
Definitions
ƒ
Calculation of SNRin and SNRout
H.-S. Lee & M.H. Perrott
iout
inout
Zout
ZL
MIT OCW
Alternative Noise Factor Expression
Rs
Equivalent output
referred current noise
(assumed to be independent
of Zout and ZL)
enRs
vin
vx
Zin
Linear,Time Invariant
Circuit
(Noiseless)
ƒ
From previous slide
ƒ
Calculation of Noise Factor
H.-S. Lee & M.H. Perrott
iout
inout
Zout
ZL
MIT OCW
Thevenin Computation Model For Noise (from Lec 10)
iout
D
Iout
G
D
G
S
Zg
Zg
Zgs
vgs
Cgs
gmvgs
indg
Zdeg
S
Zdeg
H.-S. Lee & M.H. Perrott
MIT OCW
Thevenin Computation Model For Noise (from Lec 10)
iout
D
Iout
G
D
G
S
Zg
Zg
Zgs
vgs
Cgs
gmvgs
indg
Zdeg
S
Zdeg
ƒ
We analyzed a non-degenerated CMOS amplifier in Lec 10
- Broadband amplifiers: gate noise not significant
- Narrowband amplifiers:
ƒ Assumed in analysis that we operated at resonance
ƒ Q turned out to be key design parameter
Can we simultaneously design amplifiers for optimal noise
match and optimal power match?
H.-S. Lee & M.H. Perrott
MIT OCW
Input Referred Noise Model
Equivalent output
referred current noise
(assumed to be independent
of Zout and ZL)
enRs
Rs
vin
vx
Zin
Linear,Time Invariant
Circuit
(Noiseless)
iout
inout
Zout
ZL
en
iin
is
Ys
vx
in
Zin
Linear,Time Invariant
Circuit
(Noiseless)
iout
en
Can remove the signal source
since Noise Factor can be
expressed as the ratio of total
output noise to input noise
H.-S. Lee & M.H. Perrott
is
Ys
in
iin,sc=
iout
β
MIT OCW
Input-Referred Noise Figure Expression
en
is
Ys
in
iin,sc=
iout
β
ƒ
We know that
ƒ
Let’s express the above in terms of input short circuit
current
H.-S. Lee & M.H. Perrott
MIT OCW
Calculation of Noise Factor
en
is
Ys
in
ƒ
By inspection of above figure
ƒ
In general, en and in will be correlated
-Y
c
iout
iin,sc=
β
is called the correlation admittance
H.-S. Lee & M.H. Perrott
MIT OCW
Noise Factor Expressed in Terms of Admittances
en
is
ƒ
Ys
Yc
iu
iout
iin,sc=
β
We can replace voltage and current noise currents
with impedances and admittances
H.-S. Lee & M.H. Perrott
MIT OCW
Optimal Source Admittance for Minimum Noise Factor
ƒ
Express admittances as the sum of conductance, G,
and susceptance, B
ƒ
Take the derivative with respect to source admittance
and set to zero (to find minimum F), which yields
ƒ
Plug these values into expression above to obtain
H.-S. Lee & M.H. Perrott
MIT OCW
Optimal Source Admittance for Minimum Noise Factor
ƒ
After much algebra (see Appendix L of Gonzalez*
book for derivation), we can derive
- Contours of constant noise factor are circles centered
about (G ,B ) in the admittance plane
- They are also circles on a Smith Chart (see pp 299-302
opt
opt
of Gonzalez for derivation and examples)
ƒ
How does (Gopt,Bopt) compare to admittance achieving
maximum power transfer?
*Guillermo Gonzalez, Microwave Transistor Amplifiers:
Analysis and Design, Prentice Hall, 1996
H.-S. Lee & M.H. Perrott
MIT OCW
Optimizing For Noise Figure versus Power Transfer
Signal
iin
Source
Source
conductance susceptance
is
Gs
en
Bs
vx
in
Zin
Source noise produced
by source conductance
iout
Bs
Example source
admittance for maximum
Bopt
power transfer
Circles of constant
Noise Factor
(Fmin at the center)
Bmax
Gmax Gopt
ƒ
Linear,Time Invariant
Circuit
(Noiseless)
Gs
One cannot generally achieve minimum noise figure if
maximum power transfer is desired
H.-S. Lee & M.H. Perrott
MIT OCW
Optimal Noise Factor for MOS Transistor Amp
ƒ
Consider the common source MOS amp (no
degeneration) considered in Lecture 10
- In Tom Lee’s book (pp. 272-276 (1
st
ed.), pp. 364-369 (2nd
ed.)), the noise impedances are derived as
- The optimal source admittance values to minimize noise
factor are therefore
H.-S. Lee & M.H. Perrott
MIT OCW
Optimal Noise Factor for MOS Transistor Amp (Cont.)
ƒ
Optimal admittance consists of a resistor and
inductor (wrong frequency behavior – broadband
match fundamentally difficult)
- If there is zero correlation, inductor value should be set
ƒ
to resonate with Cgs at frequency of operation
Minimum noise figure
- Exact if one defines w = g /C
t
H.-S. Lee & M.H. Perrott
m
gs
MIT OCW
Recall Noise Factor Comparison Plot From Lecture 10
Noise Factor Scaling Coefficient Versus Q for 0.18 µ NMOS Device
8
Noise Factor Scaling Coefficient
7
6
c = -j0
c = -j0.55
5
Achievable values as
a function of Q under
the constraint that
1
= wo
LgCgs
c = -j1
c = -j0
4
c = -j0.55
3
1
0
Minimum across
all values of Q and
1
Note: curves
meet if we
approximate
Q2+1 Q2
2
1
2
H.-S. Lee & M.H. Perrott
3
c = -j1
LgCgs
4
5
6
Q
7
8
9
10
MIT OCW
Example: Noise Factor Calculation for Resistor Load
Source
Source
Rs
Rs
enRs
enRL
vin
RL
vout
RL
ƒ
Total output noise
ƒ
Total output noise due to source
ƒ
Noise Factor
H.-S. Lee & M.H. Perrott
vnout
MIT OCW
Comparison of Noise Figure and Power Match
Source
Source
Rs
Rs
enRs
enRL
vin
RL
vout
RL
ƒ
To achieve minimum Noise Factor
ƒ
To achieve maximum power transfer
H.-S. Lee & M.H. Perrott
vnout
MIT OCW
Example: Noise Factor Calculation for Capacitor Load
Source
Source
Rs
Rs
vin
CL vout
ƒ
Total output noise
ƒ
Total output noise due to source
ƒ
Noise Factor
H.-S. Lee & M.H. Perrott
enRs
CL
vnout
MIT OCW
Example: Noise Factor with Zero Source Resistance
Source
RL
RL
vin
CL vout
ƒ
Total output noise
ƒ
Total output noise due to source
ƒ
Noise Factor
H.-S. Lee & M.H. Perrott
enRL
CL
vnout
MIT OCW
Example: Noise Factor Calculation for RC Load
Source
Source
Rs
Rs
enRs
enRL
vin
CL
RL vout
ƒ
Total output noise
ƒ
Total output noise due to source
ƒ
Noise Factor
H.-S. Lee & M.H. Perrott
CL
RL
vnout
MIT OCW
Example: Resistive Load with Source Transformer
Source
RS
Vs
Rin=
N
RL
Vx
1
2
Vout=NVx
2
RL
Rout=N Rs
1:N
Source
enRs
RS
Rin=
1
N
enRL
Vx
2
Rout=N2Rs
RL
Vnout=NVx
RL
1:N
ƒ
For maximum power transfer (as derived in Lecture 3)
H.-S. Lee & M.H. Perrott
MIT OCW
Noise Factor with Transformer Set for Max Power Transfer
Source
enRs
RS
enRL
Vx
Rin= Rs
Rout=RL
1:N=
RL
RL
V
Rs x
RL
Rs
ƒ
Total output noise
ƒ
Total output noise due to source
ƒ
Noise Factor
H.-S. Lee & M.H. Perrott
Vnout=
MIT OCW
Observations
Source
RS
enRs
enRL
Vx
Rin= Rs
Rout=RL
1:N=
ƒ
ƒ
Vnout=
RL
RL
V
Rs x
RL
Rs
If you need to power match to a resistive load, you
must pay a 3 dB penalty in Noise Figure
- A transformer does not alleviate this issue
What value does a transformer provide?
- Almost-true answer: maximizes voltage gain given the
-
power match constraint, thereby reducing effect of
noise of following amplifiers
Accurate answer: we need to wait until we talk about
cascaded noise factor calculations
H.-S. Lee & M.H. Perrott
MIT OCW
Nonlinearities in Amplifiers
ƒ
We can generally break up an amplifier into the
cascade of a memoryless nonlinearity and an input
and/or output transfer function
Vdd
Memoryless
Nonlinearity
RL
Lowpass
Filter
Vout
Vin
Id
Vin
M1
CL
Id
-RL
Vout
1+sRLCL
ƒ
Impact of nonlinearities with sine wave input
ƒ
Impact of nonlinearities with several sine wave inputs
- Causes harmonic distortion (i.e., creation of harmonics)
- Causes harmonic distortion for each input AND
intermodulation products
H.-S. Lee & M.H. Perrott
MIT OCW
Analysis of Amplifier Nonlinearities
ƒ
Focus on memoryless nonlinearity block
- The impact of filtering can be added later
Memoryless
Nonlinearity
x
ƒ
y
Model nonlinearity as a Taylor series expansion up to
its third order term (assumes small signal variation)
- For harmonic distortion, consider
- For intermodulation, consider
H.-S. Lee & M.H. Perrott
MIT OCW
Harmonic Distortion
ƒ
Substitute x(t) into polynomial expression
Fundamental
ƒ
Harmonics
Notice that each harmonic term, cos(nwt), has an
amplitude that grows in proportion to An
Very small for small A, very large for large A
H.-S. Lee & M.H. Perrott
MIT OCW
Frequency Domain View of Harmonic Distortion
3
Memoryless
Nonlinearity
A
0
ƒ
3c A
Afund = c1A + 3
4
w
x
y
0
w
2w 3w
Harmonics cause “noise”
- Their impact depends highly on application
ƒ LNA – typically not of consequence
ƒ Power amp – can degrade spectral mask
ƒ Audio amp – depends on your listening preference!
ƒ
Gain for fundamental component depends on input
amplitude!
H.-S. Lee & M.H. Perrott
MIT OCW
1 dB Compression Point
3
Memoryless
Nonlinearity
A
0
ƒ
ƒ
3c A
Afund = c1A + 3
4
w
x
Definition: input signal level
such that the small-signal
gain drops by 1 dB
y
0
w
2w 3w
20log(Afund)
- Input signal level is high!
1 dB
A1-dB
20log(A)
Typically calculated from simulation or measurement
rather than analytically
- Analytical model must include many more terms in Taylor
series to be accurate in this context
H.-S. Lee & M.H. Perrott
MIT OCW
Harmonic Products with An Input of Two Sine Waves
ƒ
DC and fundamental components
ƒ
Second and third harmonic terms
ƒ
Similar result as having an input with one sine wave
- But, we haven’t yet considered cross terms!
H.-S. Lee & M.H. Perrott
MIT OCW
Intermodulation Products
ƒ
Second-order intermodulation (IM2) products
ƒ
Third-order intermodulation (IM3) products
- These are the troublesome ones for narrowband
systems
H.-S. Lee & M.H. Perrott
MIT OCW
Corruption of Narrowband Signals by Interferers
Memoryless
Nonlinearity
X(w)
0
Interferers
Desired
Narrowband
Signal
y
W
w1 w 2
Y(w)
x
Corruption of desired signal
W
w1 w2
2w1 2w2
3w1 3w2
0 w2-w1
2w1-w2 2w2-w1 w1+w2 2w1+w2 2w2+w1
ƒ
Wireless receivers must select a desired signal that is
accompanied by interferers that are often much larger
- LNA nonlinearity causes the creation of harmonic and
intermodulation products
- Must remove interference and its products to retrieve
desired signal
H.-S. Lee & M.H. Perrott
MIT OCW
Use Filtering to Remove Undesired Interference
Memoryless
Nonlinearity
X(w)
0
Interferers
w1 w 2
Y(w)
Desired
Narrowband
Signal
x
y
Bandpass
Filter
z
W
Corruption of desired signal
W
w1 w2
2w1 2w2
3w1 3w2
0 w2-w1
2w1-w2 2w2-w1 w1+w2 2w1+w2 2w2+w1
Z(w)
Corruption of desired signal
W
2w1 2w2
3w1 3w2
w1 w2
0 w2-w1
2w1-w2 2w2-w1 w1+w2 2w1+w2 2w2+w1
ƒ
Ineffective for IM3 term that falls in the desired signal
frequency band
H.-S. Lee & M.H. Perrott
MIT OCW
Characterization of Intermodulation
ƒ
Magnitude of third order products is set by c3 and
input signal amplitude (for small A)
ƒ
Magnitude of first order term is set by c1 and A (for
small A)
ƒ
Relative impact of intermodulation products can be
calculated once we know A and the ratio of c3 to c1
- Problem: it’s often hard to extract the polynomial
coefficients through direct DC measurements
ƒ Need an indirect way to measure the ratio of c3 to c1
H.-S. Lee & M.H. Perrott
MIT OCW
Two Tone Test
ƒ
Input the sum of two equal amplitude sine waves into
the amplifier (assume Zin of amplifier = Rs of source)
vin(w)
Equal Amplitude
Sine Waves
2A
0
w 1 w2
Note: v (w)
in
vx(w) =
2
W
first-order output
Vout(w)
third-order IM term
Amplifier
Rs
Vx
Vout
vin
Vbias
Zin=Rs
2
3
Vout=co+c1Vx+c2Vx+c3Vx
W
w1 w2
2w1 2w2
3w1 3w2
0 w2-w1
2w1-w2 2w2-w1 w1+w2 2w1+w2 2w2+w1
ƒ
On a spectrum analyzer, measure first order and third
order terms as A is varied (A must remain small)
- First order term will increase linearly
Third order IM term will increase as the cube of A
H.-S. Lee & M.H. Perrott
MIT OCW
Input-Referred Third Order Intercept Point (IIP3)
ƒ
Plot the results of the two-tone test over a range of A
(where A remains small) on a log scale (i.e., dB)
- Extrapolate the results to find the intersection of the
first and third order terms
20log(Afund)
1 dB
First-order
output = c1A
Third-order
3 c A3
IM term = 4 3
A1-dB
Aiip3
20log(A)
- IIP3 defined as the input power at which the
extrapolated lines intersect (higher value is better)
ƒ Note that IIP3 is a small signal parameter based on
extrapolation, in contrast to the 1-dB compression point
H.-S. Lee & M.H. Perrott
MIT OCW
Relationship between IIP3, c1 and c3
ƒ
Intersection point
ƒ
Solve for A (gives Aiip3)
20log(Afund)
1 dB
First-order
output = c1A
Third-order
3 c A3
IM term = 4 3
A1-dB
ƒ
Aiip3
20log(A)
Note that A corresponds to the peak value of the two
cosine waves coming into the amplifier input node (Vx)
- Would like to instead like to express IIP3 in terms of power
H.-S. Lee & M.H. Perrott
MIT OCW
IIP3 Expressed in Terms of Power at Source
ƒ
IIP3 referenced to
Vx (peak voltage)
vin(w)
0
ƒ
Note: v (w)
in
vx(w) =
2
Equal Amplitude
Sine Waves
2A
w 1 w2
W
Rs
Amplifier
Vx
Vout
vin
IIP3 referenced to Vx
(rms voltage)
Vbias
Zin=Rs
2
3
Vout=co+c1Vx+c2Vx+c3Vx
ƒ
Power across Zin = Rs
H.-S. Lee & M.H. Perrott
ƒ
Note: Power from vin
MIT OCW
IIP3 as a Benchmark Specification
ƒ
ƒ
Since IIP3 is a convenient parameter to describe the level
of third order nonlinearity in an amplifier, it is often
quoted as a benchmark spec
Measurement of IIP3 on a discrete amplifier would be
done using the two-tone method described earlier
- This is rarely done on integrated amplifiers due to poor
access to the key nodes
- Instead, for a radio receiver for instance, one would simply
put in interferers and see how the receiver does
ƒ Note: performance in the presence of interferers is not just a
function of the amplifier nonlinearity
ƒ
Calculation of IIP3 is most easily done using a simulator
such as Hspice or Spectre
- Two-tone method is theoretically not necessary – simply
curve fit to a third order polynomial
H.-S. Lee & M.H. Perrott
MIT OCW
Impact of Differential Amplifiers on Nonlinearity
I1
vid
2
Memoryless
Nonlinearity
I2
M1
M2
vx
-vid
2
vid
Idiff = I2-I1
2Ibias
ƒ
Assume vx is approximately incremental ground
ƒ
Second order term removed and IIP3 increased!
H.-S. Lee & M.H. Perrott
MIT OCW
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