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Special Topics in Electronics Engineering
Emad HegaziProfessor, ECE
Communication Circuits Research Grouphttp://www.iclasu.edu.eg/ehgroup
Spring2014
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17!
Es/No or Eb/No=?
Spring2014
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Noise Figure Calculation
receiver
BasebandRF input
nfP
minSNR
NFinSNR
Standard Bandwidth10log(BW) Sensitivity(dBm) Noise Floor (dBm) SNRin(dB) NF(dB) SNRmin(dB)
DECT 1.70E+06 62.30 -83.00 -111.50 28.50 18.20 10.3
GSM 2.00E+05 53.01 -102.00 -120.79 18.79 9.79 9
WLAN 2.00E+06 63.01 -80.00 -110.79 30.79 15.69 15.1
BW
RdB
NE
dBSNRBW
R
NE
SNR symbolssymbols log10)()(0
min0
min
Spring2014
RF
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IP3 Calculation
10
23
3)(2
31
min3
min3
IIPdB
nfsfIIP
nfIIPsf
PP
PSNRDRP
SNRPP
DR
Standard DR SFDR IIP3 Pmax Bandwidth 10log(BW) Sensitivity(dBm)Bluetooth 50.00 36.57 -10.00 -20.00 1.00E+06 60.00 -70.00GSM 87.00 61.67 -5.00 -15.00 2.00E+05 53.01 -102.00WLAN 76.00 52.30 6.00 -4.00 2.00E+06 63.01 -80.00
Spring2014
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Simplified Transceiver Architecture
Spring2014
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Role of a Receiver
090
AD
AD
HPMX-2007
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lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
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wklhjr qlih qilh q q3wih qwklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh lihewrw
The lkhefw wlkhq wilehrwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.
Power Supply
uP/DSP
Low Noise Amplifier
Mixer
Oscillator
Baseband Processor
De-Modulator
bias
I Data
Q Data
1 .amplify received signal with min. added
noise
2 .shift to lower frequency (cost and/or
performance)
3 .LO for down conversion
4 .discard carrier and recover data
Information
bias bias
Antenna
Spring2014
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Can we use a BPF for channel selection?
• The adjacent channels are always considered as interferers. These interferes could affect the reception of the signal.
• It is important to filter the unnecessary channels • Example:
It is desired to filter the alternate channel by 35 dB using an LC-BPF. Determine the quality factor of the tank.
Solution:
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Too large cannot be achieved
Spring2014
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Band Selection
• The BPF before the LNA is used as a band select filter– Specification is relaxed compared to the case where it is used as a
channel select filter– It has a constant frequency response and does not need to be
tunable
• The BPF is implemented using:– SAW technology for frequencies below 10 GHZ– MEMS technology for mm-wave frequencies
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd EditionDesired Band
f
Band Select filter
Spring2014
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9
Band Selection
• TX-RX feedthrough can limit the performance of the receiver• Typically the received signal is in the order of -70 dBm• Feedthrough may saturate the BB blocks because of the high gain• Is an issue in full duplex transceivers• Design Targets:
– LNA must tolerate this high input level– A BPF is usually included at the output of LNA provide additional filtering
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
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10
Band Selection
• Band select filters are usually implemented in a duplexer• Single antenna transceivers use a duplexer to isolate
between TX and RX• Duplexers are two BPF, one for RX and the other for TX
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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Channel Selection Remarks
• Channel selection cannot be done before the LNA because:– It is hard to find a BPF with large quality factor, and achieving a very small
loss– Having a tunable BPF with high quality factor is hard to obtained
• Usually, there are two steps to select a channel:
– Band selection: In which the entire band is selected. This step usually comes before the LNA.
– Channel selection: In which the desired channel is selected. This step is usually done after the first mixer.
M. El-Nozahi
Spring2014
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Superheterodyne Receiver
Spring2014
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Example: AM Radio
• AM radio band: 530 to 1610 KHz• BW/2 = (1610-530)/2=1080/2=540, in band• IF has to be lower. Commonly: 455kHz• Image can be in AM band• If LO is on low side, LO tuning range is:
– (530 to 1610) – 455 = (75 to 1155)– LO lowest to highest is a factor of 15.4
• If LO is on high side, LO tuning range is:– (530 to 1610) + 455 = (985 to 2065)– LO lowest to highest is a factor of 2.01
Spring2014
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14
Typical Superheterodyne Digital Receiver
Prof. E Sanchez-Sinencio RF course slides
Advantage Disadvantages
Good selectivity High complexity
Good sensitivity High power consumption
Image problem
External components
Not suitable for multi-standard
Spring2014
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15
The Image Problem
• The image could be another user or standard• The image must be filtered out before going the mixer• Frequency planning is key
Prof. E Sanchez-Sinencio RF course slides
Spring2014
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Image Rejection Calculation
SNRmin
fIF
IRrequired
fRFfLO
Pdesired
PImage
minSNRPPIR desiredimagerequired
)all in dB’s(
Spring2014
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Mixer = Multiplying up/down conversion
• Frequency translation device• Ideal mixer:
• Doesn’t “mix”; it multiplies
A
B
AB
Spring2014
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Super-heterodyne Receiver
Spring2014
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Selection of IF
• If IF is large, – better separation between RF and image– better image rejection– easier image rejection filter design– More stages of down conversion
• Other IF selection criteria– Select IF so that image freq is outside of RF
band– IF >= (RF BW)/2
• Sometime may not be possible, if (RF BW)/2 is within RF Band
Spring2014
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• For each channel assignment, there are two choices of LO freq that meets the requirement |RF–LO|=IF.
• Q: should LO > RF, or LO < RF??
Spring2014
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Image problem converting to IF
A1cos(wRFt)
A has desired signal at wIF
plus an interference at wIM
A2cos(wIMt)
B is at wLO
And:
wRF - wLO = wLO - wIM = wIF
Both converted to IF,Can’t be cleaned once corrupted
Spring2014
RF
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Image Problem
)()(cos2
)()(cos2
)cos())(cos()()()(
)cos()(
message is )();)(cos()(
tmtAB
tmtAB
ttmtABtBtAtC
tBtB
tmtmtAtA
LOx
LOx
LOx
LO
x
?
IFLOimagex
IFLORFx
if
OKif
Spring2014
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Problem of Image Signal
IF
RFimage LO
Spring2014
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Problem of Image Signal
• Solution: Image Rejection Filter
RFimage LO
Spring2014
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25
The Image Problem
• Image Reject filter versus channel selection:
• Larger IF frequencies requires channel select filter with higher Q
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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26
Dual-IF Heterodyne Receiver
• Channel selection is done in two stages, hence relaxing the specification for each stage
• Secondary image problem– To avoid the problem, the second IF frequency is set to zero
• Is it possible to have a zero IF?
M. El-Nozahi
Spring2014
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27
Down Conversion to IF
M. El-Nozahi
AM modulation:
FM/ Digital ..etc . modulations:
Spring2014
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High Q Alternatives
• What is really needed is not really a filter.• A cancellation scheme to reject noise is
good enough
Spring2014
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Cosine wave
High Q Alternatives
• What if we use a sine wave instead
Spring2014
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j
-j
j
-j
Complex Signal Representation
Niknejad and Shana’a
Spring2014
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Orthogonality of I and Q
Niknejad and Shana’a
Spring2014
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Orthogonality
Spring2014
Des
ign
of R
F C
ircui
ts &
Sys
tem
s
Spring2014
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33
Image Reject Receivers-I
– What is a shift by 90o?
– The 90o phase shift is also called Hilbert transform
M. El-Nozahi
ffc-fc
𝐴2
𝐴2
Re
Im
f
fc
-fc
Re
Im
− 𝑗𝐴2
𝑗𝐴2
𝑋 90(𝜔)=𝑋 (𝜔) [− 𝑗 𝑠𝑔𝑛(𝜔) ]
Spring2014
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34
Hilbert transform:
• A 90o phase shift results in:– Rotating positive frequency components CW by 90o
– Rotating negative frequency components CCW by 90o
• Multiplication by +j rotates all frequency components CCW by 90o.
• Multiplication by -j rotates all frequency components CW by 90o.
• Note that for DC frequencies these transformations do not have any meaning
M. El-Nozahi
Spring2014
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35
Hilbert transform
• Assume I(t) is shifted by 90o to produce Q(t). Find I(t)+jQ(t).
M. El-Nozahi
ffc-fc
Re{I}
Im{I}
f
fc
-fc
Re{Q}
Im{Q}
f
fc
-fc
Re{jQ}
Im{jQ} Im{I+jQ}
ffc-fc
Re{I+jQ}Spring2014
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36
Image Reject Receivers
• Idea: From the previous example it seems that one could remove the image with the help of quadrature components.
M. El-Nozahi
ffs-fs
Re{I}
Im{I}
-fi fi
f
Re{I}Im{I}{
-fIF fIF
fLO
f
Re{Q}Im{Q}
-fIF fIF
Spring2014
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37
Hartley Image Reject Architecture
• A Hilbert transform is used to cancel the image• I&Q (quadrature) signals are generated for image rejection.• The generation of the 90o could be achieved using RC phase shifter each providing 45o phase shift (narrow band solution)
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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38
Hartley Image Reject Architecture
• Still in the BB we must generate another I&Q for digital demodulation
• Drawbacks:– Mismatch between the two path will result in finite image rejection– The RC solution can be used for narrow-band architectures. Wideband
architecture will result in degraded performance for the image rejection (IRR)– Typical values for IRR is lower than 35 dB.
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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Implementing the Phase ShiftHartley Architecture with simple 90 deg phase shiftor
Spring2014
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Spring2014
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IRRt
AAt
AAtx imLO
imLORFLO
RFLOA )sin(
2)sin(
2)(
)(cos2
)()(cos2
)()( tA
AtA
Atx imLOim
LORFLORF
LOB
)cos(2
)cos(2
)(
t
At
AAtx imLO
imRFLO
RFLOC
cos2
cos2
)()( t
AAt
AAtx RFLO
RFLORFLO
RFLOsig
cos2
cos2
)()( t
AAt
AAtx imLO
imLOimLO
imLOim
cos)(2)(
cos)(2)(.
22
22
2
2
LOLOLOLO
LOLOLOLO
RF
im
outsig
im
AAAA
AAAA
A
A
P
P
Input image power ratio
44
4
4
)cos1)((2
cos)(2)(
cos)(2)(
22
22
2
222
2
2
22
22
AA
AIRR
A
A
A
AA
AAAA
AAAAIRR
LO
LO
LO
LOLO
LOLOLOLO
LOLOLOLO
1
1
1
1222222
CRCCRR
CCRR
A
A
2
1
2
C
C
R
RC
CR
RC
CR
R
A
A
Gain Mismatch due to R, C errors
At w = 1/RC:
Spring2014
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47
Weaver Image Reject Architecture
• Hilbert transform is obtained using another quadrature (complex) mixing stage
• Advantages compared to Hartley:– Better accuracy in generating the additional 90o phase shift– IRR is limited to 40 dB, which is higher than Hartley architecture
• Disadvantages:– Secondary image problem
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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48
Direct Conversion Receiver
• A single step down conversion is used. The output frequency is at DC
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd EditionAdvantages Disadvantages
No image problem LO leakage
Less complex / low power consumption
DC offset
Channel selection is done with a LPF Even order distortion
Effect of mixer spurs are reduced Flicker noise
IQ mismatch
Spring2014
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49
LO Leakage
– The LO signal can be leaked to the antenna by the capacitive coupling or substrate
– For singled ended Los, the LO leakage can reach -60 dBm– Differential LO architectures have lower LO leakage (better than -
100 dBm)
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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50
Direct Conversion Receiver
• DC Offset:– The leaked LO signal can go through the antenna, LNA and down
converted – Because of the LO signal and its feedthrough signal carry the same
frequency, a DC offset is produced (this phenomena is called LO self mixing).
– BB blocks usually have high again, hence the LO self mixing may saturate the receiver– HPF are not common because they require a very low cut-off frequency
(large components, slow settling)
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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51
Even Order Distortion
M. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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52
Direct Conversion Receiver
• Flicker Noise:
• For 802.11g the channel bandwidth is 10MHz. With a noise corner frequency of 200kHz• For GSM, the channel bandwidth is 100 kHz and therefore a
large portion of noise appears due to flicker noiseM. El-Nozahi
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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53
Direct Conversion Receiver
• IQ mismatch:– mismatch in I and Q path affects SNR of received signals– Mismatch effects are more dominate at high frequencies. Reducing the
frequency at which the I and Q signal are generated enhances the SNR– Digital calibration is used to correct these mismatches
M. El-Nozahi
Amplitude mismatch:
Phase mismatch:
Spring2014
RF
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54
Low-IF Receiver
• Has all the advantages of direct conversion receivers• More difficult image rejection requirements• Minimum IF frequency is channel bandwidth• DC offset is outside the signal bandwidth
Complex Filter
LargeRequires matchingPower hungry
Spring2014
RF
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s an
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ADC
ADC
PGA
PGA
LNA
RFPLL
DIG
ITA
LF
ILT
ER
100 kHz
I
Q
sin cos
RFSAW
sin cos
270 kS/s
925-960MHz
925.1 - 960.1MHz
Low IF receiver
-Quadrature RF down conversion required
-Require higher performance ADC-Additional mixer
-Slower RF PLL settling-Even order distortion still
problem-Low freq IF filters require large
chip area
+Eliminate IF SAW, IF PLL and image filtering
+Integration
+Relaxes image rejection requirements
+Avoids DC problems, relaxes 1/f noise problem
Spring2014
RF
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Low-IF Down Conversion
LOω
Complex BPF
Mirror signal, needs removal
Spring2014
RF
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Mirror Signal Suppression
ComplexBandpass
Filter
I Q I Q
LO1 LO2
Spring2014
RF
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Complex Mixing- Real LO
Spring2014
RF
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Complex Mixing-Complex LO
Spring2014
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Complex Mixing
Spring2014
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61
Bluetooth Receiver
• Has all the advantages of direct conversion receivers• More difficult image rejection requirements• Minimum IF frequency is channel bandwidth• DC offset is outside the signal bandwidth
Spring2014
RF
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Direct Conversion Receiver
Little image problemNo IQ filter@ IF
PGA
PGA
LNA
RFSAW ADC
ADC
DIG
ITA
LF
ILT
ER
I
Q
RFPLL
sin cos
270 kS/s
925-960MHz
925 - 960MHz
Spring2014
RF
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Direct Conversion Receiver
LO is at same frequency as RF1/f noise here can end up in channel
Self mixing cause DC problem
+Eliminate IF SAW, IF PLL and image filtering+ Integration+ easier image problem
-Quadrature RF down conversion required
-DC problem -Typically requires offset or
2x LO to avoid coupling
Spring2014
RF
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DC Offset (Self-mixing)
AD w c
aLO(t)=ALOcos( w c+q)
0
w c
)(, tx LOoffset
capacitive couplingsubstrate couplingbondwire coupling
Saturates the following stages
AD w c 0
w c
)(, tx RFoffset
Spring2014
RF
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DC Offset (Self-mixing)
θωω
θωθωω
ω
tAA
tAtAA
tataAtx
cLOcrosstalk
cLOcLOcrosstalk
LOLOcrosstalkLOoffset
2cos1)(
coscos)(
)()()()(
221
,
φ)(ω2cos1)ω(
φ)(ωcos)ω(
)()()ω()(
2interferer2
1
22interferer
interfererinterfererinterferer,
tmtAA
tmtAA
tataAtx
ccrosstalk
ccrosstalk
crosstalkoffset
level
DC Offset
+
-
t
φ)(ω2cos1)ω(
φ)(ωcos)ω(
)()()ω()(
2interferer2
1
22interferer
interfererinterfererinterferer,
tmtAA
tmtAA
tataAtx
ccrosstalk
ccrosstalk
crosstalkoffset Spring2014
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DC Offset Cancellation
• Capacitive Coupling– Requires a large capacitor
• Negative Feedback– Nonlinear -A
Spring2014
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1/f noise effect
• CMOS transistors has significant 1/f noise at low to DC frequency
• Significantly noise performance of direct conversion receivers
Receive signal1/f noise
f
Spring2014
RF
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Even-Order Distortion
c
0c
0
Direct feed through
Direct feed through
Interferers
y(t) = a1 x(t) + a2 x2(t)
Dw
Dw
a2 A1A2 cos(Dw)
Spring2014
RF
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Mirror Signal
• Upper sideband and lower sideband are identical
RF
LO
0
0
Spring2014
RF
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Mirror Signal • Upper sideband and lower sideband are not
identical
RF
LO
0
0
Spring2014
RF
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Mirror Signal Suppression
• Quadrature Down Conversion
AD
090
AD
a(t)
ui(t)
uq(t)
vi(t)
vq(t)
I
Q Spring2014
RF
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Quadrature Conversion
)(
)(tan)(
))(tan()(
)(
))(sin()(
))(cos()(
)sin()()(
)cos()()(
))(cos()(
1
21
21
tv
tvtm
tmtv
tv
tmtv
tmtv
ttatu
ttatu
tmtta
i
q
i
q
q
i
LOq
LOi
RF
Spring2014
RF
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Quadrature Down Conversion
RF
LO
0
0
Spring2014
RF
Sys
tem
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ts
I/Q Mismatch
090
I
Q
Phase & Gain Error
Phase & Gain Error
Phase & Gain Error
)(, tx ILO
)(, tx QLO
)(, tx IBB
)(, tx QBB
a(t)
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
I/Q Mismatch due to LO errors
2)(sin
21
2)(
2)(cos
21
2)(
2sin
21)(
2cos
21)(
)(cos)(
,
,
,
,
tmA
tx
tmA
tx
ttx
ttx
tmtAta
QBB
IBB
cQLO
cILO
c
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
2
2ˆ
ˆ
2222
1
)(
)()(ˆ Find :Exercise
unbiased. is )(ˆ Hence,
)())(ˆ( Clearly,
0)(,))((,))(( and
0)( ,0)( Suppose
)2/)(cos()2/1(
)2/)(sin()2/1(tan)(ˆ
tm
tmtmEσ
tm
tmtmE
EσEσE
EE
tm
tmtm
def
m
m
ε
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Use of I/Q down conversion recovers the nonsymmetrical receive signal spectrumBut port isolation becomes more challengingSelfmixing and even order distortion may affect both channels and affect each other, causing additional I/Q mismatch
Spring2014
RF
Sys
tem
s an
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ircui
ts
090
a(t)
A/D
A/D
Base Band
DSP
Phase and gain mismatchcompensation
DC and 1/fcancellation
Spring2014
RF
Sys
tem
s an
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ircui
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Summary of Direct Conversion Receiver
• No need for imager reject filter• Suitable for monolithic integration with baseband • DC offsets due to crosstalk of input ports of mixer• Even order IM direct feed through to baseband• Quadrature down conversion suppresses mirror• I/Q mismatch due to mismatches in parasitics• Low power consumption attributes to less hardware
Spring2014
RF
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Balun
Spring2014
RF
Sys
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ts
Texas Instruments 2006
Phase Noise
Spring2014
RF
Sys
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s an
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ts
Texas Instruments 2006
Trsnmitter Paradigms
• Signal is strong.• We need to make sure efficient delivery
of power to the antenna.• Spectral content should be contained to
its specified limits.• Linearity matters if modulation is linear. Spring
2014
RF
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Transmit Specifications• Transmit spectrum mask
Spring2014
RF
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Transmitter Specifications
20 20
4040
Adjacent channel
alternate adjacent channel
Spring2014
RF
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Transmitter Architectures
• Direct Conversion Transmitter• Two-step Conversion Transmitter• Offset PLL Transmitter
Spring2014
RF
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tem
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d C
ircui
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Direct-conversion transmitter
090
I
QwLO
Pros: less spurious synthesizedCons: more LO pulling
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Direct-conversion transmitter with offset LO
090
I
Q
wLOw1
w2
Pros: less LO pullingCons: more spurious synthesized
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
090
I
Q
cosw1tcosw2t
w1+w2
Pros: less LO pulling superior IQ matching
Cons: required high-Q bandpass filter
Two-step transmitter
Spring2014
RF
Sys
tem
s an
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Offset PLL Transmitter
090
I
Q
cosw1tPD/LPF VCO
1/NSpring2014
RF
Sys
tem
s an
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Simplified Transceiver Architecture
Spring2014
RF
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90
Role of a Receiver
090
AD
AD
HPMX-2007
The lkhefw wlkhq wilehrwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih q
The lkhefw wlkhq wilehrwejklh wajkhrqwilu wae.esjlkh qwh wlh lihewrw
wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh lihewrw
wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh lihewrw
wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh lihewrw
wklhjr qlih qilh q q3wih qwklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh lihewrw
wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh lihewrw
wklhjr qlih qilh q q3wih qwklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh lihewrw
The lkhefw wlkhq wilehrwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.esjlkh qwh wlh
lihewrw wklhjr qlih qilh q q3wih qwejklh wajkhrqwilu wae.
Power Supply
uP/DSP
Low Noise Amplifier
Mixer
Oscillator
Baseband Processor
De-Modulator
bias
I Data
Q Data
1 .amplify received signal with min. added
noise
2 .shift to lower frequency (cost and/or
performance)
3 .LO for down conversion
4 .discard carrier and recover data
Information
bias bias
Antenna
Spring2014
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91
92
Can we use a BPF for channel selection?
• The adjacent channels are always considered as interferers. These interferes could affect the reception of the signal.
• It is important to filter the unnecessary channels • Example:
It is desired to filter the alternate channel by 35 dB using an LC-BPF. Determine the quality factor of the tank.
Solution:
B. Razavi: RF Microelectronics, 2nd Edition
Too large cannot be achieved
Spring2014
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93
Band Selection
• The BPF before the LNA is used as a band select filter– Specification is relaxed compared to the case where it is used as a
channel select filter– It has a constant frequency response and does not need to be
tunable
• The BPF is implemented using:– SAW technology for frequencies below 10 GHZ– MEMS technology for mm-wave frequencies
B. Razavi: RF Microelectronics, 2nd EditionDesired Band
f
Band Select filter
Spring2014
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94
Band Selection
• TX-RX feedthrough can limit the performance of the receiver• Typically the received signal is in the order of -70 dBm• Feedthrough may saturate the BB blocks because of the high gain• Is an issue in full duplex transceivers• Design Targets:
– LNA must tolerate this high input level– A BPF is usually included at the output of LNA provide additional filtering
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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95
Band Selection
• Band select filters are usually implemented in a duplexer• Single antenna transceivers use a duplexer to isolate
between TX and RX• Duplexers are two BPF, one for RX and the other for TX
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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96
Channel Selection Remarks
• Channel selection cannot be done before the LNA because:– It is hard to find a BPF with large quality factor, and achieving a very small
loss– Having a tunable BPF with high quality factor is hard to obtained
• Usually, there are two steps to select a channel:
– Band selection: In which the entire band is selected. This step usually comes before the LNA.
– Channel selection: In which the desired channel is selected. This step is usually done after the first mixer.
Spring2014
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Superheterodyne Receiver
Spring2014
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97
Example: AM Radio
• AM radio band: 530 to 1610 KHz• BW/2 = (1610-530)/2=1080/2=540, in band• IF has to be lower. Commonly: 455kHz• Image can be in AM band• If LO is on low side, LO tuning range is:
– (530 to 1610) – 455 = (75 to 1155)– LO lowest to highest is a factor of 15.4
• If LO is on high side, LO tuning range is:– (530 to 1610) + 455 = (985 to 2065)– LO lowest to highest is a factor of 2.01
Spring2014
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98
99
Typical Superheterodyne Digital Receiver
Prof. E Sanchez-Sinencio RF course slides
Advantage Disadvantages
Good selectivity High complexity
Good sensitivity High power consumption
Image problem
External components
Not suitable for multi-standard
Spring2014
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100
The Image Problem
• The image could be another user or standard• The image must be filtered out before going the mixer• Frequency planning is key
Prof. E Sanchez-Sinencio RF course slides
Spring2014
RF
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Image Rejection Calculation
SNRmin
fIF
IRrequired
fRFfLO
Pdesired
PImage
minSNRPPIR desiredimagerequired
)all in dB’s(
Spring2014
RF
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101
Mixer = Multiplying up/down conversion
• Frequency translation device• Ideal mixer:
• Doesn’t “mix”; it multiplies
A
B
AB
Spring2014
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102
Super-heterodyne Receiver
Spring2014
RF
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103
Selection of IF
• If IF is large, – better separation between RF and image– better image rejection– easier image rejection filter design– More stages of down conversion
• Other IF selection criteria– Select IF so that image freq is outside of RF
band– IF >= (RF BW)/2
• Sometime may not be possible, if (RF BW)/2 is within RF Band
Spring2014
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104
• For each channel assignment, there are two choices of LO freq that meets the requirement |RF–LO|=IF.
• Q: should LO > RF, or LO < RF??
Spring2014
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105
Image problem converting to IF
A1cos(wRFt)
A has desired signal at wIF
plus an interference at wIM
A2cos(wIMt)
B is at wLO
And:
wRF - wLO = wLO - wIM = wIF
Both converted to IF,Can’t be cleaned once corrupted
Spring2014
RF
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106
Image Problem
)()(cos2
)()(cos2
)cos())(cos()()()(
)cos()(
message is )();)(cos()(
tmtAB
tmtAB
ttmtABtBtAtC
tBtB
tmtmtAtA
LOx
LOx
LOx
LO
x
?
IFLOimagex
IFLORFx
if
OKif
Spring2014
RF
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tem
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ts
107
Problem of Image Signal
IF
RFimage LO
Spring2014
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108
Problem of Image Signal
• Solution: Image Rejection Filter
RFimage LO
Spring2014
RF
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109
110
The Image Problem
• Image Reject filter versus channel selection:
• Larger IF frequencies requires channel select filter with higher Q
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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tem
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111
Dual-IF Heterodyne Receiver
• Channel selection is done in two stages, hence relaxing the specification for each stage
• Secondary image problem– To avoid the problem, the second IF frequency is set to zero
• Is it possible to have a zero IF?Spring2014
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112
Down Conversion to IF
AM modulation:
FM/ Digital ..etc . modulations:
Spring2014
RF
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High Q Alternatives
• What is really needed is not really a filter.• A cancellation scheme to reject noise is
good enough
Spring2014
RF
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tem
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Cosine wave
113
High Q Alternatives
• What if we use a sine wave instead
Spring2014
RF
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114
Complex Signal Representation
Niknejad and Shana’a
Spring2014
RF
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115
Orthognality of I and Q
Niknejad and Shana’a
Spring2014
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116
Orthogonality
Spring2014
Des
ign
of R
F C
ircui
ts &
Sys
tem
s
Spring2014
RF
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117
118
Image Reject Receivers-I
– What is a shift by 90o?
– The 90o phase shift is also called Hilbert transform
ffc-fc
𝐴2
𝐴2
Re
Im
f
fc
-fc
Re
Im
− 𝑗𝐴2
𝑗𝐴2
𝑋 90(𝜔)=𝑋 (𝜔) [− 𝑗 𝑠𝑔𝑛(𝜔) ]
Spring2014
RF
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119
Hilbert transform:
• A 90o phase shift results in:– Rotating positive frequency components CW by 90o
– Rotating negative frequency components CCW by 90o
• Multiplication by +j rotates all frequency components CCW by 90o.
• Multiplication by -j rotates all frequency components CW by 90o.
• Note that for DC frequencies these transformations do not have any meaning
Spring2014
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120
Hilbert transform
• Assume I(t) is shifted by 90o to produce Q(t). Find I(t)+jQ(t).
ffc-fc
Re{I}
Im{I}
f
fc
-fc
Re{Q}
Im{Q}
f
fc
-fc
Re{jQ}
Im{jQ} Im{I+jQ}
ffc-fc
Re{I+jQ}Spring2014
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121
Image Reject Receivers
• Idea: From the previous example it seems that one could remove the image with the help of quadrature components.
ffs-fs
Re{I}
Im{I}
-fi fi
f
Re{I}Im{I}{
-fIF fIF
fLO
f
Re{Q}Im{Q}
-fIF fIF
Spring2014
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122
Hartley Image Reject Architecture
• A Hilbert transform is used to cancel the image• I&Q (quadrature) signals are generated for image rejection.• The generation of the 90o could be achieved using RC phase shifter each providing 45o phase shift (narrow band solution)
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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123
Hartley Image Reject Architecture
• Still in the BB we must generate another I&Q for digital demodulation
• Drawbacks:– Mismatch between the two path will result in finite image rejection– The RC solution can be used for narrow-band architectures. Wideband
architecture will result in degraded performance for the image rejection (IRR)– Typical values for IRR is lower than 35 dB.
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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Implementing the Phase ShiftHartley Architecture with simple 90 deg phase shiftor
Spring2014
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124
Weaver
125
126
127
Spring2014
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128
IRRt
AAt
AAtx imLO
imLORFLO
RFLOA )sin(
2)sin(
2)(
)(cos2
)()(cos2
)()( tA
AtA
Atx imLOim
LORFLORF
LOB
)cos(2
)cos(2
)(
t
At
AAtx imLO
imRFLO
RFLOC
cos2
cos2
)()( t
AAt
AAtx RFLO
RFLORFLO
RFLOsig
cos2
cos2
)()( t
AAt
AAtx imLO
imLOimLO
imLOim
129
cos)(2)(
cos)(2)(.
22
22
2
2
LOLOLOLO
LOLOLOLO
RF
im
outsig
im
AAAA
AAAA
A
A
P
P
Input image power ratio
44
4
4
)cos1)((2
cos)(2)(
cos)(2)(
22
22
2
222
2
2
22
22
AA
AIRR
A
A
A
AA
AAAA
AAAAIRR
LO
LO
LO
LOLO
LOLOLOLO
LOLOLOLO
130
1
1
1
1222222
CRCCRR
CCRR
A
A
2
1
2
C
C
R
RC
CR
RC
CR
R
A
A
Gain Mismatch due to R, C errors
At w = 1/RC:
Spring2014
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131
132
Weaver or Hartley?
• Hilbert transform is obtained using another quadrature (complex) mixing stage
• Advantages compared to Hartley:– Better accuracy in generating the additional 90o phase shift– IRR is limited to 40 dB, which is higher than Hartley architecture
• Disadvantages:– Secondary image problem
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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133
Direct Conversion Receiver
• A single step down conversion is used. The output frequency is at DC
B. Razavi: RF Microelectronics, 2nd EditionAdvantages Disadvantages
No image problem LO leakage
Less complex / low power consumption
DC offset
Channel selection is done with a LPF Even order distortion
Effect of mixer spurs are reduced Flicker noise
IQ mismatch
Spring2014
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134
LO Leakage
– The LO signal can be leaked to the antenna by the capacitive coupling or substrate
– For singled ended Los, the LO leakage can reach -60 dBm– Differential LO architectures have lower LO leakage (better than -
100 dBm)
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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135
Direct Conversion Receiver
• DC Offset:– The leaked LO signal can go through the antenna, LNA and down
converted – Because of the LO signal and its feedthrough signal carry the same
frequency, a DC offset is produced (this phenomena is called LO self mixing).
– BB blocks usually have high again, hence the LO self mixing may saturate the receiver– HPF are not common because they require a very low cut-off frequency
(large components, slow settling)
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
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136
Even Order Distortion
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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137
Direct Conversion Receiver
• Flicker Noise:
• For 802.11g the channel bandwidth is 10MHz. With a noise corner frequency of 200kHz• For GSM, the channel bandwidth is 100 kHz and therefore a
large portion of noise appears due to flicker noise
B. Razavi: RF Microelectronics, 2nd Edition
Spring2014
RF
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138
Direct Conversion Receiver
• IQ mismatch:– mismatch in I and Q path affects SNR of received signals– Mismatch effects are more dominate at high frequencies. Reducing the
frequency at which the I and Q signal are generated enhances the SNR– Digital calibration is used to correct these mismatches
Amplitude mismatch:
Phase mismatch:
Spring2014
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139
Low-IF Receiver
• Has all the advantages of direct conversion receivers• More difficult image rejection requirements• Minimum IF frequency is channel bandwidth• DC offset is outside the signal bandwidth
Complex Filter
LargeRequires matchingPower hungry
Spring2014
RF
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tem
s an
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ts
ADC
ADC
PGA
PGA
LNA
RFPLL
DIG
ITA
LF
ILT
ER
100 kHz
I
Q
sin cos
RFSAW
sin cos
270 kS/s
925-960MHz
925.1 - 960.1MHz
Low IF receiver
-Quadrature RF down conversion required
-Require higher performance ADC-Additional mixer
-Slower RF PLL settling-Even order distortion still
problem-Low freq IF filters require large
chip area
+Eliminate IF SAW, IF PLL and image filtering
+Integration
+Relaxes image rejection requirements
+Avoids DC problems, relaxes 1/f noise problem
Spring2014
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140
Low-IF Down Conversion
LOω
Complex BPF
Mirror signal, needs removal
Spring2014
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141
Mirror Signal Suppression
ComplexBandpass
Filter
I Q I Q
LO1 LO2
Spring2014
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142
Complex Mixing- Real LO
Spring2014
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Complex Mixing-Complex LO
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Complex Mixing
Spring2014
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145
146
Bluetooth Receiver
• Has all the advantages of direct conversion receivers• More difficult image rejection requirements• Minimum IF frequency is channel bandwidth• DC offset is outside the signal bandwidth
Spring2014
RF
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tem
s an
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Direct Conversion Receiver
Little image problemNo IQ filter@ IF
PGA
PGA
LNA
RFSAW ADC
ADC
DIG
ITA
LF
ILT
ER
I
Q
RFPLL
sin cos
270 kS/s
925-960MHz
925 - 960MHz
Spring2014
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tem
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147
Direct Conversion Receiver
LO is at same frequency as RF1/f noise here can end up in channel
Self mixing cause DC problem
+Eliminate IF SAW, IF PLL and image filtering+ Integration+ easier image problem
-Quadrature RF down conversion required
-DC problem -Typically requires offset or
2x LO to avoid coupling
Spring2014
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148
DC Offset (Self-mixing)
AD w c
aLO(t)=ALOcos( w c+q)
0
w c
)(, tx LOoffset
capacitive couplingsubstrate couplingbondwire coupling
Saturates the following stages
AD w c 0
w c
)(, tx RFoffset
Spring2014
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149
DC Offset (Self-mixing)
θωω
θωθωω
ω
tAA
tAtAA
tataAtx
cLOcrosstalk
cLOcLOcrosstalk
LOLOcrosstalkLOoffset
2cos1)(
coscos)(
)()()()(
221
,
φ)(ω2cos1)ω(
φ)(ωcos)ω(
)()()ω()(
2interferer2
1
22interferer
interfererinterfererinterferer,
tmtAA
tmtAA
tataAtx
ccrosstalk
ccrosstalk
crosstalkoffset
level
DC Offset
+
-
t
φ)(ω2cos1)ω(
φ)(ωcos)ω(
)()()ω()(
2interferer2
1
22interferer
interfererinterfererinterferer,
tmtAA
tmtAA
tataAtx
ccrosstalk
ccrosstalk
crosstalkoffset Spring2014
RF
Sys
tem
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ircui
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150
DC Offset Cancellation
• Capacitive Coupling– Requires a large capacitor
• Negative Feedback– Nonlinear -A
Spring2014
RF
Sys
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151
1/f noise effect
• CMOS transistors has significant 1/f noise at low to DC frequency
• Significantly noise performance of direct conversion receivers
Receive signal1/f noise
f
Spring2014
RF
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tem
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152
Even-Order Distortion
c
0c
0
Direct feed through
Direct feed through
Interferers
y(t) = a1 x(t) + a2 x2(t)
Dw
Dw
a2 A1A2 cos(Dw)
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
153
Mirror Signal
• Upper sideband and lower sideband are identical
RF
LO
0
0
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
154
Mirror Signal • Upper sideband and lower sideband are not
identical
RF
LO
0
0
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
155
Mirror Signal Suppression
• Quadrature Down Conversion
AD
090
AD
a(t)
ui(t)
uq(t)
vi(t)
vq(t)
I
Q Spring2014
RF
Sys
tem
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d C
ircui
ts
156
Quadrature Conversion
)(
)(tan)(
))(tan()(
)(
))(sin()(
))(cos()(
)sin()()(
)cos()()(
))(cos()(
1
21
21
tv
tvtm
tmtv
tv
tmtv
tmtv
ttatu
ttatu
tmtta
i
q
i
q
q
i
LOq
LOi
RF
Spring2014
RF
Sys
tem
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ircui
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157
Quadrature Down Conversion
RF
LO
0
0
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
158
I/Q Mismatch
090
I
Q
Phase & Gain Error
Phase & Gain Error
Phase & Gain Error
)(, tx ILO
)(, tx QLO
)(, tx IBB
)(, tx QBB
a(t)
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
159
I/Q Mismatch due to LO errors
2)(sin
21
2)(
2)(cos
21
2)(
2sin
21)(
2cos
21)(
)(cos)(
,
,
,
,
tmA
tx
tmA
tx
ttx
ttx
tmtAta
QBB
IBB
cQLO
cILO
c
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
160
2
2ˆ
ˆ
2222
1
)(
)()(ˆ Find :Exercise
unbiased. is )(ˆ Hence,
)())(ˆ( Clearly,
0)(,))((,))(( and
0)( ,0)( Suppose
)2/)(cos()2/1(
)2/)(sin()2/1(tan)(ˆ
tm
tmtmEσ
tm
tmtmE
EσEσE
EE
tm
tmtm
def
m
m
ε
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
161
Use of I/Q down conversion recovers the nonsymmetrical receive signal spectrumBut port isolation becomes more challengingSelfmixing and even order distortion may affect both channels and affect each other, causing additional I/Q mismatch
Spring2014
RF
Sys
tem
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ircui
ts
162
090
a(t)
A/D
A/D
Base Band
DSP
Phase and gain mismatchcompensation
DC and 1/fcancellation
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
163
Summary of Direct Conversion Receiver
• No need for imager reject filter• Suitable for monolithic integration with baseband • DC offsets due to crosstalk of input ports of mixer• Even order IM direct feed through to baseband• Quadrature down conversion suppresses mirror• I/Q mismatch due to mismatches in parasitics• Low power consumption attributes to less hardware
Spring2014
RF
Sys
tem
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ircui
ts
164
Outline
• Friis Formula• Merits of LNAs• Common Gate LNA• Common Source LNA• Highly Linear LNA• Wideband LNAs• Mixers
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Cascaded Noise Figure
• In a line-up of receiver stages, use Friis equation
• Gi is the power gain• Says that the noise factor ‘F’ is more
influenced by earlier stages Spring2014
RF
Sys
tem
s an
d C
ircui
ts
LNA Merits
• Gain• Low Noise (NF)• High Linearity (IIP3)• Low Reflection (S11)• High reverse isolation (S12)• High Stability (K)
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Gate LNA
• Input impedance is resistive (except for parasitics)
• Offers good impedance match even at low frequencies
R
vout
Cgs
Cgd
Vin
ZinRs
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Gate LNA
• Inductor @input tunes out transistor and board parasitics.
• Channel resistance offers good reverse isolation
R
vout
Cgs
Cgd
Vin
RsCpad
+ Csb L
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Gate LNA
• At matching condition, Zin = 1/gm
R
vout
Cgs
Cgd
Vin
RsCpad
+ Csb L
sms
m
RgkTR
gkTF
1
4
/41
1FSpring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Gate LNA: Lowering Power II
• Narrowband impedance transformer (L Section) allows the LNA to have Zin>50W.
• Transformer amplifies input signal by:
R
vout
Cgs
Cgd
Vin
RsCpad
+ Csb L
50 >501
o
in
Z
ZSpring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Gate LNA: Lowering Power II
• For same IIP3, Veff has to increase by
• Current is reduced by the
same factor • Bias current is given by:
R
vout
Cgs
Cgd
Vin
RsCpad
+ Csb L
50 >50
o
in
Z
Z
oin
effD
ZZ
VI
2
1
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Source Amplifier
Input impedance is purely capacitive
Resistive part appears at high frequency
No input matching is possible
R
vin
vout
Cgs
Zin= 1/jCgs
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Source Amplifier
• Rg is set to 50 W => Input Matching
• Miller Effect due to Cgd
=> Limited Bandwidth
R
vin
vout
Cgs
Rg
Cgd
p
sin j
RZ
1
)(
1
gdMgssp CACR
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Source Amplifier
• Cascode reduces Miller Effect
• Resistive Load limits linearity
R
vin
vout
Cgs
Cgd
RgSpring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Source Amplifier
• Parallel Resonance at output boasts narrow band gain without impacting linearity
• Rg produces a lot of Noise NF>3 dB
vin
Cgs
Rg
QoL
vout
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Source Amplifier
Series resonance at input creates a resistive term
Iin= jw CgsVgs
Vin=Vgs+jwLs(Iin+gmVgs)
ssgs
in LLjCj
Z
1
QoL
vin
vout
Cgs
L
LsSeries Resonance
gmVgs
Iin
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Source Amplifier
• Series resonance at input creates a resistive term
• @ RF, input is still capacitive because Ls is very small to give 50W with high wT
QoL
vin
vout
Cgs
L
LsSeries Resonance
sgs
ms
gsin L
C
gLj
CjZ
1
gs
mT C
g
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Source Amplifier
Gate inductance offers one more degree of freedom to allow matching and series resonance at the same time
Valid for
QoL
vin
vout
Cgs
L
LsSeries Resonance
Lg s
gs
mgs
gsin L
C
gLLj
CjZ
1
gss
oCL
1 Spring
2014
RF
Sys
tem
s an
d C
ircui
ts
Parasitics
Ali Niknejad ECE142
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Design Procedure for Common Source LNAs
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Common Source Amplifier
Assume an equivalent resistive load Rd
@ resonance vin
vout
Cgs
Rd = QoL
LsSeries Resonance
Lg
sgs
mgs
gsin L
C
gLLj
CjZ
1
OhmLC
gZ s
gs
min 50 Spring
2014
RF
Sys
tem
s an
d C
ircui
ts
Common Source Amplifier
Noise Figure (F) is given by
vin
vout
Cgs
Rd = QoL
LsSeries Resonance
Lg
OhmLC
gZ s
gs
min 50
Decreases with wT
Use samll Ls
Source Coils TransistorSpring2014
RF
Sys
tem
s an
d C
ircui
ts
Optimization of CS LNA
Assume
@ Input matching condition
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Optimization of CS LNA
wT Increases
Lg Noise dominates
Higher power
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Another Way to Look at It
• If Q is input quality factor
vinCgs
Ls
Lg
vinCgs
Ls
TLs
+
-Vgs
QV
V
in
gs
sTsmo
T
LRgQ
1
smRgQF
4
11
2
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Another Way to Look at It
• The input is amplified by Q before it reaches the transistor
• This reduces linearity vinCgs
Ls
Lg
vinCgs
Ls
TLs
+
-Vgs
22
333
Q
IIP
in
gs
IIPIIP FETFET
LNA
V
V
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Other Losses: Inductor Losses
• Typically Lg losses dominate• Adds in series to source noise • Independent of FET gain
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Other Losses: Gate Resistance
• Gate Resistance creates additional noise (uncorrelated with channel noise)
• Use inter-digitated layout to reduce gate electrode resistance
rg
g
mFETn
rg
kTv
42
,
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Other Losses: Gate Induced Noise
• Due to inversion layer resistance
• Partly correlated with conventional thermal noise
• Modeled as a resistance in series with gate
GateSource Drain
oxeffinv CWV
Lr
5
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Other Losses: Gate Induced Noise
• The effective Q is lowered by losses
• Higher Q is achieved through lower Cgs
• Smaller Cgs raises rinv and also gate resistance
• There is an optimum W at each current
vin
Cgs
Ls
Lg
+
-Vgs
rinv
W
FQ increases
Fopt
Other losses dominate
FETDominates
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Other Losses: Substrate Coupling
• BSIM3V3 models do NOT capture Cgb• Gate to bulk capacitance is an additional path for
noise Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Other Losses: Substrate Coupling
• Hole distribution in the depletion layer are modulated by gate voltage
• Same effect on electrons in the inversion layer which reflects back on depletion region Spring
2014
RF
Sys
tem
s an
d C
ircui
ts
Wideband CS LNA
• Uses an LC ladder filter to widen BW
• Uses a large number of inductors
• Excellent noise performance
`
M1
M2
+r
Rs
Vs
Vo
Vbias
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Resistive Feedback
• Feedback widens BW and lowers Zin
• Power consumption is very high
• Noise Cancellation can be employed
+r
Rs
Vs
+r
M1 M2
M3
X
Y
VsRs
Vout Spring2014
RF
Sys
tem
s an
d C
ircui
ts
Capacitive Cross Coupling Technique
,1
2
12
11 mmin gg
R
+ IN
M1 M2C1 C2
1
21
2
4
4
mn
sns
g
KTv
KTRv
+ r
vn1
vns
in_diffout
Rs Rs
M1 M2
+r
•Differential input impedance:
•Two voltage noise sources: vns & vn1 in each
half circuit
Spring2014
RF
Sys
tem
s an
d C
ircui
ts
• The output differential noise current square due to each noise source is given by:
• Then:
• Using the input power matchingcondition:
+ r
vn1
vns
in_diffout
Rs Rs
M1 M2
+r
2
22
4
1
s
nsns_diffout R
vi
2
212
1 16
1
s
n_diffoutn R
vi
smns_diffout
_diffoutn
Rgi
iF
12
21
4
111
2
11F
Capacitive Cross-Coupling Technique
Spring2014
RF
Sys
tem
s an
d C
ircui
ts