FEATURES
Integrated RF and Baseband AGC Amplifiers
Quadrature Phase Accuracy 1ⴗ Typ
I/Q Amplitude Balance 0.3 dB Typ
Third Order Intercept (IIP3) +11.5 dBm @ Min Gain
Noise Figure 11 dB @ Max Gain
AGC Range 69.5 dB
Baseband Level Control Circuit
Low LO Drive –8 dBm
ADC Compatible I/Q Outputs
Single Supply 2.7 V–5.5 V
Power-Down Mode
Package 28-Lead TSSOP
APPLICATIONS
Cellular Basestations
Radio Links
Wireless Local Loop
IF Broadband Demodulator
RF Instrumentation
Satellite Modems
AD8347
FUNCTIONAL BLOCK DIAGRAM
LOIN
VPS1
IOPN
IOPP
VCMO
IAIN
COM3
IMXO
COM2
RFIN
RFIP
VPS2
IOFS
VREF
1
2
3
4
5
6
7
8
9
10
11
12
13
14
AD8347
SPLITTER
SPLITTER
BIAS
PHASE
PHASE
DET
GAIN
CONTROL
LOIP
28
COM1
27
26
QOPN
25
QOPP
24
QAIN
23
COM3
22
QMXO
21
VPS3
20
VDT1
19
VAGC
18
VDT2
17
VGIN
16
QOFS
15
ENBL
*
GENERAL DESCRIPTION
The AD8347 is a broadband Direct Quadrature Demodulator
with RF and baseband Automatic Gain Control (AGC) amplifiers.
It is suitable for use in many communications receivers,
performing Quadrature demodulation directly to baseband
frequencies. The input frequency range is 800 MHz to 2.7 GHz.
The outputs can be connected directly to popular A-to-D converters
such as the AD9201 and AD9283.
The RF input signal goes through two stages of variable gain
amplifiers prior to two Gilbert-cell Mixers. The LO quadrature
phase splitter employs polyphase filters to achieve high quadrature accuracy and amplitude balance over the entire operating
frequency range. Separate I & Q channel variable-gain amplifiers
follow the baseband outputs of the mixers. The RF and baseband
*U.S. Patents Issued and Pending
amplifiers together provide 69.5 dB of gain control. A precision
control circuit sets the Linear-in-dB RF gain response to the gain
control voltage.
Baseband level detectors are included for use in an AGC loop to
maintain the output level. The demodulator dc offsets are
minimized by an internal loop, whose time constant is controlled
by external capacitor values. The offset control can also be
overridden by forcing an external voltage at the offset nulling pins.
The baseband variable gain amplifier outputs are brought off-chip
for filtering before final amplification. By inserting a channel
selection filter before each output amplifier high-level out-ofchannel interferers can be eliminated. Additional internal circuitry
also allows the user to set the dc common-mode level at the
baseband outputs.
REV. 0
Information furnished by Analog Devices is believed to be accurate and
reliable. However, no responsibility is assumed by Analog Devices for its
use, nor for any infringements of patents or other rights of third parties that
may result from its use. No license is granted by implication or otherwise
under any patent or patent rights of Analog Devices.
Maximum Junction Temperature . . . . . . . . . . . . . . . . 150°C
Operating Temperature Range . . . . . . . . . . . –40°C to +85°C
Storage Temperature Range . . . . . . . . . . . . –65°C to +150°C
Lead Temperature (Soldering 60 sec) . . . . . . . . . . . . . 300°C
*Stresses above those listed under Absolute Maximum Ratings may cause perma-
nent damage to the device. This is a stress rating only; functional operation of the
device at these or any other conditions above those indicated in the operational
section of this specification is not implied. Exposure to absolute maximum rating
conditions for extended periods may affect device reliability.
AD8347ARU–40°C to +85°CTube (28-Lead TSSOP) ThinRU-28
AD8347ARU-REEL13" Tape and Reel
AD8347ARU-REEL77" Tape and Reel
AD8347-EVALEvaluation Board
PIN CONFIGURATION
1
LOIN
2
VPS1
3
IOPN
4
IOPP
5
VCMO
6
IAIN
COM3
IMXO
COM2
RFIN
RFIP
VPS2
IOFS
VREF
7
8
9
10
11
12
13
14
AD8347
TOP VIEW
(Not to Scale)
Shrink Small Outline Package
LOIP
28
COM1
27
26
QOPN
25
QOPP
24
QAIN
23
COM3
22
QMXO
21
VPS3
20
VDT1
19
VAGC
18
VDT2
17
VGIN
16
QOFS
15
ENBL
VPS3
DET 1
VREF
VREF
DET 2
VDT2QMXOQOPPQOFSVAGCVDT1QAIN
VREF
PHASE
SPLITTER
VREF
IAIN
2
VCMO
IOPPIOFSIOPN
PHASE
SPLITTER
1
VCMO
QOPN
ENBL
RFIN
RFIP
VGIN
VPS2IMXO
VPS1
AD8347
BIAS
CELL
GAIN
CONTROL
INTERFACE
Figure 1. Block Diagram
CAUTION
ESD (electrostatic discharge) sensitive device. Electrostatic charges as high as 4000 V readily
accumulate on the human body and test equipment and can discharge without detection. Although
the AD8347 features proprietary ESD protection circuitry, permanent damage may occur on
devices subjected to high-energy electrostatic discharges. Therefore, proper ESD precautions are
recommended to avoid performance degradation or loss of functionality.
VCMO
LOIN
LOIP
COM3
COM2
COM3
COM1
WARNING!
ESD SENSITIVE DEVICE
–4–
REV. 0
Page 5
AD8347
PIN FUNCTION DESCRIPTIONS
PinEquiv.
No.MnemonicCir.Description
1, 28LOIN, LOIPALO Input. For optimum performance, these inputs should be driven differentially. Typical input
drive level is equal to –8 dBm. To improve the match to a 50 Ω source, connect a 200 Ω shunt
resistor between LOIP and LOIN. A single-ended drive is also possible but this will slightly
increase LO leakage.
2VPS1Positive Supply for LO Section. This pin should be decoupled with 0.1 µF and 100 pF capacitors.
3, 4IOPN, IOPPB
5VCMOCBaseband Amplifier Common-Mode Voltage. The voltage applied to this pin sets the output
6IAINDI Channel Baseband Amplifier Input. This pin, which has a high input impedance, should be
7, 23COM3Ground for Biasing and Baseband Sections
8, 22IMXO, QMXOBI & Q Channel Baseband Mixer/VGA Outputs. These are low impedance outputs whose bias
9COM2RF Section Ground
10, 11RFIN, RFIPERF Input. RFIN must be ac-coupled to ground. The RF input signal should be ac-coupled into
12VPS2Positive Supply for RF Section. This pin should be decoupled with 0.1 µF and 100 pF capacitors.
13, 16IOFS, QOFSFI Channel and Q Channel Offset Nulling Inputs. To null the dc-offset on the I Channel and
14VREFGReference Voltage Output. This output voltage (1 V) is the main bias level for the device and
15ENBLHChip Enable Input. Active high.
17VGINCGain Control Input. The voltage on this pin controls the gain on the RF and baseband VGAs.
18, 20VDT2, VDT1DDetector Inputs. These pin are the inputs to the on-board detector. VDT2 and VDT1, which
19VAGCIAGC Output. This pin provides the output voltage from the on-board detector. In AGC mode,
21VPS3Positive Supply for Biasing and Baseband Sections. This pin should be decoupled with 0.1 µF
24QAINDQ Channel Baseband Amplifier Input. This pin, which has a high input impedance, should be
25, 26QOPP, QOPNBQ Channel Differential Baseband Output. Typical output swing is equal to 1 V p-p differential.
27COM1LO Section Ground
I Channel Differential Baseband Output. Typical output swing is equal to 760 mV p-p differential
in AGC mode
common-mode level of the baseband amplifiers. This pin can either be connected to VREF
(Pin 14) or to a reference voltage from another device (typically an ADC).
biased to VREF (approximately 1 V). If IAIN is connected directly to IMXO, biasing will be
provided by IMXO. If an ac-coupled filter is placed between IMXO and IAIN, this pin can be
biased from VREF through a 1 kΩ resistor. The gain from IAIN to the differential outputs
IOPN/IOPP is 30 dB.
levels are equal to VREF. IMXO and QMXO are typically connected to IAIN and QAIN
respectively, either directly or through filters. These outputs have a maximum current limit of
about 1.5 mA. This allows for a 600 mV p-p swing into a 200 Ω load. This corresponds to an
input level of –40 dBm @ max gain of 39.5 dB. At lower output levels, IMXO and QMXO, can
drive a lower load resistance, subject to the same current limit.
RFIP. For a broadband 50 Ω input impedance, connect a 200 Ω resistor from the signal side of
RFIP’s coupling capacitor to ground. Please note that RFIN and RFIP are not interchangeable
differential inputs. RFIN is the ground reference for the input system.
Q Channel Mixer Outputs (IMXO, QMXO), connect a 0.1 µF capacitor from these pins to
ground. Alternately, a forced voltage of approximately 1 V on these pins will disable the offset
compensation circuit.
can be used to externally bias the inputs and outputs of the baseband amplifiers.
The gain control is applied in parallel to all VGAs. The gain control voltage range is from 0.2 V
to 1.2 V and corresponds to a gain range from +39.5 dB to –30 dB. This is the gain to the output
of the baseband VGAs (i.e., QMXO and IMXO). There is an additional 30 dB of gain in the
baseband amplifiers. Note that the gain control function has a negative sense (i.e., increasing
control voltage decreases gain). In AGC mode, this pin is connected directly to VAGC.
have high input impedances, are normally connected to IMXO and QMXO respectively.
this pin is connected directly to VGIN.
and 100 pF capacitors.
biased to VREF (approximately 1 V). If QAIN is connected directly to QMXO, biasing will be
provided by QMXO. If an ac-coupled filter is placed between QMXO and QAIN, this pin can
be biased from VREF through a 1 kΩ resistor. The gain from QAIN to the differential outputs
QOPN/QOPP is 30 dB.
The common-mode level on these pins is programmed by the voltage on VCMO.
. The common mode level on these pins is programmed by the voltage on VCMO.
REV. 0
–5–
Page 6
AD8347
VPS3
VAGC
COM3
EQUIVALENT CIRCUITS
LOIN
LOIP
VPS1
COM1
IAIN
QAIN
VPS3
Circuit A
PHASE
SPLITTER
CONTINUES
RFIP
RFIN
VPS2
COM3
Circuit B
VPS3
IOPP, IOPN,
QOPP, QOPN,
IMXO, QMXO
VCMO
IOFS
QOFS
VPS3
CURRENT MIRROR
COM3
Circuit C
VPS3
CURRENT MIRROR
Circuit D
COM3
Circuit G
COM3
VPS3
VREF
COM2
Circuit E
VPS3
ENBL
COM3
Circuit H
Figure 2. Equivalent Circuits
COM3
Circuit F
Circuit I
–6–
REV. 0
Page 7
RF AMP AND DEMODULATOR
BASEBAND FREQUENCY – MHz
1
GAIN – dB
100
30
31
32
33
34
35
36
37
38
10
39
40
41
42
VS = 5V,
TA = +25ⴗC
VS = 2.7V, TA = –40ⴗC
VS = 2.7V, TA = +25ⴗC
VS = 5V, TA = –40ⴗC
VS = 2.7V, T
A
= +85ⴗC
VS = 5V, TA = +85ⴗC
Typical Performance Characteristics–
AD8347
45
40
35
30
25
20
15
10
–5
MIXER GAIN – dB
–10
–15
–20
–25
–30
–35
TA = –40ⴗC
TA = +85ⴗC
TA = +25ⴗC
5
0
TA = +25ⴗC
TA = +85ⴗC
0.2
0.30.4 0.5 0.60.7 0.80.9 1.01.1 1.2
V
– V
GIN
TPC 1. Gain and Linearity Error vs. V
= 1900 MHz, FBB = 1 MHz
F
LO
45
MIXER GAIN – dB
–10
–15
–20
–25
–30
–35
40
35
30
25
20
15
10
5
0
–5
0.2
TA = –40ⴗC
TA = +85ⴗC
TA = –40ⴗC
TA = +25ⴗC
TA = +85ⴗC
0.3 0.40.5 0.60.7 0.80.9 1.01.1 1.2
TA = +25ⴗC
V
– V
GIN
TPC 2. Gain and Linearity Error vs. V
F
= 1900 MHz, FBB = 1 MHz
LO
TA = –40ⴗC
, VS = 5 V,
GIN
, VS = 2.7 V,
GIN
14
12
10
8
6
4
2
0
–2
–4
–6
–8
–10
–12
14
12
10
8
6
4
2
0
–2
–4
–6
–8
–10
LINEARITY ERROR – dB
LINEARITY ERROR – dB
3.0
2.5
2.0
1.5
VS = 2.7V, TA = –40ⴗC
1.0
GAIN – dB
0.5
VS = 5V, TA = –40ⴗC
0
–0.5
–1.0
800
1000 1200 1400 1600 1800 2000 2200
TPC 4. Gain vs. FLO, V
–27
–28
VS = 2.7V, TA = +25ⴗC
–29
–30
–31
–32
GAIN – dB
–33
VS = 5V, TA = +85ⴗC
–34
–35
–36
–37
800
1000 1200 1400 1600 1800 2000 2200
TPC 5. Gain vs. FLO, V
VS = 2.7V, TA = +25ⴗC
VS = 5V,
T
RF FREQUENCY – MHz
VS = 5V,
T
VS = 5V, TA = –40ⴗC
RF FREQUENCY – MHz
= +25ⴗC
A
VS = 5V, TA = +85ⴗC
VS = 2.7V, TA = +85ⴗC
2400 2600
= 0.7 V, FBB = 1 MHz
GIN
= +25ⴗC
A
GIN
VS = 2.7V, TA = –40ⴗC
VS = 2.7V, TA = +85ⴗC
2400 2600
= 1.2 V, FBB = 1 MHz
REV. 0
40
39
VS = 2.7V, TA = –40ⴗC
38
37
36
VS = 2.7V, TA = +85ⴗC
35
GAIN – dB
34
33
32
31
30
800
1000 1200 1400 1600 1800 2000 2200
VS = 2.7V, TA = +25ⴗC
VS = 5V, TA = +85ⴗC
RF FREQUENCY – MHz
TPC 3. Gain vs. FLO, V
VS = 5V,
= +25ⴗC
T
A
VS = 5V, TA = –40ⴗC
2400 2600
= 0.2 V , FBB = 1 MHz
GIN
–7–
TPC 6. Gain vs. FBB, V
= 0.2 V, FLO = 1900 MHz
GIN
Page 8
AD8347
10
9
8
7
6
5
4
3
2
GAIN – dB
1
0
–1
–2
–3
–4
–5
1
VS = 2.7V, TA = +25ⴗC
VS = 5V, TA = –40ⴗC
VS = 5V, TA = +85ⴗC
VS = 2.7V, TA = –40ⴗC
BASEBAND FREQUENCY – MHz
TPC 7. Gain vs. FBB, V
–25
–26
–27
VS = 5V,
–28
= +25ⴗC
T
A
–29
–30
GAIN – dB
–31
–32
VS = 2.7V,
–33
TA = +85ⴗC
–34
–35
1
BASEBAND FREQUENCY – MHz
TPC 8. Gain vs. FBB, V
VS = 2.7V, TA = +85ⴗC
VS = 5V,
= +25ⴗC
T
A
10
= 0.7 V, FLO = 1900 MHz
GIN
VS = 2.7V,TA = –40ⴗC
VS = 2.7V,
= +25ⴗC
T
A
VS = 5V,
= –40ⴗC
T
A
VS = 5V,TA = +85ⴗC
10
= 1.2 V, FLO = 1900 MHz
GIN
100
100
15
VS = 2.7V,
14
= +85ⴗC
T
A
13
12
11
10
VS = 2.7V, TA = +25ⴗC
IIP3 – dBm
9
8
7
6
5
8002400 26001000 1200 1400 1600 1800 2000 2200
TPC 10. IIP3 vs. FLO, V
–10
–12
VS = 5V, TA = +25ⴗC
–14
–16
–18
–20
IIP3 – dBm
–22
–24
V
= 5V, TA = –40ⴗC
S
–26
–28
–30
8002400 26001000 1200 1400 1600 1800 2000 2200
TPC 11. IIP3 vs. FLO, V
VS = 5V, TA = +85ⴗC
VS = 5V, TA = +25ⴗC
VS = 2.7V, TA = –40ⴗC
VS = 5V, TA = –40ⴗC
RF FREQUENCY – MHz
VS = 2.7V,
T
A
VS = 2.7V, TA = –40ⴗC
VS = 5V, TA = +85ⴗC
RF FREQUENCY – MHz
= 1.2 V, FBB = 1 MHz
GIN
= +85ⴗC
= 0.2 V, FBB = 1 MHz,
GIN
VS = 2.7V,
T
= +25ⴗC
A
0
–5
–10
–15
–20
INPUT P1dB – dBm
–25
–30
–35
0.20
VS = 5V,
= –40ⴗC
T
A
VS = 2.7V, TA = –40ⴗC
0.30
VS = 2.7V, TA = +85ⴗC
= 5V,
V
S
= +85ⴗC
T
A
VS = 2.7V,
= +25ⴗC
T
A
VS = 5V,
= +25ⴗC
T
A
1.20
V
– V
GIN
1.101.000.900.800.700.600.500.40
TPC 9. Input 1 dB Compression Point (OP1 dB) vs. V
TPC 14. IIP2 vs. FLO, V
Tone1 = 5 MHz, –10 dBm, Baseband Tone2 = 6 MHz,
–10 dBm, Temperature = 25ⴗC, VS = 5 V
13.0
12.5
12.0
11.5
11.0
NOISE FIGURE – dB
10.5
REV. 0
10.0
800
1000 1200 1400 1600 1800 2000 2200 2400 2600
TPC 15. Noise Figure vs. LO Frequency (FLO),
Temperature = 25
RF FREQUENCY – MHz
= 1.2 V, Baseband
GIN
VS = 5V
V
= 2.7V
S
LO FREQUENCY – MHz
ⴗ
C, V
= 0.2 V, FBB = 1 MHz
GIN
–9–
2.5
2.0
1.5
1.0
0.5
0
–0.5
–1.0
LO FREQUENCY = 800MHz
–1.5
–2.0
QUADRATURE PHASE ERROR – Degrees
–2.5
–20
–18 –16 –14 –12 –10 –8–6–4
LO FREQUENCY = 2700MHz
LO FREQUENCY = 1900MHz
–20
LO INPUT LEVEL – dBm
TPC 17a. Quadrature Error vs. LO Power Level,
ⴗ
C,
V
Temperature = 25
14.0
13.5
13.0
12.5
12.0
11.5
11.0
NOISE FIGURE – dB
10.5
10.0
9.5
9.0
–20
–18 –16 –14 –12 –10 –8–6–4
2700MHz
1900MHz
LO INPUT LEVEL – dBm
= 0.2 V, VS = 5 V
GIN
800MHz
–20
TPC 17b. Noise Figure vs. LO Input Level,
Temperature = 25
ⴗ
C, V
= 0.2 V, VS = 5 V
GIN
Page 10
AD8347
BASEBAND OUTPUT AMPLIFIERS
34
TA = –40ⴗC, V
32
30
28
TA = +85ⴗC, VS = 2.7V
26
24
GAIN – dB
22
20
18
16
110010
= 5V
S
TA = +25ⴗC, VS = 5V
BASEBAND FREQUENCY – MHz
TPC 18. Gain vs. FBB, V
5
TA = –40ⴗC, VS = 5V
0
–5
–10
OP1 – dBV rms
–15
–20
–25
110010
TA = –40ⴗC, VS = 2.7V
TA = +25ⴗC, VS = 2.7V
TA = +85ⴗC, VS = 2.7V
BASEBAND FREQUENCY – MHz
TPC 19. OP1 vs. FBB, V
TA = –40ⴗC, VS = 2.7V
TA = +25ⴗC, VS = 2.7V
TA = +85ⴗC, VS = 5V
= 1 V
VCMO
TA = +85ⴗC, VS = 5V
TA = +25ⴗC,
= 5V
V
S
= 1 V
VCMO
20
15
10
5
0
–5
–10
–15
–20
–25
BASEBAND AMPLIFIER OUTPUT IP3 – dBV rms
–30
–2
COMMON-MODE OFFSET – mV
–4
–6
VS = 5V, TA = –40ⴗC
VS = 2.7V, TA = +25ⴗC
VS = 2.7V,
T
1
= +85ⴗC
A
VS = 2.7V, TA = –40ⴗC
BASEBAND FREQUENCY – MHz
TPC 20. OIP3 vs. FBB, V
8
VS = 2.7V, MEAN +
6
4
2
0
VS = 2.7V, MEAN –
0.53.52.0
VS = 2.7V, MEAN
VS = 5V, MEAN
1.01.52.53.0
V
VCMO
VS = 5V, TA = 25ⴗC
10
VCMO
VS = 5V, MEAN –
– V
VS = 5V,
T
= 1 V
= +85ⴗC
A
VS = 5V,
MEAN +
100
TPC 21. Common-Mode Output Offset Voltage vs. V
ⴗ
Temperature = 25
C ( = 1 Standard Deviation)
VCMO
,
–10–
REV. 0
Page 11
BASEBAND FREQUENCY – MHz
I TO Q AMPLITUDE MISMATCH – dB
0
–0.2
–0.8
–0.4
–0.6
0
0.2
5 10152025303540
0.4
–1.0
0.6
0.8
1.0
TA = +25ⴗC
TA = –40ⴗC
TA = +85ⴗC
RF AMP/DEMOD AND BASEBAND OUTPUT AMPLIFIERS
AD8347
75
65
55
VS = 2.7V,
= +85ⴗC
T
45
A
35
25
VOLTAGE GAIN – dB
15
5
–5
0.20.80.5
0.3 0.40.6 0.7
VS = 5V, TA = +85ⴗC
VS = 2.7V, TA = –40ⴗC
= 5V, TA = –40ⴗC
V
S
V
= 2.7V, TA = +25ⴗC
S
V
= 5V, TA = +25ⴗC
S
V
GIN
TPC 22. Voltage Gain vs. V
= 1 MHz
F
BB
2.5
2.0
1.5
1.0
0.5
0
–0.5
–1.0
–1.5
QUADRATURE PHASE ERROR – Degrees
–2.0
–2.5
800
VS = 5V, TA = +25ⴗC
VS = 5V, TA = +85ⴗC
1000 1200 1400 1600 1800 2000 2200
RF FREQUENCY – MHz
– V
0.9 1.01.1 1.2
, FLO = 1900 MHz,
VGIN
VS = 5V, TA = –40ⴗC
2400 2600
TPC 25. I/Q Amplitude Imbalance vs. FBB,
ⴗ
Temperature = 25
0
C, VS = 5 V
–2
–4
–6
–8
RETURN LOSS – dBm
–10
–12
RF WITH TERMINATION
RF WITHOUT TERMINATION
1000 1200 1400 1600 1800 2000 2200
800
RF FREQUENCY – MHz
2400 2600
TPC 23. Quadrature Phase Error vs. FLO, V
V
= 5 V
S
2.5
2.0
1.5
1.0
0.5
QUADRATURE PHASE ERROR – Degrees
–0.5
–1.0
–1.5
–2.0
–2.5
0
0
5 10152025303540
TA = +85ⴗC
TA = –40ⴗC
BASEBAND FREQUENCY – MHz
TPC 24. Quadrature Phase Error vs. FBB, V
V
= 5 V
S
REV. 0
TA = +25ⴗC
VGIN
VGIN
= 0.7 V,
= 0.7 V,
TPC 26. Return Loss of RFIP vs. FRF, V
2.7GHz
2.7GHz
WITH TERMINATION
800MHz
WITHOUT TERMINATION
TPC 27. S11 of RFIN vs. FRF, V
–11–
VGIN
800MHz
= 0.7 V, VS = 5 V
VGIN
= 0.7 V, VS = 5 V
Page 12
AD8347
0
–2
–4
–6
–8
RETURN LOSS – dBm
–10
–12
–14
800
TPC 28. Return Loss of LOIP vs. FLO, V
LO PORT WITHOUT TERMINATION
LO PORT WITH TERMINATION
1000 1200 1400 1600 1800 2000 2200
RF FREQUENCY – MHz
WITH TERMINATION
800MHz
2.7GHz
WITHOUT TERMINATION
2.7GHz
800MHz
2400 2600
= 0.7 V, VP = 5 V
VGIN
30
25
20
15
10
5
MIXER OUTPUT VOLTAGE – mV p-p
0
–70
TA = +85ⴗC
TA = –40ⴗC
TA = +25ⴗC
TA = +85ⴗC
TA = +25ⴗC
TA = –40ⴗC
–60–50–40–30–20–10010
RF INPUT POWER – dBm
1.20
1.00
0.80
0.60
0.40
0.20
0
TPC 30. AGC Voltage and Mixer Output Level vs. RF Input
Power, F
= 1900 MHz, F
LO
85
= 1 MHz, VS = 5 V
BB
80
75
70
VP = 5.5V
65
60
SUPPLY CURRENT – mA
55
50
45
–40
VP = 2.7V
–30 –20 –100 102030
VP = 5V
VP = 3V
TEMPERATURE – ⴗC
40 50
60 70 80
AGC VOLTAG E – V
TPC 29. S11 of LOIN vs. FLO, V
= 0.7 V, VS = 5 V
VGIN
TPC 31. Supply Current vs. Temperature, V
= 1 V
V
VCMO
VGIN
= 0.7 V,
–12–
REV. 0
Page 13
VPS3
VPS2IMXO
VPS1
VREF
IAIN
AD8347
IOPPIOFSIOPN
AD8347
ENBL
RFIN
RFIP
VGIN
BIAS
CELL
GAIN
CONTROL
INTERFACE
DET 1
VREF
DET 2
VDT2QMXOQOPPQOFSVAGCVDT1QAIN
Figure 3. Block Diagram
CIRCUIT DESCRIPTION
OVERVIEW
The AD8347 is a direct I/Q demodulator usable in digital
wireless communication systems including Cellular, PCS, and
Digital Video receivers. An RF signal in the frequency range of
800 MHz–2700 MHz is directly downconverted to the I & Q
components at baseband using a Local Oscillator (LO) signal at
the same frequency as the RF signal.
The RF input signal goes through two stages of variable gain
amplifiers before splitting up to reach two Gilbert-cell Mixers.
The mixers are driven by a pair of Local Oscillator (LO)
signals which are in quadrature (90 degrees of phase difference).
The outputs of the mixers are applied to baseband I & Q channel
variable-gain amplifiers. The outputs from these baseband
variable
filtering.
fixed-gain
outputs from the external filters
A-to-D Converters.
gain amplifiers are brought out to pins for external
The filter outputs are then applied to a pair of on-chip,
baseband amplifiers. These amplifiers gain up the
to a level compatible with most
A sum-of-squares detector is available for
use in an Automatic Gain Control (AGC) loop to set the output
level. The RF and baseband amplifiers provide approximately
69.5 dB of gain control range. Additional on-chip circuits allow
the setting of the dc level at the I & Q channel baseband outputs, as well as nulling the dc offset at each channel.
RF Variable Gain Amplifiers (VGA)
These amplifiers use the patented X-AMP approach with NPNdifferential pairs separated by sections of resistive attenuators.
The gain control is achieved through a gaussian interpolator
where the control voltage sets the tail currents to be supplied to
the different differential pairs according to the gain desired. In
the first amplifier, the combined output currents from the transconductance cells go through a cascode stage to resistive loads
with inductive peaking. In the second amplifier the differential
currents are split and fed to the two Gilbert-cell mixers through
separate cascode stages.
Mixers
Two double balanced Gilbert-cell mixers, one for each channel,
perform the In-phase (I) and Quadrature (Q) down conversion.
Each mixer has four cross-connected transistor pairs which are
X-AMP is a registered trademark of Analog Devices, Inc.
REV. 0
–13–
VREF
VCMO
LOIN
LOIP
COM3
COM2
COM3
COM1
PHASE
SPLITTER
VREF
2
VCMO
PHASE
SPLITTER
1
VCMO
QOPN
terminated in resistive loads and feed the differential baseband
variable gain amplifiers for each channel. The bases of the mixer
transistors are driven by the quadrature LO signals.
Baseband Variable Gain Amplifiers
The baseband VGA’s also use the X-AMP approach with NPNdifferential pairs separated by sections of resistive attenuators.
The same interpolator controlling the RF amplifiers controls the
tail currents of the differential pairs. The outputs of these amplifiers are provided off chip for external filtering. Automatic offset
nulling minimizes the dc offsets at both I & Q channels. The
common-mode output voltage is set to be the same as the reference
voltage (1.0 V) generated in the Bias section, also made available
at the VREF pin.
Output Amplifiers
The output amplifiers gain up the signal coming back from each
of the external filters to a level compatible with most high speed
A-to-D converters. These amplifiers are based on an active-feedback
design to achieve the high gain bandwidth and low distortion.
LO and Phase-Splitters
The incoming LO signal is applied to a polyphase phase-splitter
to generate the LO signals for the I channel and Q channel
mixers. The polyphase phase-splitters are RC networks connected in a cyclical manner to achieve gain balance and phase
quadrature. The wide operating frequency range of these phasesplitters is achieved by cascading multiple sections of these
networks with staggered RC constants. Each branch goes through
a buffer to make up for the loss and high frequency roll-off. The
output from the buffers then go into another polyphase phasesplitter to enhance the accuracy of phase quadrature. Each LO
signal gets buffered again to drive the mixers.
Output Level Detector
Two signals proportional to the square of each output channel
are summed together and compared to a built-in threshold to
create an AGC voltage (VAGC). The inputs to this rms detector
are referenced to VREF.
Bias
An accurate reference circuit generates the reference currents
used by the different sections. The reference circuit is controlled
by an external power-up (ENBL) logic signal which, when set
low, puts the whole chip into a sleep mode typically requiring
Page 14
AD8347
less than
of 1.0 V,
baseband circuits, is made available for external use.
400 µA of supply current. The reference voltage (VREF)
which serves as the common-mode reference for the
RF Input and Matching
The RF input signal should be ac-coupled into the RFIP pin and
RFIN should be ac-coupled to ground. To improve broadband
matching to a 50 Ω source, a 200 Ω resistor may be connected
OPERATING THE AD8347
Basic Connections
Figure 4 shows the basic connections for operating the AD8347.
The device is powered through three power supply pins: VPS1,
VPS2, and VPS3. These pins supply current to different parts of
the overall circuit. VPS1 and VPS2 power the Local Oscillator (LO)
and RF sections, respectively, while VPS3 powers the baseband
amplifiers. While all of these pins should be connected to the same
supply voltage, each pin should be separately decoupled
using two
capacitors. 100 pF and 0.1 µF are recommended (values close
to these may also be used).
A supply voltage in the range 2.7 V to 5.5 V should be used. The
quiescent current is 64 mA when operating from a 5 V supply.
By pulling the ENBL pin low, the device goes into its power- down
mode. The power-down current is 400 µA when operating on a
5 V supply and 80 µA on a 2.7 V supply.
Like the supply pins, the individual sections of the circuit are
separately grounded. COM1, COM2, and COM3 provide ground
for the LO, RF, and baseband sections respectively. All of these
from the signal side of RFIP’s coupling capacitor to ground.
LO Drive Interface
For optimum performance the LO inputs, LOIN and LOIP,
should be driven differentially. M/A-COM balun, ETC1-1-13
is recommended. Unless an (ac-coupled) transformer is being
used to generate the differential LO, the inputs must be ac-coupled
as shown. To improve broadband matching to a 50 Ω source, a
200 Ω shunt resistor may be connected between LOIP and LOIN.
An LO drive level of –8 dBm is recommended. TPC 17a shows
the relationship between LO drive level, LO frequency, and
quadrature error for a typical device.
A single-ended drive is also possible as shown in Figure 5, but
this will slightly increase LO leakage. The LO signal should be
applied through a coupling capacitor to LOIP, and LOIN should
be ac-coupled to ground. Because the inputs are fully differential, the drive orientation can be reversed. As in the case of the
differential drive, a 200 Ω resistor connected across LOIP and
LOIN improves the match to a 50 Ω source.
pins should be connected to the same low impedance ground.
RF INPUT
0.8GHz–2.7GHz
0dBm MAX
(AGC MODE)
C1
100pF
R1
200⍀
100pF
+V
S
(2.7V–5.5V)
C9
C6
0.1F
C5
100pF
VPS1
C7
0.1F
C8
100pF
VPS2
0.1F
C10
100pF
VPS3
VREF
IMXO
AD8347
BIAS
ENBL
RFIN
RFIP
C2
VGIN
CELL
GAIN
CONTROL
INTERFACE
DET 1
VAGCVDT1
VREF
DET 2
VDT2
QMXOQOPP
C15
0.1F
24mV p-p
(AGC MODE)
1V BIAS (VREF)
C13
0.1F
IOFS
VREF
SPLITTER
VREF
QOFS
C14
0.1F
24mV p-p
(AGC MODE)
1V BIAS (VREF)
IAIN
PHASE
2
VCMO
QAIN
IOPP
PHASE
SPLITTER
VCMO
1
IOPN
QOPN
VCMO
LOIN
LOIP
COM3
COM2
COM3
COM1
C4
100pF
R17
200⍀
C3
100pF
ETC 1-1-13
(M/A-COM)
IOPP
760mV p-p
DIFFERENTIAL
(AGC MODE)
= 1V
V
CM
IOPN
LO INPUT
–8dBm
0.8GHz–2.7GHz
3
4
15
T1
QOPN
760mV p-p
DIFFERENTIAL
(AGC MODE)
= 1V
V
CM
Figure 4. Basic Connections
–14–
QOPP
REV. 0
Page 15
AD8347
100pF
LO
200⍀
100pF
LOIN
AD8347
LOIP
Figure 5. Single-Ended LO Drive
Operating the VGA
A three-stage VGA sets the gain in the RF section. Two of the
three stages come before the mixer while the third amplifies the
mixer output. All three stages are driven in parallel. The gain
range of the first RF VGA and that of the second RF VGA
combined with the mixer are both –13 dB to +10 dB. The
gain range of the baseband VGA is –4 dB to +19.5 dB. So the
overall gain range from the RF input to the IMXO/QMXO pins
is –30 dB to approximately +39.5 dB.
The gain of the VGA is set by the voltage on the VGIN pin,
which is a high impedance input. The gain control function
(which is linear-in-dB) and linearity are shown in TPC 1 and
TPC 2 at 1.9 GHz. Note that the sense of the gain control
voltage is negative so as the gain control voltage ranges from 0.2 V
to 1.2 V, the gain decreases from +39.5 dB to –30 dB.
Mixer Output Level and Drive Capability
I & Q channel baseband outputs, IMXO and QMXO are low
impedance outputs (R
, the voltage on Pin 14. The achievable output level on
V
VREF
@ 3 Ω) whose bias level is equal to
OUT
IMXO/QMXO is limited by their current drive capability of
1.5 mA max. This would allow for a 600 mV p-p swing into a
200 Ω load. At lower output levels, IMXO and QMXO can
drive smaller load resistances, subject to the same current limit.
These output stages are not, however, designed to drive 50 Ω
loads directly.
Operating the VGA in AGC Mode
While the VGA can be driven by an external source such as a
DAC, the AD8347 has an on-board sum of squares detector
which allows the AD8347 to operate in an automatic leveling
mode. The connections for operating in this mode are shown in
Figure 4. The two mixer outputs are connected to the detector
inputs VDT1 and VDT2. The summed detector output drives
an internal integrator which in turn delivers a gain correction
voltage to the VAGC pin. A 0.1 µF capacitor from VAGC to
ground sets the dominant pole of the integrator circuit. VAGC,
which should be connected to VGIN, adjusts gain until an
internal threshold is reached. This threshold corresponds to a level
at the IMXO/QMXO pins of approximately 8.5 mV rms. This
level will change slightly as a function of RF input power (see
TPC 30). For a CW (sine wave) input this corresponds to
approximately 24 mV p-p. If this signal is applied directly to the
subsequent baseband amplifier stage, the final baseband output
is 760 mV p-p differential. (See Baseband Amplifier section.)
If the VGA gain is being set from an external source, the on-board
detector inputs (VDT1 and VDT2) are not used and should be
tied to VREF.
Note that in subsequent sections, peak-to-peak calculations
assume a sine wave input. If the input signal has a higher peakto-average ratio, the mixer output peak-to-peak voltage at which
the AGC loop settles will be higher.
Changing the AGC Setpoint
The AGC circuit can be easily set up to level at voltages higher
than the nominal 24 mV p-p as shown in Figure 6. The voltages
on Pins IMXO and QMXO are attenuated before being applied
to the detector inputs. In the example shown, an attenuation
factor of 0.2 (–14 dB) between IMXO/QMXO and the detector
inputs, will cause the VGA to level at approximately 120 mV p-p
(note that resistor divider network must be referenced to V
VREF
This results in a peak-to-peak output swing at the baseband
amplifier outputs of 3.8 V differential, that is, 1.6 V to 3.4 V on
each side. Note that V
has been increased to 2.5 V to avoid
VCMO
signal clipping at the baseband outputs. Due to the attenuation
between the mixer output and the detector input, the variation
in the settled mixer output level, versus RF input power, will be
greater than the variation shown in TPC 30. The variation will
be greater by a factor equal to the inverse of the attenuation factor.
Baseband Amplifiers
The final baseband amplifier stage takes the signals from IMXO/
The differential output offset voltages of the baseband amplifiers
are typically ±50 mV. This offset voltage results from both input
and output effects.
The overall signal-to-noise ratio can be improved by increasing
the VGA gain by driving it with an external voltage or by changing
the setpoint of the AGC circuit. (See Changing the AGC Setpoint.)
Driving Capacitive Loads
In applications where the baseband amplifiers are driving unbalanced capacitive loads, some series resistance should be placed
between the amplifier and the capacitive load. For example, for
a 10 pF load, four 220 Ω series resistors (one in each baseband
output) should be used.
External Baseband Amplification
The baseband output offset voltage and noise can be reduced by
bypassing the internal baseband amplifiers and amplifying the
mixer output signal using a high quality differential amplifier. In
the example shown in Figure 7, two AD8132 differential ampli-
).
fiers are used to gain the mixer output signals up by 20 dB. In this
example, the setpoint of the AGC circuit has been increased so that
the input to the external amplifiers is approximately 72 mV p-p.
This results in final baseband output signals of 720 mV p-p.
The closed-loop bandwidth of the amplifiers in Figure 7 is equal
to roughly 20 MHz. Higher bandwidths are achievable, but at
the cost of lower closed-loop gain. In Figure 7, the output common
mode levels (VOCM, Pin 2) of the differential amplifiers are set
by the AD8347’s VREF (approximately 1 V). The output common
mode levels can also be set externally (e.g., by the reference voltage
from an ADC).
QMXO and amplifies them by 30 dB, or a factor of 31.6. This
results in a maximum system gain of 69.5 dB. When the VGA is
in AGC mode, the baseband I & Q outputs (IOPN, IOPP,
QOPN, and QOPP) deliver a differential voltage of approximately 760 mV p-p (380 mV p-p on each side).
The single-ended input signal to the baseband amplifiers is
applied at the high impedance inputs IAIN and QAIN. As can
be seen in Figure 4, the baseband amplifier operates internally
as a differential amplifier, with the second input being driven by
V
. As a result, the input signal to the baseband amplifier
VREF
should be biased at V
VREF
.
The output common-mode level of the baseband amplifiers is
set by the voltage on Pin 5, VCMO. This pin can either be
connected to VREF (Pin 14) or to an external reference voltage
from a device such as an analog-to-digital converter (ADC).
V
has a nominal range from 0.5 V to 2.5 V. However, since
VCMO
the baseband amplifiers can only swing down to 0.4 V, higher
values of V
will generally be required to avoid low-end
VCMO
signal clipping. On the other hand, the positive swing at each
output is limited to 1.3 V below the supply voltage. So the max
p-p swing is given by 2 ⫻ (V
– 1.3 – 0.4) V differentially.
PS
For example, in order for the baseband output amplifier to be able
to deliver an output swing of 2 V p-p (1 V p-p on each side),
V
must be in the range from 0.9 V to 2.5 V.
VCMO
+5V
AD8347
IMXO
VDT1
VREF
VDT2
QMXO
72mV p-p
R23
10k⍀
R25
20k⍀
72mV p-p
R22
20k⍀
R24
10k⍀
R17A
499⍀
R18A
499⍀
R17B
499⍀
R18B
499⍀
R19A
4.99k⍀
AD8132
4.99k⍀
R20A
4.99k⍀
R19B
4.99k⍀
R20B
AD8132
–5V
0.1F
0.1F
–5V
+5V
0.1F
0.1F
10F
720mV p-p
DIFFERENTIAL
= 1V
V
CM
10F
10F
720mV p-p
DIFFERENTIAL
= 1V
V
CM
10F
Figure 7. External Baseband Amplification Example
–16–
REV. 0
Page 17
AD8347
Filter Design Considerations
Baseband low-pass or band-pass filtering can be conveniently
performed between the mixer outputs (IMXO/QMXO) and the
input to the baseband amplifiers. Because the output impedance
of the mixer is low (roughly 3 Ω) and the input impedance of
the baseband amplifier is high, it is not practical to design a
filter which is reactively matched to these impedances. An LC
filter can be matched by placing a series resistor at the mixer
output and a shunt resistor (terminated to V
) at the input to
VREF
the baseband amplifier.
Because the mixer output drive level is limited to a maximum current of 1.5 mA, the characteristic impedance of the filter should be
greater than 50 Ω, especially if larger signal swings are to be achieved.
Figure 8 shows the schematic for a 100 Ω, fourth order elliptic
low-pass filter with a 3 dB cutoff frequency of 20 MHz. Source
and load impedances of approximately 100 Ω ensure that the
filter sees a matched source and load. This also ensures that the
mixer output is driving an overall load of 200 Ω. Note that the
shunt termination resistor is tied to VREF and not to ground.
The frequency response and group delay of this filter are shown
in Figures 9 and 10.
IMXO
AD8347
RS
95.3⍀
4.7pF
L
1
0.68H
C1
R3
2⍀
C3
8.2pF
L
R4
3
2⍀
1.2H
C2
150pF
C4
82pFRL100⍀
VREFVDT1
IAIN
(SEE
TEXT)
Figure 8. Typical Baseband Low-Pass Filter
0
–10
–20
–30
–40
–50
ATTENTUATION – dB
–60
–70
–80
110010
FREQUENCY – MHz
Figure 9. Frequency Response of 20 MHz Baseband
Low-Pass Filter
50
45
40
35
30
25
20
GROUP DELAY – ns
15
10
5
0
110010
FREQUENCY – MHz
Figure 10. Group Delay of 20 MHz Baseband Low-Pass
Filter
If the VGA is operating in AGC mode, the detector input (VDT1/
VDT2) can be tied either to the input or output of the filter.
Connecting the detector input to the input of the filter (i.e.,
IMXO and QMXO) will cause the VGA leveling point to be
determined by the composite of the wanted signal and any unfiltered
components such as blockers or signal harmonics. Connecting
VDT1/VDT2 to the outputs of the filters ensures that the leveling
point of the AGC circuit is based upon the amplitude of the
filtered output only. The latter option is more desirable as it
results in a more constant baseband output. However, when
using this method, the leveling point of the AGC should be set
so that out-of-band blockers do not overdrive the mixer output.
DC Offset Compensation
Feedthrough of the LO signal to the RF input port results in
self-mixing of the LO signal. This produces a dc component
at the mixer output that is frequency-dependent.
The AD8347 includes an internal circuit which actively nulls
out any dc offsets that appear at the mixer output. The dc-bias
level of the mixer output (which should ideally be equal to V
VREF
,
the bias level for the baseband sections of the chip) is continually
being compared to V
output level and V
VREF
. Any differences between the mixer
VREF
, will force a compensating voltage on to
the mixer output.
The time constant of this correction loop is set by the capacitors
which are connected to pins IOFS and QOFS (each output can
be compensated separately). For normal operation 0.1 µF capacitors
are recommended. The corner frequency of the compensation
loop is given approximately by the equation
f
dB
3
CinF
()
OFS
OFS
C
40
=µ
The corner frequency must be set to a frequency that is much
lower than the symbol rate of the demodulated data. This prevents
the compensation loop from falsely interpreting the data stream
as a changing offset voltage.
To disable the offset compensation circuits, IOFS and QOFS
should be tied to VREF.
REV. 0
–17–
Page 18
AD8347
Evaluation Board
Figure 11 shows the schematic of the AD8347 evaluation board.
Note that uninstalled components are indicated with the “open”
designation. The board is powered by a single supply in the
range of 2.7 V to 5.5 V. Table I details the various configuration
options of the evaluation board.
Figure 13. Layout of Component SideFigure 14. Layout of Circuit Side
–19–
Page 20
AD8347
Table I. Evaluation Board Configuration Options
ComponentFunctionDefault Condition
TP1, TP4, TP5Power Supply and Ground Vector PinsNot Applicable
TP2, TP6IOFS and QOFS Probe PointsNot Applicable
TP3VREF Probe PointNot Applicable
LK1, J11Baseband Amplifier Output Bias: Installing this link connects VREFLK1 Installed
to VCMO. This sets the bias level on the baseband amplifiers to VREF,
which is equal to approximately 1 V. Alternatively, the bias level of the
baseband amplifiers can be set by applying an external voltage to SMA
connector J11.
LK2, LK6, LK3, J9, J10AGC Mode: Installing LK2 and LK6 connects the mixer outputs IMXOLK2, LK6, LK3 Installed
and QMXO to the detector inputs VDT2 and VDT1. By installing LK3,
which connects VGIN to VAGC, the AGC mode is activated. The AGC
voltage can be observed on SMA connector J9. With LK3 removed, the
gain control signal for the internal variable gain amplifiers should be
applied to SMA connector J10.
LK4, LK5Baseband Filtering: Installing LK4 and LK5, connects the mixerLK4, LK5 Installed
R6, R33,outputs IMXO and QMXO directly to the baseband amplifier inputsR6 = R33 = 0 Ω (Size 0603)
L1–L5IAIN and QAIN. With R6 and R33 installed (0 Ω), IAIN and QAINL1–L5 = Open (Size 0805)
C4, C17–C22, C25–C31
can be observed on SMA connectors J7 and J8. By removing LK4 and LK5
R8, R34, R39, R40and installing R8 and R34, LC filters can be inserted between theOpen (Size 0805)
mixer outputs and the baseband amplifier inputs. R8 and R34 can beR8 = R34 = Open (0603)
used to increase the effective output impedance of IMXO and QMXO.R39 = R40 = Open (0603)
(These outputs have low output impedances.) R39 and R40 can be used
to provide terminations for the filter at IAIN and QAIN. (IAIN and QAIN
are high impedance inputs.) R39 and R40 are terminated to VREF.