Wide bandwidth: 1 MHz to 10 GHz
Dual-channel and channel difference output ports
Integrated accurate scaled temperature sensor
62 dB dynamic range (±3 dB)
>50 dB with ±1 dB up to 8 GHz
Stability over temperature: ±0.5 dB (−40
Low noise detector/controller outputs
Pulse response time: 6 ns/8 ns (fall time/rise time)
Supply operation: 3.3 V to 5.5 V @ 60 mA
Fabricated using high speed SiGe process
Small footprint, 5 mm × 5 mm, 32-lead LFCSP
Operating temperature range: −40
APPLICATIONS
RF transmitter power amplifier linearization and
gain/power control
Power monitoring in radio link transmitters
Dual-channel wireless infrastructure radios
Antenna VSWR monitor
RSSI measurement in base stations, WLAN, WiMAX, radar
GENERAL DESCRIPTION
The ADL5519 is a dual-demodulating logarithmic amplifier that
incorporates two AD8317s. It can accurately convert an RF input
signa
l into a corresponding decibel-scaled output. The ADL5519
provides accurately scaled, independent, logarithmic output voltages for both RF measurement channels. The device has two
additional output ports, OUTP and OUTN, that provide the
measured differences between the OUTA and OUTB channels.
The on-chip channel matching makes the log amp outputs
insensitive to temperature and process variations.
The temperature sensor pin provides a scaled voltage that is
portional to the temperature over the operating temperature
pro
range of the device.
The ADL5519 maintains accurate log conformance for signals
m 1 MHz to 8 GHz and provides useful operation to 10 GHz.
fro
The ±3 dB dynamic range is typically 62 dB and has a ±1 dB
dynamic range of >50 dB (re: 50 ). The ADL5519 has a response
time of 6 ns/8 ns (fall time/rise time) that enables RF burst detection to a pulse rate of greater than 50 MHz. The device provides
unprecedented logarithmic intercept stability vs. ambient
o
C to +85oC)
o
C to +125oC
Detector/Controller
ADL5519
FUNCTIONAL BLOCK DIAGRAM
INHA
INLA
COMR
PWDN
COMR
COMR
INLB
INHB
COM
COM
2423222120191817
ADL5519
25
26
CHANNEL A
LOG DETECTOR
27
28
29
30
31
32
OUTA
OUTB
CHANNEL B
LOG DETECTOR
12345678
COMR
COMR
VPSA
VPSB
ADJA
TEMP
BIAS
ADJB
Figure 1.
VPSR
VREF
TEMP
VLVL
temperature conditions. A supply of 3.3 V to 5.5 V is required
to power the device. Current consumption is typically 60 mA,
and it decreases to less than 1 mA when the device is disabled.
The device is capable of supplying four log amp measurements
sim
ultaneously. Linear-in-dB measurements are provided at OUTA
and OUTB with conveniently scaled slopes of −22 mV/dB. The log
amp difference between OUTA and OUTB is available as differential or single-ended signals at OUTP and OUTN. An optional
voltage applied to VLVL provides a common-mode reference level
to offset OUTP and OUTN above ground. The broadband output
pins can support many system solutions.
Any of the ADL5519 output pins can be configured to provide
rol voltage to a variable gain amplifier (VGA). Special
a cont
attention has been paid to minimize the broadband noise of the
output pins so that they can be used for controller applications.
The ADL5519 is fabricated on a SiGe bipolar IC process and is
ava
ilable in a 5 mm × 5 mm, 32-lead LFCSP with an operating
temperature range of −40°C to +125°C.
VSTA
CLPA
16
NC
15
OUTA
14
FBKA
13
OUTP
12
OUTN
11
FBKB
10
OUTB
9
NC
VSTB
CLPB
06198-001
Rev. 0
Information furnished by Analog Devices is believed to be accurate and reliable. However, no
responsibility is assumed by Anal og Devices for its use, nor for any infringements of patents or ot her
rights of third parties that may result from its use. Specifications subject to change without notice. No
license is granted by implication or otherwise under any patent or patent rights of Analog Devices.
Trademarks and registered trademarks are the property of their respective owners.
SIGNAL INPUT INTERFACE INHA, INHB (Pin 25, Pin 32)
Specified Frequency Range 0.001 10 GHz
DC Common-Mode Voltage VP − 0.7 V
MEASUREMENT MODE,
100 MHz OPERATION
ADJA (Pin 21) = 0.65 V, ADJB (Pin 4) = 0.7 V; OUTA, OUTB
(Pin 15, Pin 10) shorted to VSTA, VSTB (Pin 17, Pin 8);
OUTP, OUTN (Pin 13, Pin 12) shorted to FBKA, FBKB
(Pin 14, Pin 11), respectively; sinusoidal input signal;
error referred to best-fit line using linear regression
between P
Input Impedance 1670||0.47 Ω||pF
OUTA, OUTB ± 1 dB Dynamic Range 51 dB
−40°C < TA < +85°C 42 dB
OUTA, OUTB Maximum Input Level ±1 dB error −1 dBm
OUTA, OUTB Minimum Input Level ±1 dB error −52 dBm
OUTA, OUTB, OUTP, OUTN Slope
OUTA, OUTB Intercept
1
1
−22 mV/dB
22 dBm
Output Voltage (High Power In) OUTA, OUTB @ P
Output Voltage (Low Power In) OUTA, OUTB @ P
OUTP, OUTN Dynamic Gain Range ±1 dB error 50 dB
−40°C < TA < +85°C 44 dB
Temperature Sensitivity Deviation from OUTA, OUTB @ 25°C
−40°C < TA < +85°C, P
25°C < TA < 85°C, P
−40°C < TA < +25°C, P
Distribution of OUTP, OUTN from 25°C
25°C < T
typical error = −0.09 dB
−40°C < T
typical error = 0.25 dB
25°C < TA < 85°C, P
typical error = 0.05 dB
−40°C < T
typical error = −0.23 dB
Input A-to-Input B Isolation 80 dB
Input A-to-OUTB Isolation
Input B-to-OUTA Isolation
MEASUREMENT MODE,
900 MHz OPERATION
Frequency separation = 1 kHz, P
P
INHA
Frequency separation = 1 kHz, P
P
INHB
ADJA = 0.6 V, ADJB = 0.65 V; OUTA, OUTB shorted to
VSTA, VSTB; OUTP, OUTN shorted to FBKA, FBKB, respectively;
sinusoidal input signal; error referred to best fit line using
linear regression between P
Input Impedance 925||0.54 Ω||pF
OUTA, OUTB ± 1 dB Dynamic Range 54 dB
−40°C < TA < +85°C 49 dB
OUTA, OUTB Maximum Input Level ±1 dB error −2 dBm
OUTA, OUTB Minimum Input Level ±1 dB error −56 dBm
OUTA, OUTB, OUTP, OUTN Slope
OUTA, OUTB Intercept
1
1
−22 mV/dB
20.3 dBm
Output Voltage (High Power In) OUTA, OUTB @ P
Output Voltage (Low Power In) OUTA, OUTB @ P
= 1000 pF, TA = 25°C, 50 Ω termination resistor at INHA, INHB, unless otherwise noted.
LPF
, P
= −40 dBm and −10 dBm
INHB
, P
INHA
INHA
= −16 dBm 0.7 V
INHB
, P
= −40 dBm 1.37 V
INHB
, P
INHA
, P
INHA
INHA
= −16 dBm, P
INHA
INHA
= −40 dBm, P
INHA
INHA
= −16 dBm ±0.25 dB
INHB
= −40 dBm +0.16 dB
INHB
, P
= −40 dBm −0.6 dB
INHB
= −30 dBm,
B
INHB
= −16 dBm, P
= −40 dBm, P
INHB
= −30 dBm, B
INHB
INHB
= −50 dBm,
INHA
when OUTB/Slope = 1 dB
= −50 dBm,
INHB
when OUTA/Slope = 1 dB
= −30 dBm,
= −30 dBm,
B
±0.25 dB
±0.4 dB
±0.25 dB
±0.45 dB
60 dB
60 dB
– P
– P
INHA
< 85°C, P
A
< +25°C, P
A
< +25°C, P
A
INHB
INHA
, P
= −40 dBm and −10 dBm B
INHA
INHB
, P
INHA
INHA
= −10 dBm 0.67 V
INHB
, P
= −40 dBm 1.34 V
INHB
Rev. 0 | Page 3 of 40
ADL5519
www.BDTIC.com/ADI
Parameter Conditions Min Typ Max Unit
OUTP, OUTN Dynamic Gain Range ±1 dB error 55 dB
−40°C < TA < +85°C 48 dB
Temperature Sensitivity Deviation from OUTA, OUTB @ 25°C
−40°C < TA < +85°C, P
25°C < TA < 85°C, P
−40°C < TA < +25°C, P
Distribution OUTP, OUTN from 25°C
25°C < T
< 85°C, P
A
typical error = −0.08 dB
−40°C < TA < +25°C, P
typical error = 0.3 dB
25°C < T
< 85°C, P
A
typical error = 0.17 dB
−40°C < T
< +25°C, P
A
typical error = −0.19 dB
Input A-to-Input B Isolation 75 dB
Input A-to-OUTB Isolation
Input B-to-OUTA Isolation
MEASUREMENT MODE,
1.9 GHz OPERATION
Frequency separation = 1 kHz, P
P
– P
INHA
when OUTB/Slope = 1 dB
INHB
Frequency separation = 1 kHz, P
P
– P
INHB
when OUTA/Slope = 1 dB
INHA
ADJA = 0.5 V, ADJB = 0.55 V; OUTA, OUTB shorted to
VSTA, VSTB; OUTP, OUTN shorted to FBKA, FBKB, respectively;
sinusoidal input signal; error referred to best fit line using
linear regression between P
Input Impedance 525||0.36 Ω||pF
OUTA, OUTB ± 1 dB Dynamic Range 55 dB
−40°C < TA < +85°C 49 dB
OUTA, OUTB Maximum Input Level ±1 dB error −4 dBm
OUTA, OUTB Minimum Input Level ±1 dB error −59 dBm
OUTA, OUTB, OUTP, OUTN Slope
OUTA, OUTB Intercept
1
Output Voltage (High Power In) OUTA, OUTB @ P
Output Voltage (Low Power In) OUTA, OUTB @ P
1
−22 mV/dB
18 dBm
INHA
INHA
OUTP, OUTN Dynamic Gain Range ±1 dB error 55 dB
−40°C < TA < +85°C 48 dB
Temperature Sensitivity Deviation from OUTA, OUTB @ 25°C
−40°C < TA < +85°C, P
25°C < TA < 85°C, P
−40°C < TA < +25°C, P
Distribution of OUTP, OUTN from 25°C
25°C < T
< 85°C, P
A
typical error = −0.07 dB
−40°C < T
< +25°C, P
A
typical error = 0.23 dB
25°C < TA < 85°C, P
typical error = 0.16 dB
−40°C < TA < +25°C, P
typical error = −0.22 dB
Input A-to-Input B Isolation 65 dB
Input A-to-OUTB Isolation
Input B-to-OUTA Isolation
Frequency separation = 1 kHz, P
P
– P
INHA
when OUTB/Slope = 1 dB
INHB
Frequency separation = 1 kHz, P
P
– P
INHB
when OUTA/Slope = 1 dB
INHA
, P
INHA
, P
INHA
INHA
= −16 dBm, P
INHA
INHA
= −40 dBm, P
INHA
INHA
= −16 dBm ±0.25 dB
INHB
= −40 dBm +0.25 dB
INHB
, P
= −40 dBm −0.5 dB
INHB
±0.25 dB
±0.4 dB
±0.25 dB
±0.4 dB
50 dB
50 dB
= −16 dBm, P
INHB
= −40 dBm, P
INHA
= −50 dBm,
INHB
= −30 dBm,
B
INHB
= −30 dBm
INHB
= −30 dBm,
B
= −30 dBm,
B
INHB
= −50 dBm,
, P
= −40 dBm and −10 dBm B
INHA
INHB
, P
= −10 dBm 0.62 V
INHB
, P
= −40 dBm 1.28 V
INHB
, P
INHA
, P
INHA
INHA
= −16 dBm, P
INHA
INHA
= −40 dBm, P
INHA
INHA
= −16 dBm ±0.2 dB
INHB
= −40 dBm +0.25 dB
INHB
, P
= −40 dBm −0.5 dB
INHB
±0.3 dB
±0.4 dB
±0.3 dB
±0.4 dB
46 dB
46 dB
= −16 dBm, P
INHB
= −40 dBm, P
INHA
= −50 dBm,
INHB
= −30 dBm,
B
INHB
= −30 dBm,
INHB
= −30 dBm, B
= −30 dBm, B
INHB
= −50 dBm,
Rev. 0 | Page 4 of 40
ADL5519
www.BDTIC.com/ADI
Parameter Conditions Min Typ Max Unit
MEASUREMENT MODE,
2.2 GHz OPERATION
ADJA = 0.48 V, ADJB = 0.6 V; OUTA, OUTB shorted to
VSTA, VSTB; OUTP, OUTN shorted to FBKA, FBKB, respectively;
sinusoidal input signal; error referred to best fit line using
linear regression between P
INHA
, P
INHB
= −40 dBm and −10 dBm B
Input Impedance 408||0.34 Ω||pF
OUTA, OUTB ± 1 dB Dynamic Range 55 dB
−40°C < TA < +85°C 50 dB
OUTA, OUTB Maximum Input Level ±1 dB error −5 dBm
OUTA, OUTB Minimum Input Level ±1 dB error −60 dBm
OUTA, OUTB, OUTP, OUTN Slope
OUTA, OUTB Intercept
1
Output Voltage (High Power In) OUTA, OUTB @ P
Output Voltage (Low Power In) OUTA, OUTB @ P
1
−22 mV/dB
16.9 dBm
, P
INHA
INHA
= −10 dBm 0.6 V
INHB
, P
= −40 dBm 1.26 V
INHB
OUTP, OUTN Dynamic Gain Range ±1 dB error 56 dB
−40°C < TA < +85°C 40 dB
Temperature Sensitivity Deviation from OUTA, OUTB @ 25°C
−40°C < TA < +85°C, P
25°C < TA < 85°C, P
−40°C < TA < +25°C, P
INHA
, P
INHA
, P
INHA
= −16 dBm ±0.28 dB
INHB
= −40 dBm +0.3 dB
INHB
, P
= −40 dBm −0.5 dB
INHB
Distribution of OUTP, OUTN from 25°C
25°C < T
< 85°C, P
A
= −16 dBm, P
INHA
= −30 dBm,
B
INHB
typical error = −0.07 dB
−40°C < T
< +25°C, P
A
= −16 dBm, P
INHA
= −30 dBm,
INHB
typical error = 0.25 dB
25°C < T
< 85°C, P
A
= −40 dBm, P
INHA
= −30 dBm,
B
INHB
typical error = 0.17 dB
−40°C < T
< +25°C, P
A
= −40 dBm, P
INHA
= −30 dBm
B
INHB
typical error = −0.22dB
Input A-to-Input B Isolation 60 dB
Input A-to-OUTB Isolation
Input B-to-OUTA Isolation
MEASUREMENT MODE,
3.6 GHz OPERATION
Frequency separation = 1 kHz, P
P
– P
INHA
when OUTB/Slope = 1 dB
INHB
Frequency separation = 1 kHz, P
P
– P
INHB
when OUTA/Slope = 1 dB
INHA
ADJA = 0.35 V ADJB = 0.42; OUTA, OUTB shorted to
VSTA, VSTB; OUTP, OUTN shorted to FBKA, FBKB, respectively;
= −50 dBm,
INHA
= −50 dBm,
INHB
sinusoidal input signal; error referred to best fit line using
linear regression between P
INHA
, P
INHB
= −40 dBm and −10 dBm B
Input Impedance 187||0.66 Ω||pF
OUTA, OUTB ± 1 dB Dynamic Range 54 dB
−40°C < TA < +85°C 44 dB
OUTA, OUTB Maximum Input Level ±1 dB error −4 dBm
OUTA, OUTB Minimum Input Level ±1 dB error −58 dBm
OUTA, OUTB, OUTP, OUTN Slope
OUTA, OUTB Intercept
1
Output Voltage (High Power In) OUTA, OUTB @ P
Output Voltage (Low Power In) OUTA, OUTB @ P
1
−22.5 mV/dB
17 dBm
, P
INHA
INHA
= −10 dBm 0.62 V
INHB
, P
= −40 dBm 1.31 V
INHB
OUTP, OUTN Dynamic Gain Range ±1 dB error 52 dB
−40°C < TA < +85°C 42 dB
±0.25 dB
±0.4 dB
±0.25 dB
±0.4 dB
46 dB
46 dB
Rev. 0 | Page 5 of 40
ADL5519
www.BDTIC.com/ADI
Parameter Conditions Min Typ Max Unit
Temperature Sensitivity Deviation from OUTA, OUTB @ 25°C
−40°C < TA < +85°C, P
25°C < TA < 85°C, P
−40°C < TA < +25°C, P
Distribution of OUTP, OUTN from 25°C
25°C < T
< 85°C, P
A
typical error = −0.07 dB
−40°C < T
< +25°C, P
A
typical error = 0.27 dB
25°C < T
< 85°C, P
A
typical error = 0.31 dB
−40°C < T
< +25°C, P
A
typical error = −0.14 dB
Input A-to-Input B Isolation 40 dB
Input A-to-OUTB Isolation
Input B-to-OUTA Isolation
MEASUREMENT MODE,
5.8 GHz OPERATION
Frequency separation = 1 kHz, P
P
– P
INHA
when OUTB/Slope = 1 dB
INHB
Frequency separation = 1 kHz, P
P
– P
INHB
when OUTA/Slope = 1 dB
INHA
ADJA = 0.58 V, ADJB = 0.7 V; OUTA, OUTB shorted to
VSTA, VSTB; OUTP, OUTN shorted to FBKA, FBKB respectively;
sinusoidal input signal; error referred to best fit line using
linear regression between P
Input Impedance 28||1.19 Ω||pF
OUTA, OUTB ± 1 dB Dynamic Range 53 dB
−40°C < TA < +85°C 45 dB
OUTA, OUTB Maximum Input Level ±1 dB error −2 dBm
OUTA, OUTB Minimum Input Level ±1 dB error −55 dBm
OUTA, OUTB, OUTP, OUTN Slope
OUTA, OUTB Intercept
1
Output Voltage (High Power In) OUTA, OUTB @ P
Output Voltage (Low Power In) OUTA, OUTB @ P
1
−22.5 mV/dB
20 dBm
INHA
INHA
OUTP, OUTN Dynamic Gain Range ±1 dB error 53 dB
−40°C < TA < +85°C 46 dB
Temperature Sensitivity Deviation from OUTA, OUTB @ 25°C
−40°C < TA < +85°C, P
25°C < TA < 85°C, P
−40°C < TA < +25°C, P
Distribution of OUTP, OUTN from 25°C
25°C < T
< 85°C, P
A
typical error = 0.02 dB
−40°C < T
< +25°C, P
A
typical error = 0.25 dB
25°C < T
< 85°C, P
A
typical error = 0.13 dB
−40°C < T
< +25°C, P
A
typical error = 0.06 dB
Input A-to-Input B Isolation 45 dB
Input A-to-OUTB Isolation
Input B-to-OUTA Isolation
Frequency separation = 1 kHz, P
P
– P
INHA
when OUTB/Slope = 1 dB
INHB
Frequency separation = 1 kHz, P
P
– P
INHB
when OUTA/Slope = 1 dB
INHA
, P
INHA
, P
INHA
INHA
= −16 dBm, P
INHA
INHA
= −40 dBm, P
INHA
INHA
= −16 dBm ±0.4 dB
INHB
= −40 dBm +0.6 dB
INHB
, P
= −40 dBm −0.45 dB
INHB
±0.25 dB
±0.45 dB
±0.3 dB
±0.5 dB
20 dB
20 dB
= −16 dBm, P
INHB
= −40 dBm, P
INHA
= −50 dBm,
INHB
= −30 dBm,
B
INHB
= −30 dBm,
INHB
= −30 dBm,
B
= −30 dBm,
B
INHB
= −50 dBm,
, P
= −40 dBm and −20 dBm B
INHA
INHB
, P
= −10 dBm 0.68 V
INHB
, P
= −40 dBm 1.37 V
INHB
, P
INHA
, P
INHA
INHA
= −16 dBm, P
INHA
INHA
= −40 dBm, P
INHA
INHA
= −16dBm ±0.25 dB
INHB
= −40 dBm +0.25 dB
INHB
, P
= −40 dBm −0.4 dB
INHB
±0.3 dB
±0.4 dB
±0.3 dB
±0.5 dB
48 dB
48 dB
= −16 dBm, P
INHB
= −40 dBm, P
INHA
= −50 dBm,
INHB
= −30 dBm,
B
INHB
= −30 dBm,
INHB
= −30 dBm,
B
= −30 dBm,
B
INHB
= −50 dBm,
Rev. 0 | Page 6 of 40
ADL5519
www.BDTIC.com/ADI
Parameter Conditions Min Typ Max Unit
MEASUREMENT MODE,
8 GHz OPERATION
ADJA = 0.72 V, ADJB = 0.82 V to GND; OUTA, OUTB shorted
to VSTA, VSTB; OUTP, OUTN shorted to FBKA, FBKB, respectively;
sinusoidal input signal; error referred to best fit line using
linear regression between P
INHA
, P
INHB
= −40 dBm and −20 dBm B
Input Impedance +10||−1.92 Ω||pF
OUTA, OUTB ± 1 dB Dynamic Range 48 dB
−40°C < TA < +85°C 38 dB
OUTA, OUTB Maximum Input Level ±1 dB error 0 dBm
OUTA, OUTB Minimum Input Level ±1 dB error −48 dBm
OUTA, OUTB, OUTP, OUTN Slope
OUTA, OUTB Intercept
1
Output Voltage (High Power In) OUTA, OUTB @ P
Output Voltage (Low Power In) OUTA, OUTB @ P
1
−22 mV/dB
26 dBm
, P
INHA
INHA
= −10 dBm 0.81 V
INHB
, P
= −40 dBm 1.48 V
INHB
OUTP, OUTN Dynamic Gain Range ±1 dB error 50 dB
−40°C < TA < +85°C 42 dB
Temperature Sensitivity Deviation from OUTA, OUTB @ 25°C
−40°C < TA < +85°C, P
25°C < TA < 85°C, P
−40°C < TA < +25°C, P
INHA
, P
INHA
, P
INHA
= −16 dBm ±0.4 dB
INHB
= −40 dBm −0.1 dB
INHB
, P
= −40 dBm +0.5 dB
INHB
Distribution of OUTP, OUTN from 25°C
25°C < T
< 85°C, P
A
= −16 dBm, P
INHA
= −30 dBm,
B
INHB
typical error = 0.2dB
−40°C < T
< +25°C, P
A
= −16 dBm, P
INHA
= −30 dBm,
INHB
typical error = 0.09dB
25°C < T
< 85°C, P
A
= −40 dBm, P
INHA
= −30 dBm,
B
INHB
typical error = −0.07dB
−40°C < T
< +25°C, P
A
= −40 dBm, P
INHA
= −30 dBm,
B
INHB
typical error = 0.17 dB
Input A-to-Input B Isolation 45 dB
Input A-to-OUTB Isolation
Input B-to-OUTA Isolation
Frequency separation = 1 kHz, P
P
– P
INHA
when OUTB/Slope = 1 dB
INHB
Frequency separation = 1 kHz, P
P
– P
INHB
when OUTA/Slope = 1 dB
INHA
= −50 dBm,
INHA
= −50 dBm,
INHB
OUTPUT INTERFACE OUTA, OUTB; OUTP, OUTN
OUTA, OUTB Voltage Range VSTA, VSTB = 1.7 V, RF in = open 0.3 V
VSTA, VSTB = 0 V, RF in = open VP − 0.4 V
OUTP, OUTN Voltage Range FBKA, FBKB = open and OUTA < OUTB, RL ≥ 240 Ω to ground 0.09 V
FBKA, FBKB = open and OUTA > OUTB, RL ≥ 240 Ω to ground VP − 0.15 V
Source/Sink Current Output held at 1 V to 1% change 10 mA
Capacitance Drive 1 nF
Output Noise
INHA, INHB = 2.2 GHz, −10 dBm, f
= 100 kHz,
NOISE
CLPA, CLPB = open
Fall Time
Input level = no signal to −10 dBm, 80% to 20%,
CLPA, CLPB = 10 pF
Input level = no signal to −10 dBm, 80% to 20%,
CLPA, CLPB = open
Rise Time
Input level = −10 dBm to no signal, 20% to 80%,
CLPA, CLPB = 10 pF
Input level = −10 dBm to no signal, 20% to 80%,
CLPA, CLPB = open
Video Bandwidth
10 MHz
(or Envelope Bandwidth)
SETPOINT INTERFACE VSTA, VSTB
Nominal Input Range Input level = 0 dBm, measurement mode 0.38 V
Input level = –50 dBm, measurement mode 1.6 V
Input Resistance Controller mode, sourcing 50 μA 40 kΩ
Rev. 0 | Page 7 of 40
±0.3 dB
±0.5 dB
±0.3 dB
±0.5 dB
30 dB
30 dB
10 nV/√Hz
12 ns
6 ns
16 ns
8 ns
ADL5519
www.BDTIC.com/ADI
Parameter Conditions Min Typ Max Unit
DIFFERENCE LEVEL ADJUST VLVL (Pin 6)
Input Voltage OUTP, OUTN = FBKA, FBKB VP − 1 V
Input Resistance OUTP, OUTN = FBKA, FBKB 100 kΩ
TEMPERATURE COMPENSATION ADJA, ADJB
Input Resistance ADJA, ADJB = 0.9 V, sourcing 50 μA 13 kΩ
Disable Threshold Voltage ADJA, ADJB = open VP − 0.4 V
VOLTAGE REFERENCE VREF (Pin 5)
Output Voltage 1.15 V
Temperature Sensitivity −40°C < TA < +25°C; relative TA = 25°C +26 μV/°C
25°C < TA < 85°C; relative TA = 25°C −26 μV/°C
Current Limit Source/Sink 3/3 mA
TEMPERATURE REFERENCE TEMP (Pin 19)
Output Voltage 1.36 V
Temperature Sensitivity −40°C < TA < +125°C 4.5 mV/°C
Current Limit Source/Sink 4/50 mA/μA
POWER-DOWN INTERFACE PWDN (Pin 28)
Logic Level to Enable Logic low enables 0 V
Logic Level to Disable Logic high disables VP − 0.2 V
Input Current Logic high PWDN = 5 V 2 μA
Logic low PWDN = 0 V 20 μA
Enable Time
Disable Time
POWER INTERFACE VPSA, VPSB, VPSR
Supply Voltage 3.3 5.5 V
Quiescent Current 60 mA
vs. Temperature −40°C ≤ TA ≤ +85°C 147 μA/°C
Disable Current ADJA, ADJB = PWDN = VP <1 mA
1
Slope and intercept are determined by calculating the best-fit line between the power levels of −40 dBm and −10 dBm at the specified input frequency.
PWDN low to OUTA, OUTB at 100% final value,
CLPA, CLPB = open, RF in = −10 dBm
PWDN high to OUTA, OUTB at 10% final value,
CLPA, CLPB = open, RF in = 0 dBm
0.4 μs
0.25 μs
Rev. 0 | Page 8 of 40
ADL5519
www.BDTIC.com/ADI
ABSOLUTE MAXIMUM RATINGS
Table 2.
Parameter Rating
Supply Voltage: VPSA, VPSB, VPSR 5.7 V
V
Voltage: VSTA, VSTB 0 to V
SET
Input Power (Single-Ended, Re: 50 Ω)
INHA, INLA, INHB, INLB
Internal Power Dissipation 420 mW
θ
JA
Maximum Junction Temperature 142°C
Operating Temperature Range −40°C to +125°C
Storage Temperature Range −65°C to +150°C
Lead Temperature (Soldering, 60 sec) 260°C
P
12 dBm
42°C/W
Stresses above those listed under Absolute Maximum Ratings
y ca
use permanent damage to the device. This is a stress
ma
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.
1 COMR Connect via low impedance to common.
2 COMR Connect via low impedance to common.
3 VPSB Positive Supply for Channel B. Apply 3.3 V to 5.5 V supply voltage.
4 ADJB Dual-Function Pin: Temperature Adjust Pin for Channel B and Power-Down Interface for OUTB.
5 VREF Voltage Reference (1.15 V).
6 VLVL DC Common-Mode Adjust for Difference Output.
7 CLPB Loop Filter Pin for Channel B.
8 VSTB Setpoint Control Input for Channel B.
9 NC No Connect.
10 OUTB Output Voltage for Channel B.
11 FBKB Difference Op Amp Feedback Pin for OUTN Op Amp.
12 OUTN Difference Output (OUTB − OUTA + VLVL).
13 OUTP Difference Output (OUTA − OUTB + VLVL).
14 FBKA Difference Op Amp Feedback Pin for OUTP Op Amp.
15 OUTA Output Voltage for Channel A.
16 NC No Connect.
17 VSTA Setpoint Control Input for Channel A.
18 CLPA Loop Filter Pin for Channel A.
19 TEMP Temperature Sensor Output (1.3 V with 4.5 mV/°C Slope).
20 VPSR Positive Supply for Difference Outputs and Temperature Sensor. Apply 3.3 V to 5.5 V supply voltage.
21 ADJA Dual-Function Pin: Temperature Adjust Pin for Channel A and Power-Down Interface for OUTA.
22 VPSA Positive Supply for Channel A. Apply 3.3 V to 5.5 V supply voltage.
23 COMR Connect via low impedance to common.
24 COMR Connect via low impedance to common.
25 INHA AC-Coupled RF Input for Channel A.
26 INLA AC-Coupled RF Common for Channel A.
27 COMR Connect via low impedance to common.
28 PWDN Power-Down for Difference Output and Temperature Sensor.
29 COMR Connect via low impedance to common.
30 COMR Connect via low impedance to common.
31 INLB AC-Coupled RF Common for Channel B.
32 INHB AC-Coupled RF Input for Channel B.
Paddle Internally connected to COMR.
Figure 48. Output Response Using Power-Down Mode for Various
RF Input Levels, C
0.06
0.05
0.04
0.03
0.02
SUPPLY CURRENT (A)
0.01
0
3.03.23.43.63.84.04.24.44.64.85.0
Figure 49. Supply Current vs. V
arrier Frequency = 900 MHz, CLPA = 0.1 μF
INCREASING
DECREASING
PWDN, ADJA, ADJB VO LTAGE ( V)
, V
ADJA
, V
PWDN
2.4
ADJB
22.5
20.0
17.5
15.0
12.5
10.0
7.5
5.0
2.5
INPUT VOLTAGE PWDN PULSE (V)
0
–2.5
2.6
2.8
3.0
06198-148
06198-150
Rev. 0 | Page 18 of 40
ADL5519
R
R
www.BDTIC.com/ADI
THEORY OF OPERATION
The ADL5519 is a dual-channel, six-stage demodulating logarithmic amplifier that is specifically designed for use in RF
measurement and power control applications at frequencies
up to 10 GHz. The ADL5519 is a derivative of the
logari
thmic detector/controller core. The ADL5519 maintains
AD8317
tight intercept variability vs. temperature over a 50 dB range.
Each measurement channel offers performance equivalent to
that of the
shown in Fi
INHA
INLA
COMR
PWDN
COMR
COMR
INLB
INHB
AD8317. The complete circuit block diagram is
gure 50.
COM
COM
2423222120191817
ADL5519
25
26
27
28
29
30
31
32
CHANNEL A
LOG DETECTOR
OUTA
OUTB
CHANNEL B
LOG DETECTOR
12345678
COMR
COMR
VPSA
VPSB
ADJA
TEMP
BIAS
ADJB
Figure 50. Block Diagram
VPSR
VREF
TEMP
VLVL
VSTA
CLPA
VSTB
CLPB
16
15
14
13
12
11
10
9
NC
OUTA
FBKA
OUTP
OUTN
FBKB
OUTB
NC
Each measurement channel is a full differential design using
a proprietary, high speed SiGe process that extends high frequency
performance.
signal pa
Figure 51 shows the basic diagram of the Channel A
th; its functionality is identical to that of the Channel B
signal path.
VI
DETDETDETDET
INHA
INLA
Figure 51. Single Channel Block Diagram
VSTA
VI
OUTA
CLPA
06198-041
06198-042
The maximum input with ±1 dB log conformance error is typically
−5 dBm (re: 50 Ω). The noise spectral density referred to the input
is 1.15 nV/√Hz, which is equivalent to a voltage of 118 µV rms
in a 10.5 GHz bandwidth or a noise power of −66 dBm (re: 50 Ω).
This noise spectral density sets the lower limit of the dynamic
range. However, the low end accuracy of the ADL5519 is enhanced
by specially shaping the demodulating transfer characteristic to
partially compensate for errors due to internal noise. The common
pins provide a quality, low impedance connection to the printed
circuit board (PCB) ground. The package paddle, which is internally connected to the COMR pins, should also be grounded to
the PCB to reduce thermal impedance from the die to the PCB.
The logarithmic function is approximated in a piecewise fashion
by six cas
tion of the logarithm approximation, refer to the
sheet
caded gain stages. For a more comprehensive explana-
AD8307 data
. The cells have a nominal voltage gain of 9 dB each, with
a 3 dB bandwidth of 10.5 GHz. Using precision biasing, the gain
is stabilized over temperature and supply variations. The overall
dc gain is high because of the cascaded nature of the gain stages.
An offset compensation loop is included to correct for offsets
within the cascaded cells. At the output of each gain stage,
a square-law detector cell is used to rectify the signal.
The RF signal voltages are converted to a fluctuating differential
cur
rent, having an average value that increases with signal level.
Along with the six gain stages and detector cells, an additional
detector is included at the input of each measurement channel,
providing a 54 dB dynamic range in total. After the detector
currents are summed and filtered, the following function is
formed at the summing node:
× log10(VIN/V
I
D
) (1)
INTERCEPT
where:
I
is the internally set detector current.
D
V
is the input signal voltage.
IN
V
is the intercept voltage (that is, when VIN = V
INTERCEPT
INTERCEPT
the output voltage would be 0 V, if it were capable of going to 0 V).
,
Rev. 0 | Page 19 of 40
ADL5519
www.BDTIC.com/ADI
USING THE ADL5519
BASIC CONNECTIONS
The ADL5519 is specified for operation up to 10 GHz. As a result,
low impedance supply pins with adequate isolation between
functions are essential. A power supply voltage between 3.3 V
and 5.5 V should be applied to VPSA, VPSB, and VPSR. Power
supply decoupling capacitors of 100 pF and 0.1 µF should be
connected close to these power supply pins (see
Figure 53).
The paddle of the LFCSP package is internally connected to
COMR. F
or optimum thermal and electrical performance, the
paddle should be soldered to a low impedance ground plane.
INPUT SIGNAL COUPLING
The ADL5519 inputs are differential but were characterized
and are generally used single ended. When using the ADL5519
in single-ended mode, the INHA, INHB pins must be ac-coupled,
and INLA, INLB must be ac-coupled to ground. Suggested
coupling capacitors are 47 nF, ceramic 0402-style capacitors for
input frequencies of 1 MHz to 10 GHz. The coupling capacitors
should be mounted close to the INHA, INHB and INLA, INLB
pins. The coupling capacitor values can be increased to lower
the input stage high-pass cutoff frequency.
The high-pass corner is set by the input coupling capacitors and the
inter
nal 10 pF high-pass capacitor. The dc voltage on INHA, INHB
and INLA, INLB is approximately one diode voltage drop below
the supply voltage.
Although the input can be reactively matched, in general this
reactive matching is not necessary. An external 52.3 Ω shunt
resistor (connected on the signal side of the input coupling capacitors, as shown in
input
The coupling time constant, 50 × C
with a 3 dB attenuation at f
C2 = C3 = C4 = C
pass corner is ~68 kHz. In high frequency applications, f
be as large as possible to minimize the coupling of unwanted low
frequency signals. In low frequency applications, a simple RC
network forming a low-pass filter should be added at the input
for similar reasons. This low-pass filter should generally be placed
at the generator side of the coupling capacitors, thereby lowering
the required capacitance value for a given high-pass corner
frequency.
VPSA
5pF5pF
18.7kΩ18.7kΩ
INHA
INLA
Figure 52. Single-Channel Input Interface
CURRENT
Gm
STAGE
2kΩ
FIRST
GAIN
STAGE
A = 9dB
OFFSET
COMP
6198-044
Figure 53) combines with the relatively high
impedance to give an adequate broadband match of 50 Ω.
/2, forms a high-pass corner
C
= 1/(2π × 50 × CC ), where C1 =
HP
. Using the typical value of 47 nF, this high-
C
should
HP
Rev. 0 | Page 20 of 40
ADL5519
VPSR
www.BDTIC.com/ADI
C15
0.1µF
TEMP SENSOR
C9
100pF
VSTA
CLPATEMPVPSRADJA
16
NC
15
OUTA
14
FBKA
13
OUTP
OUTPUT
VOLTAGE B
SETPOINT
VOLTAGE B
DIFF OUT+
INHA
PWDN
VPSA
52.3Ω
ADJA
C12
0.1µF
C4
47nF
R5
C3
47nF
C7
100pF
2423
COMR
COMR
25
INHA
26
INLA
27
COMR
28
PWDN
222120191817
VPSA
C8
100pF
ADL5519ACPZ
12
C10
100pF
VSTB
OUTN
FBKB
OUTB
NC
11
10
9
VPOS
DIFF OUT–
OUTPUT
VOLTAGE B
SETPOINT
VOLTAGE B
VPSA
VPSB
VPSR
06198-043
INHB
52.3Ω
29
COMR
30
COMR
C2
47nF
31
C1
47nF
INLB
32
INHB
COMR
COMR
12
C16
100pF
C11
0.1µF
R6
EXPOSED PADDLE
345678
C5
0.1µF
VPSB
VREFADJB
CLPBVLVLVREFADJBVPSB
VLVL
Figure 53. Basic Connections for Operation in Measurement Mode
Rev. 0 | Page 21 of 40
ADL5519
P
VPSR
V
V
www.BDTIC.com/ADI
TEMPERATURE SENSOR INTERFACE
The ADL5519 provides a temperature sensor output capable of
driving 4 mA. The temperature scaling factor of the output voltage
is ~4.48 mV/°C. The typical absolute voltage at 27°C is approximately 1.36 V.
INTERNAL
VPTAT
12kΩ
4kΩ
COMR
Figure 54. TEMP Interface Simplified Schematic
TEM
06198-045
VREF INTERFACE
The VREF pin provides a highly stable voltage reference. The
voltage on the VREF pin is 1.15 V, which is capable of driving
3 mA. An equivalent internal resistance is connected from
VREF to COMR for 3 mA sink capability.
POWER-DOWN INTERFACE
The operating and stand-by currents for the ADL5519 at 27°C
are approximately 60 mA and less than 1 mA, respectively. To
completely power down the ADL5519, the PWDN and ADJA,
ADJB pins must be pulled within 200 mV of the supply voltage.
When powered on, the output reaches to within 0.1 dB of its
steady-state value in about 0.5 μs; the reference voltage is available to full accuracy in a much shorter time.
This wake-up response time varies, depending on the input
coupling network and the capacitance at the CLPA, CLPB pins.
PWDN disables the OUTP, OUTN, VREF, and TEMP pins. The
power-down pin, PWDN, is a high impedance pin.
The ADJA and ADJB pins, when pulled within 200 mV of the
supply voltage, disable OUTA and OUTB, respectively.
SETPOINT INTERFACE—VSTA, VSTB
The VSTA, VSTB inputs are high impedance (40 kΩ) pins that
drive inputs of internal op amps. The V
the internal 1.5 kΩ resistor to generate a current, I
portion of V
−I
= V
If V
SET
is applied to VSTA, VSTB, the feedback loop forces
The slope is given by −ID × 2x × 1.5 kΩ = −22 mV/dB × x. For
example, if a resistor divider to ground is used to generate a V
voltage of V
/2, then x = 2. The slope is set to −880 V/decade
OUT
SET
or −44 mV/dB. See the Altering the Slope section for additional
information.
OUTPUT INTERFACE—OUTA, OUTB
The OUTA, OUTB pins are driven by a push-pull output stage.
The rise time of the output is limited mainly by the slew on CLPA,
CLPB. The fall time is an RC-limited slew given by the load capacitance and the pull-down resistance at OUTA, OUTB. There is
an internal pull-down resistor of 1.6 kΩ The resistive load at
OUTA, OUTB can be placed in parallel with the internal pulldown resistor to reduce the discharge time. OUTA, OUTB can
source greater than 10 mA.
The ADL5519 incorporates two operational amplifiers with rail-torail output capability to provide a channel difference output.
As in the case of the output drivers for OUTA, OUTB, the output
stages have the capability of driving greater than 10 mA. OUTA
and OUTB are internally connected through 1 kΩ resistors to the
inputs of each op amp. The VLVL pin is connected to the positive
terminal of both op amps through 1 kΩ resistors to provide
level shifting. The negative feedback terminal is also made
available through a 1 kΩ resistor. The input impedance of VLVL
is 1 kΩ, and the input impedance of FBKA, FBKB is 1 kΩ. See
Figure 57 for the connections of these pins.
Figure 58. Op Amp Connections (All Resistors Are 1 kΩ ± 20%)
1kΩ
1kΩ
FBKA COMR
1kΩ
1kΩ
FBKB COMR
1kΩ
1kΩ
1kΩ
OUTP
VPSRVLVL
OUTN
06198-050
14
FBKA
13
OUTP
12
OUTN
11
FBKB
06198-051
DESCRIPTION OF CHARACTERIZATION
The general hardware configuration used for most of the ADL5519
characterization is shown in Figure 59. The signal sources used
in this example are the E8251A from Agilent Technologies. The
INHA, INHB input pins are driven by Agilent signal sources,
and the output voltages are measured using a voltmeter.
SIGNAL
SOURCE
SIGNAL
SOURCE
–3dB
–3dB
INA
ADL5519
CHARACTERIZATI ON
BOARD
INB
COMPUTER
CONTROLL ER
Figure 59. General Characterization Configuration
OUTA
OUTB
OUTP
OUTN
VREF
TEMP
AGILENT
34970A
METER/
SWITCHING
6198-052
BASIS FOR ERROR CALCULATIONS
The input power and output voltage are used to calculate the
slope and intercept values. The slope and intercept are calculated
using linear regression over the input range from −40 dBm to
−10 dBm. The slope and intercept terms are used to generate an
ideal line. The error is the difference in measured output voltage
compared to the ideal output line. This is a measure of the linearity
of the device. Refer to the Device Calibration section for more
information on calculating slope, intercept, and error.
Error from the linear response to the CW waveform is not
a measure of absolute accuracy because it is calculated using
the slope and intercept of each device. However, error verifies the
linearity and the effects of modulation on device response.
Similarly, at temperature extremes, error represents the output
voltage variations from the 25°C ideal line performance. Data
presented in the graphs is the typical error distribution observed
during characterization of the ADL5519.
Pulse response of the ADL5519 is 6 ns/8 ns rise/fall times. For
the fastest response time, the capacitance on OUTA, OUTB should
be kept to a minimum. Any capacitance on the output pins should
be counterbalanced with an equal capacitance on the CLPA, CLPB
pins to prevent ringing on the output.
In this configuration, all four measurements, OUTA, OUTB,
OUTP, and OUTN, are available simultaneously. A differential
output can be taken from OUTP − OUTN, and VLVL can be
used to adjust the common-mode level for an ADC connection.
This is convenient not only for driving a differential ADC but
also for removing any temperature variation on VLVL.
Rev. 0 | Page 23 of 40
ADL5519
www.BDTIC.com/ADI
DEVICE CALIBRATION
The measured transfer function of the ADL5519 at 2.2 GHz is
shown in Figure 60. The figure shows plots of both output voltage
t power and calculated error vs. input power. As the input
vs. inpu
power varies from −60 dBm to −5 dBm, the output voltage varies
from 1.7 V to about 0.5 V.
2.00
1.75
1.50
1.25
V
OUT1
1.00
0.75
V
OUT2
OUTPUT VOLTAGE (V)
0.50
0.25
0
–60–50–40–30–20010
Figure 60. Transfer Function at 2.2 GHz with Calibration Points
P
PIN (dBm)
IN1
–10
P
IN2
Because slope and intercept vary from device to device, boardlevel calibration must be performed to achieve the highest
accuracy. The equation for output voltage can be written as
= Slope × (PIN − Intercept) (6)
V
OUT
where:
Slop
input power, P
h
e change in output voltage divided by the change in
e is t
, expressed in decibels (dB).
IN
Intercept is the calculated power at which the output voltage
would be 0 V. Note that an output voltage of 0 V can never be
achieved.
In general, calibration is performed by applying two known
signal leve
ls to the ADL5519 input and measuring the corresponding output voltages. The calibration points are generally
chosen to be within the linear-in-dB operating range of the
device (see the
Specifications section for more details).
Calculation of the slope and intercept is accomplished using the
wing equations:
follo
− V
)/(P
− P
Slope = (V
OUT1
Intercept = P
IN1
− (V
OUT2
IN1
/Slope) (8)
OUT1
) (7)
IN2
Once slope and intercept are calculated, an equation can be
wri
tten that calculates the input power based on the output
voltage of the detector.
(Unknown) = (V
P
IN
OUT1(MEASURED)
/Slope) + Intercept (9)
The log conformance error of the calculated power is given by
Error (dB) = (V
OUT(MEASURED)
− V
OUT(IDEAL)
)/Slope (10)
Figure 60 includes a plot of the error at 25°C, the temperature
ich the log amp is calibrated. Note that the error is not 0 dB
at wh
over the full dynamic range. This is because the log amp does
2.0
1.5
1.0
0.5
0
–0.5
–1.0
–1.5
–2.0
not perfectly follow the ideal V
its operating region. The error at the calibration points of −35
dBm and −11 dBm is equal to 0 dB, by definition.
Figure 60 also shows error plots for the output voltage at
−40°C and +85°C. Th
ese error plots are calculated using the
slope and intercept at 25°C. This is consistent with calibration
in a mass-production environment, where calibration over
temperature is not practical.
ADJUSTING ACCURACY THROUGH CHOICE OF
CALIBRATION POINTS
In some applications, very high accuracy is required at one
power level or over a reduced input range. For example, in a
wireless transmitter, the accuracy of the high power amplifier
ERROR (dB)
06198-053
(HPA) is most critical at or close to full power.
In applications like AGC control loops, good linearity and
temp
erature performance are necessary over a large input power
range. The temperature crossover point (the power level at which
there is no drift in performance from −40°C to −80°C) can be
shifted from high power levels to midpower levels using the
method shown in the
tion. This shift equalizes the temperature performance over
sec
Temperature Compensation Adjustment
the complete power range. The linearity of the transfer function
can be equalized by changing the calibration points.
Figure 61 demonstrates this equalization by changing the calibra
tion points used in Figure 60 to −46 dBm and −22 dBm. This
adju
stment of the calibration points changes the linearity to greater
than ±0.25 dB over a 50 dB dynamic range at the expense of a
slight decrease in linearity at power levels between −40 dBm
and −25 dBm.
Calibration points should be chosen to suit the application at hand.
In ge
neral, however, do not choose calibration points in the
nonlinear portion of the log amp transfer function (greater than
−10 dBm or less than −40 dBm, in this example).
2.00
1.75
1.50
V
OUT1
1.25
1.00
V
OUT2
0.75
OUTPUT VOLTAGE (V)
0.50
0.25
0
–60–50–40–30–20010
P
IN1
Figure 61. Dynamic Range Extension by Choosing C
Are Close to the End of the Linear Range, 2.14 GHz
vs. PIN equation, even within
OUT
PIN (dBm)
–10
P
IN2
alibration Points That
2.0
1.5
1.0
0.5
0
–0.5
–1.0
–1.5
–2.0
ERROR (dB)
06198-055
Rev. 0 | Page 24 of 40
ADL5519
V
V
www.BDTIC.com/ADI
Another way of presenting the error function of a log amp detector
is shown in Figure 62. In this example, the decibel (dB) error at
hot and cold
temperatures is calculated with respect to the output
voltage at ambient. This is a key difference when compared to the
previous plots, in which all errors have been calculated with respect
to the ideal transfer function at ambient.
2.00
1.75
1.50
2.0
1.5
1.0
Compensating the device for temperature drift by using ADJA,
B allows for great flexibility. To determine the optimal adjust
ADJ
voltage, sweep ADJA, ADJB at ambient and at the desired
temperature extremes for a couple of power levels while
monitoring the output voltage. The point of intersection
determines the best adjust voltage. Some additional minor
tweaking may be required to achieve the highest level of temperature stability. With appropriate values, a temperature drift error
of typically ±0.5 dB over the entire rated temperature range can be
achieved.
1.25
1.00
0.75
OUTPUT VOLTAGE (V)
0.50
0.25
0
–60–50–40–30–20–10010
Figure 62. Error vs. Temperature with Respect to Output
2.14 GHz (Removes Transfer Function Nonlinearities at 25°C)
PIN (dBm)
0.5
0
–0.5
–1.0
–1.5
–2.0
Voltage at 25°C,
With this alternative technique, the error at ambient becomes,
by definition, equal to 0 (see Figure 62). This value would be
valid i
f the device transfer function perfectly followed the ideal
of the V
= Slope × (PIN − Intercept) equation.
OUT
However, because an rms amp, in practice, never perfectly follows
this e
quation (especially outside of its linear operating range),
this plot tends to artificially improve linearity and extend the
dynamic range, unless enough calibration points are taken to
remove the error.
Figure 62 is a useful tool for estimating temperature drift at
ticular power level with respect to the (nonideal) output
a par
voltage at ambient.
Table 4. Recommended ADJA, ADJB Voltage Levels
Frequency Recommended ADJA, ADJB Voltage (V)
ERROR (dB)
100 MHz 0.65, 0.7
900 MHz 0.6, 0.65
1.9 GHz 0.5, 0.55
2.2 GHz 0.48, 0.6
3.6 GHz 0.35, 0.42
5.8 GHz 0.58, 0.7
06198-056
8 GHz 0.72, 0.82
Proprietary techniques are used to compensate for the temperature
drift. The absolute value of compensation varies with frequency
and circuit board material.
ADJA, ADJB are high impedance pins. The applied ADJA, ADJB
s can be supplied from VREF through a resistor divider.
voltage
Figure 63 shows a simplified schematic representation of the
, ADJB interface.
ADJA
REF
I
COMP
TADJ
ADL5519
ADJA, ADJB
TEMPERATURE COMPENSATION ADJUSTMENT
The ADL5519 temperature performance has been optimized to
ensure that the output voltage has minimum temperature drift
at −10 dBm input power. The applied voltage for the ADJA and
ADJB pins for some specified frequencies is listed in
ver, not all frequencies are represented in Table 4, and
Howe
exper
imentation may be required.
Table 4.
Rev. 0 | Page 25 of 40
Figure 63.
COMR
COMR
ADJA, ADJB Interface Simplified Schematic
06198-057
ADL5519
www.BDTIC.com/ADI
ALTERING THE SLOPE
As discussed in the Setpoint Interface—VSTA, VSTB section,
the slope can readily be increased by scaling the amount of
output voltage at OUTA, OUTB that is fed back to the setpoint
interface, VSTA, VSTB. When the full signal from OUTA,
OUTB is applied to VSTA, VSTB, the slope has a nominal value of
−22 mV/dB. This value can be increased by including a voltage
divider between the OUTA, OUTB and VSTA, VSTB pins, as
shown in Figure 64.
ADL5519
OUTA, OUTB
VSTA, VSTB
Figure 64. External Network to Raise Slope
V
OUT
R1
R2
06198-058
The approximate input resistance for VSTA, VSTB is 40 kΩ.
Scaling resistor values should be carefully selected to minimize
errors. Keep in mind that these resistors also load the output
pins and reduce the load-driving capabilities.
Equation 11 can be used to calculate the resistor values.
S
⎛
R2'R1(11)
=1
⎜
⎝
⎞
D
−
⎟
−
22
⎠
where:
S
is the desired slope, expressed in millivolts/decibels (mV/dB).
D
R2' is the value of R2 in parallel with 40 kΩ.
For example, using R1 = 1.65 kΩ and R2 = 1.69 kΩ (R2' = 1.62 kΩ),
the nominal slope is increased to −44 mV/dB.
When the slope is increased, the loop capacitor, CLPA, CLPB,
may need to be raised to ensure stability and to preserve a chosen
averaging time. The slope can be lowered by placing a voltage
divider after the output pin, following standard practices.
CHANNEL ISOLATION
Isolation must be considered when using both channels of the
ADL5519 at the same time. The two isolation requirements that
should be considered are the isolation from one RF channel input
to the other RF channel input and the isolation from one RF
channel input to the other channel output. When using both
channels of the ADL5519, care should be taken in the layout to
isolate the RF inputs, INHA and INHB, from each other. Coupling
on the PC board affects both types of isolation.
In most applications, the designer has the ability to adjust the
power going into the ADL5519 through the use of temperaturestable couplers and accurate temperature-stable attenuators of
different values. When isolation is a concern, it is useful to
adjust the input power so the lowest expected detectable power
is not far from the lowest detectable power of the ADL5519 at
the frequency of operation.
The lowest detectable power point of the ADL5519 has little
variation from part to part. This equalizes the signals on both
channels at their lowest possible power level, which reduces the
overall isolation requirements and possibly adds attenuators to the
RF inputs of the device, reducing the RF channel input isolation
requirements.
Measuring the RF channel input to the other RF channel input
isolation is straightforward and is done by measuring the loss
on a network analyzer from one input to the other input. The
outcome is shown in the Specifications section of the data sheet.
Note that adding an attenuator in series with the RF signal
increases the channel input-to-input isolation by the value of
the attenuator.
The isolation between one RF channel input and the other channel
output is a little more complicated. The easiest approach (which
was used in this datasheet) to measuring this isolation is to have
one channel set to the lowest power level it is expected to have
on its input (approximately −50 dBm in this data sheet) and
then increasing the power level on the other channel input until
the output of the low power channel changes by 22 mV. Because
−50 dBm is in the linear region of the detector, 22 mV equates
to a 1 dB change in the output.
If the inputs to both RF channels are at the same frequency, the
isolation also depends on the phase shift between the RF signals
put into the ADL5519. This relationship can be demonstrated by
placing a high power signal on one RF channel input and a low
power signal slightly offset in frequency to the other RF channel.
If the output of the low power channel is observed with an
oscilloscope, it has a ripple that looks similar to a full-wave
rectified sine wave with a frequency equal to the frequency
difference between the two channels, that is, a beat tone. The
magnitude of the ripple reflects the isolation at a specific phase
offset (note that two signals of slightly different frequencies act
like two signals with a constantly changing phase), and the
frequency of that ripple is directly related to the frequency offset.
The data shown in the Specifications section assumes worst-case
amplitude and phase offset. If the RF signals on Channel A and
Channel B are at significantly different frequencies, the input-tooutput isolation increases, depending on the capacitors placed on
CLPA, CLPB and the frequency offset of the two signals, due to
the response roll-off within the ADL5519.
Rev. 0 | Page 26 of 40
ADL5519
www.BDTIC.com/ADI
OUTPUT FILTERING PACKAGE CONSIDERATIONS
Accurate power detection for signals with RF bursts is achieved
when the ADL5519 is able to respond quickly to the change in
RF power. For applications in which maximum video bandwidth
and, consequently, fast rise time are desired, it is essential that
the CLPA, CLPB pins have very little capacitance on them (some
capacitance reduces the ringing).
The nominal output video bandwidth of 10 MHz can be reduced
nnecting a ground-referenced capacitor (C
by co
) to the CLPA,
FLT
CLPB pins, as shown in Figure 65. This is generally done to
uce output ripple (at twice the input frequency for a
red
symmetric input waveform, such as a sinusoidal signal).
3.5pF
×Ω×π
ADL5519
1
BandwidthVideo
+4
OUTA, OUTB
CLPA, CLPB
C
FLT
−
6198-059
(12)
pF5.3
I
LOGA,
I
LOGB
1.5kΩ
Figure 65. Lowering the Post Demodulation Bandwidth
C
is selected using the following equation:
FLT
C
=
FLT
()
k5.1
The video bandwidth should typically be set to a frequency less
than
or equal to approximately 1/10 the minimum input frequency.
There are no problems with putting large capacitor values on the
CLPA, CLPB pins. These large capacitor values ensure that the
output ripple of the demodulated log output, which is at twice
the input frequency, is well filtered. Signals with modulation
may need additional filtering (a larger C
capacitance) to
FLT
remove modulation bleedthrough.
The ADL5519 uses a compact, 32-lead LFCSP. A large exposed
paddle on the bottom of the device provides both a thermal
benefit and a low inductance path to ground for the circuit.
To make proper use of this packaging feature, the PCB RF/dc
common-ground reference needs to make contact with the paddle
with as many vias as possible to lower inductance and thermal
impedance.
OPERATION ABOVE 8 GHz
The ADL5519 is specified for operation up to 8 GHz, but it
provides useful measurement accuracy over a reduced dynamic
range of up to 10 GHz. Figure 66 shows the performance of the
ADL5519 o
high frequency performance is achieved using the configuration
shown in Figure 53. The dynamic range shown is reduced from the
typical de
measurement range with less than 3 dB of linearity error.
Implementing an impedance match for frequencies greater than
8 GHz can improve the sensitivity of the ADL5519 and its measurement range.
OUTPUT VOLTAGE (V)
Figure 66. V
ver temperature for a input frequency of 10 GHz. This
vice performance, but the ADL5519 can provide 30 dB of
2.00
1.75
1.50
1.25
1.00
0.75
0.50
0.25
0
–40–35–30–25–20–15–10–50
and Log Conformance vs. Input Amplitude at 10 GHz,
OUT
Over Temperature, ADJA, ADJB = 1.8 V, 1.8 V
PIN (dBm)
4.0
3.0
2.0
1.0
0
–1.0
–2.0
–3.0
–4.0
ERROR (dB)
06198-169
Rev. 0 | Page 27 of 40
ADL5519
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APPLICATIONS INFORMATION
MEASUREMENT MODE
The ADL5519 is placed in measurement mode by connecting
OUTA, OUTB to VSTA, VSTB, respectively. The part has an offset
voltage, a negative slope, and a V
OUTA, VOUTB
cept at the high end of its input signal range.
The output voltage vs. input signal voltage of the ADL5519 is
-in-dB over a multidecade range. The equation for this
linear
function is of the following form:
V
OUT
x × V
= x × V
× 20 × log10(VIN/V
SLOPE/dB
SLOPE/DEC
× log10(VIN/V
INTERCEPT
where:
x is the fe
V
V
the V
V
edback factor in V
is nominally −440 mV/decade or −22 mV/dB.
SLOPE/DEC
is the x-axis intercept of the linear-in-dB portion of
INTERCEPT
vs. VIN curve.
OUT
is 2 dBV for a sinusoidal input signal.
INTERCEPT
An offset voltage, V
OFFSET
= V
SET
OUT
, of 0.45 V is internally added to
the detector signal so that the minimum value for V
x × V
. If x = 1, the minimum V
OFFSET
The slope is very stable vs. process and temperature variation.
When
Base-10 logarithms are used, V
volts/decade. A decade corresponds to 20 dB; V
SLOPE/dB
represents the slope in V/dB. B
V
As noted in Equation 13 and Equation 14, the V
a negative slope. This is also the correct slope polarity to control
the gain of many VGAs in a negative feedback configuration.
Because both the slope and intercept vary slightly with frequency,
see the Specifications section for application-specific values for
pe and intercept.
slo
Although demodulating log amps respond to input signal
tage and not input signal power, it is customary to discuss
vol
the amplitude of high frequency signals in terms of power. In
this case, the characteristic impedance of the system, Z
be known to convert voltages to their corresponding power levels.
The following equations are used to perform this conversion:
2
P (dBm) = 10 × log
P (dBV) = 20 × log
P (dBm) = P (dBV) − 10 × log
For example, P
, for a sinusoidal input signal expressed
INTERCEPT
/(Z0 × 1 mW)) (15)
10(Vrms
/1 V
10(Vrms
rms
10(Z0
in terms of dBm (decibels referred to 1 mW), in a 50 Ω system is
P
P
2 dBV − 10 × log
(dBm) =
INTERCEPT
(dBV) − 10 × log10(Z0 × 1 mW/1 V
INTERCEPT
(50 × 10−3) = 15 dBm
10
measurement inter-
) = (13)
INTERCEPT
) (14)
/x.
is
OUT
value is 0.45 V.
OUT
represents the
SLOPE/DEC
/20 =
SLOPE/DEC
voltage has
OUT
, must
0
) (16)
rms
2
) =
rms
2
) (17)
× 1 mW/1 V
For a square wave input signal in a 200 Ω system
INTERCEPT
(dBm) =
[(200 Ω × 1 mW/1V
10
2
)] = +6 dBm
rms
P
−1 dBV − 10 × log
More information about the intercept variation dependence upon
form can be found in the AD8313 and AD8307 data sheets.
wave
As the input signals to Channel A and Channel B are swept over
ir nominal input dynamic range of −5 dBm to −55 dBm, the
the
output swings from 0.5 V to 1.6 V. The voltages of OUTA, OUTB
are also internally applied to a difference amplifier with a gain
of 1. When the input power is swept, OUTP swings from approximately 0.5 V to 1.75 V, and OUTN swings from 1.75 V to 0.5 V.
The VLVL pin sets the common-mode voltage for OUTP, OUTN.
An output common-mode voltage of ≤1.15 V can be set using
a resistor divider between the VREF and VLVL pins. Measurement
of large differences between INHA, INHB can be affected by
on-chip signal leakage.
CONTROLLER MODE
In addition to being a measurement device, the ADL5519 can
also be configured to set and control signal levels. Each of the two
log detectors can be separately configured to set and control the
output power level of a VGA or variable voltage attenuator (VVA).
See the Controller Mode section of the AD8317 datasheet for more
ation on running a single channel in controller mode.
inform
Alternatively, the two log detectors can be configured to measure
trol the gain of an amplifier or signal chain. The channel
and con
difference outputs can be used to control a feedback loop to the
ADL5519 RF inputs. A capacitor connected between FBKA and
OUTP forms an integrator, keeping in mind that the on-chip 1 kΩ
feedback resistor forms a 0. (The value of the on-chip resistors can
vary as much as ±20% with manufacturing process variation.)
If Channel A is driven and Channel B has a feedback loop from
OUTP through a VGA, OUTP integrates to a voltage value
such that
OUTB = (OUTA +
h
e output value from OUTN may or may not be useful. It is
T
give
n by
OUTN = 0 V (19)
for VLVL < OUTA/3.
Otherwise,
OUTN = (3 × VLVL − OUTA)/2 (20)
VLVL)/2 (18)
Rev. 0 | Page 28 of 40
ADL5519
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If VLVL is connected to the OUTA pin, OUTB is forced to equal
OUTA through the feedback loop. This flexibility provides the
capability to measure one channel operating at a given power
level and frequency while forcing the other channel to a desired
power level at another frequency. The voltages applied to the
ADJA, ADJB pins should be selected carefully to minimize
temperature drift of the output voltage. The temperature drift is
the statistical sum of the drift from Channel A and Channel B.
As stated previously, VLVL can be used to force the slaved
channel to operate at a different power from the other channel.
If the two channels are forced to operate at different power levels,
som
e static offset occurs due to voltage drops across metal wiring
in the IC.
If an inversion is necessary in the feedback loop, OUTN can be
used as
the integrator by placing a capacitor between OUTN,
OUTP. This changes the output equation for OUTB and OUTP to
OUTB = 2 × OUT
For VLVL < OUTA/2,
OUTN = 0 V (22)
Otherwise,
OUTN = 2 × VLVL − OUTA (23)
uation 18 to Equation 23 are valid when Channel A is driven
Eq
Channel B is slaved through a feedback loop. When Channel B
and
is driven and Channel A is slaved, these equations can be altered
by changing OUTB to OUTA and OUTN to OUTP.
A − VLVL (21)
Rev. 0 | Page 29 of 40
ADL5519
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AUTOMATIC GAIN CONTROL
Figure 67 shows how the ADL5519 can be connected to provide
automatic gain control to an amplifier or signal chain. Additional
pins are omitted for clarity. In this configuration, both detectors
are connected in measurement mode with appropriate filtering
being used on CLPA, CLPB to provide adequate filtering of the
demodulated log output. OUTA, however, is also connected to
the VLVL pin of the on-board difference amplifier. In addition,
the OUTP output of the difference amplifier drives a variable gain
element (either VVA or VGA) and is connected back to the FBKA
input via a capacitor so that it is operating as an integrator.
Assume that OUTA is much bigger than OUTB. Because OUTA
drives VLVL, this voltage is also present on the noninverting
also
input of the op amp driving OUTP. This results in a current flow
from OUTP through the integrating capacitor into the FBKA input.
This results in the voltage on OUTP increasing. If the gain control
transfer function of the VGA/VVA is positive, this increases the
gain, which in turn increases the input signal to INHA. The
output voltage on the integrator continues to increase until the
power on the two input channels is equal, resulting in a signal
chain gain of unity.
If a gain other than 0 dB is required, an attenuator can be used
in one of the RF paths, as shown in Figure 67. Alternatively,
er splitters or directional couplers of different coupling
pow
factors can be used. Another convenient option is to apply a
voltage on VLVL other than OUTA. Refer to Equation 18 and
Controller Mode section for more detail.
the
If the VGA/VVA has a negative gain control sense, the OUTN
out
put of the difference amplifier can be used with the integrating
capacitor tied back to FBKB. Alternatively, the inputs could be
swapped.
The choice of the integrating capacitor affects the response time
of t
he AGC loop. Small values give a faster response time but
may result in instability, whereas larger values reduce the response
time. Capacitors that are too large can also cause oscillations due
to the capacitive drive capability of the op amp. In automatic gain
control, the capacitors on CLPA and CLPB, which perform the
filtering of the demodulated log output, must still be used and
also affect loop response time.
Rev. 0 | Page 30 of 40
ADL5519
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DIRECTIONAL
OR
POWER SPLITTER
VGA/VVA
CLPA
ADL5519
DIRECTIONAL
OR
POWER SPLITTER
VSTA
OUTA
FBKA
OUTP
OUTN
FBKB
OUTB
VSTB
C
INT
DIFF OUT +
ATTE NUATO R
6198-063
50Ω
50Ω
0.1µF
0.1µF
0.1µF
0.1µF
INHA
INLA
INLB
INHB
CHANNEL A
LOG DETECTOR
CHANNEL B
LOG DETECTOR
VLVL
CLPB
Figure 67. Operation in Controller Mode for Automatic Gain Control
Rev. 0 | Page 31 of 40
ADL5519
www.BDTIC.com/ADI
GAIN-STABLE TRANSMITTER/RECEIVER
There are many applications for a transmitter or receiver with
a highly accurate temperature-stable gain. For example, a multicarrier, base station high power amplifier (HPA) using digital
predistortion can have a power detector and an auxiliary receiver.
The power detector and all parts associated with it can be removed
if the auxiliary receiver has a highly accurate temperature-stable
gain. With a set gain receiver, the ADC on the auxiliary receiver
can determine not only the overall power being transmitted but
also the power in each carrier for a multicarrier HPA. Without the
use of a detector, the auxiliary receiver is very difficult to calibrate
accurately over temperature due to the part-to-part variation of the
components in the auxiliary receiver.
In controller mode, the ADL5519 can be used to hold the receiver
gain constant over a broad input power/temperature range. In this
application, the difference outputs are used to hold the receiver gain
constant. Figure 69 shows an example of how this can be done.
The RF input is connected to INHB, using a 19 dB coupler, and
the down-converted output from the signal chain is connected
to INHA, using a 19 dB coupler. A 100 pF capacitor is connected
between FBKA and OUTP, forming an integrator. OUTA is
connected to VLVL, forcing OUTP to adjust the VGA so that
OUTB is equal to OUTA. The circuit gain is set by the difference
in the coupling values of the input and output couplers and the
differences in path losses to the detector. Because they are operating
at different frequencies, the appropriate voltages on the ADJA,
ADJB pins must be supplied. ADJA is set to 0.6 V and ADJB is
set to 0.65 V to set the −40
center of the input power range. Using the suggested ADJA value
for 80 MHz would put the crossover point at a higher power level.
o
C/+85oC crossover point toward the
Figure 68 shows the results of the circuit in Figure 69. The input
power is swept from −47 dBm to +8 dBm. The output power is
measured, and the gain is calculated at +25°C, −40°C and +85°C.
With equal valued couplers used on the input and output, the
expected gain is about 0 dB. Due to path loss differences and
differences due to using two separate frequencies, the average
gain is about 2.5 dB. In this configuration, approximately 50 dB of
control range with 0.2 dB drift over temperature is obtained. For
an auxiliary receiver, less than 5 dB of variation is expected over
temperature. If the power levels are chosen to coincide with the
temperature crossover point, approximately 0.1 dB of temperature
variation can be expected. Most of the gain change over input
power level is caused by performance differences at different
frequencies.
4.0
3.5
3.0
2.5
2.0
GAIN (dB)
1.5
1.0
0.5
0
–50–40–30–20–10010
Figure 68. Performance of Gain-Stable Receiver
PIN (dBm)
GAIN +85°C
GAIN +25°C
GAIN –40°C
06198-171
Rev. 0 | Page 32 of 40
ADL5519
V
www.BDTIC.com/ADI
5V
REF
C16
0.1UF
RFIN
900MHz
0.65V
C11
100PF
0Ω 0Ω
C10
0.1 UF
454Ω
19dB
COUPLING
R30
52.3
1
2
3
4
5
6
7
8
MODE SEL
0V TO 1. 2V
C4
47NF
VPSB
ADJB
VREF
VLVL
CLPB
VSTB
ADL5330
INHB
101911
C2
47NF
INLB
EXPOSED PADDLE
OUTB
FBKB
AD8342
820MHZ
POWE R DOWN
COMR
ADL5519
OUTN
0Ω 0Ω
90MHz
LPF
0.1 UF
R31
52.3
C8
100PF
C9
25
INHA
C1
47NF
24
23
22
21
20
18
17
C3
47NF
28293132
2730
26
FBKA
INLA
VPSA
ADJA
VPSR
TEMP
CLPA
VSTA
OUTA
15141213
169
PWDN
OUTP
IFOUT
80MHz
454Ω
19dB
COUPLI NG
C7
100PF
0.6V
C15
0.1UF
5V
C12
0.1UF
TEMPERATURE
SENSOR OUT
100 PF
B CHANNEL OUT
DIFF OUT–
06198-172
Figure 69. Gain-Stable Receiver Circuit
Rev. 0 | Page 33 of 40
ADL5519
www.BDTIC.com/ADI
MEASURING VSWR
Measurement of reflected power in wireless transmitters is a critical
auxiliary function that is often overlooked. The power reflected
back from an antenna is specified using either the voltage standing
wave ratio (VSWR) or the reflection coefficient (also referred to
as the return loss). Poor VSWR can cause shadowing in a TV
broadcast system because the signal reflected off the antenna
reflects again off the power amplifier and is then rebroadcast. In
wireless communications systems, shadowing produces multipathlike phenomena. Poor VSWR can degrade transmission quality;
the catastrophic VSWR that results from damage to a co-axial
cable or to an antenna can, at its worst, destroy the transmitter.
The ADL5519 delivers an output voltage proportional to the log
of the input signal over a large dynamic range. A log-responding
device offers a key advantage in VSWR measurement applications.
To compute gain or reflection loss, the ratio of the two signal
powers (either OUTPUT/INPUT or REVERSE/FORWARD)
must be calculated. An analog divider must be used to perform
this calculation with a linear-responding diode detector, but
only simple subtraction is required when using a log-responding
detector (because log(A/B) = log(A) − log(B)).
A dual RF detector has an additional advantage compared to
a discrete implementation. There is a natural tendency for two
devices (RF detectors, in this case) to behave similarly when they
are fabricated on a single piece of silicon, with both devices having
similar temperature drift characteristics, for example. At the
summing node, this drift cancels to yield a result that is more
temperature stable.
In Figure 71, two directional couplers are used, one to measure
forward power and one to measure reverse power. Additional
attenuation is required before applying these signals to the
detectors. The ADL5519 dual detector has a measurement range
of 50 dB in each detector. Care must be taken in setting the attenuation levels so the reflection coefficient can be measured over the
desired output power range.
The level planning used in this example is graphically depicted
in Figure 70. In this example, the expected output power range
from the HPA is 30 dB, from 20 dBm to 50 dBm. Over this
power range, the ADL5519 can accurately measure reflection
coefficients from 0 dB (short, open, or load) to −20 dB.
Each ADL5519 detector has a nominal input range from −5 dBm
to −55 dBm. In this example, the maximum forward power of
+50 dBm is attenuated to −10 dBm at the detector input (this
attenuation is achieved through the combined coupling factor
of the directional coupler and the subsequent attenuation). This
puts the maximum power at the detector comfortably within its
linear operating range. Also, when the HPA is transmitting at its
lowest power level of +20 dBm, the detector input power is
−40 dBm, which is still within its input operating range.
50dBm
40dBm
30dBm
20dBm
10dBm
–10dBm
–20dBm
–30dBm
–40dBm
–50dBm
–60dBm
0dBm
FORWARD
POWER
RANGE
55dB
ATTENUATION
DECTOR A/B
60dB
ATTENUATION
POWER
AT INPUT A
Figure 70. ADL5519 VSWR Level Planning
INPUT RANG E
REVERSE
POWER
RANGE
POWR
AT INPUT B
6198-075
Careful level planning should be used to match the input power
levels in a dual detector and to place these power levels within
the linear operating range of the detectors. The power from the
reverse path is attenuated by 55 dB, which means that the detector
is capable of measuring reflected power up to 0 dB. In most applications, the system is designed to shut down when the reflection
coefficient degrades below a certain minimum (for example,
10 dB). Full reflection is allowed when using the ADL5519 because
of its large dynamic range. In the case of very little reflection
(a return loss of 20 dB) and the HPA is transmitting +20 dBm, the
reverse path detector has an input power of −55 dBm.
The application circuit in Figure 71 provides a direct reading of
return loss, forward power, and reverse power. If the forward and
reverse phase difference (phase angle) is needed to optimize the
power delivered to the antenna, the AD8302 should be used.
It provides one output that represents the return loss and one
output that represents the phase difference between the two
signals. However, the AD8302 does not provide the absolute
forward or reverse power.
Rev. 0 | Page 34 of 40
ADL5519
m
www.BDTIC.com/ADI
HPA
P
= 20dBm TO 50dB
OUT
20dB20dB
40dB35dB
52.3Ω
P
= –10dBm TO
IN
–40dBm
52.3Ω
PIN = –5dBm TO
–55dBm
0.1µF
INHA
0.1µF
INHB
Figure 71.
VSTA
BIAS
TEMP
OUTA
FBKA
OUTP
OUTN
FBKB
OUTB
VSTB
RETURN
LOSS
ADL5519
CHANNEL A
LOG DETECTOR
OUTA
OUTB
CHANNEL B
LOG DETECTOR
ADL5519 Configuration for Measuring Reflection Coefficients
FORWARD
POWER
ADC
ADC
ADC
REVERSE
POWER
MICROPROCESSOR/
DSP
06198-074
Rev. 0 | Page 35 of 40
ADL5519
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EVALUATION BOARD
CONFIGURATION OPTIONS
Table 5. Evaluation Board (Rev. A) Configuration Options
Supply and Ground Connections.
VPOS, VPSB, and VPSR are internally connected.
GND, GND1, and GND3 are internally connected.
Input Interface.
The 52.3 Ω resistors in the R30 and R31 positions combine with the ADL5519
internal input impedance to give a broadband input impedance of about 50 Ω.
C1, C2, C3, and C4 are dc-blocking capacitors. A reactive impedance match can
be implemented by replacing R5, R6, R30, and R31 with an inductor and by
replacing C1, R0A and C4, R0B with appropriately valued capacitors.
Temperature Sensor Interface.
Tempera
R14 can be used as a pull-down resistor.
Temperature Compensation Interface.
A voltage source at ADJA, ADJB can be used to optimize the temperature
performance for various input frequencies. The pads for R27/R28 or R27/R29 can
be used for voltage dividers from the VREF node to set the ADJA, ADJB voltages
at different frequencies. The individual log channels can be disabled by installing
0 Ω resistors at R18 and R19.
Output Interface, Measurement Mode.
In measurement mode, a portion of the output voltage is fed back to VSTA, VSTB via
R8, R12. The magnitude of the slope of the OUTA, OUTB output voltage response
can be increased by reducing the portion of V
VSTB. The slope can be decreased by implementing a voltage divider by using
R20 and R16 or R21 and R15. R20 and R21 can also be used as a back-terminating
resistor or as part of a single-pole, low-pass filter.
Output Interface, Controller Mode.
In thi
controller mode, the ADL5519 can control the gain of an external component.
A setpoint voltage is applied to VSTA, VSTB, the value of which corresponds to
the desired RF input signal level applied to the corresponding ADL5519 RF input.
A sample of the RF output signal from this variable-gain component is selected,
typically via a directional coupler, and applied to ADL5519 RF input. The voltage
at OUTA, OUTB is applied to the gain control of the variable gain element. A control
voltage is applied to VSTA, VSTB. The magnitude of the control voltage can
optionally be attenuated via the voltage divider comprising R8, R12 and R22,
R23; or a capacitor can be installed in the R22, R23 position to form a low-pass
filter along with R8, R12.
Power Supply Decoupling.
The nominal supply decoupling consists of a 100 pF filter capacitor placed
physically close to the ADL5519 and a 0.1 μF capacitor placed nearer to each
power supply input pin.
R9 and R10 can be replaced with a capacitor to form an integrator for constant
gain con
Filter Capacitor.
The lo
lowered by placing a capacitor between CLPA, CLPB and ground. Increasing this
capacitor increases the overall rise/fall time of the ADL5519 for pulsed input
signals. See the Output Filtering section for more details.
VREF can be used to drive VLVL through a voltage divider formed using R7 and C6.
ture sensor output voltage is available at the test point labeled TEMP.
s mode, the 0 Ω resistors must be removed, leaving R8 and R12 open. In
troller mode
w-pass corner frequency of the circuit that drives OUTA, OUTB can be