AD8362ARUZ-REEL71 [ADI]

50 Hz to 2.7 GHz 60 dB TruPwr⑩ Detector; 50 Hz至2.7 GHz的60分贝TruPwr⑩探测器
AD8362ARUZ-REEL71
型号: AD8362ARUZ-REEL71
厂家: ADI    ADI
描述:

50 Hz to 2.7 GHz 60 dB TruPwr⑩ Detector
50 Hz至2.7 GHz的60分贝TruPwr⑩探测器

文件: 总36页 (文件大小:699K)
中文:  中文翻译
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50 Hz to 2.7 GHz  
60 dB TruPwr™ Detector  
AD8362  
FEATURES  
FUNCTIONAL BLOCK DIAGRAM  
DECL  
CHPF  
Complete fully calibrated measurement/control system  
Accurate rms-to-dc conversion from 50 Hz to 2.7 GHz  
Input dynamic range of >60 dB: −52 dBm to +8 dBm in 50 Ω  
Waveform and modulation independent:  
(Such as GSM/CDMA/TDMA)  
INHI  
2
x
CLPF  
VOUT  
ACOM  
INLO  
Linear-in-decibels output, scaled 50 mV/dB  
Law conformance error of 0.5 dB  
All functions temperature and supply stable  
Operates from 4.5 V to 5.5 V at 24 mA from −40°C to +85°C  
Power-down capability to 1.3 mW  
2
V
TGT  
x
VSET  
VPOS  
AD8362  
APPLICATIONS  
Power amplifier linearization/control loops  
BIAS  
VREF  
Transmitter power control  
Transmitter signal strength indication (TSSI)  
RF instrumentation  
COMM  
PWDN  
Figure 1.  
GENERAL DESCRIPTION  
The AD8362 is a true rms-responding power detector that has a  
60 dB measurement range. It is intended for use in a variety of  
high frequency communication systems and in instrumentation  
requiring an accurate response to signal power. It is easy to use,  
requiring only a single supply of 5 V and a few capacitors. It can  
operate from arbitrarily low frequencies to over 2.7 GHz and  
can accept inputs that have rms values from 1 mV to at least  
1 V rms, with peak crest factors of up to 6, exceeding the  
requirements for accurate measurement of CDMA signals.  
the input power. Optionally, the voltage at VSET may be a  
replica of the RF signals amplitude modulation, in which case  
the overall effect is to remove the modulation component prior  
to detection and low-pass filtering. The corner frequency of the  
averaging filter may be lowered without limit by adding an  
external capacitor at the CLPF pin. The AD8362 can be used to  
determine the true power of a high frequency signal having a  
complex low frequency modulation envelope (or simply as a  
low frequency rms voltmeter). The high-pass corner generated  
by its offset-nulling loop can be lowered by a capacitor added  
on the CHPF pin.  
The input signal is applied to a resistive ladder attenuator  
that comprises the input stage of a variable gain amplifier.  
The 12 tap points are smoothly interpolated using a proprietary  
technique to provide a continuously variable attenuator, which  
is controlled by a voltage applied to the VSET pin. The resulting  
signal is applied to a high performance broadband amplifier. Its  
output is measured by an accurate square-law detector cell. The  
fluctuating output is then filtered and compared with the output  
of an identical squarer, whose input is a fixed dc voltage applied  
to the VTGT pin, usually the accurate reference of 1.25 V  
provided at the VREF pin.  
Used as a power measurement device, VOUT is strapped to  
VSET, and the output is then proportional to the logarithm of  
the rms value of the input; that is, the reading is presented  
directly in decibels and is conveniently scaled 1 V per decade,  
that is, 50 mV/dB; other slopes are easily arranged. In controller  
modes, the voltage applied to VSET determines the power level  
required at the input to null the deviation from the setpoint.  
The output buffer can provide high load currents.  
The AD8362 is powered down by a logic high applied to the  
PWDN pin, i.e., the consumption is reduced to about 1.3 mW. It  
powers up within about 20 µs to its nominal operating current  
of 20 mA at 25°C. The AD8362 is supplied in a 16-lead TSSOP  
package for operation over the industrial temperature range of  
−40°C to +85°C. An evaluation board is available.  
The difference in the outputs of these squaring cells is  
integrated in a high gain error amplifier, generating a voltage at  
the VOUT pin with rail-to-rail capabilities. In a controller  
mode, this low noise output can be used to vary the gain of a  
host system’s RF amplifier, thus balancing the set point against  
Rev. B  
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.  
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.  
One Technology Way, P.O. Box 9106, Norwood, MA 02062-9106, U.S.A.  
Tel: 781.329.4700  
Fax: 781.326.8703  
www.analog.com  
© 2004 Analog Devices, Inc. All rights reserved.  
AD8362  
TABLE OF CONTENTS  
Specifications ................................................................................... 3  
Uncertainties in RIN and Power Calibration............................ 24  
Choosing the Right Value for CHPF and CLPF..................... 24  
Use of Nonstandard Target Voltages........................................ 24  
Adjusting the Intercept.............................................................. 25  
Altering the Slope....................................................................... 25  
Envelope Elimination Mode ..................................................... 26  
Operator in Controller Modes .................................................... 27  
Use of an Input Balun ................................................................ 27  
General Applications .................................................................... 29  
RMS Voltmeter with >100 dB Dynamic Range...................... 29  
RF Power Meter with 80 dB Range.......................................... 30  
High Slope Detectors Centered on a Narrow Window......... 31  
AD8362 Evaluation Board ........................................................ 32  
Outline Dimensions...................................................................... 34  
Ordering Guide .......................................................................... 34  
REVISION HISTORY  
Absolute Maximum Ratings .......................................................... 6  
ESD Caution.................................................................................. 6  
Pin Configuration and Function Description............................. 7  
Equivalent Circuits.......................................................................... 8  
Typical Performance Characteristics............................................ 9  
Characterization Setup .................................................................14  
Equipment ................................................................................... 14  
Analysis........................................................................................ 14  
Circuit Description........................................................................15  
Square-Law Detection ............................................................... 15  
Effect of Input Coupling on the Intercept Value.................... 16  
Offset Elimination...................................................................... 16  
Voltage vs. Power Calibration ................................................... 17  
Effect of Signal Waveform......................................................... 17  
Operation at Low Frequencies.................................................. 17  
Time-Domain Response of the Closed Loop ......................... 17  
Alteration of the Internal Target Voltage................................. 18  
Effects at Each End of Dynamic Range................................... 18  
Input Protection.......................................................................... 19  
Power-Enable Response Time .................................................. 19  
Using the AD8362.........................................................................20  
Basic Connections...................................................................... 20  
Main Modes of Operation............................................................21  
Operation in Measurement Modes.............................................22  
Law Conformance Error............................................................ 22  
Alternative Input Coupling Means .......................................... 23  
Using a Narrow-Band Input Match ......................................... 23  
3/04—Data Sheet Changed from Rev. A to Rev. B.  
Updated Format.................................................................Universal  
Changes to Specifications............................................................... 3  
Changes to the Offset Elimination Section................................ 16  
Changes to the Operation at Low Frequencies Section............ 17  
Changes to the Time-Domain Response of the Closed Loop  
Section............................................................................................. 17  
Changes to Equation 13................................................................ 24  
Changes to Table 5......................................................................... 31  
6/03—Data Sheet Changed from Rev. 0 to Rev. A.  
Updated Ordering Guide................................................................ 5  
Change to Analysis Section.......................................................... 12  
Updated AD8362 Evaluation Board Section ............................. 26  
2/03—Revision 0: Initial Version  
Rev. B | Page 2 of 36  
AD8362  
SPECIFICATIONS  
VS = 5 V, T = 25°C, ZO = 50 Ω, differential input drive via Balun1, VTGT connected to VREF, VOUT tied to VSET, unless otherwise noted.  
Table 1.  
Parameter  
Conditions  
Min  
Typ  
Max  
Unit  
OVERALL FUNCTION  
Maximum Input Frequency  
Input Power Range (Differential)  
2.7  
GHz  
dB Referred to 50 Ω Impedance Level,  
f ≤ 2.7 GHz, into 1:4 Balun1  
Nominal Low End of Range  
Nominal High End of Range  
Input Voltage Range (Differential)  
−52  
+8  
dBm  
dBm  
RMS Voltage at Input Terminals,  
f ≤ 2.7 GHz, into Input of the Device  
Nominal Low End of Range  
Nominal High End of Range  
Input Power Range (S-Sided)  
1.12  
1.12  
mV rms  
V rms  
Single-Ended Drive, CW Input, f ≤ 2.7 GHz,  
into Input Resistive Network2  
Nominal Low End of Range  
Nominal High End of Range  
Input Voltage Range (S-Sided)  
Nominal Low End of Range  
Nominal High End of Range  
Output Voltage Range  
Nominal Low End of Range  
Nominal High End of Range  
Output Scaling (Log Slope)  
Law Conformance Error  
RF INPUT INTERFACE  
−40  
0
dBm  
dBm  
RMS Voltage at Input Terminals, f ≤ 2.7 GHz  
2.23  
223  
mV rms  
V rms  
RL ≥ 200 Ω to Ground  
In General, VS – 0.1 V  
+100  
+4.9  
50  
mV  
V
mV/dB  
dB  
Over Central 60 dB Range, f ≤ 2.7 GHz  
Pins INHI, INLO, AC-Coupled  
Single-Ended Drive, wrt DECL  
Differential Drive  
0.5  
Input Resistance  
100  
200  
OUTPUT INTERFACE  
Available Output Range  
Absolute Voltage Range  
Nominal Low End of Range  
Nominal High End of Range  
Source/Sink Current  
Slew Rate Rising  
Pin VOUT  
RL ≥ 200 Ω to Ground  
0.1  
4.9  
V
Measurement Mode, f = 900 MHz, PIN = −52 dBm  
Measurement Mode, f = 900 MHz, PIN = +8 dBm  
VOUT Held at VS/2, to 1% Change  
CL = Open  
CL = Open  
0.2 V to 1.8 V, CLPF = 0  
1.8 V to 0.2 V, CLPF = 0  
CLPF = 1000 pF, fSPOT ≤ 100 kHz  
Pin VSET  
0.32  
3.44  
0.48  
3.52  
V
V
mA  
V/µs  
V/µs  
ns  
48  
60  
5
45  
0.4  
70  
Slew Rate Falling  
Rise Time, 10% to 90%  
Fall Time, 90% to 10%  
Wideband Noise  
µs  
nV/√Hz  
VSET INTERFACE  
Nominal Input Voltage Range  
Input Resistance  
To 1 dB Error  
0.5  
3.75  
V
kΩ  
68  
Scaling (Log Slope)  
Scaling (Log Intercept)  
f = 900 MHz  
f = 900 MHz, into 1:4 Balun  
46  
−64  
−77  
50  
−60  
−73  
54  
−56  
−69  
mV/dB  
dBm  
dBV  
VOLTAGE REFERENCE  
Output Voltage  
Pin VREF  
25°C  
−40°C ≤ TA ≤ +85°C  
1.225  
1.25  
0.08  
8
1.275  
V
Temperature Sensitivity3  
mV/°C  
Output Resistance  
Rev. B | Page 3 of 36  
 
AD8362  
Parameter  
Conditions  
Min  
Typ  
Max  
Unit  
RMS TARGET INTERFACE  
Nominal Input Voltage Range  
Input Bias Current  
Pin VTGT  
Measurement Range = 60 dB, to 1 dB Error  
VTGT = 1.25 V  
VTGT = 0 V  
0.625  
2.5  
V
−28  
−52  
52  
µA  
µA  
kΩ  
Incremental Input Resistance  
POWER-DOWN INTERFACE  
Logic Level to Enable  
Logic Level to Disable  
Input Current  
Pin PWDN  
Logic Low Enables  
Logic High Disables  
Logic High  
Logic Low  
From PWDN Low to VOUT within  
10% of Final Value, CLPF = 1000 pF  
1
V
V
µA  
µA  
ns  
3
230  
5
14.5  
Enable Time  
Disable Time  
From PWDN High to VOUT within  
10% of Final Value, CLPF = 1000 pF  
2.5  
µs  
POWER SUPPLY INTERFACE  
Supply Voltage  
Quiescent Current  
Supply Current  
Pin VPOS  
4.5  
5
20  
0.2  
5.5  
22  
V
mA  
mA  
When Disabled  
900 MHz  
Dynamic Range  
Error Referred to Best Fit Line (Linear Regression)  
1 dB Linearity, CW Input  
65  
62  
dB  
dB  
0.5 dB Linearity, CW Input  
Deviation vs. Temperature  
Deviation from Output at 25°C  
−40°C < TA < +85°C; PIN = −45 dBm  
−40°C < TA < +85°C; PIN = −20 dBm  
−40°C < TA < +85°C; PIN = +5 dBm  
−1.7  
−1.4  
−1  
dB  
dB  
dB  
Logarithmic Slope  
Logarithmic Intercept  
Deviation from CW Response  
46  
−64  
50  
−60  
0.2  
0.2  
0.5  
54  
−56  
mV/dB  
dBm  
dB  
dB  
dB  
5.5 dB Peak-to-RMS Ratio (IS95 Reverse Link)  
12 dB Peak-to-RMS Ratio (WCDMA 4 Channels)  
18 dB Peak-to-RMS Ratio (WCDMA 15 Channels)  
1.9 GHz  
Dynamic Range  
Error Referred to Best Fit Line (Linear Regression)  
1 dB Linearity, CW Input  
65  
62  
dB  
dB  
0.5 dB Linearity, CW Input  
Deviation vs. Temperature  
Deviation from Output at 25°C  
−40°C < TA < +85°C; PIN = −45 dBm  
−40°C < TA < +85°C; PIN = −20 dBm  
−40°C < TA < +85°C; PIN= +5 dBm  
−0.6  
−0.5  
−0.3  
51  
−59  
0.2  
dB  
dB  
dB  
mV/dB  
dBm  
dB  
dB  
dB  
Logarithmic Slope  
Logarithmic Intercept  
Deviation from CW Response  
5.5 dB Peak-to-RMS Ratio (IS95 Reverse Link)  
12 dB Peak-to-RMS Ratio (WCDMA 4 Channels)  
18 dB Peak-to-RMS Ratio (WCDMA 15 Channels)  
0.2  
0.5  
Rev. B | Page 4 of 36  
AD8362  
Parameter  
2.2 GHz  
Conditions  
Min  
Typ  
Max  
Unit  
Dynamic Range  
Error Referred to Best Fit Line (Linear Regression)  
±± dB Linearityꢀ ꢁC ꢂnꢃpt  
65  
65  
dB  
dB  
±ꢄ.5 dB Linearityꢀ ꢁC ꢂnꢃpt  
Deviation vs. Temꢃeratpre  
Deviation from Optꢃpt at 25°ꢁ  
−4ꢄ°ꢁ < TA < +85°ꢁ; PꢂN = −45 dBm  
−4ꢄ°ꢁ < TA < +85°ꢁ; PꢂN = −2ꢄ dBm  
−4ꢄ°ꢁ < TA < +85°ꢁ; PꢂN= +5 dBm  
−±.8  
−±.6  
−±.3  
5ꢄ.5  
−6±  
ꢄ.2  
dB  
dB  
dB  
mV/dB  
dBm  
dB  
dB  
dB  
Logarithmic Sloꢃe  
Logarithmic ꢂnterceꢃt  
Deviation from ꢁC Resꢃonse  
5.5 dB Peak-to-RMS Ratio (ꢂS95 Reverse Link)  
±2 dB Peak-to-RMS Ratio (CꢁDMA 4 ꢁhannels)  
±8 dB Peak-to-RMS Ratio (CꢁDMA ±5 ꢁhannels)  
ꢄ.2  
ꢄ.5  
2.7 GHz  
Dynamic Range  
Error Referred to Best Fit Line (Linear Regression)  
±± dB Linearityꢀ ꢁC ꢂnꢃpt  
63  
62  
dB  
dB  
±ꢄ.5 dB Linearityꢀ ꢁC ꢂnꢃpt  
Deviation vs. Temꢃeratpre  
Deviation from Optꢃpt at 25°ꢁ  
−4ꢄ°ꢁ < TA < +85°ꢁ; PꢂN = −4ꢄ dBm  
−4ꢄ°ꢁ < TA < +85°ꢁ; PꢂN = −±5 dBm  
−4ꢄ°ꢁ < TA < +85°ꢁ; PꢂN = +±5 dBm  
−5.3  
−5.5  
−4.8  
5ꢄ.5  
−58  
ꢄ.2  
dB  
dB  
dB  
mV/dB  
dBm  
dB  
dB  
dB  
Logarithmic Sloꢃe  
Logarithmic ꢂnterceꢃt  
Deviation from ꢁC Resꢃonse  
5.5 dB Peak-to-RMS Ratio (ꢂS95 Reverse Link)  
±2 dB Peak-to-RMS Ratio (CꢁDMA 4 ꢁhannels)  
±8 dB Peak-to-RMS Ratio (CꢁDMA ±5 ꢁhannels)  
ꢄ.2  
ꢄ.4  
± ±:4 balpn transformerꢀ M/A-ꢁOM ETꢁ ±.6-4-2-3.  
2 Resistive network consists of 33 Ω shpnt and 25 Ω series.  
3 See Figpre 36.  
Rev. B | Page 5 of 36  
 
AD8362  
ABSOLUTE MAXIMUM RATINGS  
Table 2.  
Parameters  
Ratings  
Stresses above those listed under Absolute Maximum Ratings  
may cause permanent 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.  
Supply Voltage VPOS  
Input Power (into Input of Device)  
Equivalent Voltage  
Internal Power Dissipation  
θJA  
Maximum Junction Temperature  
Operating Temperature Range  
Storage Temperature Range  
Lead Temperature Range (Soldering 60 sec)  
5.5 V  
13 dBm  
2 V rms  
500 mW  
125°C/W  
125°C/W  
−40°C to +85°C  
−65°C to +150°C  
300°C  
ESD 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 this product 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.  
Rev. B | Page 6 of 36  
AD8362  
PIN CONFIGURATION AND FUNCTION DESCRIPTION  
1
2
3
4
5
6
7
8
16  
15  
14  
13  
12  
11  
10  
9
COMM  
CHPF  
DECL  
INHI  
ACOM  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
ACOM  
CLPF  
AD8362  
TOP VIEW  
INLO  
(Not to Scale)  
DECL  
PWDN  
COMM  
Figure 2. Pin Configuration  
Table 3. Pin Function Descriptions  
Pin  
Equivalent  
Circuit  
No.  
1, 8  
2
Mnemonic Description  
COMM  
CHPF  
DECL  
Common Connection. Connect via low impedance to system common.  
Input HPF. Connect to common via a capacitor to determine 3 dB point of input signal high-pass filter.  
Decoupling Terminals for INHI and INLO. Connect to common via a large capacitance to complete  
input circuit.  
3, 6  
4
5
7
9
INHI  
High Signal Input Terminal. Part of a differential input port with INLO.  
Low Signal Input Terminal. Part of a differential input port with INHI.  
Disable/Enable Control Input. Apply logic high voltage to shut down the AD8362.  
Connection for loop filter integration (averaging) capacitor, the other pin of which is usually  
grounded via a resistor to improve loop stability and response time.  
Circuit A  
Circuit A  
INLO  
PWDN  
CLPF  
10, 16 ACOM  
Analog Common Connection for Output Amplifier.  
11  
VSET  
The voltage applied to this pin sets the decibel value of the required RF input voltage that results in  
zero current out of CLPF and thus the loop integrating capacitor.  
Output of Error Amplifier. In measurement mode, normally connected directly to VSET.  
Connect to 5 V Power Supply.  
The logarithmic intercept voltage is proportional to the voltage applied to this pin. The use of a lower  
target voltage increases the crest factor capacity.  
General-Purpose Reference Voltage Output of 1.25 V (usually connected only to VTGT).  
Circuit B  
Circuit C  
12  
13  
14  
VOUT  
VPOS  
VTGT  
Circuit D  
Circuit E  
15  
VREF  
Rev. B | Page 7 of 36  
AD8362  
EQUIVALENT CIRCUITS  
VPOS  
VSET  
VPOS  
VPOS  
DECL  
RAIL-TO-RAIL  
OUTPUT  
~35k  
~35kΩ  
0.7V  
COMM  
VOUT  
ACOM  
VSET  
INTERFACE  
2k  
INHI  
CLPF  
500Ω  
100  
ACOM  
COMM  
COMM  
VGA  
100Ω  
Figure 6. Circuit D  
Figure 4. Circuit B  
INLO  
VPOS  
SOURCE ONLY  
REF BUF  
VPOS  
VPOS  
COMM  
DECL  
~0.35V  
50kΩ  
50kΩ  
VOUT  
ACOM  
VTGT  
VTGT  
INTERFACE  
GAIN = 0.12  
Figure 3. Circuit A  
13kΩ  
5kΩ  
ACOM  
COMM  
COMM  
Figure 7. Circuit E  
Figure 5. Circuit C  
Rev. B | Page 8 of 36  
AD8362  
TYPICAL PERFORMANCE CHARACTERISTICS  
4.5  
4.0  
3.6  
3.0  
2.4  
100MHz  
4.0  
3.2  
2.8  
1.8  
1.2  
3.5  
3.0  
2.5  
2.0  
1.5  
1.0  
0.5  
0
2200MHz  
–40°C  
0.6  
0
2.4  
2.0  
1.6  
–0.6  
–1.2  
+85°C  
2700MHz  
+25°C  
–40°C  
1.2  
0.8  
0.4  
+25°C  
+85°C  
–1.8  
–2.4  
–3.0  
900MHz  
1900MHz  
0
–60 –55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
0
5
10 15  
–60 –55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
0
5
10 15  
INPUT AMPLITUDE (dBm)  
INPUT AMPLITUDE (dBm)  
Figure 8. Output Voltage (VOUT) vs. Input Amplitude (dBm),  
Frequencies 100 MHz, 900 MHz, 1900 MHz, 2200 MHz, 2700 MHz,  
Sine Wave, Differential Drive  
Figure 11. VOUT and Law Conformance vs. Input Amplitude, Frequency  
1900 MHz, Sine Wave, Temperature −40°C, +25°C, and +85°C  
3.0  
2.5  
2.0  
1.5  
4.0  
3.6  
3.0  
2.4  
3.2  
2.8  
1.8  
1.2  
–40°C  
1.0  
0.5  
100MHz  
0.6  
0
2.4  
2.0  
1.6  
0
–0.5  
–1.0  
–1.5  
–2.0  
–2.5  
–3.0  
+25°C  
+25°C  
–0.6  
–1.2  
2200MHz  
900MHz  
1900MHz  
1.2  
0.8  
0.4  
+85°C  
–40°C  
–1.8  
–2.4  
–3.0  
+85°C  
2700MHz  
0
–60  
–60 –55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10 15  
–10  
–50 –45 –40 –35 –30 –25 –20 –15  
–5  
0
5
10 15  
–55  
INPUT AMPLITUDE (dBm)  
Figure 9. Logarithmic Law Conformance vs. Input Amplitude  
Frequencies 100 MHz, 900 MHz, 1900 MHz, 2200 MHz, 2700 MHz,  
Sine Wave, Differential Drive  
Figure 12. VOUT and Law Conformance vs. Input Amplitude, Frequency  
2200 MHz, Sine Wave, Temperature −40°C, +25°C, and +85°C  
4.0  
3.0  
2.4  
4.0  
3.5  
3.6  
3.2  
2.8  
2.4  
2.0  
1.6  
1.2  
0.8  
0.4  
0
1.8  
1.2  
CW  
3.0  
–40°C  
2.5  
0.6  
IS95 REVERSE LINK  
+25°C  
WCDMA 8-CHANNEL  
2.0  
0
+85°C  
–40°C  
–0.6  
WCDMA 15-CHANNEL  
1.5  
1.0  
0.5  
0
–1.2  
–1.8  
–2.4  
+85°C  
+25°C  
–3.0  
–55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10 15  
–10  
–5  
–60 –55 –50 –45 –40 –35 –30 –25 –20 –15  
INPUT AMPLITUDE (dBm)  
0
5
10 15  
Figure 10. VOUT and Law Conformance vs. Input Amplitude, Frequency  
900 MHz, Sine Wave, Temperature −40°C, +25°C, and +85°C  
Figure 13. VOUT vs. Input Amplitude with Different Waveforms, CW, IS95  
Reverse Link, WCDMA 8-Channel, WCDM 15-Channel, Frequency 900 MHz  
Rev. B | Page 9 of 36  
 
 
AD8362  
3.0  
2.5  
3.0  
2.5  
WCDMA  
8-CHANNEL  
2.0  
2.0  
1.5  
1.5  
WCDMA 8-CHANNEL  
1.0  
1.0  
IS95 REVERSE LINK  
0.5  
0.5  
CW  
0
0
–0.5  
–1.0  
–1.5  
–2.0  
–2.5  
–3.0  
–0.5  
–1.0  
–1.5  
–2.0  
–2.5  
WCDMA 15-CHANNEL  
WCDMA  
15-CHANNEL  
–3.0  
–60  
–60 –55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10 15  
–55 –50 –45 –40 –35 –30 –25 –20 –15  
–5  
0
5
10 15  
–10  
INPUT AMPLITUDE (dBm)  
Figure 14. Output Error from CW Linear Reference vs. Input Amplitude  
with Different Waveforms, CW, IS95 Reverse Link, WCDMA 8-Channel,  
WCDMA 15-Channel, Frequency 900 MHz  
Figure 17. Output Error from CW Linear Reference vs. Input Amplitude,  
3 Sigma to Either Side of Mean, with WCDMA 8-Channel,  
15-Channel, Frequency 1900 MHz  
3.0  
2.5  
3.0  
2.5  
2.0  
1.5  
2.0  
WCDMA  
8-CHANNEL  
1.5  
WCDMA  
WCDMA  
1.0  
0.5  
1.0  
0.5  
4-CHANNEL  
8-CHANNEL  
0
0
–0.5  
–1.0  
–0.5  
–1.0  
–1.5  
–2.0  
–2.5  
–3.0  
WCDMA 15-CHANNEL  
–1.5  
WCDMA  
15-CHANNEL  
–2.0  
–2.5  
–3.0  
–60 –55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10 15  
–55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10  
Figure 15. Output Error from CW Linear Reference vs. Input Amplitude  
with Different WCDMA Channel Loading, 4-Channel, 8-Channel,  
15-Channel, Frequency 2200 MHz  
Figure 18. Output Error from CW Linear Reference vs. Input Amplitude,  
3 Sigma to Either Side of Mean, with WCDMA 8-Channel,  
WCDMA 15-Channel, Frequency 2200 MHz  
4.0  
3.5  
3.0  
2.5  
2.0  
1.5  
1.0  
0.5  
0
3.0  
2.5  
2.0  
WCDMA 8-CHANNEL  
1.5  
1.0  
0.5  
0
–0.5  
–1.0  
–1.5  
WCDMA 15-CHANNEL  
–2.0  
–2.5  
–3.0  
–60  
–55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10  
–55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10 15  
Figure 16. Output Error from CW Linear Reference vs. Input Amplitude,  
3 Sigma to Either Side of Mean, with WCDMA 8-Channel,  
WCDMA 15-Channel, Frequency 1900 MHz  
Figure 19. VOUT vs. Input Amplitude, 3 Sigma to Either Side of Mean,  
Sine Wave, Frequency 900 MHz, Part-to-Part Variation  
Rev. B | Page 10 of 36  
AD8362  
4.0  
3.5  
3.0  
2.5  
2.0  
1.5  
1.0  
0.5  
0
3.0  
2.5  
–40°C  
2.0  
1.5  
1.0  
0.5  
0
–0.5  
–1.0  
–1.5  
–2.0  
–2.5  
–3.0  
+85°C  
+25°C  
10  
–55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
–55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10  
Figure 20. VOUT vs. Input Amplitude, 3 Sigma to Either Side of Mean,  
Sine Wave, Frequency 1900 MHz, Part-to-Part Variation  
Figure 23. Logarithmic Law Conformance vs. Input Amplitude,  
3 Sigma to Either Side of Mean, Sine Wave, Frequency 2200 MHz,  
Temperature −40°C, +25°C, and +85°C  
3.0  
52.0  
–40°C  
2.5  
2.0  
1.5  
51.5  
51.0  
50.5  
50.0  
49.5  
49.0  
+85°C  
+25°C  
–40°C  
1.0  
0.5  
0
–0.5  
–1.0  
–1.5  
–2.0  
+85°C  
+25°C  
–2.5  
–3.0  
–55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10  
FREQUENCY (MHz)  
Figure 21. Logarithmic Law Conformance vs. Input Amplitude,  
3 Sigma to Either Side of Mean, Sine Wave, Frequency 900 MHz,  
Temperature −40°C, +25°C, and +85°C  
Figure 24. Logarithmic Slope vs. Frequency,  
Temperature −40°C, +25°C, and +85°C  
3.0  
–53  
–54  
–55  
–56  
–57  
–58  
–59  
–60  
–61  
–62  
–63  
–45°C  
2.5  
2.0  
+85°C  
1.5  
1.0  
0.5  
0
+25°C  
–0.5  
–1.0  
–1.5  
–2.0  
–2.5  
–3.0  
–40°C  
+25°C  
+85°C  
–55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10  
FREQUENCY (MHz)  
Figure 25. Logarithmic Intercept vs. Frequency,  
Temperature −40°C, +25°C, and +85°C  
Figure 22. Logarithmic Law Conformance vs. Input Amplitude,  
3 Sigma to Either Side of Mean, Sine Wave, Frequency 1900 MHz,  
Temperature −40°C, +25°C, and +85°C  
Rev. B | Page 11 of 36  
AD8362  
3.0  
2.5  
80  
70  
60  
50  
40  
30  
20  
900MHz  
2.0  
1.5  
1900MHz  
1.0  
0.5  
0
–0.5  
–1.0  
–1.5  
–2.0  
–2.5  
–3.0  
10  
0
2200MHz  
–61.0  
–60.5  
–60.0  
–59.5  
–59.0  
–58.5  
–58.0  
–40 –30 –20 –10  
0
10 20 30 40 50 60 70 80 90  
TEMPERATURE (°C)  
INTERCEPT (dBm)  
Figure 26. Change in Logarithmic Slope vs. Temperature, 3 Sigma to Either  
Side of Mean, Frequencies 900 MHz, 1900 MHz, 2200 MHz  
Figure 29. Logarithmic Intercept Distribution, Frequency 900 MHz  
2.0  
1.5  
1.0  
5.0  
6
4.5  
4.0  
3.5  
3.0  
2.5  
2.0  
1.5  
1.0  
0.5  
0
RF BURST  
ENABLE  
4
2V/DIV  
2
0
900MHz  
1900MHz  
+2dBm  
0.5  
0
–2  
–4  
–6  
–8  
–10  
–12  
–14  
VOUT  
–10dBm  
–20dBm  
–0.5  
–1.0  
–1.5  
–2.0  
–30dBm  
0.5V/DIV  
2200MHz  
–40 –30 –20 –10  
0
10 20 30 40 50 60 70 80 90  
TEMPERATURE (°C)  
0
2
4
6
8
10  
TIME (  
12  
14  
16  
18  
20  
µ
s)  
Figure 30. Output Response to RF Burst Input for Various  
RF Input Levels, Carrier Frequency 900 MHz, CLPF = 0.1 µF  
Figure 27. Change in Logarithmic Intercept vs. Temperature, 3 Sigma to  
Either Side of Mean, Frequencies 900 MHz, 1900 MHz, 2200 MHz  
5.0  
4.5  
4.0  
3.5  
3.0  
2.5  
2.0  
1.5  
1.0  
0.5  
0
6
100  
80  
60  
40  
20  
0
4
RF BURST  
2V/DIV  
ENABLE  
2
0
+2dBm  
–10dBm  
–2  
–4  
VOUT  
–20dBm  
–6  
–30dBm  
–8  
–10  
0.5V/DIV  
–12  
–14  
48  
49  
50  
51  
52  
53  
0
2
4
6
8
10  
12  
14  
16  
18  
20  
SLOPE (mV/dB)  
TIME (ms)  
Figure 31. Output Response to RF Burst Input for Various RF Input Levels,  
Carrier Frequency 900 MHz, CLPF = 0.1 µF  
Figure 28. Slope Distribution, Frequency 900 MHz  
Rev. B | Page 12 of 36  
 
 
AD8362  
90  
5.0  
4.5  
4.0  
3.5  
3.0  
2.5  
2.0  
1.5  
1.0  
0.5  
0
6
4
60  
120  
POWER-  
DOWN  
PIN  
2V/DIV  
2
0
150  
30  
+2dBm  
VOUT  
–2  
–4  
–6  
–8  
–10  
–12  
–14  
–10dBm  
–20dBm  
180  
0
0.5V/DIV  
–30dBm  
210  
330  
240  
300  
0
2
4
6
8
10  
TIME (µs)  
12  
14  
16  
18  
20  
270  
Figure 32. Output Response Using Power-Down Mode for Various RF Input  
Levels, Carrier Frequency 900 MHz, CLPF = 0  
Figure 35. Input Impedance, ZO = 50 Ω, Differential Drive  
5.0  
4.5  
4.0  
3.5  
3.0  
2.5  
2.0  
1.5  
1.0  
0.5  
0
6
5
0
4
2V/DIV  
2
0
–5  
+2dBm  
–2  
–4  
–6  
–8  
–10  
–12  
–14  
–10  
–15  
–20  
–25  
–30  
–10dBm  
–20dBm  
–30dBm  
0.5V/DIV  
0
2
4
6
8
10  
12  
14  
16  
18  
20  
–40 –30 –20 –10  
0
10 20 30 40 50 60 70 80 90  
TIME (ms)  
TEMPERATURE (°C)  
Figure 33. Output Response Using Power-Down Mode for Various RF Input  
Levels, Carrier Frequency 900 MHz, CLPF = 0.1 µF  
Figure 36. Change in VREF vs. Temperature, 3 Sigma to Either Side of Mean  
5.5  
5.0  
4.5  
4.0  
3.5  
3.0  
2.5  
2.0  
1.5  
1.0  
0
6
300  
250  
200  
150  
100  
50  
4
2V/DIV  
VPOS  
2
0
–2  
–4  
–6  
–8  
–10  
–12  
–14  
+2dBm  
1V/DIV  
–10dBm  
–20dBm  
–30dBm  
0
1.230  
1.235 1.240  
1.245 1.250  
VREF (V)  
1.255 1.260  
1.265 1.270  
0
2
4
6
8
10  
TIME (ms)  
12  
14  
16  
18  
20  
Figure 37. VREF Distribution  
Figure 34. Output Response to Gating on Power Supply for Various RF Input  
Levels, Carrier Frequency 900 MHz, CLPF = 0  
Rev. B | Page 13 of 36  
 
 
AD8362  
CHARACTERIZATION SETUP  
EQUIPMENT  
TEK TDS5104  
SCOPE  
AD8362  
The general hardware configuration used for most of the  
AD8362 characterization is shown in Figure 38. The signal  
source used was a Rohde & Schwarz SMIQ03B. A 1:4 balun  
transformer was used to transform the single-ended RF signal  
to differential form. For the response measurements in Figure  
30 and Figure 31, the configuration shown in Figure 39 was  
used; for Figure 32 and Figure 33, the configuration shown in  
Figure 40 was used; and for Figure 34, the configuration shown  
in Figure 41 was used.  
TEK P5050  
VOLTAGE PROBE  
COMM  
ACOM  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
ACOM  
CLPF  
CHPF  
DECL  
INHI  
C1  
HPE3631A  
POWER  
SUPPLY  
SMT03  
SIGNAL  
GENERATOR  
BALUN  
C2  
3dB  
INLO  
DECL  
PWDN  
COMM  
C3  
RF 50  
C4  
AD8362  
CHARACTERIZATION  
BOARD  
SMIQ03B  
RF SOURCE  
MULTIMETER  
HP34401A  
3dB  
RFIN  
VOUT  
Figure 39. Response Measurement Setup for Modulated Pulse  
TEK TDS5104  
AD8362  
SCOPE  
TEK P5050  
VOLTAGE PROBE  
COMM  
CHPF  
DECL  
INHI  
ACOM  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
ACOM  
CLPF  
PC  
CONTROLLER  
C1  
Figure 38. Primary Characterization Setup  
HPE3631A  
POWER  
SUPPLY  
SMT03  
SIGNAL  
BALUN  
C2  
3dB  
ANALYSIS  
GENERATOR  
INLO  
The slope and intercept are derived using the coefficients  
of a linear regression performed on data collected in its  
central operating range. Error is stated in two forms: error  
from linear response to CW waveform and output delta  
from 25°C performance.  
DECL  
PWDN  
COMM  
RF 50  
C3  
HP8112A  
PULSE  
GENERATOR  
C4  
The error from linear response to CW waveform is the  
decibel difference in output from the ideal output defined by  
the conversion gain and output reference. This is a measure of  
the linearity of the device response to both CW and modulated  
waveforms. The error in dB is calculated by  
Figure 40. Response Measurement Setup for Power-Down Step  
HP8112A  
PULSE  
AD811  
GENERATOR  
50  
732Ω  
VOUT Slope ×  
(
PIN PZ  
)
Error dB =  
( )  
Slope  
AD8362  
TEK TDS5104  
SCOPE  
where PZ is the x intercept, expressed in dBm.  
COMM  
ACOM  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
ACOM  
CLPF  
Error from the linear response to CW waveform is not a  
measure of absolute accuracy since it is calculated using the  
slope and intercept of each device. However, it verifies the  
linearity and the effect of modulation on the device response.  
Error from 25°C performance uses the performance of a given  
device and waveform type as the reference; it is predominantly a  
measurement of output variation with temperature.  
CHPF  
DECL  
INHI  
TEK P5050  
VOLTAGE  
PROBE  
C1  
0.01µF  
100pF  
BALUN  
C2  
3dB  
INLO  
DECL  
PWDN  
COMM  
C3  
SMT03  
SIGNAL  
GENERATOR  
C4  
RF 50Ω  
Figure 41. Response Measurement Setup for Gated Supply  
Rev. B | Page 14 of 36  
 
 
 
AD8362  
CIRCUIT DESCRIPTION  
The AD8362 is a fully calibrated, high accuracy, rms-to-dc  
converter providing a measurement range of over 60 dB. It is  
capable of operation from signals as low in frequency as a few  
Hertz to at least 2.7 GHz. Unlike earlier rms-to-dc converters,  
the response bandwidth is completely independent of the signal  
magnitude. The −3 dB point occurs at about 3.5 GHz. The  
capacity of this part to accurately measure waveforms having a  
high peak-to-rms ratio (crest factor) is independent of either  
the signal frequency or its absolute magnitude, over a wide  
range of conditions.  
shown how this basic range may be shifted either up or down,  
and even extended to >80 dB. The VGA gain has the form  
(
GSET = GO exp VSET VGNS  
)
(1)  
where GO is a basic fixed gain and VGNS is a scaling voltage that  
defines the gain slope (the dB change per volt). Note that the  
gain decreases with VSET. The VGA output is  
(
VSIG = GSETVIN = GOVIN exp VSET VGNS  
)
(2)  
where VIN is the ac voltage applied to the input terminals  
of the AD8362.  
This unique combination allows the AD8362 be to used with  
equal ease as a calibrated RF wattmeter covering a power ratio  
of >1,000,000:1, as a power controller in closed-loop systems, or  
as a general-purpose rms-responding voltmeter, and in many  
other low frequency applications.  
As is later explained more fully, the input drive may be  
either single-sided or differential but optimum performance at  
input drive. The effect of HF imbalances when using a single-  
sided drive is less apparent at low frequencies (from 50 Hz  
to 500 MHz), but the peak input voltage capacity is always  
halved relative to differential operation (see the Using the  
AD8362 section).  
AMPLITUDE TARGET  
FOR V  
–25dB TO +43dB  
SIG  
MATCH WIDE-  
BAND SQUARERS  
VTGT  
INHI  
2
2
X
VGA  
× 0.06  
V
X
TGT  
V
V
ATG  
SIG  
I
ACOM  
INLO  
SQUARE-LAW DETECTION  
I
SQU  
TGT  
The output of the variable-gain amplifier, VSIG, is  
G
SET  
CHPF  
applied to a wideband square law detector, which provides a  
true rms response to this alternating signal that is essentially  
independent of waveform up to crest factors of 6. Its output  
is a fluctuating current, ISQU, having a positive mean value. This  
current is integrated by an on-chip capacitance, CF; this is  
usually augmented by an external capacitance, CLPF, to extend  
the averaging time. The resulting voltage is buffered by a gain-  
of-5, dc-coupled amplifier whose rail-to-rail output, VOUT, may  
be used either for measurement or control purposes.  
OFFSET  
NULLING  
V
OUT  
C
F
OUTPUT  
FILTER  
VOUT  
V
SET  
SETPOINT  
VSET  
VREF  
INTERFACE  
CLPF  
INTERNAL RESISTORS  
SET BUFFER GAIN TO 5  
V
REF  
BAND GAP  
REFERENCE  
1.25V  
C
LPF  
EXTERNAL  
In most applications, the AGC loop is closed via the setpoint  
interface pin, VSET, to which the VGA gain-control voltage  
VSET is applied. In measurement modes, the closure is direct  
and local by a simple connection from the output the VOUT  
pin to the VSET pin. In controller modes, the feedback path is  
around some larger system, but the operation is the same.  
ACOM  
Figure 42. Basic Structure of the AD8362  
The part comprises the core elements of a high performance  
AGC loop (Figure 42), laser-trimmed during manufacture to  
close tolerances while fully operational at a test frequency of  
100 MHz. Its linear, wideband, variable gain amplifier (VGA)  
provides a general voltage gain, GSET; this may be controlled in a  
precisely exponential (linear-in-dB) manner over the full 68 dB  
range from −25 dB to +43 dB by a voltage VSET. However, to  
provide adequate guard-banding, only the central 60 dB of this  
range, from −21 dB to +39 dB, is normally used. Later, it is  
The fluctuating current, ISQU, is balanced against a fixed setpoint  
target current, ITGT, using current mode subtraction. With the  
exact integration provided by the capacitor(s), the AGC loop  
equilibrates when  
MEAN  
(
ISQU  
)
= ITGT  
(3)  
The current ITGT is provided by a second-reference squaring  
cell whose input is the amplitude-target voltage VATG. This is a  
fraction of the voltage VTGT applied to a special interface that  
accepts this input at the VTGT pin. Since the two squaring cells  
are electrically identical and are carefully implemented in the  
IC, process and temperature-dependent variations in the  
detailed behavior of the two square-law functions cancel.  
Rev. B | Page 15 of 36  
 
AD8362  
4.0  
3.5  
3.0  
2.5  
2.0  
1.5  
1.0  
0.5  
Accordingly, VTGT (and its fractional part VATG) determines the  
output that must be provided by the VGA for the AGC loop to  
settle. Since the scaling parameters of the two squarers are  
accurately matched, it follows that Equation 3 is satisfied only  
when  
2
2
MEAN  
(
VSIG  
)
= VATG  
(4)  
In a formal solution, one would then extract the square root of  
both sides to provide an explicit value for the root-mean-square  
(rms) value. However, it is apparent that by forcing this identity,  
through varying the VGA gain and extracting the mean value  
by the filter provided by the capacitor(s), the system inherently  
establishes the relationship  
0
100µV  
1mV  
10mV  
100mV  
1V  
10V  
RMS INPUT VOLTAGE (100µV TO 3.2V)  
Figure 43. Ideal Response of the AD8362  
rms  
(
VSIG  
)
=VATG  
(5)  
EFFECT OF INPUT COUPLING ON THE INTERCEPT  
VALUE  
Substituting the value of VSIG from Equation 2, we have  
Reductions of VIN due to coupling losses directly affect VZ. In  
high frequency applications, several factors contribute to the  
coupling of the source into the IC, including the board and  
package resonances and attenuation. Any uncertainties in the  
input impedance result in the intercept expressed in power  
terms, which is nominally −57 dBm for a 50 Ω system, being  
less accurately determined than when stated in dBV (that is, in  
pure voltage) terms. On the other hand, the slope VSLP is  
unaffected by all such impedance or coupling uncertainties.  
rms  
[
GOVIN exp  
(
VSET VGNS  
)
]
=VATG  
(6)  
As a measurement device, VIN is the unknown quantity and all  
other parameters can be fixed by design. Solving Equation 6:  
rms  
[
GOVIN VATG  
]
= exp  
(
VSET VGNS  
)
(7)  
so  
VSET =VGNS log  
[
rms  
(VIN  
)
VZ  
]
(8)  
OFFSET ELIMINATION  
The quantity VZ = VATG/GO is defined as the intercept voltage  
because VSET must be 0 when rms (VIN) = VZ.  
To address the small dc offsets that arise in the variable gain  
amplifier, an offset-nulling loop is used. The high-pass corner  
frequency of this loop is internally preset to 1 MHz, sufficiently  
low for most HF applications. When using the AD8362 in LF  
applications, the corner frequency can be reduced as needed by  
the addition of a capacitor from the CHPF pin to ground having  
a nominal value of 200 µF/Hz. For example, to lower the high-  
pass corner frequency to 150 Hz, a capacitance of 1.33 µF is  
required. The offset voltage varies depending on the actual gain  
at which the VGA is operating, and thus, on the input signal  
amplitude.  
When connected as a measurement device, the output of the  
buffer is tied directly to VSET, which closes the AGC loop.  
Making the substitution VOUT = VSET and changing the log  
base to 10, as needed in a decibel conversion, we have  
VOUT =VSLP log10  
[
rms  
(VIN  
)
VZ  
]
(9)  
where VSLP is the slope voltage, that is, the change in output  
voltage for each decade of change in the input amplitude.  
(Note that VSLP = VGNS log (10) = 2.303 VGNS). In the AD8362,  
V
SLP is laser trimmed to 1 V using a 100 MHz test signal.  
Baseline variations of this sort are a common aspect of all  
VGAs, although more evident in the AD8362 because of the  
method of its implementation, which causes the offsets to  
ripple along the gain axis with a period of 6.33 dB. When an  
excessively large value of CHPF is used, the offset correction  
process may lag the more rapid changes in the VGA’s gain,  
which may increase the time required for the loop to fully settle  
for a given steady input amplitude.  
Because a decade corresponds to 20 dB, this slope may also be  
stated as 50 mV/dB. It is later shown how the effective value of  
VSLP may be altered by the user.  
Likewise, the intercept VZ is also laser trimmed to 316 µV  
(−70 dBV). In an ideal system, VOUT would cross zero for an  
rms input of that value. In a single-supply realization of the  
function, VOUT cannot run fully down to ground; here, VZ is  
the extrapolated value. In measurement modes, the output  
ranges from 0.5 V for VIN = 1 mV (input values are stated as  
rms, outputs values as dc), up to a voltage 60 dB × 50 mV/dB =  
3 V above this for VIN = 1 V, that is, to 3.5 V. Figure 43 shows the  
ideal form of Equation 9 scaled as in the AD8362.  
Rev. B | Page 16 of 36  
 
AD8362  
In such cases, the input coupling capacitors should be large  
VOLTAGE VS. POWER CALIBRATION  
enough so that the lowest frequency components of the signal  
that are to be included in the measurement are minimally  
attenuated. For example, for a 3 dB reduction at 1.5 kHz,  
capacitances of 1 µF are needed because the input resistance is  
100 Ω at each input pin (200 Ω differentially) and we calculate  
1/(2π × 1.5 kΩ × 100) = 1 µF. Also, to lower the high-pass  
corner frequency of the VGA, a capacitor of value 200 µF-Hz  
should be used between the CHPF pin and ground; to provide a  
similar 1.5 kHz high-pass corner, a capacitor of 133 nF should  
be used.  
The AD8362 can be used as an accurate rms voltmeter  
from arbitrarily low frequencies to microwave frequencies.  
For low frequency operation, the input is usually specified  
either in volts rms or in dBV (decibels relative to 1 V rms).  
Driven differentially, the specified input range in dBV runs  
from −60 dBV to 0 dBV (1 mV to 1 V rms). In these terms,  
the intercept is at −70 dBV.  
At high frequencies, signal levels are commonly specified  
in power terms. In these circumstances, the source and  
termination impedances are an essential part of the overall  
scaling. To set the AD8362s input impedance to 50 Ω, it is  
necessary to add a resistor of 66.7 Ω across the internal 200 Ω  
differential input impedance of the IC. (This is discussed  
further in later sections.) For this condition, the intercept  
occurs at a nominal power level of −57 dBm, and VOUT  
can be stated in this way:  
TIME-DOMAIN RESPONSE OF THE CLOSED LOOP  
The external low-pass averaging capacitance, CLPF, added at  
the output of the squaring cell, is chosen to provide adequate  
filtering of the fluctuating detected signal. The optimum value  
depends on the application; as a guideline, a value of roughly  
900 µF-Hz should be used. For example, a capacitance of 5 µF  
provides adequate filtering down to 180 Hz. Note that the  
fluctuation in the quasi-dc output of a squaring cell operating  
on a sine wave input is a raised cosine at twice the signal  
frequency, easing this filtering function.  
VOUT =  
(
PIN + 57  
)
× 50 mV dB  
(10)  
where PIN is expressed in dBm. For example, an input of  
−30 dBm generates an output of 1.35 V.  
In the standard connections for the measurement mode,  
the VSET pin is tied to VOUT. For small changes in input  
amplitude (a few decibels), the time-domain response of this  
loop is essentially linear, with a 3 dB low-pass corner frequency  
of nominally fLP = 1/(CLPF × 1.1 kΩ). Internal time delays  
around this local loop set the minimum recommended value of  
this capacitor to about 300 pF, giving fLP = 3 MHz.  
EFFECT OF SIGNAL WAVEFORM  
The measurement accuracy of an rms-responding device is  
ideally unaffected by the waveform of the input signal. This is a  
valuable asset in wideband CDMA systems and in many other  
modulation modes where there is a significant amount of  
random variation of the RF carrier amplitude at baseband  
frequencies. The high accuracy of the AD8362 in such cases is  
indicated by the Typical Performance Characteristics graphs  
and in the Specifications table. Note that at low frequencies, it is  
customary to provide a specification of measurement errors due  
to waveform effects as a function of the crest factor (σ) rather  
than in terms of a system-specific modulation mode.  
When large and abrupt changes of input amplitude occur,  
the loop response becomes nonlinear and exhibits slew rate  
limitations. Further, due to the fundamentals of a system using  
transconductance squaring cells as employed in the AD8362,  
the slewing is asymmetric for increasing and decreasing inputs.  
Figure 44 shows typical waveforms for VOUT for three values  
of VIN using CLPF = 1 nF.  
When measuring signals whose waveforms have high but  
brief peak values (that is, having high crest factors), these  
peaks may be clipped, causing a reduction in the apparent value  
of the input being measured. This issue is discussed further in  
connection with the detailed description of the input system.  
3.0  
2.8  
2.6  
2.4  
2.2  
2.0  
1.8  
1.6  
OPERATION AT LOW FREQUENCIES  
In conventional rms-to-dc converters based on junction  
techniques, the effective signal bandwidth is proportional to the  
signal amplitude. For a 1 MHz rms-to-dc converter, this is the  
full-scale bandwidth. However, at an input 60 dB below full-  
scale, the bandwidth could be as low as 1 kHz. In sharp contrast,  
the 3.5 GHz bandwidth of the VGA in the AD8362 is  
independent of its gain. Since this amplifier is internally dc-  
coupled, the system can also be used as a high accuracy rms  
voltmeter at low frequencies, retaining its temperature-stable  
decibel-scaled output, for example, in seismic, audio, and sonar  
instrumentation.  
1.4  
1.2  
1.0  
0.8  
0.6  
0.4  
0.2  
0
8
16 24 32 40 48 56 64 72 80 88 96  
0
TIME (µs)  
Figure 44. Typical Large-Scale Response  
Rev. B | Page 17 of 36  
 
AD8362  
3.7  
3.2  
2.7  
2.2  
1.7  
1.2  
0.7  
0.2  
10  
The most satisfactory way to quantify slew-rate limitations is by  
considering the peak currents that can be generated by the  
squaring cells. During a fast increase in input level, the peak  
current into the integrating (loop filter) capacitance, CLPF, is  
approximately 2.5 mA. The actual value depends on several  
factors, including the size of the step, and extremes in chip  
temperature. The voltage across the 1 nF capacitor thus  
increases at a rate of nominally 2.5 V/µs. Because the output  
buffer has a gain of 5, the output slew rate is 12.5 V/µs. The peak  
rate persists up to a point about 10 dB below the final value,  
after which the response gradually converges on the linear  
system response, as noted previously.  
VTGT = 300mV  
5
0
VTGT = 533mV  
VTGT = 949mV  
VTGT = 1.69V  
VTGT = 3.0V  
10m  
–5  
–10  
100µ  
1m  
0.1  
1
10  
On the other hand, during a fast decrease in input level, the  
peak current in CLPF in the opposite (discharging) direction is  
much smaller; it is roughly 25 µA. Thus, the slew rate for VOUT  
in the descending direction is only about 0.125 V/µs for CLPF =  
1 nF. Discharging over the full 3 V range (a 60 dB reduction of  
input) requires a time interval of ~24 µs. These figures are  
verified in the results shown in Figure 44.  
RMS INPUT VOLTAGE (V)  
Figure 45. Response with VTGT Varied from 0.3 V to 3 V in 5 dB Steps,  
Showing the Proportional Shift in Intercept  
EFFECTS AT EACH END OF DYNAMIC RANGE  
All AGC loops have a limited minimum and maximum input  
beyond which the system cannot respond correctly. However,  
the output of a well-behaved system is in error in such a way as  
to avoid anomalous measurements. For an input below its  
minimum capability, the output should not turn around to  
falsely indicate a higher input value; for inputs above its  
maximum capability, the output should not fold over and return  
to some lower value.  
ALTERATION OF THE INTERNAL TARGET VOLTAGE  
The AD8362 incorporates several features that extend its  
versatility. One of these is the ability to alter the target  
voltage. As noted, the output of the VGA is forced to a  
value set by the internal bias voltage (VATG = 0.06 × VTGT)  
applied to the reference squaring cell. It is normally set to 75  
mV dc by connecting VTGT to the 1.25 V reference voltage at  
the VREF pin. However, it may optionally be varied from 0 V  
up to 0.24 V ( 4 V at VTGT). Note that the sign of this input  
is unimportant, because it is internally squared.  
The actual behavior of the AD8362 under these conditions can  
be seen in the set of plots in Figure 45, the lower panel of which  
shows the deviation from the ideal response with a slope of  
50 mV/dB. For inputs below a certain level corresponding to the  
point at which the VGA is operating at its maximum gain, its  
output can no longer meet the rms amplitude target set by  
VTGT, so the output moves quickly to its minimum value in an  
attempt to provide the needed extra gain. As VTGT is altered,  
the corresponding end-limit voltage moves to the left or to the  
right.  
By lowering VATG, the output of the VGA needed to balance the  
output currents of the two matched squaring cells is similarly  
lowered. This reduces the intercept in precisely the same ratio.  
Thus, if we halve the setpoint target voltage by halving the  
voltage applied to the VTGT pin, the intercept moves to the left  
(to a smaller input level) by 6.02 dB. This effectively doubles the  
measurement system’s sensitivity.  
On the other hand, when the input is above a certain upper  
limit where the VGA gain has been driven to its minimum  
gain, any further increase drives its output well above the target  
voltage needed to balance the loop. The resulting integration of  
this internal error signal causes VOUT to rise abruptly. In either  
case, this output takes on a safe value and does not fold back  
under any conditions.  
Furthermore, because the signal amplitude needed to drive the  
squaring cell is halved, the output stage of the VGA now has  
twice the dynamic headroom (before clipping) and can handle  
waveforms having crest factors that are twice as large. Figure 45  
shows the overall response for an illustrative set of values of  
VTGT = 0.3 V, 0.533 V, 0.949 V, 1.687 V, and 3.0 V. While this is  
usually a fixed dc voltage, it can also be a time-varying, unipolar  
or bipolar voltage, in which case the overall operation is rather  
more complex. For example, when VTGT is derived from  
VOUT, the dynamic range can be extended to over 80 dB.  
Examples of such uses of this feature are presented later.  
The dynamic range, the “dB distance” between these limits, is  
not basically dependent on VTGT. The middle line in the plots  
of Figure 45 (VTGT = 0.949 V) extends from 0.5 mV to 1.5 V  
between the 1% error points; the dynamic range is thus  
slightly over 68 dB. For other values of VTGT, this basic 68 dB  
range just moves to the left or to the right.  
Rev. B | Page 18 of 36  
 
AD8362  
VPOS  
An unavoidable consequence of this method is that the diodes  
will forward-conduct when the input amplitude is sufficient.  
This is not an all-or-nothing effect, of course; they shunt the  
input progressively as the signal increases. This conduction is  
strongest at high temperatures when the forward drop voltage  
of these diodes is lowest. The overall consequence is that high  
amplitude peaks are clamped to a greater or lesser degree. This  
affects the measurement accuracy at the top extreme of the  
dynamic range whenever the signal waveform has a high crest  
factor. These effects are, of course, included in the overall  
performance specifications.  
DECL  
COMM  
INHI  
VGA  
VIN  
INLO  
POWER-ENABLE RESPONSE TIME  
COMM  
The operating and standby currents for the AD8362 at 27°C  
are 24 mA and 275 µA, respectively. The power-down mode  
is activated by a logic high on the PWDN pin. When the  
shutdown feature is used, the normal operating conditions  
are restored relatively quickly when this pin is taken low.  
DECL  
VPOS  
Figure 46. Input Protection at INHI and INLO Pins  
INPUT PROTECTION  
Figure 47 shows typical response times for a midscale signal  
(VIN = 50 mV). The output rises to within 0.1 dB of its steady-  
state value in about 20 µs; the reference voltage is available to  
full accuracy in a much shorter time. This wake-up response  
varies in detail depending on the input coupling means and the  
capacitances CDEC, CHPF, and CLPF. These results are for a  
measurement system operating in the 0.8 GHz to 2 GHz range,  
balun coupled at the input port, with CDEC = 1 nF, CHPF = 0,  
and CLPF = 1 nF.  
Like all robust ICs, the AD8362 requires input protection  
against high voltage transients at the input (ESD). However, the  
techniques normally used for this purpose, based on breakdown  
diodes from the input pins INHI and INLO to the supply pins  
VPOS and COMM, cannot be used here because this raises the  
risk of excessive signal coupling to internal nodes at the upper  
end of the frequency range due to feedthrough in the  
capacitances of these diodes. Package inductances cause all  
internal nodes, including the supply and common lines, to have  
a significant impedance back to the external ground plane; even  
small disturbances on these nodes can cause anomalous  
operation.  
24.00mA  
10.00mA  
This risk is particularly evident because the main amplifier  
in the AD8362s VGA (an advanced X-AMP®) operates at full  
gain under all conditions, while the signal input is variably  
attenuated. Because this attenuation may be as high as 70 dB,  
very small feedthrough effects in the 0.5 GHz to 3 GHz range  
can have a pronounced impact on measurement accuracy.  
1.00mA  
0.27mA  
0.10mA  
2.20V  
OUTPUT VOLTAGE  
1dB  
2.19V  
2.18V  
1.26V  
REFERENCE VOLTAGE  
Figure 46 shows the protection method used. The multiple  
diodes arranged in back-to-back pairs limit the voltage swing  
on the input pins by clamping to the two DECL pins, which  
form a common ac low impedance node for the attenuators,  
independently grounded via two external capacitors. The HF  
currents in the capacitances of these diodes are thus shunted  
directly to a signal null point.  
1.25V  
1.24V  
0
10  
20  
30  
40  
TIME (µs)  
Figure 47. Typical Wake-Up Response; t0 = 10 µs  
Rev. B | Page 19 of 36  
 
 
AD8362  
USING THE AD8362  
V
S
The AD8362 requires a single supply of nominally 5 V; its  
performance is essentially unaffected by variations of up to  
10%, the range over which the stated specifications apply.  
Supplies as low as 2.7 V may be used with some loss of  
performance at high inputs and at temperature extremes.  
+5V nom, @ 24mA  
AD8362  
3.3Ω  
1
2
3
4
COMM ACOM 16  
CHPF  
VREF 15  
C
C
DEC  
0.1µF  
14  
DECL  
INHI  
VTGT  
DEC  
1nF  
V
VPOS 13  
VOUT 12  
SIGNAL INPUT  
Z = 2 × 100Ω  
The AD8362 is disabled by a logic high on the PWDN pin,  
which may be directly grounded for continuous operation,  
when the supply current at 27°C is nominally 24 mA and  
essentially independent of supply voltage. When powered  
down by a logic low on PWDN, the supply current is reduced  
to about 275 µA.  
C
CPL  
5
6
INLO  
DECL  
1mV – 1V rms  
OUT  
11  
VSET  
C
DEC  
LOGIC HIGH FOR  
POWER-DOWN  
7
8
PWDN ACOM 10  
COMM CLPF  
9
C
LPF  
Figure 48. Basic Measurement Mode Connections  
BASIC CONNECTIONS  
The supply is connected to the VPOS pin using the decoupling  
network shown in Figure 48, whose capacitors must provide a  
low impedance over the full frequency range of the input, and  
should be placed as close as possible to the VPOS pin. Two  
different capacitors are used in parallel to reduce the overall  
impedance since these have different resonant frequencies.  
However, the measurement accuracy is not critically dependent  
on supply decoupling because the high frequency signal path is  
confined to the relevant input pins. It is more important that the  
lead lengths to INHI and INLO, and in the decoupling  
capacitors from both of the DECL pins to ground, and the  
connections from COMM to the ground plane all use the  
shortest possible connections.  
Rev. B | Page 20 of 36  
 
AD8362  
MAIN MODES OF OPERATION  
V
S
Both measurement and controller modes are supported by the  
AD8362. Typical connections for the measurement mode,  
which may also be viewed as the rms voltmeter mode, are also  
illustrated in Figure 48. The output, VOUT, is proportional to  
the logarithm of the rms magnitude of the input signal (that is,  
a linear-on-dB response). When used in an accurately known  
system impedance (but only then), the output is a scaled decibel  
measurement of the power represented by the input voltage.  
+5V nom, @ 24mA  
AD8362  
NO CONNECTION  
FOR f >10MHz  
3.3  
1
2
3
4
5
6
7
8
COMM ACOM 16  
NC  
CHPF  
DECL  
INHI  
VREF 15  
VTGT 14  
VPOS 13  
VOUT 12  
VSET 11  
0.1µF  
1nF  
1nF  
V
SIGNAL INPUT  
Z = 2 × 100Ω  
1mV – 1V rms  
C
CPL  
RAIL-TO-RAIL  
OUT  
INLO  
DECL  
CONTROL OUTPUT  
SETPOINT INPUT  
0V–3.5V  
1nF  
PWDN ACOM 10  
COMM CLPF  
The choice of the capacitances CCPL, CDEC, CHPF, and CLPF  
depends on the lowest frequency to be included in the  
measurement spectrum. The default values shown support  
operation down to 100 Hz. Using a large enough value of CLPF  
(10 µF) to ensure sufficient filtering at this low input frequency,  
the response time is approximately 20 ms over most of the  
dynamic range. In high frequency applications, this capacitor is  
much smaller and is usually chosen to minimize the response  
time, consistent with well-behaved, large-signal behavior. In this  
figure, CHPF is also shown as 10 µF, to lower the high-pass  
corner to about 90 Hz. However, no capacitor will be needed  
here in most HF applications since the internally set high-pass  
corner is at about 2 MHz.  
THIS CONNECTION  
SETS CHIP-ENABLE  
9
300pF  
Figure 49. Basic Controller Mode Connections  
Controller mode operation is more closely analogous to that of  
a classical proportional/integral/derivative (PID) loop. The  
error corresponding to the decibel deviation from the setpoint  
is integrated by current into a capacitor (the sum of the internal  
and external capacitance CLPF) until such deviation is nulled.  
This action provides the fundamental proportional part of the  
loop response (although VOUT has decibel scaling). The Q of  
this system can be adjusted to minimize the loop response time  
by including a resistor in series with CLPF, generating a  
transmission zero, which provides the derivative term of a  
standard PID loop.  
Comparing the controller mode illustrated in Figure 49, the  
AD8362 is used here to monitor the output of a variable gain  
(or variable output power) signal processing element, frequently  
a power amplifier, and adjust its output to a desired target value  
(the setpoint) under the control of VSET. In this mode, its  
function is somewhat like an RF comparator. With the path  
from VOUT to VSET broken, any input larger than the  
corresponding setpoint causes VOUT to rail to its maximum  
value (which might loosely be viewed as a logic high). For  
inputs smaller than the setpoint, the controllers output falls to a  
near-ground level (logic low). Using the AD8362 simply as a  
threshold detector, this viewpoint may be useful, but in most  
applications, it is an oversimplification. The AD8362 invariably  
operates with the control loop closed, either locally with VOUT  
connected to VSET (as in measurement mode), or globally via  
some external nonlinear element (as in controller mode).  
As a simple example, assume that the AD8362 operates at an  
input power level of −20 dBm re: 50 Ω. Connected in the  
measurement mode, it generates a VOUT of 2.00 V, because this  
input is +40 dB above the intercept at −60 dBm and is scaled to  
50 mV/dB. Rearranged to the controller mode with exactly this  
voltage now externally applied to the VSET pin, the loop forces  
VOUT to the control voltage required by the gain element to  
provide a power sample of −20 dBm.  
Of course, any control loop of this sort operates correctly  
only if VSET corresponds to a power level (or a small sample of  
such) that can actually be provided by the external gain element.  
When this is a power amplifier, including the required amount  
of RF attenuation ensures this condition. In certain instrument-  
ation situations, it may be necessary to provide some low noise  
gain ahead of the AD8362s input.  
These two primary modes of use are discussed in more detail,  
with emphasis on practical considerations.  
Rev. B | Page 21 of 36  
 
AD8362  
OPERATION IN MEASUREMENT MODES  
Figure 50 shows the general connections for operating the  
AD8362 as an RF power detector, more correctly viewed  
as an accurate measurement system. The full performance  
potential of this part, particularly at very high frequencies  
(above 500 MHz), is realized only when the input is presented  
to the AD8362 in differential (balanced) form. In this example, a  
flux-coupled transformer is used at the input. Having a 1:4  
impedance ratio (1:2 turns ratio), the 200 Ω differential input  
resistance of the AD8362 becomes 50 Ω at the input to the  
transformer, whose outputs can be connected directly to INHI  
and INLO. If a center-tapped transformer is used, connect the  
tap to the DECL pins, which are biased to the same potential as  
the inputs (~3.6 V). Over the 0.9 GHz to 2.2 GHz range, a  
transmission line transformer (balun) may be used, as explained  
later. (The evaluation board is supplied with a M/A-COM  
ETC1.6-4-2-3, 0.5 GHz to 2.5 GHz, 4:1 balun.)  
LAW CONFORMANCE ERROR  
In practice, the response deviates slightly from the ideal straight  
line suggested by Equation 11. This deviation is called the law  
conformance error. In defining the performance of high  
accuracy measurement devices, it is customary to provide plots  
of this error. In general terms, it is computed by extracting the  
best straight line to the measured data using linear regression  
over a substantial region of the dynamic range and under  
clearly specified conditions.  
3.0  
3.8  
3.5  
2.5  
2.0  
1.5  
1.0  
0.5  
–40°C  
3.2  
2.9  
2.6  
2.3  
0
2.0  
1.7  
1.4  
1.1  
0.8  
0.5  
0.2  
V
S
–0.5  
–1.0  
–1.5  
–2.0  
–2.5  
–3.0  
+25°C  
+5V nom, @ 24mA  
+85°C  
AD8362  
–40°C  
1:4 Z-RATIO  
(1:2 TURNS RATIO)  
3.3  
1
2
3
4
5
6
7
8
COMM ACOM 16  
+25°C  
+85°C  
NC  
CHPF  
DECL  
INHI  
VREF 15  
VTGT 14  
VPOS 13  
0.1µF  
SIGNAL INPUT  
Z = 50Ω  
1nF  
1nF  
–60 –55 –50 –45 –40 –35 –30 –25 –20 –15 –10 –5  
INPUT AMPLITUDE (dBm)  
0
5
10 15  
200Ω  
12  
INLO  
DECL  
VOUT  
V
RAIL-TO-RAIL  
OUT  
CONTROL OUTPUT  
VSET 11  
Figure 51. Output Voltage and Law Conformance Error,  
at TA = −40°C, +25°C, and +85°C  
1nF  
PWDN ACOM 10  
COMM CLPF  
9
Figure 51 shows the output of the circuit of Figure 50 over the  
full input range. The agreement with the ideal function (law  
conformance) is also shown. This was determined by linear  
regression on the data points over the central portion of the  
transfer function (35 mV to 250 mV rms) for the 25°C data.  
The error at +25°C, −40°C, and +85°C was then calculated by  
subtracting the ideal output voltage at each input signal level  
from the actual output and dividing this quantity by the mean  
slope of the regression equation to provide a measurement of  
the error in decibels (scaled on the right-hand axis of Figure 51).  
300pF  
Figure 50. Connections for RF Power Measurement  
The output in this mode of use is a continuous, decibel-scaled  
voltage ranging from about 0.5 V to 3.5 V.  
VOUT =  
(
PIN PZ  
)
× 50 mV dB  
(11)  
The equivalent input power, PIN, is expressed in dBm (decibels  
above 1 mW) in a particular system impedance, which in this  
case is 50 Ω. The intercept, PZ, is that input power for which  
the back-extrapolated output crosses zero. Expressed as a  
voltage, it is 0.447 mV rms (−67 dBV, laser-calibrated at  
100 MHz), corresponding to a PZ of −60 dBm in 200 Ω.  
However, the 1:2 turns ratio of the transformer halves the  
required input voltage, which moves the intercept down by  
6 dB to 0.224 mV rms (−73 dBV) at the transformers input.  
The error curves generated in this way reveal not only the  
deviations from the ideal transfer function at a nominal  
temperature but also all of the additional errors caused by  
temperature changes. Notice there is a small temperature  
dependence in the intercept (the vertical position of the error  
plots); this variation is within 0.5 dB at high powers.  
Figure 51 further reveals that there is a periodic ripple in the  
conformance curves. This is due to the interpolation technique  
used to select the signals from the attenuator, not only at  
discrete tap points, but anywhere in between, thus providing  
continuous attenuation values. The selected signal is then  
applied to the 3.5 GHz, 40 dB fixed gain amplifier in the  
remaining stages of the AD8362s VGA.  
Impedance mismatches and attenuation in the coupling  
elements significantly affect the intercept position. This error  
is stable over temperature and time, and thus can be removed  
during calibration in a specific system. The logarithmic slope of  
50 mV/dB varies only slightly with frequency; corrected values  
for several common frequencies are provided in the  
Specifications section.  
Rev. B | Page 22 of 36  
 
 
AD8362  
An approximate schematic of the signal input section of the  
AD8362 is shown in Figure 52. The ladder attenuator is  
composed of 11 sections (12 taps), each of which progressively  
attenuates the input signal by 6.33 dB. Each tap is connected to  
a variable transconductance cell whose bias current determines  
the signal weighting given to that tap. The interpolator  
determines which stages are active by generating a discrete set  
of bias currents, each having a Gaussian profile. These are  
arranged to move from left to right, thereby determining the  
attenuation applied to the input signal as the gain is  
progressively lowered over the 69.3 dB range under control of  
the VSET input. The detailed manner in which the  
transconductance of adjacent stages varies as the virtual tap  
point slides along the attenuator accounts for the ripple  
observed in the conformance curves. Its magnitude is slightly  
temperature dependent and also varies with frequency (see  
Figure 10 to Figure 12). Notice that the system’s responses to  
signal inputs at INHI and INLO are not completely  
independent; these pins do not constitute a fully floating  
differential input.  
AD8362  
THIS INPUT  
IS DRIVEN  
1
2
3
4
5
6
7
8
16  
15  
14  
13  
12  
11  
10  
9
COMM ACOM  
NC  
CHPF  
DECL  
INHI  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
1nF  
RF INPUT  
Z = 50Ω  
R
SH  
INLO  
DECL  
1nF  
PWDN ACOM  
COMM CLPF  
DECL AND  
INLO ARE  
NOT DRIVEN  
Figure 53. Input Coupling from a Single-Ended Source  
Figure 53 illustrates one of many ways of coupling the signal  
source to the AD8362. Because the input pins are biased to  
about 3.6 V (for VS = 5 V) dc-blocking capacitors are required  
when driving from a grounded source. For signal frequencies  
>5 MHz, a value of 1 nF is adequate. While either INHI or  
INLO may be used, INHI is chosen here, and INLO is  
connected to the low side of the source. The resistor RSH is not  
needed if a 100 Ω termination is acceptable. The corresponding  
intercept is still −67 dBV, that is, 447 µV rms. However, specified  
in power terms at 100 Ω, the PZ is now at 2 nW or −57 dBm.  
ATTENUATION  
GUASSIAN INTERPOLATOR  
CONTROL  
For a source termination of 50 Ω, the internal 100 Ω from INHI  
to DECL must be shunted by a chip resistor of 100 Ω. At high  
frequencies, a low attenuation pad at the input improves the  
VSWR. For example, with a resistor of RSH = 33 Ω and an added  
resistor of 25 Ω from the source to INHI, a termination of 50 Ω  
is provided, with 6 dB of attenuation, raising the intercept to  
−48 dBm.  
TO FIXED  
GAIN STAGE  
gm  
gm  
gm  
gm  
INHI  
DECL  
USING A NARROW-BAND INPUT MATCH  
INLO  
While transformers offer the simplest method for providing  
single-sided to balanced conversion, a good alternative is  
using a specially designed narrow-band LC network, shown in  
Figure 54, which also provides an input match. Using this basic  
formulation, the match is to 50 Ω, with a voltage gain of 1.5  
(3.56 dB) from the input connector to the AD8362. This  
network is specially designed to provide a high degree of  
amplitude balance at INHI and INLO as well as an exact phase  
inversion. The narrow-band match provides a useful degree of  
frequency selectivity, and the capacitors also serve to provide  
the required dc blocking.  
STAGE 1  
6.33dB  
STAGE 11  
6.33dB  
STAGE 2  
6.33dB  
Figure 52. Simplified Input Circuit  
ALTERNATIVE INPUT COUPLING MEANS  
The input stages of the AD8362 are optimally driven from a  
fully balanced source, which should be provided wherever  
possible. The ac low sides of both halves of the attenuator  
internally connect to the DECL pin, which is therefore the RF  
signal low terminal for both INHI and INLO. In many cases,  
unbalanced sources can be applied directly to one or the other  
of these two pins. The chief disadvantage of this driving method  
is a reduction in dynamic range, particularly at very high  
frequencies.  
AD8362  
1
2
3
4
5
6
7
8
16  
15  
14  
13  
12  
11  
10  
9
COMM  
CHPF  
DECL  
INHI  
ACOM  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
ACOM  
CLPF  
NC  
C1  
RF INPUT  
Z = 50Ω  
100Ω  
L
INLO  
DECL  
PWDN  
COMM  
C2  
THESE INPUTS ARE  
EQUAL IN AMPLITUDE  
AND OF OPPOSITE SIGN  
Figure 54. Narrow-Band Reactive Input Coupling  
Rev. B | Page 23 of 36  
 
 
 
AD8362  
The network can readily be scaled to other frequencies by  
varying the product LC, while keeping the ratio L/C constant to  
preserve a 50 Ω input impedance. Table 4 provides some spot  
values; these take into account the reactive ZIN of the AD8362.  
CHOOSING THE RIGHT VALUE FOR CHPF AND  
CLPF  
The AD8362s 3.5 GHz variable gain amplifier includes an offset  
cancellation loop, which introduces a high-pass filter effect in  
its transfer function. The corner frequency, fHP, of this filter  
must be below that of the lowest input signal in the desired  
measurement bandwidth frequency to properly measure the  
amplitude of the input signal. The required value of the external  
capacitor is given by  
Table 4. Suggested Components for Narrow-Band 50 Ω  
Match  
Frequency (MHz)  
L (nH)  
21850  
10925  
4370  
2185  
1093  
437  
220  
100  
40  
C1 (pF)  
2230  
1115  
446  
223  
112  
45  
22  
10  
3.9  
C2 (pF)  
2765  
1383  
553  
276  
138  
55  
27  
12  
4.7  
1
2
5
10  
20  
50  
100  
200  
500  
CHPF = 200μF fHP  
(
fHP in Hz  
)
(12)  
Thus, for operation at frequencies down to 100 kHz, CHPF  
should be 2 nF.  
In the standard connections for the measurement mode, the  
VSET pin is tied to VOUT. For small changes in input amplitude  
(a few decibels), the time-domain response of this loop is  
essentially linear with a 3 dB low-pass corner frequency of  
nominally fLP = 1/(CLPF × 1.1 kΩ). Internal time delays around  
this local loop set the minimum recommended value of this  
capacitor to about 300 pF, making fLP = 3 MHz.  
This coupling method can be used down to much lower  
frequencies than shown in Table 4 simply by multiplying the  
1 MHz component values proportionally. The effects of the  
reactive components of the AD8362s inputs above 500 MHz  
may require some fine tuning of the suggested values. In the  
gigahertz region, the input coupling is usually more effectively  
implemented using a balun.  
For operation at lower signal frequencies, or whenever the  
averaging time needs to be longer, use  
UNCERTAINTIES IN RIN AND POWER CALIBRATION  
CLPF = 900μF fLP  
(
fLP in Hz  
)
(13)  
In all the cases where a 50 Ω to 200 Ω transformation is  
implemented, the voltage gain is only nominally ×2 (6 dB). This  
ideal is impaired by the fact that the input resistances of the  
AD8362 are not precise; variations of 20% can be expected  
from lot to lot. Therefore, it is necessary to use a calibration step  
whenever an accurate value for the power intercept, PZ, must be  
established.  
When the input signal exhibits large crest factors, such as a  
WCDMA signal, CLPF must be much larger than might at  
first seem necessary. This is due to the presence of significant  
low frequency components in the complex, pseudo-random  
modulation, which generates fluctuations in the output of  
the AD8362.  
When driven differentially, a significant improvement in  
intercept accuracy can be achieved by shunting the 200 Ω  
resistance from INHI to INLO with a 66.5 Ω resistor to set the  
differential input resistance to 50 Ω. Assuming a tolerance of  
20% for the basic RIN and 1% for the chip resistor, the net  
input resistance could exhibit an error of 2.5%. The resulting  
error in PZ (and thus in the absolute power measurement) may  
vary from −0.26 dB to +0.21 dB.  
USE OF NONSTANDARD TARGET VOLTAGES  
An external connection between VREF and VTGT sets up  
the internal target voltage, that is, the rms voltage that must  
be provided by the VGA to balance the AGC feedback loop. In  
the default scheme, the VREF of 1.25 V positions this target to  
0.06 × 1.25 V = 75 mV. In principle, however, VTGT may be  
driven by any voltage in the range −4 V to +4 V (the sign is  
ignored) to alter this target, either in a fixed or dynamic way.  
These precautions regarding input impedance do not apply  
when the input is presented in voltage form, as is often the case  
at low frequencies, or when the source impedance is low  
compared to 200 Ω. For example, when using a feedback  
amplifier as an impedance buffer ahead of the input, as in the  
example in Figure 61, the loss at the interface at moderate  
frequencies is negligible.  
For example, if this pin is supplied from VREF via a simple  
resistive attenuator of 1 kΩ:1 kΩ, the output required from the  
VGA is halved (to 37.5 mV rms), which moves the nominal  
intercept to −73 dBV. Under these conditions, the effective  
headroom in the signal path that drives the squaring cell is  
doubled. In principle, this doubles the peak crest factor that may  
be handled by the system.  
If VTGT is reduced too far, the accuracy and stability of the  
intercept are compromised. The currents generated by the  
transconductance mode squaring cells become smaller by the  
square of the ratio. Thus, a factor of 5 reduction in VTGT  
Rev. B | Page 24 of 36  
 
AD8362  
lowers the signal currents in the squaring cells by a factor of 25.  
As well as making the system more sensitive to small static  
errors (offsets) in the postdetection circuitry, such a reduction  
also reduces the peak slew rate. A suitable adjustment to the  
value of CLPF is needed to maintain a given AGC loop  
bandwidth. On the other hand, increasing the target voltage can  
improve the accuracy and stability of the intercept for low crest  
factor signals. Thus, using VTGT = 2.5 V, the peak output  
currents of the squaring cell are quadrupled and the peak slew  
rate is increased by the same factor. CLPF should be increased  
to maintain an adequate stability margin in the AGC loop.  
Also, it is worth remembering that these shifts in intercept are  
equivalent, in most respects, to a dc offset applied to the  
AD8362s output, with the main differences being that:  
Varying VTGT affects the crest factor capacity to some  
extent  
This technique makes better use of the available output  
range than a post-VOUT adjustment would  
5V  
AD8362  
1
2
3
4
5
6
7
8
4.02k  
16  
15  
14  
13  
12  
11  
COMM ACOM  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
CHPF  
DECL  
INHI  
4.02kΩ  
5.75kΩ  
In many applications, it is useful to use a nonstandard value of  
VTGT to shift the measurement range by a constant amount to  
accommodate either a reduced or increased range of signal  
inputs. The dynamic span remains >60 dB for such changes.  
This technique is particularly useful when the sensitivity can be  
lowered by raising VTGT, and there is little expectation of high  
crest factor signals.  
VR1  
20kΩ  
INLO  
DECL  
PWDN  
COMM  
ACOM 10  
CLPF  
9
Figure 55. Adjustments of the Intercept by 3 dB  
ADJUSTING THE INTERCEPT  
ALTERING THE SLOPE  
Another way to take advantage of the effect of VTGT is to use it  
to introduce an adjustment to the log intercept, represented by  
the voltage VZ in Equation 14. Formally, this can be expressed in  
terms of a modified value of VZ'.  
None of the changes in operating conditions discussed so far  
affect the logarithmic slope, VSLP, in Equation 9. However, this  
can readily be altered by controlling the fraction of VOUT that  
is fed back to the setpoint interface at the VSET pin. When the  
full signal from VOUT is applied to VSET, the slope assumes its  
nominal value of 50 mV/dB. It can be increased by including an  
attenuator between these pins, as shown in Figure 56. Moder-  
ately low resistance values should be used to minimize scaling  
errors due to the 70 kΩ input resistance at the VSET pin. Keep  
in mind that this resistor string also loads the output, and it  
eventually reduces the load-driving capabilities if very low  
values are used. To calculate the resistor values, use  
VZ' =VZVTGT 1.25V  
(14)  
A lower VTGT effectively increases the sensitivity of the  
measurement system, which is just another way of stating that the  
intercept moves to a lower value. This raises VOUT for all input  
amplitudes, as demonstrated by the plots in Figure 45. This  
control of the measurement system’s intercept could therefore be  
brought about by applying the output of a DAC to the VTGT pin,  
if that suits the overall objectives of an application.  
R1= R2'  
(
SD 50 1  
)
(15)  
For many purposes, a small manual adjustment range of 3 dB  
is sufficient. This can be implemented as shown in Figure 55.  
Here, the largest fraction of VTGT is still provided by the built-  
in reference to minimize the sensitivity to supply voltage  
variations. Now a variable component is provided by the trim  
network. For a 5 V supply, this added component of VTGT is 0  
when VR1 is centered. With the slider closest to ground, VTGT  
is lowered by 366 mV, which corresponds to a 3 dB decrease in  
intercept; in the opposite condition, it is raised by 518 mV,  
which increases the intercept by 3 dB. That is, VTGT ranges  
from 1.25 V/√2 to √2 × 1.25 V.  
where SD is the desired slope, expressed in mV/dB, and  
R2' is the value of R2 in parallel with 70 kΩ. For example, using  
R1 = 1.65 kΩ and R2 = 1.69 kΩ (R2' = 1.649 kΩ), the nominal  
slope is increased to 100 mV/dB. This choice of scaling is useful  
when the output is applied to a digital voltmeter because the  
displayed number reads as a decibel quantity directly, with only  
a decimal point shift.  
AD8362  
COMM ACOM  
1
2
3
4
5
6
7
8
16  
15  
14  
13  
12  
11  
10  
9
CHPF  
DECL  
INHI  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
Other adjustment ranges can be readily calculated from this  
example. The resistance at the VTGT pin is nominally 52 kΩ;  
resistor values should be calculated with this in mind. In some  
situations, this control interface might be driven from a  
programmable source. In the simplest case, a logic level could  
provide two intercept values, differing by say, 10 dB, thus  
providing essentially two switched input ranges.  
V
INLO  
DECL  
OUT  
R1  
R2  
PWDN ACOM  
COMM CLPF  
Figure 56. External Network to Raise Slope  
Rev. B | Page 25 of 36  
 
 
AD8362  
Operation at high slopes is useful when a particular subrange of  
the input is measured in greater detail. However, a measurement  
range of 60 dB would correspond to a 6 V change in VOUT at  
this slope, exceeding the capacity of the AD8362s output stage  
when operating on a 5 V supply. This requires that the intercept  
is repositioned to place the desired subrange within a window  
corresponding to an output range of 0.2 V ≤ VOUT ≤ 4.8 V,  
a 46 dB range.  
That being the case, the gain-control voltage, VSET, likewise  
does not need to change. It follows that the output is free of  
fluctuations. In measurement mode, that voltage is also the  
output, so it also remains at a constant value as the modulation  
varies the input magnitude. The bandwidth of the dc-coupled  
amplifier in the AD8362 that buffers VTGT has been kept high  
(~300 MHz) so that even fast AM modulation envelopes can be  
accurately tracked.  
Using the arrangement shown in Figure 57, an output of 0.5 V  
corresponds to the lower end of the desired subrange, and 4.5 V  
corresponds to the upper limit with 3 dB of margin at each end  
of the range, which is nominally 3 mV rms to 300 mV rms, with  
the intercept at 1.9 mV rms. Note that R2 is connected to VREF  
rather than ground. R3 is needed to ensure that the AD8362s  
reference buffer, which can sink only a small current, is  
correctly loaded.  
Figure 58 shows an example. As depicted in the top panel of  
Figure 59, the input to the AD8362 is a pure, ideal, sinusoidal  
100 MHz carrier that is amplitude modulated at 100 kHz by  
another pure sine wave. A suitably scaled sample of the  
modulation voltage is also applied to the VTGT pin. In this  
example, its average value is 1.25 V (the normal bias level for  
VTGT), and the amplitude is 0.75 V. Therefore VTGT ranges  
from 0.5 V to 2 V, corresponding to a factor of 4 change (16 dB)  
in the target voltage over each cycle of the modulation. The  
resulting VOUT waveform is of essentially constant value at  
about 2.5 V, as shown in Figure 59; this is compared with the  
deeply fluctuating output for a fixed VTGT of 1.25 V.  
It is apparent that a variable attenuation factor based on this  
scheme could provide a manual adjustment of the slope, but  
there are few situations in which this is of value. When the slope  
is raised by some factor, the loop capacitor, CLPF, should be  
raised by the same factor to ensure stability and to preserve a  
chosen averaging time. The slope can be lowered by placing a  
two-resistor attenuator after the output pin, following standard  
practice.  
BASEBAND REPLICA  
OF MODULATED INPUT  
SIGNAL ENVELOPE  
V
S
+5V nom,  
@ 24mA  
AD8362  
3.3  
1
2
3
4
5
6
7
8
16  
15  
14  
13  
12  
11  
10  
9
COMM ACOM  
NC  
CHPF  
DECL  
INHI  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
NC  
AMPLITUDE  
0.1µF  
MODULATED  
SIGNAL INPUT  
AD8362  
R3  
2k  
1nF  
1
2
16  
15  
14  
13  
12  
11  
10  
9
COMM ACOM  
1nF  
CHPF  
DECL  
INHI  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
INLO  
DECL  
V
OUT  
3
4
5
6
7
8
R2  
4.32kΩ  
1nF  
PWDN ACOM  
COMM CLPF  
V
INLO  
DECL  
OUT  
R1  
C
4.02kΩ  
LPF  
PWDN ACOM  
COMM CLPF  
Figure 58. Envelope Elimination Using the VTGT Interface  
Figure 57. Scheme Providing 100 mV/dB Slope for Operation  
over a 3 mV to 300 mV Input Range  
0.2  
0
ENVELOPE ELIMINATION MODE  
–0.2  
The VTGT input can be used to track the AM modulation  
envelope on an RF signal to affect a form of envelope  
FIXED TARGET VOLTAGE (1.25V)  
elimination. The modulation waveform must be known and a  
sample must be available as a baseband voltage. Using this  
voltage as VTGT, the AD8362 tracks this envelope when  
demodulation is realized by the squaring cell. So if the envelope  
output of the main amplifier should, for example, double over  
some interval while the target voltage that satisfies the AGC  
loop criterion also doubles, the net effect is that the gain of the  
amplifier does not need to change to keep the loop balanced.  
2
1
VARYING TARGET VOLTAGE  
0
3
2
1
WITH FIXED TARGET  
VOLTAGE  
WITH VARYING TARGET VOLTAGE  
0
10  
20  
30  
40  
TIME (µs)  
Figure 59. Waveforms for Envelope Elimination Scheme  
Rev. B | Page 26 of 36  
 
 
 
AD8362  
OPERATOR IN CONTROLLER MODES  
In order to fully understand this section, it is important to first  
read the preceding discussion of measurement modes, because  
there are only a few differences in operation and connections.  
When used in controller applications, the basic objective is to  
use the AD8362 as a level-sensing element in such a way that its  
output, here VAPC, moves in a direction that increases the  
controlled signal when the input sample is too low, and vice  
versa. A general scheme is shown in Figure 60.  
Every value of VSET maps uniquely to a specific rms value at its  
input. Thus, the major loop shown in Figure 60 forces the  
system being controlled to deliver exactly this level (which may  
be either in voltage form or as a sample of the power output).  
This mode of operation is therefore just an extension of the  
measurement mode, having exactly the same scaling (slope and  
intercept) at the VSET pin.  
When the system in Figure 60 is an RF power amplifier (PA), a  
practical consideration immediately comes to our attention.  
Frequently, the gain (and thus output power) is arranged to  
increase in response to an increasing positive voltage applied to  
the gain control pin. However, the AD8362’s output tends  
toward higher values as its input crosses over the level  
corresponding to the setpoint, which would cause the PA’s  
output to increase further. In other words, the feedback polarity  
is reversed, forcing the control loop to latch up at one of its  
power extremes.  
CONTROLLED SYSTEM  
(OUTPUT POWER  
DECREASES AS V  
APC  
INCREASES)  
SYSTEM  
OUTPUT  
SYSTEM  
INPUT  
OUTPUT  
INPUT  
V
APC  
R
= 100  
SH  
V
S
FOR 50Ω  
TERMINATION  
AD8362  
COMM ACOM 16  
3.3Ω  
1
2
3
4
An increasing number of modular PAs feature a control polarity  
that reduces the power output with increases in control voltage.  
These can be controlled directly from the VOUT pin of the  
AD8362. Elsewhere, it is necessary to provide the sign inversion  
using a low noise buffer. This amplifier may also include  
provisions to ensure that the PA is never driven beyond its safe  
limits. The complete details of such a control system depends  
on many factors, and this example shows only generic aspects of  
the design.  
NC  
CHPF  
DECL  
INHI  
VREF 15  
VTGT 14  
0.1µF  
1nF  
1nF  
VPOS  
13  
R
1nF  
SH  
5
6
7
8
INLO  
VOUT 12  
VSET 11  
1nF  
1nF  
SETPOINT  
VOLTAGE INPUT  
0.5V TO 3.5V  
DECL  
PWDN ACOM 10  
COMM CLPF  
9
C
LPF  
Figure 60. Generalized Control Loop Using the AD8362  
USE OF AN INPUT BALUN  
Because the AD8362 integrates any input error relative to the  
setpoint, and ideally would fully null this error over an  
appropriate time interval, it follows that VAPC swings rail-  
to-rail over a very narrow range of inputs. In practice, a few  
millidecibels of amplitude deviation at the input fully swing the  
output.  
A balun (balance to unbalance) is used either to transform  
differential RF signals to single-ended form or in reverse to  
convert single-sided signals to differential form. A typical balun  
consists of a short length of transmission line (miniature coaxial  
or twisted pair) through which the signal passes without  
significant degradation, wound on a core (often a ferrite) to  
generate a series mode inductor having a high reactive  
impedance, compared to the through-mode impedance of the  
transmission line, which is often 50 Ω.  
The signal input level at which this occurs (the setpoint) is  
determined by the control voltage, VSET. This voltage defines  
the narrow range of the ac input over which the AD8362s  
output is most sensitive to the absolute input magnitude. In base  
stations, for example, VSET is often delivered by the ramp DAC,  
and the setpoint is a rapidly varying sequence of levels during  
the ramp-up and ramp-down intervals of each burst as well as  
with output power demand variations from one channel to  
another.  
High frequency common-mode voltages applied to the input of  
this line are sustained across this series reactance and do not  
appear at the loaded side of the line. On the other hand, the  
through-mode bandwidth is very high, and the losses incurred  
in a short line of this sort are trivial.  
Baluns of slightly more elaborate construction can provide an  
impedance transformation (usually designated by their  
impedance ratio, for example, 4:1, which becomes a 1:4 ratio  
when used in reverse) in order to convert a single-sided signal  
to the balanced form, as is desirable in driving the AD8362,  
while also presenting a 50 Ω input interface.  
Rev. B | Page 27 of 36  
 
AD8362  
The evaluation board for the AD8362 includes a 1:4 balun,  
part number M/A-COM ETC1.6-4-2-3, providing low loss  
coupling from 0.5 GHz to 2.5 GHz and an impedance  
transformation from the board’s 50 Ω input (at the SMA  
connector) to the 200 Ω differential input resistance of the  
AD8362. At high frequencies, the actual impedance at the  
connector is influenced by reactive aspects of the ICs input  
impedance. Because these can alter the magnitude of the input  
voltage, the logarithmic intercept cannot be precisely specified.  
However, the shift is temperature stable.  
Note that the balun used here increases the signal voltage by the  
square root of its impedance ratio of 4:1, in this case by a factor  
of 2. The use of a transformer to match the 500 Ω source to the  
200 Ω load presented by the AD8362 thus increases the effective  
sensitivity of the measurement system by 6 dB, whether  
specified in dBV or dBm at the input to the transformer.  
Rev. B | Page 28 of 36  
AD8362  
GENERAL APPLICATIONS  
The unusual versatility of the AD8362 opens up many new  
possibilities whenever an element having an accurate rms  
response is needed. Developed primarily to address the need for  
true power measurement in communications systems operating  
at frequencies as high as 2.7 GHz, the AD8362 is capable of  
meeting the requirements of instrumentation at much lower  
frequencies. As noted earlier, the AD8362 is unique in providing  
rms-to-dc conversion with a completely constant bandwidth  
regardless of signal amplitude and in providing a calibrated  
linear-in-dB measurement.  
The basic gain of the AD8330 varies from 0 dB to 50 dB. Here it  
is raised 8 dB by driving VMAG from the 1.25 V available from  
the AD8362, whose 200 Ω loading on the 150 Ω ROUT of the  
AD8330 in turn lowers the overall gain by 5 dB. The peak gain  
is thus ~53 dB. (Mismatches between the on-chip resistors in  
each IC can cause a gain error of up to 1.3 dB.)  
Using the AD8330s inverse gain mode (MODE pin low), its  
gain decreases on a slope of 30 mV/dB to a minimum value of  
3 dB for a gain voltage (VDBS) of 1.5 V. VDBS is 40% of the  
AD8362s output. Over the 3 V range from 0.5 V to 3.5 V, the  
gain of the AD8330 varies by (0.4 × 3 V)/(30 mV/dB), that is,  
40 dB. Combined with the 60 dB gain span of the AD8362, this  
results in a 100 dB variation for a 3 V change in VOUT. The  
overall log slope is therefore 30 mV/dB.  
Caution: The applications shown in Figure 61 are provided only  
for illustrative purposes and should not be regarded as ready for  
immediate incorporation into a users system. They have been  
validated for the present purpose by simulation studies.  
The full gain noise-spectral density at the AD8330s input is  
5 nV/√Hz which is raised (by 53 dB) to 2.2 mV/√Hz at its  
output. To realize the full 100 dB potential, the noise at the  
AD8362s input must be much less than 1 mV rms. This  
requires limiting the AD8330s noise bandwidth to ~100 kHz  
(when eN = 0.7 mV rms) provided by a single-pole, low-pass  
section at the coupling interface, formed by CFLT = 18 nF and  
the net differential resistance of 86 Ω (that is, 150 Ω || 200 Ω).  
RMS VOLTMETER WITH >100 dB DYNAMIC RANGE  
The 60 dB range of the AD8362 can be extended by adding a  
standalone VGA as a preamplifier whose gain control input is  
derived directly from VOUT. This extends the dynamic range  
by the gain control range of this second amplifier. When this  
VGA also provides a linear-in-dB (exponential) gain control  
function, the overall measurement remains linearly scaled in  
decibels. The VGA gain must decrease with an increase in its  
gain bias, like the AD8362. It is convenient to select a VGA  
needing only a single 5 V supply and capable of generating a  
fully balanced differential output. All of these conditions are  
met by the AD8330. Figure 61 shows the schematic. The signal  
can be applied to the AD8330 in either single-ended or  
differential form by using a variety of coupling arrangements  
(see the AD8330 data sheet for more information).  
5V  
3.3  
3.3Ω  
3.3Ω  
AD8362  
3.6V  
ENBL OFST VPOS CNTR  
1
2
3
4
5
6
7
8
16  
15  
14  
13  
12  
11  
10  
9
COMM ACOM  
10µF  
CHPF  
DECL  
INHI  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
C
18nF  
FLT  
VPS1  
VPS0  
INHI  
OPHI  
INPUT  
(SEE AD8330  
DATA SHEET)  
3.6V  
AD8330  
INLO  
OPLO  
V
OUT  
INLO  
DECL  
MODE  
CMOP  
PWDN ACOM  
COMM CLPF  
VDBS CMGN COMM VMAG  
10µF  
6.04kΩ  
402kΩ  
ALL UNMARKED CAPACITORS ARE 0.1µF  
Figure 61. RMS Voltmeter with >100 dB Dynamic Range  
Rev. B | Page 29 of 36  
 
AD8362  
If optimized for use at lower frequencies, CFLT should be  
increased accordingly; for audio applications, use 0.1 µF. In RF  
measurements where the carrier frequency is known, the  
coupling and bandwidth limiting between the ICs might be  
provided by a narrow-band SAW filter. Figure 62 shows the  
output and law conformance error for this AD8330/AD8362  
collaboration. The dynamic range extends from 5 µV to 0.5 V  
rms between the 0.5 dB error points in this simulation.  
For example, a 10:1 change of VTGT from 0.35 V to 3.5 V shifts  
the intercept by 20 dB. This has the effect of stretching the  
measurement range by the same amount, from >60 dB to more  
than 80 dB. So the slope decreases to about 40 mV/dB because a  
larger input range is now represented by the same 3.15 V. The  
simulation results shown in Figure 64 compare the expanded  
range response with that for a fixed VTGT. The upper end of  
the measurement range is extended from 1.5 V to over 4 V  
(limited by the input protection).  
4
3
2
1
4
3
V
= V  
OUT  
TGT  
V
= 1.25V  
2
1
TGT  
0
3
2
0
15  
1
0
10  
5
V
= V  
OUT  
TGT  
–1  
–2  
–3  
V
= 1.25V  
TGT  
0
500m  
5µ  
50µ  
500µ  
5m  
50m  
RMS INPUT VOLTAGE (V)  
100µ  
1m  
10m  
0.1  
1
10  
RMS INPUT VOLTAGE (V)  
Figure 62. Output and Conformance for the AD8330/AD8362 Collaboration  
Figure 64. Dynamic Range Expansion Using VTGT = VOUT  
RF POWER METER WITH 80 DB RANGE  
However, it is apparent that the transfer function is no  
longer a simple logarithmic law; further consideration shows  
that the modified function is nonanalytic. Nevertheless, this  
function is dependable, and it remains as stable over supply  
and temperature variations as in the normal mode. A good  
approximation is provided by  
According to simulations, the basic 60 dB measurement range  
of the AD8362 can be extended by up to 20 dB by using a target  
voltage, VTGT, that increases progressively with the input level.  
In the simplest case, this can be achieved by connecting VTGT  
to the output VOUT/VSET. Figure 63 shows the connections;  
for present purposes, R1 is omitted and R2 is short-circuited.  
3
VOUT = VSLP  
{
log10  
(
VIN VZ  
)
11.3m  
[
log10  
(
VIN  
)
]
}
(16)  
For small signal inputs, VOUT is also small, and the target is  
well below the normal 75 mV (with 1.25 V applied to VTGT).  
The lower target means that the AD8362s VGA output does  
not have to be as large as normal, which increases the input  
sensitivity. As the signal and thus VOUT increases, so does the  
target voltage, which progressively shifts the required VGA  
input to a higher level.  
where the modified slope voltage VSLP'' is 0.868 V, that is,  
43.4 mV/dB. Using this expression, the dynamic range is 86 dB  
to the 0.5 dB error points (0.2 mV ≤ VIN ≤ 4 V). The actual  
range is reduced in practice by the effects of the AD8362s  
input-referred noise at low inputs. If the basic 60 dB+ range is  
only slightly less than required in a particular application, then  
a fraction of VOUT can be summed with a part of VREF to the  
VTGT pin, which is why R1 and R2 were included. The output  
now conforms in general terms to the formula  
AD8362  
1
2
3
4
5
6
7
8
16  
15  
14  
13  
12  
11  
10  
9
COMM ACOM  
CHPF  
DECL  
INHI  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
R1  
R2  
3
VOUT =VSLP  
{
log10  
(
VIN VZ  
)
KC  
[
log10  
(
VIN  
)
]
}
(17)  
V
INLO  
DECL  
OUT  
where the correction factor KC introduces the required  
PWDN ACOM  
COMM CLPF  
nonlinear correction to minimize the law-conformance error.  
Table 5 provides several representative spot values using  
progressively greater amounts of dynamic range extension.  
Figure 63. RF Power Meter with 80 dB Range  
Rev. B | Page 30 of 36  
 
 
 
AD8362  
Table 5. Suggested Values for Use in Scheme of Figure 63  
4
3
2
1
R1 (Ω)  
R2 (Ω)  
VSLP' (V/decade)  
VZ' (mV)  
0.334  
0.336  
0.333  
0.340  
0.355  
0.380  
KC (m)  
11.3  
10.4  
6.5  
O/C  
S/C  
0.868  
1904  
1346  
872  
480  
200  
96  
654  
1128  
1520  
1800  
0.870  
0.890  
0.914  
0.942  
0
3.7  
1.5  
0.5  
30  
20  
10  
0.972  
0
HIGH SLOPE DETECTORS CENTERED ON A  
NARROW WINDOW  
–10  
–20  
–30  
The situation often arises in system monitoring in which an  
input signal varies by much less than 60 dB, and the highest  
possible sensitivity and accuracy of measurement is required  
within a narrow window of input magnitudes. Adapting the  
AD8362 to this task requires that the slope be increased and the  
intercept repositioned. Using an attenuator from VOUT to  
VSET, any slope >50 mV/dB can be realized. Then, using a  
fraction of VREF (or external reference voltage), the particular  
region of the dynamic range to be measured can be positioned  
wherever desired. In these high slope applications, the full rail-  
to-rail output swing of the AD8362 can be exploited.  
100µ  
1m  
10m  
0.1  
1
10  
RMS INPUT VOLTAGE (V)  
Figure 66. Illustrative Results for Slope of 100 mV/dB  
4
3
2
1
0
30  
SLOPE  
R1  
R2  
AD8362  
(V/dec)  
2
4
5
(k)  
4.02  
8.66  
8.66  
9.1  
(k)  
4.32  
3.01  
2.15  
1.02  
20  
10  
1
2
3
4
5
16  
15  
14  
13  
12  
11  
10  
9
COMM ACOM  
CHPF  
DECL  
INHI  
VREF  
VTGT  
VPOS  
VOUT  
VSET  
0
10  
–10  
–20  
–30  
V
INLO  
DECL  
OUT  
R1  
R2  
100µ  
1m  
10m  
0.1  
1
10  
6
7
8
RMS INPUT VOLTAGE (V)  
PWDN ACOM  
COMM CLPF  
INTERCEPT OFFSET  
VOLTAGE, V  
Figure 67. Illustrative Results for Slope of 200 mV/dB  
SHIFT  
Figure 65. Slope and Intercept Adjustment  
4
3
2
1
Figure 65 shows the basic connections for this mode of use; the  
intercept repositioning voltage VSHIFT can be introduced by  
adding a third resistor from VREF to VSET with recalculated  
values of R1 and R2 or by using an external voltage source.  
Figure 66 presents the simulation results for a log slope of  
100 mV/dB (2 V/dec) covering two-decade spans over several  
sub-ranges, while Figure 67 shows the results for a slope of  
200 mV/dB (4 V/dec), providing just a one-decade span.  
0
30  
20  
10  
0
To accurately reposition the range (intercept) when very high  
slopes are used, a low output impedance DAC can be used to  
provide VSHIFT. Figure 68 shows simulated results for a slope of  
500 mV/dB (10 V/dec) presuming this configuration. In all  
cases, the fixed-pattern ripple in the log conformance remains  
unchanged in dB terms. Residual fluctuations due to insufficient  
averaging (in low frequency applications) are likewise  
unaffected in their equivalent decibel value, though greater in  
absolute voltage terms.  
–10  
–20  
–30  
100µ  
1m  
10m  
0.1  
1
10  
RMS INPUT VOLTAGE (V)  
Figure 68. Illustrative Results for Slope of 10 mV/dec  
Rev. B | Page 31 of 36  
 
 
 
 
AD8362  
AD8362 EVALUATION BOARD  
The AD8362 evaluation board provides for a number of  
different operating modes and configurations, including many  
of those described in this data sheet. The measurement mode is  
set up by positioning SW2 as shown in Figure 69. The AD8362  
can be operated in controller mode by flipping SW2 to its  
alternate position, thereby connecting the VSET pin to the  
VSET connector and applying the setpoint voltage to the VSET  
connector.  
In measurement mode, the slope of the response at VOUT may  
be increased through the use of a voltage divider implemented  
with the appropriately valued resistors, as explained in this data  
sheet, in Positions R17 and R9, and with SW2 switched to its  
alternate position.  
The AD8362 is powered up with SW3 in the position shown in  
Figure 69 and connector PWDN open. The part can be powered  
down either by connecting a logic high voltage to connector  
PWDN with SW3 in the position shown in Figure 69 or by  
switching SW3 to its alternate position.  
The internal voltage reference is used for the target voltage  
when SW1 is in the position shown in Figure 69. This voltage  
may optionally be reduced via a voltage divider implemented  
with R4 and R5, with LK1 in place as shown in Figure 69 and  
SW1 switched to its alternate position. Alternatively, an external  
target voltage may be used with SW1 switched to its alternate  
position, LK1 removed, and the external target voltage applied  
to the VTGT connector.  
Balun Transformer T1 may be removed and replaced by two  
capacitors and an inductor, as shown in Figure 54, or by two 0 Ω  
resistors (links, size 0402): one in series with Capacitors C6 and  
C10, and the other in series with C5 and a 100 Ω resistor installed  
in Position R16, to implement the circuit shown in Figure 53.  
R1  
0Ω  
AGND  
VPOS  
C1  
0.1µF  
C2  
100pF  
R14  
OPEN  
R15  
0Ω  
AD8362  
1
2
3
4
5
6
7
8
COMM  
ACOM  
16  
15  
R4  
0Ω  
C8  
1000pF  
C7  
1000pF  
VREF  
CHPF  
DECL  
INHI  
VREF  
R5  
10kΩ  
C10  
1000pF  
C6  
100pF  
VTGT 14  
VPOS  
LK1  
SW1  
T1  
R6  
0Ω  
RFIN  
13  
VTGT  
VOUT  
R16  
OPEN  
INLO  
VOUT 12  
VSET 11  
R8  
R17  
R7  
0Ω  
C5  
100pF  
0Ω  
OPEN  
DECL  
PWDN  
COMM  
SW2  
R9  
10kΩ  
C4  
1000pF  
ACOM  
CLPF  
10  
9
VSET  
C3  
0.1µF  
SW3  
PDWN  
R10  
R13  
10kΩ  
0Ω  
C9  
OPEN  
Figure 69. Evaluation Board Schematic  
Rev. B | Page 32 of 36  
 
AD8362  
Figure 70. Component Side Metal of Evaluation Board  
Figure 71. Component Side Silkscreen of Evaluation Board  
Table 6. Evaluation Board Configuration Options  
Component  
Function  
Part Number  
Default Value  
T1  
C1  
C2  
C3  
C9  
M/A-COM ETC1.6-4-2-3  
Supply filtering/decoupling capacitor  
Supply filtering/decoupling capacitor  
Output low-pass filter capacitor  
Output low-pass filter capacitor  
(normally omitted, not installed)  
0.1 µF  
100 pF  
0.1 µF  
C4, C7, C10  
C5, C6  
C8  
DUT  
Input bias-point decoupling capacitors  
Input signal coupling capacitors  
Input high-pass filter capacitor  
AD8362  
1000 pF  
100 pF  
1000 pF  
AD8362ARU  
R1, R4, R6, R7, R8, R10, R15  
Jumpers  
0 Ω  
R5, R9, R13  
R16  
R17  
RA  
RB  
Optional pull-down resistors  
Not installed, see text  
Slope adjustment (not installed, see text)  
Not installed, see text  
10 kΩ  
100 Ω  
(See text)  
25 Ωor 0 Ω  
33 Ω  
Not installed, see text  
RC  
Not installed, see text  
0 Ω  
SW1  
SW2  
SW3  
Internal/external target voltage selector  
Measurement mode/controller mode selector  
Power-down/enable or external power-down selector  
Rev. B | Page 33 of 36  
AD8362  
OUTLINE DIMENSIONS  
5.10  
5.00  
4.90  
16  
9
8
4.50  
4.40  
4.30  
6.40  
BSC  
1
PIN 1  
1.20  
MAX  
0.15  
0.05  
0.20  
0.09  
0.75  
0.60  
0.45  
8°  
0°  
0.30  
0.19  
0.65  
BSC  
SEATING  
PLANE  
COPLANARITY  
0.10  
COMPLIANT TO JEDEC STANDARDS MO-153AB  
Figure 72. 16-Lead Thin Shrink Small Outline Package [TSSOP]  
(RU-16)  
Dimensions shown in millimeters  
ORDERING GUIDE  
Model  
AD8362ARU  
AD8362ARU-REEL7  
AD8362ARUZ1  
AD8362ARUZ-REEL71  
AD8362-EVAL  
Temperature Range  
−40°C to +85°C  
−40°C to +85°C  
−40°C to +85°C  
−40°C to +85°C  
Package Description  
Package Option  
RU-16  
RU-16  
RU-16  
RU-16  
16-Lead TSSOP, Tube  
16-Lead TSSOP, 7" Tape and Reel  
16-Lead TSSOP, Tube  
16-Lead TSSOP, 7" Tape and Reel  
Evaluation Board  
1 Z = Pb-free part.  
Rev. B | Page 34 of 36  
AD8362  
NOTES  
Rev. B | Page 35 of 36  
AD8362  
NOTES  
©
2004 Analog Devices, Inc. All rights reserved. Trademarks and  
registered trademarks are the property of their respective owners.  
C02923–0–3/04(B)  
Rev. B | Page 36 of 36  

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