ADL5310-EVALZ [ADI]
Dual Logarithmic Converter;型号: | ADL5310-EVALZ |
厂家: | ADI |
描述: | Dual Logarithmic Converter |
文件: | 总20页 (文件大小:570K) |
中文: | 中文翻译 | 下载: | 下载PDF数据表文档文件 |
120 dB Range (3 nA to 3 mA)
Dual Logarithmic Converter
Data Sheet
ADL5310
FEATURES
FUNCTIONAL BLOCK DIAGRAM
2 independent channels optimized for photodiode interfacing
6-decade input dynamic range
Law conformance 0.3 dB from 3 nA to 3 mA
Temperature-stable logarithmic outputs
665kΩ
VREF
VRDZ
OUT1
VSUM
IRF1
V
OUT1
COMM
Nominal slope 10 mV/dB (200 mV/dec), externally scalable
Intercepts may be independently set by external resistors
User-configurable output buffer amplifiers
Single-supply or dual-supply operation
SCL1
BIN1
V
BIAS
6.69kΩ
I
LOG
TEMPERATURE
COMPENSATION
VNEG
LOG1
451Ω
14.2kΩ
Space efficient, 24-lead 4 mm × 4 mm LFCSP
Low power: <10 mA quiescent current
I
INP1
IRF2
PD1
OUT2
REFERENCE
GENERATOR
0.5V
2.5V
V
OUT2
APPLICATIONS
20kΩ
COMM
80kΩ
Gain and absorbance measurements
Multichannel power monitoring
General-purpose baseband log compression
SCL2
BIN2
V
BIAS
14.2kΩ
I
LOG
TEMPERATURE
VNEG
COMPENSATION
LOG2
451Ω
6.69kΩ
I
INP2
PD2
COMM
VSUM
665kΩ
VREF
Figure 1.
GENERAL DESCRIPTION
The ADL53101 low cost, dual logarithmic amplifier converts input
current over a wide dynamic range to a linear-in-dB output
voltage. It is optimized to determine the optical power in wide-
ranging optical communication system applications, including
control circuitry for lasers, optical switches, atten-uators, and
amplifiers, as well as system monitoring. The device is equivalent
to a dual AD8305 with enhanced dynamic range (120 dB). While
the ADL5310 contains two independent signal channels with
individually configurable transfer function constants (slope and
intercept), internal bias circuitry is shared between channels for
improved power consumption and channel matching. Dual
converters in a single, compact LFCSP package yield space-
efficient solutions for measuring gain or attenuation across
optical elements. Only a single supply is required; optional
dual-supply operation offers added flexibility.
VSUM potential. The VSUM potential is internally set to 500 mV
but may be externally grounded for dual-supply operation, and
for additional applications requiring voltage inputs.
The logarithmic slope is set to 10 mV/dB (200 mV/decade)
nominal and can be modified using external resistors and the
independent buffer amplifiers. The logarithmic intercepts for
each channel are defined by the individual reference currents,
which are set to 3 μA nominal for maximum input range by
connecting 665 kΩ resistors between the 2.5 V VREF pins and
the IRF1 and IRF2 inputs. Tying VRDZ to VREF effectively sets
the x-intercept four decades below the reference current, which
is typically 300 pA for a 3 µA reference.
The use of individually optimized reference currents may be
valuable when using the ADL5310 for gain or absorbance measure-
ments where each channel input has a different current range
requirement. The reference current inputs are also fully functional
dynamic inputs, allowing log ratio operation with the reference
input current as the denominator. The ADL5310 is specified for
operation from –40°C to +85°C.
The ADL5310 employs an optimized translinear structure that
use the accurate logarithmic relationship between a bipolar
transistor’s base emitter voltage and collector current, with
appropriate scaling by precision currents to compensate for the
inherent temperature dependence. Input and reference current
pins sink current ranging from 3 nA to 3 mA (limited to 60 dB
between input and reference) into a fixed voltage defined by the
1 Protected by US Patents 4,604,532, and 5,519,308. Other patents pending.
Rev. B
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Tel: 781.329.4700 ©2003–2018 Analog Devices, Inc. All rights reserved.
Technical Support
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ADL5310
Data Sheet
TABLE OF CONTENTS
Features .............................................................................................. 1
Theory.......................................................................................... 11
Managing Intercept and Slope.................................................. 12
Response Time and Noise Considerations ............................. 12
Applications Information.............................................................. 13
Calibration................................................................................... 14
Minimizing Crosstalk ................................................................ 14
Relative and Absolute Power Measurements.......................... 15
Characterization Methods ........................................................ 16
Evaluation Board ............................................................................ 17
Outline Dimensions....................................................................... 20
Ordering Guide .......................................................................... 20
Applications....................................................................................... 1
Functional Block Diagram .............................................................. 1
General Description......................................................................... 1
Revision History ............................................................................... 2
Specifications..................................................................................... 3
Absolute Maximum Ratings............................................................ 4
ESD Caution.................................................................................. 4
Pin Configuration and Function Descriptions............................. 5
Typical Performance Characteristics ............................................. 6
General Structure ........................................................................... 11
REVISION HISTORY
4/2018—Rev. A to Rev. B
Changes to Figure 2 and Table 3..................................................... 5
Changes to Figure 40...................................................................... 18
Updated Outline Dimensions ....................................................... 20
Changes to Ordering Guide .......................................................... 20
9/2004—Rev. 0 to Rev. A
Changes to Ordering Guide .......................................................... 20
11/2003—Revision 0: Initial Version
Rev. B | Page 2 of 20
Data Sheet
ADL5310
SPECIFICATIONS
VP = 5 V, V N = 0 V, T A = 25°C, RREF = 665 kΩ, and VRDZ connected to VREF, unless otherwise noted.
Table 1.
Parameter
Test Conditions/Comments
Pin 1 to Pin 6: INP1 and INP2, IRF1 and IRF2, VSUM
Flows toward INP1 pin or INP2 pin
Flows toward INP1 pin or INP2 pin
Flows toward IRF1 pin or IRF2 pin
Internally preset; user alterable
–40°C < TA < +85°C
Min
Typ
Max
Unit
INPUT INTERFACE
Specified Current Range, IPD
Input Current Min/Max Limits
Reference Current, IREF, Range
Summing Node Voltage
Temperature Drift
3 n
3 m
10 m
3 m
A
A
A
V
3 n
0.46
0.5
0.030
0.54
mV/°C
mV
Input Offset Voltage
+20
VIN − VSUM, VIREF − VSUM
−20
LOGARITHMIC OUTPUTS
Logarithmic Slope
Pin 15 and Pin 16: LOG1 and LOG2
190
185
165
40
200
300
210
215
535
1940 pA
0.4
0.6
mV/dec
mV/dec
pA
–40°C < TA < +85°C
Logarithmic Intercept1
Law Conformance Error
–40°C < TA < +85°C
10 nA < IPD < 1 mA
3 nA < IPD < 3 mA
IPD > 3 µA; output referred
IPD = 3 µA
0.1
0.3
0.5
1.5
1.7
0.10
5
dB
dB
µV/√Hz
MHz
V
Wideband Noise2
Small Signal Bandwidth2
Maximum Output Voltage
Minimum Output Voltage
Output Resistance
Limited by VN = 0 V
V
4.375
5.625 kΩ
REFERENCE OUTPUT
Voltage wrt Ground
Pin 7 and Pin 24 (internally shorted): VREF
2.45
2.42
2.5
2.55
2.58
V
V
–40°C < TA < +85°C
Maximum Output Current
Incremental Output Resistance
OUTPUT BUFFERS
Sourcing (grounded load)
Load current < 10 mA
20
4
mA
Ω
Pins 12 to 14 and 17 to 19: OUT2, SCL2, BIN2, BIN1, SCL1,
and OUT1
Input Offset Voltage
Input Bias Current
Incremental Input Resistance
Incremental Output Resistance
Output High Voltage
Output Low Voltage
Peak Source/Sink Current
Small-Signal Bandwidth
Slew Rate
−20
+20
mV
µA
MΩ
Ω
Flowing out of Pins 13, 14, 17, and 18
0.4
35
0.5
Load current < 10 mA; gain = 1
RL = 1 kΩ to ground
V
VP − 0.1
0.10
30
15
15
RL = 1 kΩ to ground
V
mA
MHz
V/µs
Gain = 1
0.2 V to 4.8 V output swing
Pins 8 and 9: VPOS; Pins 10, 11, and 20: VNEG
(VP – VN ) ≤ 12 V
Input currents < 10 µA
(VP – VN ) ≤ 12 V
POWER SUPPLY
Positive Supply Voltage
Quiescent Current
3
5
9.5
0
12
11.5
V
mA
V
Negative Supply Voltage (Optional)
−5.5
1 Other values of logarithmic intercept can be achieved by adjustment of RREF
2 Output noise and incremental bandwidth are functions of input current; measured using output buffer connected for GAIN = 1.
.
Rev. B | Page 3 of 20
ADL5310
Data Sheet
ABSOLUTE MAXIMUM RATINGS
Table 2.
Stresses at or above those listed under Absolute Maximum
Ratings may cause permanent damage to the product. This is a
stress rating only; functional operation of the product at these
or any other conditions above those indicated in the operational
section of this specification is not implied. Operation beyond
the maximum operating conditions for extended periods may
affect product reliability.
Parameter
Rating
12 V
Supply Voltage VP − VN
Input Current
Internal Power Dissipation
θJA
Maximum Junction Temperature
Operating Temperature Range
Storage Temperature Range
Lead Temperature Range (Soldering 60 sec)
20 mA
500 mW
35°C/W1
125°C
–40°C to +85°C
−65°C to +150°C
300°C
ESD CAUTION
1 With paddle soldered down.
Rev. B | Page 4 of 20
Data Sheet
ADL5310
PIN CONFIGURATION AND FUNCTION DESCRIPTIONS
1
18 SCL1
BIN1
VSUM
INP1 2
17
ADL5310
16 LOG1
15 LOG2
3
4
5
6
IRF1
IRF2
DUAL LOG AMP
TOP VIEW
(Not to Scale)
INP2
14
BIN2
VSUM
CL2
13 S
NOTES
1. EXPOSED PAD. THE EXPOSED PAD MUST
BE CONNECTED TO ANALOG GROUND
VIA A LOW IMPEDANCE PATH.
Figure 2. 24-Lead LFCSP Pin Configuration
Table 3. Pin Function Descriptions
Pin No.
Mnemonic Function
1, 6
VSUM
Guard Pin. Used to shield the INP1 and INP2 input current lines, and for optional adjustment of the input
summing node potentials. Pin 1 and Pin 6 are internally shorted.
2
INP1
Channel 1 Numerator Input. Accepts (sinks) photodiode current IPD1. Usually connected to photodiode anode
such that photocurrent flows into INP1.
3
4
5
IRF1
IRF2
INP2
Channel 1 Denominator Input. Accepts (sinks) reference current, IRF1
Channel 2 Denominator Input. Accepts (sinks) reference current, IRF2
Channel 2 Numerator Input. Accepts (sinks) photodiode current IPD2. Usually connected to photodiode anode
such that photocurrent flows into INP2.
.
.
7, 24
8, 9
10, 11, 20
VREF
VPOS
VNEG
Reference Output Voltage of 2.5 V. Pin 7 and Pin 24 are internally shorted.
Positive Supply, (VP – VN) ≤ 12 V. Both pins must be connected externally.
Optional Negative Supply, VN. These pins are usually grounded. For more details, see the General Structure and
Applications Information sections. All VNEG pins must be connected externally.
12
13
14
15
16
17
18
19
OUT2
SCL2
BIN2
LOG2
LOG1
BIN1
SCL1
OUT1
COMM
VRDZ
Buffer Output for Channel 2.
Buffer Amplifier Inverting Input for Channel 2.
Buffer Amplifier Noninverting Input for Channel 2.
Output of the Logarithmic Front End for Channel 2.
Output of the Logarithmic Front End for Channel 1.
Buffer Amplifier Noninverting Input for Channel 1.
Buffer Amplifier Inverting Input for Channel 1.
Buffer Output for Channel 1.
21, 22
23
Analog Ground. Pin 21 and Pin 22 are internally shorted.
Intercept Shift Reference Input. The top of a resistive divider network that offsets VLOG to position the intercept.
Normally connected to VREF; may also be connected to ground when bipolar outputs are to be provided.
EPAD
Exposed Pad. The exposed pad must be connected to analog ground via a low impedance path.
Rev. B | Page 5 of 20
ADL5310
Data Sheet
TYPICAL PERFORMANCE CHARACTERISTICS
VP = 5 V, V N = 0 V, R REF = 665 kΩ, TA = 25°C, unless otherwise noted.
1.6
2.0
1.5
T
V
= –40°C, 0°C, +25°C, +70°C, +85°C
= 0V
A
IN
1.4
1.2
1.0
0.8
0.6
0.4
0.2
0
1.0
+85°C
+70°C
+25°C
0.5
0
–0.5
–1.0
–1.5
–2.0
0°C
–40°C
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
I
I
INP
INP
Figure 3. VLOG vs. IINP for Multiple Temperatures
Figure 6. Law Conformance Error vs. IINP for Multiple Temperatures,
Normalized to 25°C
1.8
1.6
1.4
1.2
1.0
0.8
0.6
0.4
0.2
0
2.0
1.5
1.0
T
V
= –40°C, 0°C, +25°C, +70°C, +85°C
= 0V
A
IN
+85°C
+70°C
0.5
0
+25°C
–0.5
–1.0
–1.5
–2.0
–40°C
0°C
1m
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
1n
10n
100n
1µ
10µ
(A)
100µ
10m
I
I
REF
REF
Figure 4. VLOG vs. IREF for Multiple Temperatures (IINP = 3 µA)
Figure 7. Law Conformance Error vs. IREF for Multiple Temperatures,
Normalized to 25°C (IINP = 3 µA)
1.8
1.6
1.4
1.2
1.0
0.8
0.6
0.4
0.2
0
1.0
0.8
3mA
300µA
0.6
0.4
3µA
30µA
300nA
3µA
30nA
3nA
0.2
0
–0.2
–0.4
–0.6
–0.8
–1.0
300nA
3mA
300µA
30µA
3nA
30nA
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
I
I
INP
INP
Figure 8. Law Conformance Error vs. IINP for Multiple Values of IREF
Decade Steps from 3 nA to 3 mA
,
Figure 5. VLOG vs. IINP for Multiple Values of IREF
Decade Steps from 3 nA to 3 mA
,
Rev. B | Page 6 of 20
Data Sheet
ADL5310
1.8
1.6
1.4
1.2
1.0
1.0
0.8
3nA
30nA
0.6
300nA
30µA
0.4
3µA
300µA
0.2
3µA
3mA
0
0.8
3mA
–0.2
–0.4
–0.6
–0.8
–1.0
3nA
0.6
3mA
30nA
300µA
300nA
0.4
0.2
0
3µA
30µA
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
I
I
REF
REF
Figure 9. VLOG vs. IREF for Multiple Values of IINP
,
Figure 12. Law Conformance Error vs. IREF for Multiple Values of IINP
Decade Steps from 3 nA to 3 mA
,
Decade Steps from 3 nA to 3 mA
1.0
0.8
2.0
T
= 25°C
A
1.5
1.0
+5V, 0V
+12V, 0V
0.6
+12V, 0V
0.4
+9V, 0V
+3V, 0V
0.5
MEAN + 3σ
MEAN – 3σ
0.2
0
0
–0.2
–0.4
–0.6
–0.8
–1.0
–0.5
–1.0
–1.5
–2.0
+5V, –5V
+5V, –5V
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
I
I
INP
PD
Figure 10. Law Conformance Error vs. IINP for Various Supply Conditions
Figure 13. Law Conformance Error Distribution (3σ to Either Side of Mean)
2.0
4
T
= 0°C, 70°C
T
= –40°C, 85°C
A
A
1.5
1.0
3
2
MEAN + 3σ AT –40°C
MEAN + 3σ AT 70°C
0.5
1
MEAN + 3σ AT +85°C
0
MEAN ± 3σ AT 0°C
0
–0.5
–1.0
–1.5
–2.0
–1
–2
–3
–4
MEAN – 3σ AT 70°C
MEAN – 3σ AT –40°C
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
I
I
PD
PD
Figure 11. Law Conformance Error Distribution (3σ to Either Side of Mean)
Figure 14. Law Conformance Error Distribution (3σ to Either Side of Mean)
Rev. B | Page 7 of 20
ADL5310
Data Sheet
15
10
1.6
1.4
1.2
1.0
0.8
0.6
0.4
0.2
0
30nA
300nA
5
3nA
T-RISE < 1µs T-FALL < 1µs
T-RISE < 1µs T-FALL < 1µs
300µA TO 3mA
30µA
0
–5
30µA TO 300µA
3µA TO 30µA
–10
–15
–20
–25
–30
–35
–40
–45
300µA
T-RISE < 1µs T-FALL < 5µs
T-RISE < 5µs T-FALL < 10µs
T-RISE < 10µs T-FALL < 40µs
300nA TO 3µA
30nA TO 300nA
3mA
3µA
T-RISE < 30µs T-FALL < 80µs
3nA TO 30nA
–50
100
0
20
40
60
80
100 120 140 160 180 200
TIME (µs)
1k
10k
100k
1M
10M
100M
FREQUENCY (Hz)
Figure 15. Small Signal AC Response, IINP to VOUT (AV = 1)
(5% Sine Modulation, Decade Steps from 3 nA to 3 mA)
Figure 18. Pulse Response—IINP to VOUT (AV = 1)
in Consecutive 1-Decade Steps
1.6
1.4
1.2
1.0
0.8
0.6
0.4
0.2
0
15
10
30nA
300nA
3mA
5
T-RISE < 80µs T-FALL < 30µs
T-RISE < 40µs T-FALL < 10µs
3nA TO 30nA
0
–5
30nA TO 300nA
300µA
3nA
–10
–15
–20
–25
–30
–35
–40
–45
–50
T-RISE < 10µs T-FALL < 5µs
T-RISE < 1µs T-FALL < 1µs
T-RISE < 1µs T-FALL < 1µs
300nA TO 3µA
3µA TO 30µA
30µA TO 300µA
3µA
30µA
T-RISE < 1µs T-FALL < 1µs
300µA TO 3mA
0
20
40
60
80
100 120 140 160 180 200
TIME (µs)
100
1k
10k
100k
1M
10M
100M
FREQUENCY (Hz)
Figure 16. Small Signal AC Response, IREF to VOUT (AV = 1)
(5% Sine Modulation, Decade Steps from 3 nA to 3 mA)
Figure 19. Pulse Response—IREF to VOUT (AV = 1)
in Consecutive 1-Decade Steps
5.0
4.0
3.0
2.0
1.0
0
100
10
3nA
30nA
1
3µA
300nA
0.1
30µA
3mA
300µA
0.01
100
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
1k
10k
100k
1M
10M
FREQUENCY (Hz)
I
INP
Figure 17. Spot Noise Spectral Density at VOUT vs. Frequency (AV = 1)
for IINP in Decade Steps from 3 nA to 3 mA
Figure 20. Total Wideband Noise Voltage at VOUT vs. IINP (AV = 1)
Rev. B | Page 8 of 20
Data Sheet
ADL5310
25
20
5
4
3
15
2
10
MEAN + 3σ
1
MEAN + 3σ
5
0
0
–1
–2
–3
–4
–5
–6
MEAN – 3σ
–5
–10
–15
–20
MEAN – 3σ
–25
–40 –30 –20 –10
0
10 20 30 40 50 60 70 80 90
TEMPERATURE (°C)
–40 –30 –20 –10
0
10 20 30 40 50 60 70 80 90
TEMPERATURE (°C)
Figure 21. VREF Drift vs. Temperature (3σ to Either Side of Mean)
Normalized to 25°C
Figure 24. VINPT Drift vs. Temperature (3σ to Either Side of Mean)
Normalized to 25°C
6
5
4
3
7
6
5
4
3
2
1
MEAN + 3σ
2
1
MEAN + 3σ
0
0
–1
–2
–3
–4
–5
–6
–1
–2
–3
–4
–5
–6
MEAN – 3σ
MEAN – 3σ
–40 –30 –20 –10
0
10 20 30 40 50 60 70 80 90
TEMPERATURE (°C)
–40 –30 –20 –10
0
10 20 30 40 50 60 70 80 90
TEMPERATURE (°C)
Figure 22. Slope Drift vs. Temperature (3σ to Either Side of Mean)
Normalized to 25°C
Figure 25. Slope Mismatch Drift vs. Temperature
(VY1 – VY2, 3σ to Either Side of Mean) Normalized to 25°C
200
200
150
100
50
150
100
50
MEAN + 3σ
MEAN + 3σ
0
0
–50
–100
–150
–200
MEAN – 3σ
MEAN – 3σ
–50
–100
–150
–40 –30 –20 –10
0
10 20 30 40 50 60 70 80 90
TEMPERATURE (°C)
–40 –30 –20 –10
0
10 20 30 40 50 60 70 80 90
TEMPERATURE (°C)
Figure 26. Intercept Mismatch Drift vs. Temperature
(IZ1 – IZ2, 3σ to Either Side of Mean) Normalized to 25°C
Figure 23. Intercept Drift vs. Temperature
(3σ to Either Side of Mean) Normalized to 25°C
Rev. B | Page 9 of 20
ADL5310
Data Sheet
450
400
350
300
250
200
150
100
50
700
600
500
400
300
200
100
0
0
190
–9
–6
–3
0
3
6
9
195
200
205
210
SLOPE MISMATCH (mV/dec)
SLOPE (mV/dec)
Figure 27. Distribution of Logarithmic Slope
Figure 30. Distribution of Channel-to-Channel Slope Mismatch (VY1 – VY2)
600
500
400
300
200
100
500
400
300
200
100
0
0
–300
–200
–100
0
100
200
300
100
200
300
400
500
INTERCEPT MISMATCH (pA)
INTERCEPT (pA)
Figure 28. Distribution of Logarithmic Intercept
Figure 31. Distribution of Channel-to-Channel Intercept Mismatch (IZ1 – IZ2)
500
700
600
500
400
300
200
100
0
400
300
200
100
0
–9
–6
–3
0
3
6
9
2.46
2.48
2.50
2.52
2.54
V
– V VOLTAGE (mV)
SUM
VREF VOLTAGE (V)
INPT
Figure 29. Distribution of VREF (RL = 100 kΩ)
Figure 32. Distribution of Offset Voltage (VINPT – VSUM)
Rev. B | Page 10 of 20
Data Sheet
ADL5310
GENERAL STRUCTURE
The ADL5310 addresses a wide variety of interfacing conditions
to meet the needs of fiber optic supervisory systems and is useful
in many nonoptical applications. These notes explain the structure
of this unique style of translinear log amp. Figure 33 shows the
key elements of one of the two identical on-board log amps.
THEORY
The base-emitter voltage of a bipolar junction transistor (BJT)
can be expressed by Equation 1, which immediately shows its
basic logarithmic nature:
V
BE = kT/q ln(IC/IS)
(1)
BIAS
GENERATOR
where:
IC is the collector current.
IREF
PHOTODIODE
INPUT
V
V
BE1
TEMPERATURE
COMPENSATION
(SUBTRACT AND
DIVIDE BY T°K)
IS is a scaling current, typically only 10–17 A.
kT/q is the thermal voltage, proportional to absolute
temperature (PTAT), and is 25.85 mV at 300 K.
2.5V
VREF
CURRENT
I
REF
BE2
80kΩ
0.5V
20kΩ
COMM
I
PD
IS is never precisely defined and exhibits an even stronger temper-
ature dependence, varying by a factor of roughly a billion between
−35°C and +85°C. Thus, to make use of the BJT as an accurate
logarithmic element, both of these temperature dependencies
must be eliminated.
VSUM
44µA/dec
INP1
(INP2)
0.5V
14.2kΩ 451Ω
VRDZ
VLOG
0.5V
Q1
V
V
Q2
BE2
6.69kΩ
BE1
The difference between the base-emitter voltages of a matched
pair of BJTs, one operating at the photodiode current IPD and
the other operating at a reference current IREF, can be written as
COMM
VNEG (NORMALLY GROUNDED)
Figure 33. Simplified Schematic of Single Log Amp
V
BE1 – VBE2 = kT/q ln(IPD/IS) – kT/q ln(IREF/IS)
The photodiode current IPD is received at either Pin INP1 or
Pin INP2. The voltages at these nodes are approximately equal
to the voltage on the adjacent guard pins, VSUM, as well as reference
inputs IRF1 and IRF2, due to the low offset voltage of the JFET
operational amplifiers. Transistor Q1 converts IPD to a corre-
sponding logarithmic voltage, as shown in Equation 1. A finite
positive value of VSUM is needed to bias the collector of Q1 for
the usual case of a single-supply voltage. This is internally set to
0.5 V, one-fifth of the 2.5 V reference voltage that appears on
Pin VREF. Both VREF pins are internally shorted, as are both
VSUM pins. The resistance at the VSUM pin is nominally 16 kΩ;
this voltage is not intended as a general bias source.
= ln(10) kT/q log10(IPD/IREF
= 59.5 mV log10(IPD/IREF) (T = 300 K)
)
(2)
The uncertain, temperature-dependent saturation current, IS,
that appears in Equation 1 has therefore been eliminated. To
eliminate the temperature variation of kT/q, this difference
voltage is processed by what is essentially an analog divider.
Effectively, it puts a variable under Equation 2. The output of
this process, which also involves a conversion from voltage
mode to current mode, is an intermediate, temperature-
corrected current:
I
LOG = IY log10(IPD/IREF
)
(3)
The ADL5310 also supports the use of an optional negative supply
voltage, VN, at Pin VNEG. When VN is 0.5 V or more negative,
VSUM may be connected to ground; thus, INP1, INP2, IRF1,
and IRF2 assume this potential. This allows operation as a voltage-
input logarithmic converter by the inclusion of a series resistor
at either or both inputs. Note that the resistor setting IREF for
each channel needs to be adjusted to maintain the intercept value.
Also, note that the collector-emitter voltages of Q1 and Q2 are
the full VN and effects due to self-heating cause errors at large
input currents.
where IY is an accurate, temperature-stable scaling current that
determines the slope of the function (change in current per
decade).
For the ADL5310, IY is 44 µA, resulting in a temperature-
independent slope of 44 µA/decade for all values of IPD and IREF
This current is subsequently converted back to a voltage-mode
output, VLOG, scaled 200 mV/decade.
.
It is apparent that this output is 0 for IPD = IREF and must swing
negative for smaller values of input current. To avoid this, IREF
would need to be as small as the smallest value of IPD. Accordingly,
an offset voltage is added to VLOG to shift it upward by 0.8 V when
VRDZ is directly connected to VREF. This moves the intercept
to the left by four decades (at 200 mV/decade), from 3 μA to
300 pA:
The input-dependent VBE1 of Q1 is compared with the reference
VBE2 of a second transistor, Q2, operating at IREF. IREF is generated
externally to a recommended value of 3 µA. However, other
values over a several-decade range can be used with a slight
degradation in law conformance.
I
LOG = IY log10(IPD/IINTC
)
(4)
where IINTC is the operational value of the intercept current.
Rev. B | Page 11 of 20
ADL5310
Data Sheet
Because values of IPD < IINTC result in a negative VLOG, a negative
supply of sufficient value is required to accommodate this
situation.
Thus, the effective intercept current IINTC is only one ten-
thousandth of IREF, corresponding to 300 pA when using the
recommended value of IREF = 3 μA.
The voltage VLOG is generated by applying ILOG to an internal
resistance of 4.55 kΩ, formed by the parallel combination of a
6.69 kΩ resistor to ground and a 14.2 kΩ resistor to Pin VRDZ
(typically tied to the 2.5 V reference, VREF). At the LOG1
(LOG2) pin, the output current ILOG generates a voltage of
The slope can be reduced by attaching a resistor between the log
amp output pin, LOG1 or LOG2, and ground. This is strongly
discouraged given that the on-chip resistors do not ratio
correctly to the added resistance. In addition, it is rare that one
would wish to lower the basic slope of 10 mV/dB; if this is
needed, it should be effected at the low impedance output of the
buffer amps, which are provided to avoid such miscalibration
and to allow higher slopes to be used.
V
LOG = ILOG × 4.55 kΩ
= 44 μA × 4.55 kΩ × log10(IPD/IINTC
= VY log10(IPD/IINTC
)
(5)
)
Each buffer of the ADL5310 is essentially an uncommitted
operational amplifier with rail-to-rail output swing, good load
driving capabilities, and a typical unity-gain bandwidth of 15 MHz.
In addition to allowing the introduction of gain, using standard
feedback networks and thereby increasing the slope voltage VY,
the buffer can be used to implement multipole, low-pass filters,
threshold detectors, and a variety of other functions. Further
details on these applications can be found in the AD8304 data
sheet.
where VY = 200 mV/decade or 10 mV/dB.
Note that any resistive loading on LOG1 (LOG2) lowers this
slope and results in an overall scaling uncertainty. This is due to
the variability of the on-chip resistors compared to the off-chip
load. As a consequence, this practice is not recommended.
VLOG may also swing below ground when dual supplies (VP and
VN) are used. When VN = −0.5 V or larger, the input Pins INP1
(INP2) and IRF1 (INP2) may be positioned at ground level
simply by grounding VSUM. Care must be taken to limit the
power consumed by the input BJT devices when using a larger
negative supply, because self heating degrades the accuracy at
higher currents.
RESPONSE TIME AND NOISE CONSIDERATIONS
The response time and output noise of the ADL5310 are funda-
mentally a function of the signal current, IPD. For small currents,
the bandwidth is proportional to IPD, as shown in Figure 15. The
output low frequency voltage-noise spectral-density is a function
of IPD (see Figure 17) and increases for small values of IREF. Details
of the noise and bandwidth performance of translinear log amps
can be found in the AD8304 data sheet.
MANAGING INTERCEPT AND SLOPE
When using a single supply, VRDZ should be directly connected
to VREF to allow operation over the entire 6-decade input current
range. As noted in the Theory section, this introduces an accurate
offset voltage of 0.8 V at the LOG1 and LOG2 pins, equivalent
to four decades, resulting in a logarithmic transfer function that
can be written as
V
LOG = VY log10(104 × IPD/IREF) = VY log10(IPD/IINTC
where IINTC = IREF/104.
)
(6)
Rev. B | Page 12 of 20
Data Sheet
ADL5310
APPLICATIONS INFORMATION
5V
VPOS
COMM
665kΩ
0.5log (I
)
PD1
1nA
VREF
VRDZ
OUT1
SCL1
VSUM
10
V
OUT1
I
RF1
12kΩ
IRF1
8kΩ
2kΩ
4.7nF
BIAS
6.69kΩ
BIN1
I
V
LOG
LOG1
TEMPERATURE
COMPENSATION
VNEG
C
451Ω
FLT1
10 nF
14.2kΩ
I
PD1
INP1
0.5log (I
)
1kΩ
PD2
1nA
OUT2
SCL2
10
1nF
REFERENCE
GENERATOR
0.5V
2.5V
V
OUT2
20kΩ
80kΩ
12kΩ
COMM
IRF2
8kΩ
2kΩ
14.2kΩ
BIN2
4.7nF
BIAS
I
V
LOG
LOG2
TEMPERATURE
COMPENSATION
VNEG
C
451Ω
FLT2
10 nF
I
RF2
6.69kΩ
COMM
I
PD2
INP2
1kΩ
VSUM
VREF
VNEG
COMM
1nF
1nF
665kΩ
Figure 34. Basic Connections for Fixed Intercept Use
The ADL5310 is easy to use in optical supervisory systems and in
similar situations where a wide-ranging current is to be converted
to its logarithmic equivalent, that is, represented in decibel terms.
Basic connections for measuring a single current at each input
are shown in Figure 34, which also includes various nonessential
components, as explained next.
In addition, each input and reference pin (INP1, INP2, IRF1,
and IRF2) has a compensation network made up of a series
resistor and capacitor. The junction capacitance of the photo-
diode along with the network capacitance of the board artwork
around the input system creates a pole that varies widely with
input current. The RC network stabilizes the system by simul-
taneously reducing this pole frequency and inserting a zero to
compensate an additional pole inherent in the input system. In
general, the 1 nF, 1 kΩ network handles almost any photodiode
interface. In situations where larger active area photodiodes are
used, or when long input traces are used, the capacitor value may
need to be increased to ensure stability. Although the signal and
reference input systems are similar, additional care is required
to ensure stable operation of the reference inputs at temperature
extremes across the full current range of IRF1 (IRF2). It is recom-
mended that filter components of 4.7 nF and 2 kΩ should be
used from Pin IRF1 (IRF2) to ground. Temperature-stable compo-
nents should always be used in critical locations, such as the
compensation networks. Y5V-type chip capacitors are to be
avoided due to their poor temperature stability.
The 2 V difference in voltage between the VREF and Input Pins
INP1 and INP2, in conjunction with the external 665 kΩ resistors
RRF1 and RRF2, provides 3 µA reference currents IRF1 and IRF2 into
Pins IRF1 and IRF2. Connecting VRDZ to VREF raises the
voltage at LOG1 and LOG2 by 0.8 V, effectively lowering each
intercept current IINTC by a factor of 104 to position it at 300 pA.
A wide range of other values for IREF, from 3 nA to 3 mA, may
be used. The effect of such changes is shown in Figure 5 and
Figure 8.
Any temperature variation in RRF1 (RRF2) must be taken into account
when estimating the stability of the intercept. Also, the overall
noise increases when using very low values of IRF1 (IRF2). In fixed
intercept applications, there is little benefit in using a large reference
current, because doing so only compresses the low current end
of the dynamic range when operated from a single supply. The
capacitor between VSUM and ground is strongly recommended
to minimize the noise on this node, to reduce channel-to-channel
crosstalk, and to help provide clean reference currents.
The optional capacitor from LOG1 (LOG2) to ground forms a
single-pole, low-pass filter in combination with the 5 kΩ resis-
tance at this pin. For example, when using a CFLT of 10 nF, the
3 dB corner frequency is 3.2 kHz. Such filtering is useful in
Rev. B | Page 13 of 20
ADL5310
Data Sheet
minimizing the output noise, particularly when IPD is small.
Multipole filters are more effective in reducing the total noise;
examples are provided in the AD8304 data sheet.
Figure 35 shows the improvement in accuracy when using a
2-point calibration method. To perform this calibration, apply
two known currents, I1 and I2, in the linear operating range
between 10 nA and 1 mA. Measure the resulting output, V1 and
V2, respectively, and calculate the slope m and the intercept b:
Because the basic scaling at LOG1 (LOG2) is 0.2 V/decade, and
a 4 V swing at the buffer output would correspond to 20 decades,
it is often useful to raise the slope to make better use of the rail-
to-rail voltage range. For illustrative purposes, both channels in
Figure 34 provide a 0.5 V/decade overall slope (25 mV/dB).
Thus, using IREF = 3 μA, VLOG runs from 0.2 V at IPD = 3 nA to
1.4 V at IPD = 3 mA; the buffer output runs from 0.5 V to 3.5 V,
corresponding to a dynamic range of 120 dB (electrical, that is,
60 dB optical power).
m = (V1 – V2)/[log10(I1) – log10(I2)]
b = V1 – m × log10(I1)
(7)
(8)
The same calibration can be performed with two known optical
powers, P1 and P2. This allows for calibration of the entire
measurement system while providing a simplified relationship
between the incident optical power and VLOG voltage:
m = (V1 – V2)/(P1 – P2)
b = V1 – m × P1
(9)
(10)
Further information on adjusting the slope and intercept, using
a negative supply, and additional operations can be found in the
AD8305 data sheet.
The uncalibrated error line in Figure 35 was generated assuming
that the slope of the measured output was 200 mV/decade when
in fact it was actually 194 mV/decade. Correcting for this discre-
pancy decreased measurement error up to 3 dB.
CALIBRATION
Each channel of the ADL5310 has a nominal slope and intercept
at LOG1 (LOG2) of 200 mV/decade and 300 pA, respectively,
when configured as shown in Figure 34. These values are
untrimmed and the slope alone may vary by as much as 7.5%
over temperature. For this reason, it is recommended that a
simple calibration be done to achieve increased accuracy. While
the ADL5310 offers improved slope and intercept matching
compared to a randomly selected pair of AD8305 log amps, the
specified accuracy can only be achieved by calibrating each
channel individually.
MINIMIZING CROSSTALK
Combining two high-dynamic-range logarithmic converters in
one IC carries potential pitfalls concerning channel-to-channel
isolation. Special care must be taken in several areas to ensure
acceptable crosstalk performance, particularly when one or
both channels may operate at very low input currents. Fastidious
supply bypassing, which is also necessary for overall stability,
and careful board layout are important first steps for
minimizing crosstalk.
1.4
1.2
1.0
0.8
0.6
0.4
0.2
0
4
While the shared bias circuitry improves channel-to-channel
matching and reduces power consumption, it is also a source of
crosstalk that must be mitigated. The VSUM pins, which are inter-
nally shorted, should be bypassed with at least 1 nF to ground,
and 20 nF is recommended for operation at the lowest currents
(<30 nA). VSUM is of particular importance because it acts as a
reference voltage input for each input system, but without the
bandwidth limitation at low currents that the primary inputs incur.
Disturbances at the VSUM pin that are well within the bandwidth
of the input are tracked by the loop and do not generate distur-
bances at the output (aside from the generally minor perturbation
in reference currents caused by voltage variations at IRF1 and
IRF2).
UNCALIBRATED ERROR
3
2
MEASURED OUTPUT
1
0
CALIBRATED ERROR
–1
–2
–3
IDEAL OUTPUT
1n
10n
100n
1µ
10µ
(A)
100µ
1m
10m
I
PD
Figure 35. Using 2-Point Calibration to Increase Measurement Accuracy
For this reason, the pole frequency at VSUM, which has a 16 kΩ
typical source resistance, should be set below the minimum input
system bandwidth for the lowest input current to be encountered.
Because the low frequency noise at VSUM is also tracked by the
loop within its available bandwidth, this is also a criterion for
reducing the noise contribution at the output from the thermal
noise of the 16 kΩ source resistance at VSUM.
Rev. B | Page 14 of 20
Data Sheet
ADL5310
A 10 nF capacitor on each VSUM pin (20 nF parallel equivalent)
combined with the 16 kΩ source resistance yields a 500 Hz pole,
which is sufficiently below the bandwidth for the minimum
input current of 3 nA.
voltage, followed by differencing of the two signal levels in the
digital domain for a relative gain or absorbance measurement.
A more straightforward analog implementation includes the use
of a current mirror, as shown in Figure 37. The current mirror
is used to feed an opposite polarity replica of the cathode photo-
current of PD2 into Channel 2 of the ADL5310. This allows one
channel to be used as an absolute power meter for the optical
signal incident on PD2, while the opposite channel is used to
directly compute the log ratio of the two input signals.
Residual crosstalk disturbance is particularly problematic at the
lowest currents for two reasons. First, the loop is unable to reject
summing node disturbances beyond the limited bandwidth.
Second, the settling response at the lowest currents to any residual
disturbance is significantly slower than that for input currents
even one or two decades higher (see Figure 18).
5V
VPOS
COMM
5V
0.1µF
Φ *
OUT2
2
VSUM
12
1.2
1.0
0.8
0.6
0.4
0.2
0
ACTIVE CHANNEL OUTPUT PULSE, 1-DECADE STEP
3µA TO 30µA
ADL5310
1nF
9
I
IN2
*Φ (V) ≅ 0.2log
(
)
2
10
100pA
I
=I
6
IN2 PD2
SCL2
log
log
INP2
I
– 3nA
I
INP
1kΩ
BIN2
3
– 10nA
I
– 100nA
INP
4.7nF
INP
I
LOG2
LOG2
TEMPERATURE
COMPENSATION
1nF
0
I
– 30nA
IRF2
INP
2MΩ
–3
–6
INACTIVE CHANNEL RESPONSE
α
**
21
OUT1
SCL1
VRDZ
VREF
1kΩ
BIAS
GENERATOR
4.7nF
0
0.5
1.0
1.5
2.0
2.5
TIME (ms)
I
IN1
**α (V) ≅ 0.2log
(
)
21
10
I
PD2
Figure 36. Crosstalk Pulse Response for Various Input Current Values
I
PD2
IRF1
log
log
PD2
InGaAs PIN
Figure 36 shows the measured response of an inactive channel
(dc input) to a 1-decade current step on the input of the active
channel for several inactive channel dc current values. Additional
system considerations may be necessary to ensure adequate
settling time following a known transient when one or both
channels are operating at very low input currents.
BIN1
1kΩ
4.7nF
I
LOG1
LOG1
TEMPERATURE
COMPENSATION
1nF
5V
PD1
InGaAs PIN
I
IN1
INP1
1kΩ
COMM
COMM
0.1µF
4.7nF
VSUM
VNEG
RELATIVE AND ABSOLUTE POWER
MEASUREMENTS
1nF
Figure 37. Absolute and Relative Power Measurement Application
Using Modified Wilson Current Mirror
When properly calibrated, the ADL5310 provides two independent
channels capable of accurate absolute optical power measurements.
Often, it is desirable to measure the relative gain or absorbance
across an optical network element, such as an optical amplifier
or variable attenuator. If each channel has identical logarithmic
slopes and intercepts, this can easily be done by differencing the
output signals of each channel. In reality, channel mismatch can
result in significant errors over a wide range of input levels if
left uncompensated. Postprocessing of the signal can be used to
account for individual channel characteristics. This requires a
simple calculation of the expected input level for a measured log
The presented current mirror is a modified Wilson mirror. Other
current mirror implementations would also work, though the
modified Wilson mirror provides fairly constant performance
over temperature. It is essential to use matched pair transistors
when designing the current mirror to minimize the effects of
temperature gradients and beta mismatch.
Rev. B | Page 15 of 20
ADL5310
Data Sheet
The solution in Figure 37 is no longer subject to potential channel
mismatch issues. Individual channel slope and intercept charac-
teristics can be calibrated independently. The accuracy was verified
using a pair of calibrated current sources. The performance of
the circuit depicted in Figure 37 is shown in Figure 38 and
Figure 39. Multiple transfer functions and error plots are provided
for various power levels. The accuracy is better than 0.1 dB over
a 5-decade range. The dynamic range is slightly reduced for strong
IIN input currents. This is due to the limited available swing of
the VLOG pin and can be recovered through careful selection
of input and output optical tap coupling ratios.
CHARACTERIZATION METHODS
During the characterization of the ADL5310, the device was
treated as a precision current-input logarithmic converter, because
it is impractical to generate accurate photocurrents by illumin-
ating a photodiode. The test currents were generated by using
either a well calibrated current source, such as the Keithley 236,
or a high value resistor from a voltage source to the input pin.
Great care is needed when using very small input currents. For
example, the triax output connection from the current generator
was used with the guard tied to VSUM. The input trace on the
PC board was guarded by connecting adjacent traces to VSUM.
1.8
These measures are needed to minimize the risk of leakage current
paths. With 0.5 V as the nominal bias on the INP1 (INP2) pin, a
leakage-path resistance of 1 GΩ to ground would subtract 0.5 nA
from the input, which amounts to a −1.6 dB error for a 3 nA source
current. Additionally, the very high sensitivity at the input pins
and the long cables commonly needed during characterization
allow 60 Hz and RF emissions to introduce substantial measure-
ment errors. Careful guarding techniques are essential to reducing
the pickup of these spurious signals.
1.6
φ
WHEN I = 100µA
PD1
2
1.4
1.2
1.0
0.8
0.6
0.4
0.2
0
α
FOR MULTIPLE VALUES OF I
PD1
21
Additional information, including test setups, can be found in
the AD8305 and ADL5306 data sheets.
–20
–10
0
10
LOG [I
20
/I
30
40
50
60
] (dB)
10 PD1 PD2
Figure 38. Absorbance and Absolute Power Transfer Functions for
Wilson Mirror ADL5310 Combination
0.5
0.4
0.3
I
= 1µA
PD1
0.2
0.1
0
I
= 10µA
–0.1 PD1
–0.2
–0.3
I
= 100µA
PD1
0
–0.4
–0.5
–40
–30 –20 –10
10
20
30
40
50
60
LOG [I
/I
] (dB)
10 PD1 PD2
Figure 39. Log Conformance for Wilson Mirror ADL5310 Combination,
Normalized to 10 mA Channel 1 Input Current, IIN1
Rev. B | Page 16 of 20
Data Sheet
ADL5310
EVALUATION BOARD
An evaluation board is available for the ADL5310 (Figure 40 shows the schematic). It can be configured for a wide variety of experiments.
The gain of each buffer amp is factory-set to unity, providing a slope of 200 mV/dec, and the intercept is set to 300 pA. Table 4 describes
the various configuration options.
Table 4. Evaluation Board Configuration Options
Component
Function
Default Condition
P1
Supply Interface. Provides access to the Supply Pins VNEG, COMM, and
VPOS.
P1 = installed
P2, R1, R3, R8, R9,
Monitor Interface. By adding 0 Ω resistors to R1, R3, R8, R9, R17, R22, and
P2 = not installed
R17, R22, R25, R30 R25, the VRDZ, VREF, VSUM, BIN1, BIN2, OUT1, and OUT2 pin voltages
can be monitored using a high impedance probe. VBIAS allows for the
external bias voltages to be applied to J1 and J2. If R30 = 0 Ω,
VBIAS = VREF.
R1 = R3 = R8 = open (size 0402)
R9 = R17 = open (size 0402)
R22 = R25 = R30 = open (size 0402)
R5, R6, R7, R16,
R18, R19, R20,
R21, R31, R32, C4,
C14, C15, C16,
C19, C20
Buffer Amplifier/Output Interface. The logarithmic slopes of the ADL5310
can be altered using each buffer’s gain-setting resistors, R5 and R6, and
R18 and R19. R7, R16, R31, R32, C19, and C20 allow for variation in the
buffer loading. R20, R21, C4, C14, C15, and C16 are provided for a variety
of filtering applications.
R5 = R19 = 0 Ω (size 0402)
R7 = R16 = 0 Ω (size 0402)
R20 = R21 = 0 Ω (size 0402)
R6 = R18 = open (size 0402)
R31 = R32 = open (size 0402)
C4 = C14 = open (size 0402)
C19 = C20 = open (size 0402)
C15 = C16 = open (size 0402)
LOG1 = OUT1 = installed
LOG2 = OUT2 = installed
R2, R28, R29
Intercept Adjustment. The voltage dropped across Resistors R28 and R29
determines the intercept reference current for each log amp, nominally
set to 3 µA using a 665 kΩ 1% resistor. R2 can be used to adjust the output
offset voltage at the LOG1 and LOG2 outputs.
R28 = R29 = 665 kΩ (size 0402)
R2 = 0 Ω (size 0402)
R4, R10, R11, C2,
C3, C5, C6, C8, C9
Supply Decoupling.
C2 = C5 = C9 = 100 pF (size 0402)
C3 = C6 = C8 = 0.01 µF (size 0402)
R4 = R10 = R11 = 0 Ω (size 0402)
C1, C7
Filtering VSUM.
C1 = C7 = 0.01 µF (size 0402)
R12, R13, R14,
R15, C10, C11,
C12, C13
Input Compensation. Provides essential HF compensation at the Input
Pins INP1, INP2, IRF1, and IRF2.
R12 = R15 = 1 kΩ (size 0402)
R13 = R14 = 2 kΩ (size 0402)
C10 = C13 = 1 nF (size 0402)
C11 = C12 = 4.7 nF (size 0402)
IREF, INPT
J1, J2
Input Interface. The test board is configured to accept current through the IREF = INPT = installed
SMA connectors labeled INP1 and INP2. Through-holes are provided to
connect photodiodes in place of the INP1 and INP2 SMAs for optical
interfacing. By removing R28 (R29 for INP2), a second current can be
applied to the IRF1 (IRF2 for INP2) input (also SMA) for evaluating the
ADL5310 in log ratio applications.
SC-Style Photodiode. Provides for the direct mounting of SC-style
photodiodes.
J1 = J2 = open
Rev. B | Page 17 of 20
ADL5310
Data Sheet
VRDZ
VNEG
C3 0.01µF
R7 0Ω
OUT1
OUT1
R32
OPEN
C20
OPEN
R3
OPEN
R2
3
R4
0Ω
C2
2
1
J2
PHOTODIODE
0Ω
VBIAS
R29
R8 OPEN
C4 OPEN
100pF
21
R5 0Ω
C1 0.01µF
R28
C16
OPEN
24
23
22
20
19
665kΩ 665kΩ
R20
R24
LOG1
LOG1
0Ω
0Ω
R1
R6
VSUM
INP1
1
2
3
4
5
6
18
17
16
15
14
13
VSUM
INP1
IRF1
SCL1
BIN1
OPEN
OPEN
R26 0Ω
R27 0Ω
R25
BIN1
LOG2
BIN2
LOG1
LOG2
BIN2
ADL5310
OPEN
IRF1
IRF2
INP2
IRF2
R21
R22
INP2
VSUM
0Ω
OPEN
R23
R18
C14
OPEN
C15
SCL2
OPEN
OPEN
LOG2
0Ω
R19
0Ω
7
8
9
10
11
12
R15 R14 R13 R12
1kΩ 2kΩ 2kΩ 1kΩ
R9
OPEN
1
2
3
4
5
6
OUT1
VREF
C5 100pF
C9 100pF
R17
OPEN
C13 C12 C11 C10
1nF 4.7nF 4.7nF 1nF
BIN1
LOG1
LOG2
BIN2
R11
0Ω
C8 0.01µF
R10
0Ω
C6 0.01µF
OUT2
OUT2
R16 0Ω
3
R31
OPEN
C19
OPEN
2
1
J1
VBIAS
PHOTODIODE
AGND
2
OUT2
VPOS
1
3
VNEG
7
8
VREF
C7 0.01µF
R30 OPEN
P1
VBIAS
P2
Figure 40. Evaluation Board Schematic
Rev. B | Page 18 of 20
Data Sheet
ADL5310
Figure 41. Component-Side Layout
Figure 42. Component-Side Silkscreen
Rev. B | Page 19 of 20
ADL5310
Data Sheet
OUTLINE DIMENSIONS
DETAIL A
(JEDEC 95)
4.10
4.00 SQ
3.90
0.30
0.25
0.20
PIN 1
INDICATOR
PIN 1
24
19
18
INDIC ATOR AREA OPTIONS
(SEE DETAIL A)
1
0.50
BSC
2.20
2.10 SQ
2.00
EXPOSED
PAD
13
12
6
7
0.50
0.40
0.30
0.20 MIN
TOP VIEW
SIDE VIEW
BOTTOM VIEW
FOR PROPER CONNECTION OF
THE EXPOSED PAD, REFER TO
THE PIN CONFIGURATION AND
FUNCTION DESCRIPTIONS
0.80
0.75
0.70
0.05 MAX
0.02 NOM
COPLANARITY
0.08
SECTION OF THIS DATA SHEET.
SEATING
PLANE
0.203 REF
COMPLIANT TO JEDEC STANDARDS MO-220-WGGD-8.
Figure 43. 24-Lead Lead Frame Chip Scale Package [LFCSP]
4 mm × 4 mm Body and 0.75 mm Package Height
(CP-24-10)
Dimensions shown in millimeters
ORDERING GUIDE
Model
Temperature Range
Package Description
Package Option
ADL5310ACPZ-REEL7
ADL5310-EVALZ
–40°C to +85°C
24-Lead Lead Frame Chip Scale Package [LFCSP]
Evaluation Board
CP-24-10
©2003–2018 Analog Devices, Inc. All rights reserved. Trademarks and
registered trademarks are the property of their respective owners.
D04415-0-4/18(B)
Rev. B | Page 20 of 20
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