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參數資料
型號: ADL5317ACPZ-REEL7
廠商: Analog Devices Inc
文件頁數: 9/16頁
文件大小: 541K
描述: IC CURRENT MONITOR 16LFCSP
設計資源: Interfacing ADL5317 High Side Current Mirror to a Translinear Logarithmic Amplifier in an Avalanche Photodiode Power Detector
標準包裝: 1
功能: 電流監控器
檢測方法: 高端
輸入電壓: 10 V ~ 80 V
工作溫度: -40°C ~ 85°C
安裝類型: 表面貼裝
封裝/外殼: 16-VFQFN 裸露焊盤,CSP
供應商設備封裝: 16-LFCSP-VQ
包裝: 標準包裝
產品目錄頁面: 772 (CN2011-ZH PDF)
其它名稱: ADL5317ACPZ-REEL7DKR
 
ADL5317
 
Rev. 0 | Page 9 of 16
THEORY OF OPERATION
The ADL5317 is designed to address the need for high voltage
bias control and precision optical power monitoring in optical
systems using avalanche photodiodes. It is optimized for use
with the Analog Devices, Inc. family of translinear logarithmic
amplifiers that take advantage of the wide input current range
of the ADL5317. This arrangement allows the anode of the
photodiode to connect directly to a transimpedance amplifier
for the extraction of the data stream without need for a separate
optical power monitoring tap. Figure 19 shows the basic
connections for the ADL5317.
1
FALT
2
V
SET
3
4
11
IPDM
12
NC
10
NC
9
GARD
5
6
7
8
15
16
14
13
ADL5317
FALT
VSET
VPLV
VPHV
MIRROR CURRENT
OUTPUT
0.01?/SPAN>F
APD
1nF
1k?/SPAN>
I
APD
0.1?/SPAN>F
0.01?/SPAN>F
HIGH VOLTAGE
SUPPLY
0?/SPAN>
LOW VOLTAGE
SUPPLY
10k?/SPAN>
0?/SPAN>
0.01?/SPAN>F
0.1?/SPAN>F
 
Figure 19. Basic Connections 
At the heart of the ADL5317 is a precision attenuating current
mirror with a voltage following characteristic that provides
precision biasing at the monitor input. This architecture uses a
JFET-input amplifier to drive the bipolar mirror and maintain
stable V
APD
 voltage, while offering very low leakage current at
the VAPD pin. The mirror attenuates the current sourced
through VAPD by a factor of 5 to limit power dissipation under
high voltage operation and delivers the mirrored current to the
IPDM monitor output pin. Proprietary mirroring and cascoding
techniques maintain the linearity vs. the input current and
stability of the mirror ratio over a very wide range of supply and
V
APD
 voltages.
BIAS CONTROL INTERFACE
In the linear operating mode, the voltage at VAPD is referenced
to ground, and follows the simplified equation
V
APD
 = 30 ?V
SET
GARD is driven to the same potential as VAPD for use in
shielding the highly sensitive VAPD pin from leakage currents.
The GARD and VAPD pins are clamped to within approxi-
mately 40 V below the VPHV supply to prevent internal device
breakdowns, and VAPD is clamped to within a volt of GARD.
The VAPD adjustment range for a given high voltage supply,
VPHV, is limited to approximately 33 V (or less, for V
PHV
 <
41 V). For example, VAPD is specified from 40 V to 73.5 V for
a 75 V supply, and 6 V (the minimum allowed) to 28.5 V for a
30 V supply. When VAPD is driven to its lower clamp voltage
via the VSET pin, the mirror can continue to operate, but the
VAPD bias voltage no longer responds to incremental changes
in VSET.
GARD INTERFACE
The GARD pins primarily shield the VAPD trace from leakage
currents and filter noise from the bias control interface. GARD
is driven by the VSET amplifier through a 20 k?resistor. This
resistor forms an RC network with an external capacitor from
GARD to ground that filters the thermal noise of the amplifiers
feedback network and provides additional power supply
rejection. The series components, RCOMP and CCOMP, shown in
Figure 20, are necessary to ensure essential high frequency
compensation at the VAPD input pin over the full operating
range of the ADL5317.
V
SET
 AMPLIFIER
GARD
C
GRD
ADL5317
X30
VAPD
C
COMP
R
COMP
20k?/SPAN>
 
Figure 20. Filtering VAPD Using the GARD Interface
The cutoff frequency of the GARD interface for small signals
and noise is defined by
GRD
3dB
C
F
?/DIV>
?/DIV>
=
k?/DIV>
20
2?/DIV>
1
 
where:
F
3dB
 is the cutoff frequency of the low-pass filter formed by the
on-board 20 k?and C
GRD
.
C
GRD
 is the filter capacitor installed from GARD to ground.
A larger value for C
GRD
 (up to approximately 0.01 糉) provides
superior noise performance at the lowest input current levels,
but also slows the response time to changes in VSET.
The pull-up of the VSET amplifier is limited to approximately
2.5 mA, resulting in a slew limited region for large signals,
followed by an RC decay for the final 700 mV. This decay
corresponds to the above single-pole equation. The pull-down
of the V
SET
 amplifier is largely resistive, equivalent to
approximately 90 k?in parallel with 70 糀 to ground.
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