AD8033/AD8034
Rev. D | Page 19 of 24
APPLICATIONS INFORMATION
HIGH SPEED PEAK DETECTOR
The low input bias current and high bandwidth of the AD8033/
AD8034 make the parts ideal for a fast settling, low leakage peak
detector. The classic fast-low leakage topology with a diode in
the output is limited to ~1.4 V p-p maximum in the case of the
AD8033/AD8034 because of the protection diodes across the
inputs, as shown in Figure 54.
AD8033/
AD8034
V
IN
~1.4V p-p MAX
V
OUT
02924-054
Figure 54. High Speed Peak Detector with Limited Input Range
Using the AD8033/AD8034, a unity gain peak detector can
be constructed that captures a 300 ns pulse while still taking
advantage of the low input bias current and wide common-
mode input range of the AD8033/AD8034, as shown in Figure 55.
Using two amplifiers, the difference between the peak and the
current input level is forced across R2 instead of either amplifier’s
input pins. In the event of a rising pulse, the first amplifier
compensates for the drop across D2 and D3, forcing the voltage
at Node 3 equal to Node 1. D1 is off and the voltage drop across
R2 is zero. Capacitor C3 speeds up the loop by providing the
charge required by the input capacitance of the first amplifier,
helping to maintain a minimal voltage drop across R2 in the
sampling mode. A negative going edge results in D2 and D3
turning off and D1 turning on, closing the loop around the
first amplifier and forcing V
OUT
− V
IN
across R2. R4 makes
the voltage across D2 zero, minimizing leakage current and
kickback from D3 from affecting the voltage across C2.
The rate of the incoming edge must be limited so that the output
of the first amplifier does not overshoot the peak value of V
IN
before the output of the second amplifier can provide negative
feedback at the summing junction of the first amplifier. This
is accomplished with the combination of R1 and C1, which
allows the voltage at Node 1 to settle to 0.1% of V
IN
in 270 ns.
The selection of C2 and R3 is made by considering droop
rate, settling time, and kickback. R3 prevents overshoot from
occurring at Node 3. The time constants of R1, C1 and R3, C2
are roughly equal to achieve the best performance. Slower time
constants can be selected by increasing C2 to minimize droop
rate and kickback at the cost of increased settling time. R1 and
C1 should also be increased to match, reducing the incoming
pulses effect on kickback.
AD8034
1/2
C3
10pF
R2
1k
R1
1k
AD8034
1/2
–V
S
+V
S
C1
39pF/
120pF
LS4148
V
IN
R5
49.9
D1
4.7pF
C4
R4
6k
D3
LS4148
–V
S
+V
S
LS4148
R3
200
C2
180pF/
560pF
V
OUT
D2
0
2924-056
Figure 55. High Speed, Unity Gain Peak Detector Using AD8034
AD8033/AD8034
Rev. D | Page 20 of 24
1V/DIV 100ns/DIV
02924-055
OUTPUT
INPUT
2
Figure 56. Peak Detector Response 4 V, 300 ns Pulse
Figure 56 shows the peak detector in Figure 55 capturing a
300 ns, 4 V pulse with 10 mV of kickback and a droop rate of
5 V/s. For larger peak-to-peak pulses, increase the time constants
of R1, C1 and R3, C3 to reduce overshoot. The best droop rate
occurs by isolating parasitic resistances from Node 3, which can
be accomplished using a guard band connected to the output of the
second amplifier that surrounds its summing junction (Node 3).
Increasing both time constants by a factor of 3 permits a larger
peak pulse to be captured and increases the output accuracy.
1V/DIV 200ns/DIV
02924-057
OUTPUT
INPUT
2
Figure 57. Peak Detector Response 5 V, 1 μs Pulse
Figure 57 shows a 5 V peak pulse being captured in 1 µs with
less than 1 mV of kickback. With this selection of time constants,
up to a 20 V peak pulse can be captured with no overshoot.
ACTIVE FILTERS
The response of an active filter varies greatly depending on the
performance of the active device. Open-loop bandwidth and
gain, along with the order of the filter, determines the stop-band
attenuation as well as the maximum cutoff frequency, while
input capacitance can set a limit on which passive components
are used. Topologies for active filters are varied, and some are
more dependent on the performance of the active device than
others are.
The Sallen-Key topology is the least dependent on the active
device, requiring that the bandwidth be flat to beyond the stop-
band frequency because it is used simply as a gain block. In the
case of high Q filter stages, the peaking must not exceed the open-
loop bandwidth and the linear input range of the amplifier.
Using an AD8033/AD8034, a 4-pole cascaded Sallen-Key filter
can be constructed with f
C
= 1 MHz and over 80 dB of stop-band
attenuation, as shown in Figure 58.
–V
S
+V
S
C2
10pF
–V
S
+V
S
V
IN
R1
4.22k
AD8034
1/2
AD8034
1/2
R2
6.49k
R5
49.9
C1
27pF
C3
33pF
R4
4.99k
R3
4.99k
C4
82pF
V
OUT
02924-058
Figure 58. 4-Pole Cascade Sallen-Key Filter
Component values are selected using a normalized cascaded,
2-stage Butterworth filter table and Sallen-Key 2-pole active
filter equations. The overall frequency response is shown in
Figure 59.
10M1M10k
FREQUENCY (Hz)
–100
REF LEVEL (dB)
–90
–80
–70
–60
–50
–40
–30
–20
–10
0
100k
0
2924-059
Figure 59. 4-Pole Cascade Sallen-Key Filter Response
AD8033/AD8034
Rev. D | Page 21 of 24
When selecting components, the common-mode input capacitance
must be taken into consideration.
Filter cutoff frequencies can be increased beyond 1 MHz using the
AD8033/AD8034 but limited open-loop gain and input impedance
begin to interfere with the higher Q stages. This can cause early
roll-off of the overall response.
Additionally, the stop-band attenuation decreases with decreasing
open-loop gain.
Keeping these limitations in mind, a 2-pole Sallen-Key Butterworth
filter with f
C
= 4 MHz can be constructed that has a relatively
low Q of 0.707 while still maintaining 15 dB of attenuation an
octave above f
C
and 35 dB of stop-band attenuation. The filter
and response are shown in Figure 60 and Figure 61, respectively.
–V
S
+V
S
V
IN
R1
2.49k
C3
22pF
V
OUT
AD8033
R2
2.49k
R5
49.9
C1
10pF
02924-060
Figure 60. 2-Pole Butterworth Active Filter
100M100k 1M
FREQUENCY (Hz)
–45
GAIN (dB)
–40
–35
–30
–25
–20
–15
–10
–5
0
5
0
2924-061
10M
Figure 61. 2-Pole Butterworth Active Filter Response
WIDEBAND PHOTODIODE PREAMP
Figure 62 shows an I/V converter with an electrical model of a
photodiode.
The basic transfer function is
FF
F
PHOTO
OUT
RsC
R
I
V
+
×
=
1
where I
PHOTO
is the output current of the photodiode, and the
parallel combination of R
F
and C
F
sets the signal bandwidth.
C
S
R
SH
= 10
11
V
B
I
PHOTO
02924-062
R
F
C
F
V
OUT
C
M
R
F
C
M
C
D
C
F
+ C
S
Figure 62. Wideband Photodiode Preamp
The stable bandwidth attainable with this preamp is a function
of R
F
, the gain bandwidth product of the amplifier, and the total
capacitance at the summing junction of the amplifier, including
C
S
and the amplifier input capacitance. R
F
and the total capacitance
produce a pole in the loop transmission of the amplifier that
can result in peaking and instability. Adding C
F
creates a zero
in the loop transmission that compensates for the effect of the
pole and reduces the signal bandwidth. It can be shown that the
signal bandwidth resulting in a 45°phase margin (f
(45)
) is defined
by the expression
S
F
CR
CR
f
f
××π
=
2
)45(
where:
f
CR
is the amplifier crossover frequency.
R
F
is the feedback resistor.
C
S
is the total capacitance at the amplifier summing junction
(amplifier + photodiode + board parasitics).
The value of C
F
that produces f
(45)
is
CR
F
S
F
fR
C
C
××π
=
2
The frequency response in this case shows about 2 dB of
peaking and 15% overshoot. Doubling C
F
and cutting the
bandwidth in half results in a flat frequency response, with
about 5% transient overshoot.

AD8034ARTZ-R2

Mfr. #:
Manufacturer:
Analog Devices Inc.
Description:
Operational Amplifiers - Op Amps SOT23 Hi-Speed Dual FET Input Amplifier
Lifecycle:
New from this manufacturer.
Delivery:
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