Tsop 48
Tsop 48
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IR Receiver Modules for Remote Control Systems
DESCRIPTION
This IR receiver series is optimized for long burst remote
control systems in different environments. The customer
can chose between different IC settings (AGC variants), to
find the optimum solution for his application. The higher the
AGC, the better noise is suppressed, but the lower the code
compatibility.
The devices contain a PIN diode and a preamplifier
assembled on a lead frame. The epoxy package contains an
IR filter. The demodulated output signal can be directly
connected to a microprocessor for decoding. These
components have not been qualified to automotive
specifications.
FEATURES
• Individual IC settings to reach maximum
performance
• Immunity against noise (lamps, LCD TV, Wi-Fi)
LINKS TO ADDITIONAL RESOURCES • Low supply current
• Photo detector and preamplifier in one package
Product Page Marking Packages Holders Bends and Cuts • Supply voltage: 2.0 V to 5.5 V
• Material categorization:
for definitions of compliance please see
www.vishay.com/doc?99912
APPLICATIONS
• Infrared remote control systems
BLOCK DIAGRAM
VS
30 kΩ
OUT
Band Demo-
Input AGC
pass dulator
GND
PIN Control circuit
16833-22
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TSOP22.., TSOP24.., TSOP48.., TSOP44..
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MECHANICAL DATA ORDERING CODE
Pinning for TSOP44.., TSOP48..: TSOP2..., TSOP4... - 2160 pieces in tubes
1 = OUT, 2 = GND, 3 = VS
Pinning for TSOP22.., TSOP24..: APPLICATION CIRCUIT
1 = OUT, 2 = VS, 3 = GND 17170-14
R1
Transmitter IR receiver
with VS + VS
TSALxxxx
C1
Circuit
µC
OUT
VO
GND GND
PARTS TABLE
LEGACY, FOR RECOMMENDED FOR
AGC
LONG BURST REMOTE CONTROLS (AGC2) LONG BURST CODES (AGC4)
30 kHz TSOP4830 TSOP2230 TSOP4430 TSOP2430
33 kHz TSOP4833 TSOP2233 TSOP4433 TSOP2433
Carrier 36 kHz TSOP4836 TSOP2236 TSOP4436 (1)(2)(3) TSOP2436 (1)(2)(3)
frequency 38 kHz TSOP4838 TSOP2238 TSOP4438 (4)(5)(6)(9)(10) TSOP2438 (4)(5)(6)(9)(10)
40 kHz TSOP4840 (8) TSOP2240 (8) TSOP4440 TSOP2440
56 kHz TSOP4856 (11) TSOP2256 (11) TSOP4456 (6)(7) TSOP2456 (6)(7)
Package Mold
Pinning 1 = OUT, 2 = GND, 3 = VS 1 = OUT, 2 = VS, 3 = GND 1 = OUT, 2 = GND, 3 = VS 1 = OUT, 2 = VS, 3 = GND
Dimensions (mm) 6.0 W x 6.95 H x 5.6 D
Mounting Leaded
Application Remote control
(1) RC-5 (2) RC-6 (3) Panasonic (4) NEC (5) Sharp (6) r-step (7) Thomson RCA
Best choice for (8) Sony (9) Mitsubishi (10) Sejin 4PPM (11) Cisco
• Narrow optical filter: www.vishay.com/doc?81590
Special options
• Wide optical filter: www.vishay.com/doc?82726
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t t
600 µs 600 µs
tpi (1)
T t = 60 ms
(1)
tpi ≥ 10/f0
94 8134
Output Signal 16110-12 Output Signal, (see Fig. 4)
VO (2) VO
7/f0 < td < 13/f0
(3)
VOH tpi - 4/f0 < tpo < tpi + 4/f0 VOH
VOL
VOL
td (2) tpo (3) t
t
t on t off
0.80
0.6
0.70
1000 1000
0.60 0.5
toff
2nd line
2nd line
1st line
1st line
2nd line
2nd line
Fig. 2 - Pulse Length and Sensitivity in Dark Ambient Fig. 4 - Output Pulse Diagram
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Axis Title
Axis Title
1.0 10000
1.2 10000
f = 38 kHz, Ee = 2 mW/m2
0.9
Ee min./Ee - Relative Responsivity
2nd line
2nd line
1st line
2nd line
1st line
2nd line
0.6 AGC 2
0.5
0 10 0.1
0.7 0.8 0.9 1.0 1.1 1.2 1.3
0 10
16925 f/f0 - Relative Frequency
0 20 40 60 80 100 120 140
Burst Length (Number of Cycles/Burst)
Fig. 5 - Frequency Dependence of Responsivity Fig. 8 - Max. Envelope Duty Cycle vs. Burst Length
2nd line
1st line
1st line
2nd line
2nd line
1
0.2
100 100
0.1
0 10 0 10
0.01 0.1 1 10 100 -30 -10 10 30 50 70 90
Ee - Ambient DC Irradiance (W/m2) Tamb - Ambient Temperature (°C)
0.9
S(λ)rel. - Relative Spectral Sensitivity
0.7
0.8
0.6
0.7
1000 1000
0.5 f = f0 0.6
2nd line
2nd line
1st line
1st line
2nd line
2nd line
f = 30 kHz
0.4 0.5
f = 10 kHz
0.3 f = 100 Hz 0.4
100 100
0.3
0.2
0.2
0.1 0.1
0 10 0 10
1 10 100 1000 750 850 950 1050 1150
∆VS RMS - AC Voltage on DC Supply Voltage (mV) 23180 λ - Wavelength (nm)
Fig. 7 - Sensitivity vs. Supply Voltage Disturbances Fig. 10 - Relative Spectral Sensitivity vs. Wavelength
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Axis Title
0° 10° 20° 0.8 10000
30°
0.6
40° 1000
1.0 0.5
2nd line
2nd line
1st line
0.9 50° 0.4
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SUITABLE DATA FORMAT
This series is designed to suppress spurious output pulses Axis Title
7 10000
due to noise or disturbance signals. The devices can
distinguish data signals from noise due to differences in 6
frequency, burst length, and envelope duty cycle. The data
signal should be close to the device’s band-pass center 5
IR Signal Amplitude
1000
frequency (e.g. 38 kHz) and fulfill the conditions in the table
2nd line
4
1st line
below.
2nd line
When a data signal is applied to the product in the 3
presence of a disturbance, the sensitivity of the receiver 100
is automatically reduced by the AGC to insure that no 2
spurious pulses are present at the receiver’s output. Some
1
examples which are suppressed are:
• DC light (e.g. from tungsten bulbs sunlight) 0 10
0 5 10 15 20
• Continuous signals at any frequency
16920 Time (ms)
• Strongly or weakly modulated patterns from fluorescent
lamps with electronic ballasts (see Fig. 13 or Fig. 14). Fig. 13 - IR Disturbance from Fluorescent Lamp
With Low Modulation
• 2.4 GHz and 5 GHz Wi-Fi
Axis Title
40 10000
20
IR Signal Amplitude
1000
0
2nd line
2nd line
1st line
-20
100
-40
-60 10
0 5 10 15 20
16921 Time (ms)
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PACKAGE DIMENSIONS in millimeters
3.9
6
5.3
6.95
8.25
(5.55)
30.5 ± 0.5
0.85 max.
1
0.89
0.5 max.
2.54 nom.
1.3
0.7 max.
4.1
2.54 nom.
5.6
marking area
Not indicated tolerances ± 0.2
technical drawings
according to DIN
specifications
R 2.5
Drawing-No.: 6.550-5169.01-4
Issue: 9; 03.11.10
13655
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