TSL245RSM TAOS [TEXAS ADVANCED OPTOELECTRONIC SOLUTIONS], TSL245RSM Datasheet - Page 4
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TSL245RSM
Manufacturer Part Number
TSL245RSM
Description
INFRARED LIGHT-TO-FREQUENCY CONVERTER
Manufacturer
TAOS [TEXAS ADVANCED OPTOELECTRONIC SOLUTIONS]
Datasheet
1.TSL245RSM.pdf
(10 pages)
TSL245R
INFRARED LIGHT-TO-FREQUENCY CONVERTER
TAOS060D − SEPTEMBER 2007
Power-supply considerations
Device Operational Details
Output interface
Measuring the frequency
4
Copyright E 2007, TAOS Inc.
Power-supply lines must be decoupled by a 0.01-μF to 0.1-μF capacitor with short leads placed close to the
TSL245R (Figure 5). A low-noise power supply is required to minimize jitter on output pulse.
The frequency at the output pin (OUT) is given by:
where:
f
represents a light-independent term in the total output frequency f
can be a significant portion of f
any given device over the full output range, the value of f
later subtracted from subsequent light measurement (see Figure 1).
The output of the device is designed to drive a standard TTL or CMOS logic input over short distances. If lines
greater than 12 inches are used on the output, a buffer or line driver is recommended.
The choice of interface and measurement technique depends on the desired resolution and data-acquisition
rate. For maximum data-acquisition rate, period-measurement techniques are used.
Period measurement requires the use of a fast reference clock with available resolution directly related to
reference-clock rate. The technique is employed to measure rapidly varying light levels or to make a fast
measurement of a constant light source.
Maximum resolution and accuracy may be obtained using frequency-measurement, pulse-accumulation,
or integration techniques. Frequency measurements provide the added benefit of averaging out random- or
high-frequency variations (jitter) resulting from noise in the light signal. Resolution is limited mainly by available
counter registers and allowable measurement time. Frequency measurement is well suited for slowly varying
or constant light levels and for reading average light levels over short periods of time. Integration, the
accumulation of pulses over a very long period of time, can be used to measure exposure — the amount of light
present in an area over a given time period.
D
is an output frequency resulting from leakage currents. As shown in the equation above, this frequency
f
f
R
E
O
D
e
e
is the output frequency
is the output frequency for dark condition (E
is the device responsivity for a given wavelength of light given in kHz/(μW/cm
is the incident irradiance in μW/cm
0.1 μF
Figure 5. Typical TSL245R Interface to a Microcontroller
f
O
O
. The dark frequency is temperature dependent. For optimum performance of
= f
APPLICATION INFORMATION
TSL245R
D
r
V
+ (R
DD
2
1
e
) (E
www.taosinc.com
2
e
)
3
e
= 0)
D
should be measured (in the absence of light) and
Timer / Port
O
. At very low light levels, this dark frequency
MCU
r
The LUMENOLOGY r Company
2
)