Data Sheet
Page 14 ams Datasheet 
Document Feedback [v1-00] 2016-Jul-13
TCS3200, TCS3210 − Application Information
The output goes high upon the next subsequent pulse of the 
principal frequency, beginning a new valid period. This 
minimizes the time delay between a change on the input lines 
and the resulting new output period. The response time to an 
input programming change or to an irradiance step change is 
one period of new frequency plus 1μs. The scaled output 
changes both the full-scale frequency and the dark frequency 
by the selected scale factor.
The frequency-scaling function allows the output range to be 
optimized for a variety of measurement techniques. The 
scaled-down outputs may be used where only a slower 
frequency counter is available, such as low-cost 
microcontroller, or where period measurement techniques are 
used.
Measuring the Frequency
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.
Output data can be collected at a rate of twice the output 
frequency or one data point every microsecond for full-scale 
output. Period measurement requires the use of a fast reference 
clock with available resolution directly related to reference 
clock rate. Output scaling can be used to increase the resolution 
for a given clock rate or to maximize resolution as the light input 
changes. Period measurement is used to measure rapidly 
varying light levels or to make a very 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.










