Cooling an array detector with a built-in thermoelectric cooler
(TEC) is an effective way to reduce dark current and noise as well
as to enhance the dynamic range and detection limit. The graph below
shows the dark current and noise for an un-cooled versus cooled CCD
detector at an integration time of 60 s. When operating at room
temperature, the dark current nearly saturates the un-cooled CCD.
When the CCD is cooled down only to 10
°C
by the TEC, the dark current is reduced by about four times and the
dark shot noise is reduced by about two times. This makes the CCD
capable of operating at a long integration time to detect weak
optical signals. When a CCD based spectrometer is involved in
non-demanding high light level situations such as LED measurement
applications, the dark noise reduction due to TE cooling is minimal
because of the relatively short integration time used. The
temperature regulation of detector arrays under these conditions
will provide benefit for long term baseline stability.
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