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The nature of photoconductive effects at wavelengths longer than 100 μ is discussed with particular reference to n-type InSb in (a) zero magnetic field, (b) magnetic fields too low to produce magneto-optical resonance absorption, and (c) large magnetic fields. The performance of practical detectors using these effects is described and is compared with that of other submillimeter detectors.
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E H Putley (1965) studied this question.
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