1 May 1994 Photoresponse of low-background extrinsic infrared detector arrays
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The operation of low-background lR extrinsic photoconductor detectors and detector arrays is essentially dependent on the process of spreading time-dependent photocurrent, which is due to low non-steady-state screening of the electric charges in the detectors. The spreading leads to an increase in the photoresponse time, an essential difference between the non-steady-state photocurrents in the circuits of the source contacts injecting free-charge carriers into the detectors and those in the circuits of the contacts that serve as drains for the carriers, and a high non-steady-state cross talk in the detector arrays. The results of the experimental study of all these effects and some others in 36- and 48-element linear arrays (Si:Ga) as well as their theoretical description are presented. The theory developed is in satisfactory agreement with the experimental data. Some consequences of the results obtained, which are important in space-based astronomy applications of such detectors, are discussed.
Boris I. Fouks, Boris I. Fouks, Vasily F. Kocherov, Vasily F. Kocherov, Igor I. Taubkin, Igor I. Taubkin, Leonid A. Vinokurov, Leonid A. Vinokurov, Nicolas B. Zaletaev, Nicolas B. Zaletaev, } "Photoresponse of low-background extrinsic infrared detector arrays," Optical Engineering 33(5), (1 May 1994). https://doi.org/10.1117/12.165801 . Submission:


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