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Proceedings Paper

Optimization of PhCCD structure for star sensor
Author(s): Alexandre I. Baklanov; Anatoli V. El'tsov; Vjacheslav V. Kolotkov; Andre A. Pugachev; Victor A. Shilin
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Paper Abstract

Star sensor have special performance which allows to monitor point images for low illumination levels. For the CCD sensor, this means that all of the charge generated by image photons incident on a given pixel should be collected within that pixel. Two main physical processes are determined the expected charge-collection efficiency: 3D diffusion of generated electrons and charge-transfer inefficiency. The ability of perception of low illumination stars depends on the star temperature (this temperature influences the spectral distribution of photons), quantum efficiency, and noises of the imager.

Paper Details

Date Published: 8 April 1996
PDF: 1 pages
Proc. SPIE 2790, Fifth Conference on Charge-Coupled Devices and CCD Systems, (8 April 1996); doi: 10.1117/12.238218
Show Author Affiliations
Alexandre I. Baklanov, OPTEKS Research Institute (Russia)
Anatoli V. El'tsov, OPTEKS Research Institute (Russia)
Vjacheslav V. Kolotkov, OPTEKS Research Institute (Russia)
Andre A. Pugachev, OPTEKS Research Institute (Russia)
Victor A. Shilin, OPTEKS Research Institute (Russia)


Published in SPIE Proceedings Vol. 2790:
Fifth Conference on Charge-Coupled Devices and CCD Systems
Vladimir A. Karasev; Yuri A. Kuznetsov; Victor A. Shilin, Editor(s)

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