High radiometric performance CCD for the third-generation stratospheric aerosol and gas experiment

Details High radiometric performance CCD for the third-generation stratospheric aerosol and gas experiment High radiometric performance CCD for the third-generation stratospheric aerosol and gas experiment

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991spie.1447..204d&link_type=abstract

Proc. SPIE Vol. 1447, p. 204-213, Charge-Coupled Devices and Solid State Optical Sensors II, Morley M. Blouke; Ed.

Computer Science

Scientific paper

A third-generation SAGE instrument is about to be designed as part of the NASA Earth Observational System. Previous instruments have used individual diodes as detectors. The new instrument will use a custom design CCD to dramatically enhance the study of the gas and aerosol components of the upper atmosphere. The CCD is a 3 X 400 imaging array that has a single serial register and an exposure control drain. It will be used at the focal plane of a spectrometer covering the spectral range from 288 nm to 1.02 micrometers .

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