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CLAES focal plane arrayThe Cryogenic Limb Array Etalon Spectrometer for the NASA Upper Atmospheric Research Satellite uses solid-state focal plane arrays to detect emission from the earth's atmosphere over the IR wavelength range 3.5 to 13 microns. This paper discusses the design of the focal plane detector assembly and compares calculated performance with measurements. Measurements were made of focal plane noise and responsivity as functions of frequency (2 to 500 Hz) and temperature (12 to 19 K), pixel-to-pixel and across-array crosstalk, and linearity over a dynamic range of 100,000. The measurements demonstrate that the arrays satisfy the science requirements, and that, in general, there is reasonable agreement between the measurements and the analytical model.
Document ID
19900024231
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Roche, A. E.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Sterritt, L. W.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Kumer, J. B.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Callary, P. C.
(Lockheed Missiles and Space Co., Inc. Research and Development Div., Palo Alto, CA, United States)
Nielsen, R. L.
(Hughes Santa Barbara Research Center Goleta, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Subject Category
Spacecraft Instrumentation
Meeting Information
Meeting: Cryogenic Optical Systems and Instruments III
Location: San Diego, CA
Country: United States
Start Date: August 17, 1988
End Date: August 19, 1988
Sponsors: SPIE
Accession Number
90A11286
Funding Number(s)
CONTRACT_GRANT: NAS5-27752
Distribution Limits
Public
Copyright
Other

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