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Stable vacuum UV CCD detectors designed for space flight experimentsThinned, backside-illuminated, p-channel CCD images are under development which can exploit the surface potential in VUV applications, yielding enhanced quantum efficiency to wavelengths as short as 1100 A. The current goal is production of large-format, 5-micron pixel imagers for spectrographic and imaging VUV spaceflight experiments. Model predictions of the effect of device design on quantum efficiency, well capacity, and crosstalk are presented for such 5-micron-approaching pixel sizes.
Document ID
19930050448
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Socker, Dennis G. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Marchywka, Mike (U.S. Navy, Naval Research Lab. Washington, United States)
Taylor, G. C. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Levine, P. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Rios, R. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Shallcross, F. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Hughes, G. (David Sarnoff Research Center Princeton, NJ, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1993
Publication Information
Publication: In: Ultraviolet technology IV; Proceedings of the Meeting, San Diego, CA, July 20, 21, 1992 (A93-34426 13-35)
Publisher: Society of Photo-Optical Instrumentation Engineers
Subject Category
Instrumentation And Photography
Accession Number
93A34445
Funding Number(s)
CONTRACT_GRANT: NASA ORDER S-19986-E
Distribution Limits
Public
Copyright
Other

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