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The ultraviolet imager (UVI) for ISTPWe report the design of an imager with 0.6-millirad angular resolution over an 8-deg field of view sampled with 39,500 pixels, yielding global auroral coherent imaging from above 6 R(E). High performance filters provide spectrally pure measurements of four key FUV features, with 10 exp -4 out-of-band rejection. Together with the solar blind intensified CCD detector, a net rejection of 10 exp -9 of all out-of-band emissions is achieved. The optical design comprises a three-mirror f/3 system which yields a noise equivalent sensitivity of 10 Rayleighs for a 37-sec frame rate. The instantaneous dynamic range is 1000 which can be windowed over a range of 10 exp 4.
Document ID
19930043085
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Torr, D. G.
(Alabama Univ. Huntsville, United States)
Torr, Marsha R.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Zukic, M.
(Alabama Univ. Huntsville, United States)
Spann, J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Johnson, R. B.
(Alabama Univ. Huntsville, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Instrumentation for planetary and terrestrial atmospheric remote sensing; Proceedings of the Meeting, San Diego, CA, July 23, 24, 1992 (A93-27076 09-35)
Publisher: Society of Photo-Optical Instrumentation Engineers
Subject Category
Spacecraft Instrumentation
Accession Number
93A27082
Funding Number(s)
CONTRACT_GRANT: NAS8-38145
CONTRACT_GRANT: NAS8-38146
Distribution Limits
Public
Copyright
Other

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