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Report of the ultraviolet and visible sensors panelIn order to meet the science objectives of the Astrotech 21 mission set the Ultraviolet (UV) and Visible Sensors Panel made a number of recommendations. In the UV wavelength range of 0.01 to 0.3 micro-m the focus is on the need for large format high quantum efficiency, radiation hard 'solar-blind' detectors. Options recommended for support include Si and non-Si charge coupled devices (CCDs) as well as photocathodes with improved microchannel plate readouts. For the 0.3 to 0.9 micro-m range, it was felt that Si CCDs offer the best option for high quantum efficiencies at these wavelengths. In the 0.9 to 2.5 micro-m the panel recommended support for the investigation of monolithic arrays. Finally, the panel noted that the implementation of very large arrays will require new data transmission, data recording, and data handling technologies.
Document ID
19920013373
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Timothy, J. Gethyn
(Stanford Univ. CA., United States)
Blouke, M.
(Tektronix, Inc., Beaverton OR., United States)
Bredthauer, R.
(Eastman Kodak Co. Rochester, NY., United States)
Kimble, R.
(Arizona Univ. Phoenix., United States)
Lee, T.-H.
(California Univ. Berkeley., United States)
Lesser, M.
(Stanford Univ. CA, United States)
Siegmund, O.
(Stanford Univ. CA, United States)
Weckler, G.
(Edgerton, Germeshausen and Grier, Inc., Idaho Falls ID., United States)
Date Acquired
August 15, 2013
Publication Date
August 1, 1991
Publication Information
Publication: JPL, California Inst. of Tech., Workshop Proceedings: Sensor Systems for Space Astrophysics in the 21st Century, Volume 2
Subject Category
Spacecraft Instrumentation
Accession Number
92N22616
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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