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Proceedings Paper

Imaging MAMA detector systems
Author(s): David C. Slater; J. Gethyn Timothy; Jeffrey S. Morgan; David B. Kasle
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Paper Abstract

Imaging multianode microchannel array (MAMA) detector systems with 1024 x 1024 pixel formats have been produced for visible and UV wavelengths; the UV types employ 'solar blind' photocathodes whose detective quantum efficiencies are significantly higher than those of currently available CCDs operating at far-UV and EUV wavelengths. Attention is presently given to the configurations and performance capabilities of state-of-the-art MAMA detectors, with a view to the development requirements of the hybrid electronic circuits needed for forthcoming spacecraft-sensor applications. Gain, dark noise, uniformity, and dynamic range performance data are presented for the curved-channel 'chevron', 'Z-plate', and helical-channel high gain microchannel plate configurations that are currently under evaluation with MAMA detector systems.

Paper Details

Date Published: 1 July 1990
PDF: 15 pages
Proc. SPIE 1243, Electron Image Tubes and Image Intensifiers, (1 July 1990); doi: 10.1117/12.19463
Show Author Affiliations
David C. Slater, Stanford Univ. (United States)
J. Gethyn Timothy, Stanford Univ. (United States)
Jeffrey S. Morgan, Stanford Univ. (United States)
David B. Kasle, NASA/Goddard Space Flight Ctr. (United States)


Published in SPIE Proceedings Vol. 1243:
Electron Image Tubes and Image Intensifiers
Illes P. Csorba, Editor(s)

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