MAMA detector systems - A status report

Details MAMA detector systems - A status report MAMA detector systems - A status report

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1158..104t&link_type=abstract

IN: Ultraviolet technology III; Proceedings of the Meeting, San Diego, CA, Aug. 10, 11, 1989 (A90-43258 19-35). Bellingham, WA,

Computer Science

Performance

7

Anodes, Microchannel Plates, Ultraviolet Detectors, Ultraviolet Telescopes, Hubble Space Telescope, Pixels, Soho Mission

Scientific paper

Third-generation, 224 x 960 and 360 x 1024-pixel multianode microchannel (MAMA) detectors are under development for satellite-borne FUV and EUV observations, using pixel dimensions of 25 x 25 microns. An account is presently given of the configurations, modes of operation, and recent performance data of these systems. At UV and visible wavelengths, these MAMAs employ a semitransparent, proximity-focused photocathode structure. At FUV and EUV wavelengths below about 1500 A, opaque alkali-halide photocathodes deposited directly on the front surface of the MCP furnish the best detective quantum efficiencies.

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