Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997stin...9890976t&link_type=abstract
Technical Report, NASA/CR-97-206833; NAS 1.26:206833 Center for Space Science and Astrophysics
Astronomy and Astrophysics
Astrophysics
Multi-Anode Microchannel Arrays, Spectrographs, Photometry, Imaging Techniques, Hubble Space Telescope, Systems Engineering, Quantum Efficiency, High Resolution, Far Ultraviolet Radiation, Charge Coupled Devices, Technology Utilization
Scientific paper
The development of the Multi-Anode Microchannel Array (MAMA) detector systems started in the early 1970's in order to produce multi-element detector arrays for use in spectrographs for solar studies from the Skylab-B mission. Development of the MAMA detectors for spectrographs on the Hubble Space Telescope (HST) began in the late 1970's, and reached its culmination with the successful installation of the Space Telescope Imaging Spectrograph (STIS) on the second HST servicing mission (STS-82 launched 11 February 1997). Under NASA Contract NAS5-29389 from December 1986 through June 1994 we supported the development of the MAMA detectors for STIS, including complementary sounding rocket and ground-based research programs. This final report describes the results of the MAMA detector development program for STIS.
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