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Photographic films for the Multi-Spectral Solar Telescope ArrayThe rocketborne Multi-Spectral Solar Telescope Array (MSSTA) uses an array of Ritchey-Chretien, Cassegrain, and Herschelian telescopes to produce ultrahigh-resolution full-disk images of the sun within the soft X-ray, EUV, and FUV ranges. Such imaging of the solar disk and corona out to several solar radii placed great demands on the MSSTA's data storage capabilities; in addition, its photographic films required very low outgassing rates. Results are presented from calibration tests conducted on the MSSTA's emulsions, based on measurements at NIST's synchrotron facility.
Document ID
19930055675
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Hoover, Richard B.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Walker, Arthur B. C., Jr.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Deforest, Craig E.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Allen, Maxwell J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Lindblom, Joakim F.
(Stanford Univ. CA, United States)
Gilliam, Lou
(NASA Marshall Space Flight Center Huntsville, AL, United States)
November, Larry
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Brown, Todd
(National Solar Observatory Sunspot, NM, United States)
Dewan, Clyde A.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Multilayer and grazing incidence X-ray(EUV optics; Proceedings of the Meeting, San Diego, CA, July 22-24, 1991 (A93-39658 15-74)
Publisher: Society of Photo-Optical Instrumentation Engineers
Subject Category
Instrumentation And Photography
Accession Number
93A39672
Distribution Limits
Public
Copyright
Other

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