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The Solar/Stellar Coronal Explorer and the Solar/Stellar Coronal ObservatoryThe Solar/Stellar Coronal Explorer (SSCE) carries six identical Ritchey-Chretien Telescopes of 127 mm aperture each; their images will be recorded by multianode microchannel-array detectors. The mirrors of five of the telescopes are coated with multilayer reflecting structures that select narrow XUV wavelength bands corresponding to strong emission lines emitted by solar or stellar coronal plasmas. Also noted here is a larger explorer mission concept, that of the Solar/Stellar Coronal Observatory, which will undertake more extensive spectroscopic observations.
Document ID
19930055679
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Walker, Arthur B. C., Jr. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Lindblom, Joakim F. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Timothy, J. G. (Stanford Univ. CA, United States)
Barbee, Troy W., Jr. (Lawrence Livermore National Lab. Livermore, CA, United States)
Hoover, Richard B. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Tandberg-Hanssen, Einar (NASA Marshall Space Flight Center Huntsville, AL, United States)
Wu, Shi T. (Alabama Univ. Huntsville, United States)
Sahade, J. (La Plata Univ. Argentina)
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
Astronomy
Accession Number
93A39676
Distribution Limits
Public
Copyright
Other

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IDRelationTitle19930055661Collected WorksMultilayer and grazing incidence X-ray/EUV optics; Proceedings of the Meeting, San Diego, CA, July 22-24, 1991
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