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Plasma diagnostic capabilities of the Soft X-ray Telescope on Solar-AThe predicted response of the Solar-A Soft X-ray Telescope (SXT) to various solar targets is presented. It is found that the SXT is very sensitive and should be able to observe active regions and flares at its nominal cadence with exposure times ranging from 0.0001 to 1 s. The SXT temperature diagnostic capabilities are presented for various combinations of the X-ray filters.
Document ID
19910063040
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0273-1177(91)90359-R
Authors
Strong, K. T. (Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Acton, L. W. (Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Brown, W. A. (Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Claflin, E. S. (Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Lemen, J. R. (Lockheed Solar and Astrophysics Laboratory Palo Alto, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1991
Publication Information
Publication: of the COSPAR 28th Plenary Meeting, The Hague, Netherlands, June 25-July 6, 1990. A91-47654 20-92) Advances in Space Research
ISSN: 0273-1177
Subject Category
Astronomy
Accession Number
91A47663
Funding Number(s)
CONTRACT_GRANT: NAS8-37334
Distribution Limits
Public
Copyright
Other

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