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On the absolute abundance of calcium in solar flaresThe abundance of calcium relative to hydrogen in soft X-ray-emitting solar flare plasmas is determined. Results were obtained for 25 flares. An average calcium-to-hydrogen abundance of about 5 x 10 exp -6, which is about a factor of 2 greater than measured for the photosphere, is found. This result is consistent with an enhancement of low first ionization elements in soft X-ray flare plasmas. For one flare, the calcium abundance was higher, at about 1.6 times the average results. It is inferred that the calcium abundance can vary among flares. Significant variations of the calcium abundance during the course of a flare were not detected.
Document ID
19930041439
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Sterling, Alphonse C.
(Computational Physics, Inc. Fairfax, VA, United States)
Doschek, George A.
(NASA Headquarters Washington, DC United States)
Feldman, Uri
(U.S. Navy E.O. Hulburt Center for Space Research, Washington, United States)
Date Acquired
August 16, 2013
Publication Date
February 10, 1993
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 404
Issue: 1
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
93A25436
Funding Number(s)
CONTRACT_GRANT: NASA ORDER W-14057
Distribution Limits
Public
Copyright
Other

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