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Does the emission measure decrease during the start of a soft X-ray flareIt is suggested that the apparent emission dip found in soft X-ray flare observations, interpreted as the emission from a single temperature plasma, is an artifact. According to this hypothesis, the flare phenomenon represents a combination of flare plus a stable active region plasma. A small amount of hot flare plasma will dominate the total emission, and the calculated isothermal plasma parameters will trend towards those of the hot flare plasma, so that a decrease in emission measure will be inferred. It is claimed that observed data fit the model of a stable plasma plus a flare plasma better than it does the model of a single plasma, in accordance with a chi square statistic. The model of stable plasma plus flare plasma is also supported by the observation that the plasma parameters in the postflare condition are indistinguishable from those during preflare.
Document ID
19790038299
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Wolfson, C. J.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Acton, L. W.
(Lockheed Missiles and Space Co. Palo Alto, CA, United States)
Datlowe, D. W.
(Lockheed Research Laboratories Palo Alto, Calif., United States)
Date Acquired
August 9, 2013
Publication Date
October 1, 1978
Publication Information
Publication: Solar Physics
Volume: 59
Subject Category
Solar Physics
Accession Number
79A22312
Funding Number(s)
CONTRACT_GRANT: NAS5-22411
CONTRACT_GRANT: NAS5-11360
Distribution Limits
Public
Copyright
Other

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