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Physical parameter analysis of an intense, compact subflareResults of analysis of Skylab X-ray proportional counter data (10-s averages) and X-ray telescope filtergrams for the August 9, 1973 (SN/M2) subflare from McMath 12474 (NOAA AR 185) are presented. The event flux profiles and profiles of temperature, volume emission-measure, and a quantity equivalent to thermal energy content are shown. Using the proportional counter data, a peak temperature in excess of 20,000,000 K at 1552:05 UT, a peak volume emission measure of 7 x 10 to the 48th per cu cm at 1553:25 UT, and a peak value of thermal energy content of 2 x 10 to the 16th evgs/cm to the 3/2 power at 1552:45 UT were derived. Based on the analysis of spatially-resolved X-ray images during the period near flare-peak through flare-decay, the flare is observed to be both intense and compact and to consist of at least two identifiable loops whose volumes remained essentially unchanged throughout the event.
Document ID
19790051240
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wilson, R. M.
(NASA Marshall Space Flight Center Space Sciences Laboratory, Huntsville, Ala., United States)
Smith, J. B., Jr.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Speich, D. M.
(NASA Marshall Space Flight Center Space Sciences Laboratory, Huntsville, Ala.; NOAA, Space Environment Laboratory, Boulder, Colo., United States)
Date Acquired
August 9, 2013
Publication Date
April 1, 1979
Publication Information
Publication: Astronomy and Astrophysics
Volume: 74
Issue: 2, Ap
Subject Category
Solar Physics
Accession Number
79A35253
Funding Number(s)
CONTRACT_GRANT: NASA ORDER H-12261-B
Distribution Limits
Public
Copyright
Other

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