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Spatial structure of a two-phase solar flare observed in the EUV by OSO-7Soft X-ray and hydrogen alpha observations on the structure of a solar flare show the typical flare behavior - a rapid rise to maximum and a gradual exponential decay, with good time correlation between the soft X-rays and H alpha. The emission is identified by Fe XI ion, and the emitting region is contoured on EUV maps.
Document ID
19730023147
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Thomas, R. J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: Significant Accomplishments in Sci.
Subject Category
Space Radiation
Accession Number
73N31879
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19730023135Collected WorksSignificant Accomplishments in Sciences: Goddard Space Flight Center, 1972
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