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Energy conversion in the coronal plasmaSolar and stellar X-ray emission are the observed waste products of the interplay between magnetic fields and the motion of stellar plasma. Theoretical understanding of the process of coronal heating is of utmost importance, since the high temperature is what defines the corona in the first place. Most of the research described deals with the aspects of the several rivalling theories for coronal heating. The rest of the papers deal with processes of energy conversion related to flares.
Document ID
19870011501
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Martens, P. C. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 5, 2013
Publication Date
December 1, 1986
Publication Information
Publication: Coronal and Prominence Plasmas
Subject Category
Solar Physics
Accession Number
87N20934
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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