dc.contributor.author |
Krishan, V |
|
dc.contributor.author |
Kundu, M. R |
|
dc.date.accessioned |
2008-07-31T05:16:29Z |
|
dc.date.available |
2008-07-31T05:16:29Z |
|
dc.date.issued |
1985 |
|
dc.identifier.citation |
Unstable current systems and plasma instabilities in astrophysics; Proceedings of the 107th Symposium, College Park, MD, August 8-11, 1983 Dordrecht, D. Reidel Publishing Co., pp. 299-301. |
en |
dc.identifier.issn |
A85-48801 24-90 |
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dc.identifier.uri |
http://hdl.handle.net/2248/2964 |
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dc.description.abstract |
Recent observations of the fast time variability in the hard X-ray emission from solar flares are interpreted. The fast spikes are assumed to be superimposed on the thermal X-ray emission. The rise and fall of a spike are caused by disruptions in the plasma. The rise time represents the impulsive heating time and the decay or fall time represents a quick cooling of the plasma due to the accelerating growth rate of the m = 1 tearing mode. The estimated characteristic time durations of the spike are found to be in good agreement with the observed ones. |
en |
dc.format.extent |
244392 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
International Astronomical Union |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1985IAUS..107..299K |
en |
dc.subject |
X-ray emission |
en |
dc.subject |
Solar flares |
en |
dc.title |
An Interpretation of the Millisecond time variation in Hard X-ray solar flares |
en |
dc.type |
Article |
en |