An Estimation of the Amount of Heating for Some Solar Coronal Loops

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/278

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DC Field	Value	Language
dc.contributor.author	Elwett, G	-
dc.contributor.author	Narain, Udit	-
dc.date.accessioned	2005-02-01T05:30:07Z	-
dc.date.available	2005-02-01T05:30:07Z	-
dc.date.issued	1980-03	-
dc.identifier.citation	BASI, Vol. 8, No. 1, pp. 21-26	en
dc.identifier.uri	http://hdl.handle.net/2248/278	-
dc.description.abstract	Based on the standard idea that short cooling times imply continued heating, a method of estimation of the amount of heating is developed and applied to thte five examples of Krieger (1978) assuming conduction to be the dominant cooling mechanism in plane parallel and line dipole geometries. As expected, one requires more heating in former geometry than in the latter. The required total energy supplied by heating is found to be comparable to the total thermal energy of the events under consideration.	en
dc.format.extent	557767 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of India	en
dc.subject	Solar Coronal Loops	en
dc.subject	Cooling times - Solar Coronal Loops	en
dc.title	An Estimation of the Amount of Heating for Some Solar Coronal Loops	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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