An estimation of the amount of heating in solar coronal loops II. Cooling through conduction-driven evaporation

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DC Field	Value	Language
dc.contributor.author	Narian, Udit	-
dc.date.accessioned	2005-02-05T04:45:37Z	-
dc.date.available	2005-02-05T04:45:37Z	-
dc.date.issued	1981-12	-
dc.identifier.citation	BASI, Vol. 9, No. 4, pp. 278-286	en
dc.identifier.uri	http://hdl.handle.net/2248/322	-
dc.description.abstract	In this paper a theory of cooling of solar coronal loops through conduction driven evaporation in presence of a source of heating is presented. No attempt has been made to specify the nature of the source. The theory has been applied to estimate the amount of heating for the flare kernael of 1973 September 1 for different breadths of the source of heating. These results are then compared with those of Elwert & Narian (1980).	en
dc.format.extent	631788 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of India	en
dc.subject	coronal loop	en
dc.subject	evaporative cooling	en
dc.subject	heating estimate	en
dc.title	An estimation of the amount of heating in solar coronal loops II. Cooling through conduction-driven evaporation	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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