On Heating of Solar Corona Through Magnetic Fields

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/369

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DC Field	Value	Language
dc.contributor.author	Narain, Udit	-
dc.contributor.author	Kumar, Mukul	-
dc.date.accessioned	2005-02-11T05:34:05Z	-
dc.date.available	2005-02-11T05:34:05Z	-
dc.date.issued	1986	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 127-131	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/369	-
dc.description.abstract	In this article the heating of solar corona by magnetic fields, with particular emphasis to the work done by authors has been presented. It is found that the heating of active ragions by twisting of magnetic fields (Tucker, 1973) does not seem feasible in view of very high twisting velocities predicted for the magnetic field. Further the heating by reconnection (Levine, 1974) seems interesting and needs further quantitative investigation.	en
dc.format.extent	139882 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solra Corona	en
dc.subject	Magnetic Fields	en
dc.title	On Heating of Solar Corona Through Magnetic Fields	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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