On Heating of Solar Corona Through Magnetic Fields

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