On the electric circuit approach of coronal heating: a review

dc.contributor.author	Narain, U
dc.contributor.author	Kumar, S
dc.date.accessioned	2007-04-16T09:00:00Z
dc.date.available	2007-04-16T09:00:00Z
dc.date.issued	1993-06
dc.identifier.citation	BASI, Vol. 21, No.2, pp. 85-102	en
dc.identifier.uri	http://hdl.handle.net/2248/1479
dc.description.abstract	It is now widely believed that the photosphere of the Sun and its outer atmosphere (chromosphere and corona) are electrodynamically coupled through interconnecting magnetic fields. A similar situation may exist in other stars. The electric circuit approach provides a formalism through which the coupling of inner and outer regions of stars can be adequately described, and many seemingly diverse heating mechanisms can be unified. The physics of stellar atmospheres can be better understood through electric circuit analogues because the theory of electric circuits is well understood.	en
dc.format.extent	1363483 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Sun	en
dc.subject	Stars	en
dc.title	On the electric circuit approach of coronal heating: a review	en
dc.type	Article	en