Coronal heating Efficiency for resonant (A.C.) and non-resonant (D.C.) mechanisms

dc.contributor.author	Chandra, S
dc.contributor.author	Musrif, P. G
dc.contributor.author	Prasad, L
dc.date.accessioned	2006-03-15T04:15:48Z
dc.date.available	2006-03-15T04:15:48Z
dc.date.issued	2005-09
dc.identifier.citation	BASI, Vol. 33, No. 3, pp. 275-282	en
dc.identifier.uri	http://hdl.handle.net/2248/782
dc.description.abstract	Ionson (1985a) extended his uni¯ed theory of coronal resonance heating having non-resonant (D.C.) and resonant (A.C.) components. Narain and Kumar (1995) calculated heating e±ciency for resonant and non-resonant components for coronal heating. Since some inconsistencies are noticed in these calculations, we decided to reinvestigate the work of Narain and Kumar (1995). The results are found to vary remarkably. Reasons for these variations are discussed	en
dc.format.extent	214047 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Sun: corona - Sun	en
dc.subject	magnetic fields - Sun	en
dc.subject	X-rays- MHD	en
dc.title	Coronal heating Efficiency for resonant (A.C.) and non-resonant (D.C.) mechanisms	en
dc.type	Article	en