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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/782

Title:	Coronal heating Efficiency for resonant (A.C.) and non-resonant (D.C.) mechanisms
Authors:	Chandra, S Musrif, P. G Prasad, L
Keywords:	Sun: corona - Sun magnetic fields - Sun X-rays- MHD
Issue Date:	Sep-2005
Publisher:	Astronomical Society of India
Citation:	BASI, Vol. 33, No. 3, pp. 275-282
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
URI:	http://hdl.handle.net/2248/782
Appears in Collections:	BASI Publications

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