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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/782
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dc.contributor.authorChandra, S-
dc.contributor.authorMusrif, P. G-
dc.contributor.authorPrasad, L-
dc.date.accessioned2006-03-15T04:15:48Z-
dc.date.available2006-03-15T04:15:48Z-
dc.date.issued2005-09-
dc.identifier.citationBASI, Vol. 33, No. 3, pp. 275-282en
dc.identifier.urihttp://hdl.handle.net/2248/782-
dc.description.abstractIonson (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 discusseden
dc.format.extent214047 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSun: corona - Sunen
dc.subjectmagnetic fields - Sunen
dc.subjectX-rays- MHDen
dc.titleCoronal heating Efficiency for resonant (A.C.) and non-resonant (D.C.) mechanismsen
dc.typeArticleen
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