Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/369
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dc.contributor.authorNarain, Udit-
dc.contributor.authorKumar, Mukul-
dc.date.accessioned2005-02-11T05:34:05Z-
dc.date.available2005-02-11T05:34:05Z-
dc.date.issued1986-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 6, pp. 127-131en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/369-
dc.description.abstractIn 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.extent139882 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectSolra Coronaen
dc.subjectMagnetic Fieldsen
dc.titleOn Heating of Solar Corona Through Magnetic Fieldsen
dc.typeArticleen
Appears in Collections:Kodaikanal Observatory Bulletins (1905 - 1997 )
IIAP Publications

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