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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/790
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dc.contributor.authorRavindra, B-
dc.date.accessioned2006-03-15T08:44:19Z-
dc.date.available2006-03-15T08:44:19Z-
dc.date.issued2005-09-
dc.identifier.citationBASI, Vol. 33, No. 3, pp. 333-336en
dc.identifier.urihttp://hdl.handle.net/2248/790-
dc.description.abstractThe Sun affects the terrestrial climate and weather as well as near Earth space by its high energy radiation and particle emissions. It is now becoming clear that the solar magnetic field, which controls all the physical processes in the solar atmosphere, is the driver for these two processes. In this thesis we have studied the role of the evolution of magnetic fields in the production of enhanced high energy radiation and particle emission from the Sun.en
dc.format.extent111297 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSunen
dc.subjectactivity- Sunen
dc.subjectcoronal mass ejections (CMEs) ­ -Sunen
dc.subjectoscil- lations ­ Sunen
dc.subjectmagenetic fieldsen
dc.titleEvolution of magnetic fields in the solar atmosphereen
dc.typeArticleen
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