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dc.contributor.authorAmbastha, A-
dc.contributor.authorBasu, S-
dc.contributor.authorAntia, H. M-
dc.date.accessioned2008-06-05T07:39:23Z-
dc.date.available2008-06-05T07:39:23Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 319 - 320en
dc.identifier.urihttp://hdl.handle.net/2248/2405-
dc.description.abstractSolar flares release large amounts of energy at different layers of the solar atmosphere. It is, therefore, expected that major flares would be able to excite waves, thereby affecting the p-mode oscillation characteristics. From the analysis of MDI data, we find that power in p-modes appears to increase for some flares, beyond the normal values expected from the influence of magnetic field.en
dc.format.extent67975 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..319Aen
dc.subjectSolar flaresen
dc.subjectp-mode oscillationsen
dc.titleExcitation of Solar p-mode Oscillations by Flaresen
dc.typeArticleen
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