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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2398
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dc.contributor.authorVenkatakrishnan, P-
dc.contributor.authorKumar, B-
dc.contributor.authorRavindra, B-
dc.date.accessioned2008-06-03T12:29:22Z-
dc.date.available2008-06-03T12:29:22Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 299 - 301en
dc.identifier.urihttp://hdl.handle.net/2248/2398-
dc.description.abstractWe report on the rapid variations of solar magnetic fields that appear to be enhanced significantly above the background variability, at a few locations within the solar active regions, as observed with the Michelson Doppler Imager (MDI) on board the SOHO spacecraft. The pressure fluctuations estimated to arise from this variability far exceed the general level of acoustic pressure fluctuations. The equivalent mechanical flux that could be generated from these rapid magnetic variations is more than adequate for the heating of the active region chromosphere and corona.en
dc.format.extent104647 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..299Ven
dc.subjectSunen
dc.subjectMHDen
dc.subjectPhotosphereen
dc.titleOn the Rapid Variations of Solar Magnetic Fieldsen
dc.typeArticleen
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