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Heating of solar filamentary magnetic flux tubes

dc.contributor.authorDwivedi R.; Singh R.N.
dc.date.accessioned2025-05-24T09:56:36Z
dc.description.abstractThe sunspot regions are well-known sources of energetic charged particle emissions and numerous wave mode generations. It is shown that the high frequency electromagnetic waves generated by synchrotron process, at times, could be cross-modulated by low frequency p-mode oscillations. The analyses of recorded electromagnetic field strength and seismic waves would depict interesting features of the originating sunspot regions.
dc.identifier.doiDOI not available
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/21146
dc.relation.ispartofseriesCurrent Science
dc.titleHeating of solar filamentary magnetic flux tubes

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