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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/670
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dc.contributor.authorBagare, S. P-
dc.date.accessioned2005-12-08T05:52:40Z-
dc.date.available2005-12-08T05:52:40Z-
dc.date.issued1985-12-
dc.identifier.citationBASI, Vol. 13, No. 4, pp. 394-398en
dc.identifier.urihttp://hdl.handle.net/2248/670-
dc.description.abstractWe have obtained a good time sequence of spectroheliograms and spatial sequence spectra in the K-line of Ca II using the Kodaikanal tower telescope. We have derived the two dimensional pattern of the mass motions of the plasma associated with the flare at this level in the solar atmosphere. We find that significant mass motions are practically confined to the two ribbons that developed soon after the flaring event.en
dc.format.extent605970 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar flareen
dc.subjectCa K spectraen
dc.titleSolar flare 1982 April 14en
dc.typeArticleen
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