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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1967
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dc.contributor.authorSundararaman, K-
dc.contributor.authorAleem, P. S. M-
dc.contributor.authorThiagarajan, R-
dc.date.accessioned2007-11-15T07:50:00Z-
dc.date.available2007-11-15T07:50:00Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 3, pp. 383 - 389en
dc.identifier.urihttp://hdl.handle.net/2248/1967-
dc.description.abstractSpectra taken at the solar telescope-spectrograph, Kodaikanal, are analysed to find the sight-line velocity values in the regions between the opposite polarity sunspots. Velocities in opposite directions in the range 1 - 2.5 km per second are obtained in the cases of δ - type sunspots (spots having common penumbra), whereas opposite polarity sunspots having separate structures do not show any appreciable velocity in the regions between them. The velocities in the sunspots are restricted to the penumbral boundaries.en
dc.format.extent565877 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..383Sen
dc.subjectEvershed velocityen
dc.subjectBipolar sunspotsen
dc.subjectFlaresen
dc.titleEvershed velocities in bipolar sunspotsen
dc.typeArticleen
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