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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2728
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dc.contributor.authorSingh, G. N-
dc.contributor.authorShrivastava, P. K-
dc.date.accessioned2008-07-17T10:23:57Z-
dc.date.available2008-07-17T10:23:57Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 599 - 600en
dc.identifier.urihttp://hdl.handle.net/2248/2728-
dc.description.abstractHigh speed solar· wind streams are separated into two categories : (i) Corotating (ii) Flare-generated streams. Resul ts based on this analysis indicate the occurrence of large geomagnetic and interplanetary disturbances during flare-generated streams in comparison to period of corotating streams.en
dc.format.extent56595 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar Winden
dc.subjectGeomagnetic Activityen
dc.subjectInterplanetary Disturbancesen
dc.titleEffect of solar wind streams on interplanetary features and on geomagnetic fielden
dc.typeArticleen
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