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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3370
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dc.contributor.authorDas, T. K-
dc.contributor.authorNag, T. K-
dc.contributor.authorDutta, A. K-
dc.date.accessioned2008-09-04T16:52:44Z-
dc.date.available2008-09-04T16:52:44Z-
dc.date.issued1998-
dc.identifier.citationBASI, Vol. 26, p. 311 - 315en
dc.identifier.urihttp://hdl.handle.net/2248/3370-
dc.description.abstractA study has been made about the solar proton events observed by NOAA satellite during the period 1976-1993 by considering their association with Hα-flares. The proton flux has been found to depend linearly upon the estimated flare energy output per day. The proton flux varies with the rise time also in a linear way. Study about the visual features of the proton - associated Hα-flares reveals that the proton events are connected with those kinds of flares which have multiple instabilities in the associated active regionsen
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1998BASI...26..311Den
dc.subjectSolar protonen
dc.subjectH-alpha flaresen
dc.titleSolar proton events in relation to H-alpha flaresen
dc.typeArticleen
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