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dc.contributor.authorHiremath, K. M-
dc.date.accessioned2008-07-22T11:47:30Z-
dc.date.available2008-07-22T11:47:30Z-
dc.date.issued2000-
dc.identifier.citationIAU Symposia, Vol. 195, pp. 397 - 398en
dc.identifier.issn0074-1809-
dc.identifier.urihttp://hdl.handle.net/2248/2824-
dc.description.abstractGiven the prevailing physical conditions in the cosmic environment, the similarity of solar transients and cosmic gamma-ray bursts suggests that the most promising energy source for the latter may be primordial flares, which derive energy from magnetic reconnection.en
dc.format.extent209596 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000IAUS..195..397Hen
dc.subjectPrimordial Flaresen
dc.subjectFlux Tubesen
dc.subjectGamma-ray Burstsen
dc.subjectCosmic Gamma-Ray Burstsen
dc.subjectSolar Transientsen
dc.titlePrimordial Flares, Flux Tubes, and Gamma-ray Burstsen
dc.typeArticleen
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