Primordial Flares, Flux Tubes, and Gamma-ray Bursts

dc.contributor.author	Hiremath, K. M
dc.date.accessioned	2008-07-22T11:47:30Z
dc.date.available	2008-07-22T11:47:30Z
dc.date.issued	2000
dc.identifier.citation	IAU Symposia, Vol. 195, pp. 397 - 398	en
dc.identifier.issn	0074-1809
dc.identifier.uri	http://hdl.handle.net/2248/2824
dc.description.abstract	Given 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.extent	209596 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000IAUS..195..397H	en
dc.subject	Primordial Flares	en
dc.subject	Flux Tubes	en
dc.subject	Gamma-ray Bursts	en
dc.subject	Cosmic Gamma-Ray Bursts	en
dc.subject	Solar Transients	en
dc.title	Primordial Flares, Flux Tubes, and Gamma-ray Bursts	en
dc.type	Article	en