Production of magnetic flux bundles for solar activity by cascade of energy in global torsional MHD waves

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4048

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DC Field	Value	Language
dc.contributor.author	Gokhale, M. H	-
dc.date.accessioned	2008-12-12T09:51:37Z	-
dc.date.available	2008-12-12T09:51:37Z	-
dc.date.issued	1994	-
dc.identifier.citation	Solar active region evolution: comparing models with observations. Astronomical Society of the Pacific Conference Series, volume 68, Proceedings of the Fourteenth (14th) International Summer Workshop, National Solar Observatory / Sacramento Peak, Sunspot, New Mexico, USA, 30 August - 3 September 1993,edited by K. S. Balasubramaniam and George W. Simon., pp. 102 - 106	en
dc.identifier.uri	http://hdl.handle.net/2248/4048	-
dc.description	Open Access	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	-
dc.relation.uri	http://adsabs.harvard.edu/abs/1994ASPC...68..102G	en
dc.subject	Magnetic Flux Bundles	en
dc.subject	Solar Activity	en
dc.subject	Global Torsional MHD Waves	en
dc.title	Production of magnetic flux bundles for solar activity by cascade of energy in global torsional MHD waves	en
dc.type	Article	en
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