Possible amount of magnetic flux reconnected through quiescent prominences outside the active regions

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4808

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DC Field	Value	Language
dc.contributor.author	Gokhale, M. H	-
dc.contributor.author	Sivaraman, K. R	-
dc.date.accessioned	2009-09-10T10:13:56Z	-
dc.date.available	2009-09-10T10:13:56Z	-
dc.date.issued	1979	-
dc.identifier.citation	Jensen, E., Maltby, P and Orrall, F Q. eds., Proceedings of the International Astronomical Union Colloquium No.44 OSLO August 14 - 18, 1978., pp. 189 - 192	en
dc.identifier.issn	82-990556-0-1	-
dc.identifier.uri	http://hdl.handle.net/2248/4808	-
dc.language.iso	en	en
dc.publisher	Institute of Theoretical Astrophysics	en
dc.relation.ispartofseries	International Astronomical Union Colloquium; No. 44	-
dc.subject	Magnetic Flux	en
dc.subject	Solar Magnetic Field	en
dc.subject	Solar Prominences	en
dc.subject	Filaments	en
dc.subject	Photosphere	en
dc.subject	Sunspot Cycle	en
dc.title	Possible amount of magnetic flux reconnected through quiescent prominences outside the active regions	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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