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

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