On the relation between large scale solar magnetic fields and filament positions

dc.contributor.author	Shelke, R. N.
dc.contributor.author	Pande, M. C.
dc.date.accessioned	2010-07-15T06:57:39Z
dc.date.available	2010-07-15T06:57:39Z
dc.date.issued	1983
dc.identifier.citation	This article is downloaded from ADS site	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/706
dc.description.abstract	Interrelationships of filament positions and large scale solar magnetic field structures are examined here. The broad neutral bands seem to be suitable locations for the formations and development of filaments. Filaments generally break into fragments as soon as narrow neutral bands are formed.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi11-327
dc.subject	Solar magnetic field, Filaments	en_US
dc.title	On the relation between large scale solar magnetic fields and filament positions	en_US
dc.type	Article	en_US