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	2005-12-06T05:20:15Z
dc.date.available	2005-12-06T05:20:15Z
dc.date.issued	1983-12
dc.identifier.citation	BASI, Vol. 11, No. 4, pp. 327-336	en
dc.identifier.uri	http://hdl.handle.net/2248/608
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 formation and development of filaments. Filaments generally break into fragments as soon as narrow neutral bands are formed.	en
dc.format.extent	805915 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Solar magnetic field - filaments	en
dc.title	On the relation between large scale solar magnetic fields and filament positions	en
dc.type	Article	en