1. IIA Institutional Repository
  2. Publications of Astronomical Society of India
  3. BASI Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/608
Full metadata record
DC FieldValueLanguage
dc.contributor.authorShelke, R. N-
dc.contributor.authorPande, M. C-
dc.date.accessioned2005-12-06T05:20:15Z-
dc.date.available2005-12-06T05:20:15Z-
dc.date.issued1983-12-
dc.identifier.citationBASI, Vol. 11, No. 4, pp. 327-336en
dc.identifier.urihttp://hdl.handle.net/2248/608-
dc.description.abstractInterrelationships 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.extent805915 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar magnetic field - filamentsen
dc.titleOn the relation between large scale solar magnetic fields and filament positionsen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
SHELKE.pdf787.03 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.