The Enhanced Coronal Green Line Intensity and the Magnetic Field Gradients

dc.contributor.author	Ramesh, K. B
dc.contributor.author	Nagabhushana, B. S
dc.contributor.author	Varghese, B. A
dc.date.accessioned	2008-08-12T09:02:08Z
dc.date.available	2008-08-12T09:02:08Z
dc.date.issued	2000-12
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 419 - 420	en
dc.identifier.issn	0250-6335
dc.identifier.uri	http://hdl.handle.net/2248/3079
dc.format.extent	36139 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000JApA...21..419R	en
dc.subject	Sun: Corona	en
dc.subject	Emergence of magnetic flux	en
dc.title	The Enhanced Coronal Green Line Intensity and the Magnetic Field Gradients	en
dc.type	Article	en