Optical emission from solar corona

dc.contributor.author	Raju, P. K
dc.date.accessioned	2005-01-08T05:37:01Z
dc.date.available	2005-01-08T05:37:01Z
dc.date.issued	1988
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 89-98	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/189
dc.description.abstract	In this article the methods to probe the solar corona are briefly described. The discussion is confined to continuum and the "optical" wavelength region ~ 0.3 mum to 1.1 mum.	en
dc.format.extent	272829 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Solar corona	en
dc.subject	Optical emission	en
dc.title	Optical emission from solar corona	en
dc.type	Article	en