Optical emission from solar corona

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/189

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DC Field	Value	Language
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
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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