The solar corona in the He II line

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/894

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DC Field	Value	Language
dc.contributor.author	Shylaja, B. S	-
dc.date.accessioned	2006-04-08T10:46:21Z	-
dc.date.available	2006-04-08T10:46:21Z	-
dc.date.issued	1997	-
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 111	en
dc.identifier.issn	0374-3632	-
dc.identifier.uri	http://hdl.handle.net/2248/894	-
dc.description.abstract	The corona of the sun was photographed with the filters centered at 4686Å, 4921 Å and 5812 Å, on 24th October 1995, during totality at Nim Ka Thana The PDS scans of these Images were presented The differences In the contours may be interpreted to mean the non uniform distribution of the source of the Hell emission.	-
dc.format.extent	270990 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Institute of Astrophysics	en
dc.title	The solar corona in the He II line	en
dc.type	Article	en
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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