The solar corona in the He II line

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