Spectroscopy, Multicolour Photometry and Structure of the Solar Corona during the Total Solar Eclipse on October 24, 1995

dc.contributor.author	Rusin, V
dc.contributor.author	Klocok, L
dc.contributor.author	Minarovjech, M
dc.contributor.author	Rybansky, M
dc.date.accessioned	2005-01-18T03:54:15Z
dc.date.available	2005-01-18T03:54:15Z
dc.date.issued	1997
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 79-81	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/246
dc.description.abstract	A brief description of the scientific goals and preliminary results related to the 24 October 1995 solar eclipse at Nim Ka Thana is given. The white-light corona was of a minimum type above the E- and W-limbs. Coronal holes and plumes are located around the solar poles. No CME or comet was observed.	en
dc.format.extent	69412 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Total Solar Eclipse	en
dc.subject	Coronal streamers	en
dc.subject	Coronal holes and plumes	en
dc.subject	Spectroscopy	en
dc.title	Spectroscopy, Multicolour Photometry and Structure of the Solar Corona during the Total Solar Eclipse on October 24, 1995	en
dc.type	Article	en