Narrow Band Photometry in Emission Lines during the Total Solar Eclipse of October 24, 1995

dc.contributor.author	Singh, J
dc.contributor.author	Cowsik, R
dc.contributor.author	Venkatakrishnan, P
dc.contributor.author	Srinivasan, R
dc.contributor.author	Chinnappan, V
dc.contributor.author	Raju, K. P
dc.contributor.author	Srikanth, R
dc.date.accessioned	2005-01-17T10:41:49Z
dc.date.available	2005-01-17T10:41:49Z
dc.date.issued	1997
dc.identifier.citation	Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 37-39	en
dc.identifier.issn	0374-3632
dc.identifier.uri	http://hdl.handle.net/2248/237
dc.description.abstract	To investigate the spatial variation of tempereture and density within coronal strucures, narrow band photometry in three coronal emission lines was done during this eclipse. The emission lines 6374 (FeX), 7892 (Fe XI) and 5303 Armstrong (Fe XIV) represented temperatures in the Armstrong range of 1-2 million degrees. Peltier cooled CCD camera was used to record the coronal images thorugh 5 Armstrong interference filters with pixel resolution of 11 arcsec.	en
dc.format.extent	53112 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Indian Institute of Astrophysics, Bangalore	en
dc.subject	Narrow band photometry	en
dc.subject	Emission lines	en
dc.subject	Electron density	en
dc.subject	Coronal structure	en
dc.title	Narrow Band Photometry in Emission Lines during the Total Solar Eclipse of October 24, 1995	en
dc.type	Article	en