Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/237
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dc.contributor.authorSingh, J-
dc.contributor.authorCowsik, R-
dc.contributor.authorVenkatakrishnan, P-
dc.contributor.authorSrinivasan, R-
dc.contributor.authorChinnappan, V-
dc.contributor.authorRaju, K. P-
dc.contributor.authorSrikanth, R-
dc.date.accessioned2005-01-17T10:41:49Z-
dc.date.available2005-01-17T10:41:49Z-
dc.date.issued1997-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 13, pp. 37-39en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/237-
dc.description.abstractTo 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.extent53112 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectNarrow band photometryen
dc.subjectEmission linesen
dc.subjectElectron densityen
dc.subjectCoronal structureen
dc.titleNarrow Band Photometry in Emission Lines during the Total Solar Eclipse of October 24, 1995en
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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