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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/246
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dc.contributor.authorRusin, V-
dc.contributor.authorKlocok, L-
dc.contributor.authorMinarovjech, M-
dc.contributor.authorRybansky, M-
dc.date.accessioned2005-01-18T03:54:15Z-
dc.date.available2005-01-18T03:54:15Z-
dc.date.issued1997-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 13, pp. 79-81en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/246-
dc.description.abstractA 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.extent69412 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectTotal Solar Eclipseen
dc.subjectCoronal streamersen
dc.subjectCoronal holes and plumesen
dc.subjectSpectroscopyen
dc.titleSpectroscopy, Multicolour Photometry and Structure of the Solar Corona during the Total Solar Eclipse on October 24, 1995en
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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