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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3352
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dc.contributor.authorBhatnagar, A-
dc.contributor.authorMukerji, S-
dc.contributor.authorBabu, Y. S-
dc.contributor.authorSehgal, N. K-
dc.contributor.authorKamble, V. B-
dc.contributor.authorPandya, R. P-
dc.contributor.authorPandya, N. P-
dc.contributor.authorBhavsar, K. M-
dc.contributor.authorPrajapati, R. P-
dc.date.accessioned2008-09-04T10:34:27Z-
dc.date.available2008-09-04T10:34:27Z-
dc.date.issued1997-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 13, pp. 101en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/3352-
dc.description.abstractThe objective of this project was to take intensity and polarization measurements of extended solar coronal streamers, from a height of 75,000 to 80,000 feet above the ground. Hitherto, no observations have been made of the total solar eclipse from such a height. As the scattered light in the lower atmosphere, due to the dust particles, decreases exponentially, it was expected that we could observe the extended coronal streamers, up to 12-15 solar radii from such heights. For these observations, a 70mm format Hassel lad camera with f/3.5 and f=100 mm lens was mounted on the desk board in the cockpit of MiG-25 trainer airplane of the Indian Air force.-
dc.language.isoenen
dc.publisherIndian Institute of Astrophysicsen
dc.titleTotal solar eclipse observations MiG-25 at 80,000 ften
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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