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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/245
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dc.contributor.authorPasachoff, J. M-
dc.contributor.authorBabcock, B. A-
dc.contributor.authorSebastian Diaz-
dc.contributor.authorReardon, K. P-
dc.contributor.authorKutner, E. R-
dc.date.accessioned2005-01-18T03:03:54Z-
dc.date.available2005-01-18T03:03:54Z-
dc.date.issued1997-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 13, pp. 75-77en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/245-
dc.description.abstractWe report on the Williams College expedition to Mukandgarh Fort, Rajasthan, for the total solar eclipse of 24 October 1995. The main experiments were a search for 1 Hz oscillations in coronal loops as an indication of magnetohydrodynamic theories of coronal heating and a mapping of the coronal temperature through comaprison of images at specific ultraviolet wavelengths, measuring the difference between the photospheric and coronal continuum. We also obtained a variety of coronal images.en
dc.format.extent100077 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectCoronal heatingen
dc.subjectCoronal temperatureen
dc.subjectSolar eclipseen
dc.titleCoronal Heating Experiments of the Williams College Group at Mukandgarh Fort, Rajasthanen
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )

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