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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/284
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dc.contributor.authorSmartt, R. N-
dc.contributor.authorZirker, J. B-
dc.contributor.authorMauter, H. A-
dc.date.accessioned2005-02-03T03:54:13Z-
dc.date.available2005-02-03T03:54:13Z-
dc.date.issued1980-06-
dc.identifier.citationBASI, Vol. 8, Nos. 2&3, pp. 59-61en
dc.identifier.urihttp://hdl.handle.net/2248/284-
dc.description.abstractAn experiment carried out during the February 16, 1980 total solar eclipse to measure velocities and intensity distributions associated with coronal loops is described. The optical instrumentation used consisted of a 30-cm aperture Cassegrain telescope, a solid fabry-Perot etalon, ancillary optical components and a motor-driven camera. During totality, the green corona was photographed both with and without the etalon in thte system; the first maximum of the etalon beyond the limb was recorded on three frames. A preliminary discussion of the data is presented.en
dc.format.extent1357711 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherTata Institute of Fundamental Research, Bombayen
dc.subjectCoronal Emissionen
dc.subjectInterferometric Eclipse Observationsen
dc.subjectCoronal Fe XIV Emissionen
dc.titleInterferometric Eclipse Observations of Coronal Fe XIV Emissionen
dc.typeArticleen
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