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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/295
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dc.contributor.authorLandman, Donald. A-
dc.contributor.authorJefferies, John. T-
dc.contributor.authorOrrall, Frank. Q-
dc.date.accessioned2005-02-03T06:01:49Z-
dc.date.available2005-02-03T06:01:49Z-
dc.date.issued1980-12-
dc.identifier.citationBASI, Vol. 8, No. 4, pp. 123-127en
dc.identifier.urihttp://hdl.handle.net/2248/295-
dc.description.abstractThe Institute for Astronomy's Eclipse Spectrograph was used to obrain prominence and coronal spectra throughout the wavelength range from about Lamda Lamda 3500-7000 at the February 16, 1980 total solar eclipse. The observations were made at the Japal-Rangapur Observatory near Hyderabad. The spectra will be analysed to determine the temperature, density and composition of the prominence plasma, and will also provide tests on recently developed non-LTE, multi-atom theoretical prominence models. Analysis of thet forbidden line coronal spectrum too will yield diagnostic data for the coronal plasma.en
dc.format.extent1159384 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectEclipse Spectophotometryen
dc.subjectSolar Prominencesen
dc.titleEclipse Spectrophotometry of Solar Prominencesen
dc.typeArticleen
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