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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4265
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dc.contributor.authorChandrasekhar, T-
dc.contributor.authorAshok, N. M-
dc.contributor.authorDesai, J. N-
dc.contributor.authorPasachoff, J. M-
dc.contributor.authorSivaraman, K. R-
dc.date.accessioned2009-01-16T14:15:41Z-
dc.date.available2009-01-16T14:15:41Z-
dc.date.issued1984-02-
dc.identifier.citationApplied Optics , Vol. 23, pp. 508 - 511en
dc.identifier.issn0003-6935-
dc.identifier.urihttp://hdl.handle.net/2248/4265-
dc.descriptionRestricted Access-
dc.description.abstractA dual-channel Fabry-Perot interferometric system was used to study simultaneously the coronal emission lines at 5303 Å (Fe XIV) and at 6374 Å (Fe X). Initial results indicate an emission corona confined largely within 1.2 R_sun;. Doppler temperatures derived from the width of the 5303-Å line appear to be appreciably lower than similar temperatures determined during the solar-maximum eclipse of 1980.en
dc.language.isoenen
dc.publisherOptical society of Americaen
dc.relation.urihttp://www.opticsinfobase.org/abstract.cfm?id=27279en
dc.rights© Optical Society of Americaen
dc.subjectFabry-Perot Interferometersen
dc.subjectSolar Coronaen
dc.subjectSolar Eclipsesen
dc.subjectSolar Instrumentsen
dc.subjectSolar Spectraen
dc.subjectCollimationen
dc.subjectEmission Spectraen
dc.subjectImage Filtersen
dc.titleFabry-Perot interferometric observations of the coronal red and green lines during the 1983 Indonesian eclipseen
dc.typeArticleen
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