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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2240
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dc.contributor.authorGupta, A. K-
dc.contributor.authorMohan, A-
dc.contributor.authorDwivedi, B. N-
dc.date.accessioned2008-04-21T11:18:52Z-
dc.date.available2008-04-21T11:18:52Z-
dc.date.issued1997-
dc.identifier.citationBASI, Vol. 25, No. 2, pp. 247 - 251en
dc.identifier.urihttp://hdl.handle.net/2248/2240-
dc.description.abstractWe present new calculations for N III ion for diagnostics of solar plasma. The atomic model comprising the first 15 energy levels is considered for evaluating the line emissivities as a function of electron density and temperature, taking account of various physical processes. EUV line ratios, hitherto unexplored for diagnostic study, from this ion are presented as a function of electron density at its temperature of peak ionic concentration and their diagnostic applications in the solar atmosphere are discussed.en
dc.format.extent342759 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997BASI...25..247Gen
dc.subjectLine diagnosticsen
dc.subjectEUV Emission Linesen
dc.subjectOptically Thin Plasmasen
dc.subjectExtreme Ultraviolet Radiationen
dc.titleOn the EUV Line Diagnostics From N III Solar Ionen
dc.typeArticleen
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