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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3572
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dc.contributor.authorRaju, P. K-
dc.contributor.authorVasundhara, R-
dc.date.accessioned2008-09-12T10:35:53Z-
dc.date.available2008-09-12T10:35:53Z-
dc.date.issued1990-
dc.identifier.citationIAU Symposium, No. 142, pp. 443 - 444en
dc.identifier.issn0074-1809-
dc.identifier.urihttp://hdl.handle.net/2248/3572-
dc.description.abstractThe variation of theoretical line intensity ratios with electron density for Mg VI ion is presented. This study indicates that the line intensity ratios for Mg VI can be used to infer electron density for solar plasma.en
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.urihttp://adsabs.harvard.edu/abs/1990IAUS..142..443Ren
dc.subjectElectron densityen
dc.subjectSolar Emission Linesen
dc.titleDensity Diagnostics of Solar Emission Lines from the Nitrogen-Like Mgvi Ionen
dc.typeArticleen
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