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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4264
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dc.contributor.authorRaju, P. K-
dc.contributor.authorDwivedi, B. N-
dc.date.accessioned2009-01-16T14:14:14Z-
dc.date.available2009-01-16T14:14:14Z-
dc.date.issued1990-11-
dc.identifier.citationAstrophysics and Space Science, Vol. 173, No. 1, pp. 13 - 26en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4264-
dc.description.abstractLine emissions from nitrogen-like ions NeIV, MgVI, and AlVII have been studied as a diagnostic probe for the emitting regions of astrophysical plasma. Line intensities from these ions have been calculated and compared, in this study, with available observational data for solar plasma.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1990Ap%26SS.173...13Ren
dc.relation.urihttp://dx.doi.org/10.1007/BF00642558en
dc.subjectCosmic Plasmaen
dc.subjectEmission Spectraen
dc.subjectNitrogen Ionsen
dc.subjectPlasma Diagnosticsen
dc.subjectAluminumen
dc.subjectGround Stateen
dc.subjectMagnesiumen
dc.subjectMetal Ionsen
dc.subjectMolecular Collisionsen
dc.subjectMolecular Energy Levelsen
dc.titleEmission lines from nitrogen-like ions and their diagnostic useen
dc.typeArticleen
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