Emission lines from nitrogen-like ions and their diagnostic use

dc.contributor.author	Raju, P. K
dc.contributor.author	Dwivedi, B. N
dc.date.accessioned	2009-01-16T14:14:14Z
dc.date.available	2009-01-16T14:14:14Z
dc.date.issued	1990-11
dc.identifier.citation	Astrophysics and Space Science, Vol. 173, No. 1, pp. 13 - 26	en
dc.identifier.issn	0004-640X
dc.identifier.uri	http://hdl.handle.net/2248/4264
dc.description.abstract	Line 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.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1990Ap%26SS.173...13R	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00642558	en
dc.subject	Cosmic Plasma	en
dc.subject	Emission Spectra	en
dc.subject	Nitrogen Ions	en
dc.subject	Plasma Diagnostics	en
dc.subject	Aluminum	en
dc.subject	Ground State	en
dc.subject	Magnesium	en
dc.subject	Metal Ions	en
dc.subject	Molecular Collisions	en
dc.subject	Molecular Energy Levels	en
dc.title	Emission lines from nitrogen-like ions and their diagnostic use	en
dc.type	Article	en