Emission lines from nitrogen-like ions and their diagnostic use

dc.contributor.author	Raju P.K.; Dwivedi B.N.
dc.date.accessioned	2025-05-24T09:57:38Z
dc.description.abstract	Line emissions from nitrogen-like ions Ne IV, Mg VI, and Al VII 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. © 1990 Kluwer Academic Publishers.
dc.identifier.doi	https://doi.org/10.1007/BF00642558
dc.identifier.uri	http://172.23.0.11:4000/handle/123456789/22384
dc.relation.ispartofseries	Astrophysics and Space Science
dc.title	Emission lines from nitrogen-like ions and their diagnostic use

Collections