Emission lines from O IV as a plasma diagnostic

dc.contributor.author	Dwivedi B.N.; Gupta A.K.
dc.date.accessioned	2025-05-24T09:58:10Z
dc.description.abstract	Using several density diagnostic O iv theoretical line ratios and corresponding observed values for the same source by Sandlin et al. (1984) and Sandlin, Brueckner, and Tousey (1977), we find that an emitting region has a multidensity structure. We discuss several other line ratios for density measurement in sunspots, active regions, and flares. © 1992 Kluwer Academic Publishers.
dc.identifier.doi	https://doi.org/10.1007/BF00151916
dc.identifier.uri	http://172.23.0.11:4000/handle/123456789/22992
dc.relation.ispartofseries	Solar Physics
dc.title	Emission lines from O IV as a plasma diagnostic

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