Emission lines from O IV as a plasma diagnostic

Details Emission lines from O IV as a plasma diagnostic Emission lines from O IV as a plasma diagnostic

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..138..283d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 138, no. 2, April 1992, p. 283-290.

Physics

10

Electron Density (Concentration), Emission Spectra, Line Spectra, Oxygen, Plasma Density, Plasma Diagnostics, Sunspots, Atomic Excitations, Metastable State, Physical Properties, Solar Activity, Solar Flares, Transition Probabilities

Scientific paper

Using new calculations of several diagnostic O IV line intensity ratios in terms of electron density, together with the corresponding Skylab observations of the same source (Sandlin et al. (1977, 1984)), it is shown that an emitting region has a multidensity structure. Results of electron densities for various transitions, derived from theoretical line ratio curves using observed values, are presented in a tabular form and are compared with those reported by other authors using different observational data.

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