Emission lines from nitrogen-like ions and their diagnostic use

Details Emission lines from nitrogen-like ions and their diagnostic use Emission lines from nitrogen-like ions and their diagnostic use

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.173...13r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 173, no. 1, Nov. 1990, p. 13-26.

Astronomy and Astrophysics

Astrophysics

4

Cosmic Plasma, Emission Spectra, Nitrogen Ions, Plasma Diagnostics, Aluminum, Ground State, Magnesium, Metal Ions, Molecular Collisions, Molecular Energy Levels

Scientific paper

The model solar atmosphere of Elzner (1976) is used to calculate the line intensities of Ne IV, Mg VI, and Al VII, supplementing the values for other N-like ions reported by Raju (1978) and Dwivedi and Raju (1988). The results are presented in extensive tables and graphs and characterized in detail, with reference to selected observational data. The focus is on the use of these emission lines as plasma-density diagnostics.

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