Line diagnostics for NE V and MG V solar ions

Details Line diagnostics for NE V and MG V solar ions Line diagnostics for NE V and MG V solar ions

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..158..237d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 158, no. 2, p. 237-248

Physics

3

Ions, Line Spectra, Magnesium, Neon, Solar Atmosphere, Solar Physics, Solar Spectra, Sun, Astronomical Spectroscopy, Extreme Ultraviolet Radiation, Ratios, Soho Mission, Spectrum Analysis

Scientific paper

Spectroscopic diagnostics for the Ne V and Mg V solar ions have been investigated. The theoretical forbidden line ratios from these ions are presented for estimating the Ne/Mg variation in different solar structures. Calculations for density and temperature line diagnostics of these ions are given for the several spectral line ratios and their applications are discussed with the help of available solar observations in space. Future observations from the CDS and the SUMER experiments aboard the SOHO satellite are also discussed.

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