Densities in the quiet sun and coronal holes using EUV emission lines

Details Densities in the quiet sun and coronal holes using EUV emission lines Densities in the quiet sun and coronal holes using EUV emission lines

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..124..185d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 124, no. 1, 1989, p. 185-188.

Physics

Coronal Holes, Extreme Ultraviolet Radiation, Line Spectra, Plasma Diagnostics, Solar Activity, Solar Spectra, Atmospheric Models, Electron Density (Concentration), Emission Spectra, Magnesium, Silicon, Solar Atmosphere, Sulfur

Scientific paper

The density dependence of solar EUV line intensity ratios from Mg VIII, Si VII, S IX and Si IX ions have been used to determine electron densities in the quiet sun and coronal holes. The line intensity values have been computed using a model atmosphere of Kopp and Orrall (1976) in order to emphasize the utility of the lines studied which could be compared with observational data that future missions might provide.

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