Electron density from MG VIII emission lines

Details Electron density from MG VIII emission lines Electron density from MG VIII emission lines

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..116..405d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 116, no. 2, 1988, p. 405-408.

Physics

9

Chromosphere, Electron Density (Concentration), Electron Plasma, Emission Spectra, Line Spectra, Solar Corona, Coronal Holes, Extreme Ultraviolet Radiation, Magnesium, Plasma Diagnostics, Solar Activity

Scientific paper

The Mg VIII emission line intensity ratio I(430.47)/I(436.62) is used to provide data on the quiet sun and coronal holes. Using the model of Kopp and Orrall (1976), electron densities of 10 to the 9th/cu cm for the quiet sun and 4.6 x 10 the 8th/cu cm for the coronal holes are found. The results support the previous density findings of Dwivedi and Raju (1980), derived using Mg VIII emission line data.

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