On the electron density in sunspot plumes

Details On the electron density in sunspot plumes On the electron density in sunspot plumes

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..123..385d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 123, no. 2, 1989, p. 385-387.

Physics

1

Electron Density (Concentration), Extreme Ultraviolet Radiation, Solar Wind, Sunspots, Magnesium, Plasma Diagnostics, Skylab Program, Solar Corona

Scientific paper

The Noyes et al. (1985) EUV line intensity observations in sunspot plumes are presently used to determine electron densities from theoretical curves of the Mg VI and Mg VIII density-sensitive line ratios. It is found that, in general, the curves for Mg VI are clearly good candidates for diagnosing events whose apparent density lies above 10 to the 10th/cu cm. The curves for Mg VI show a large variation in density according to the density-sensitive ratio used as a diagnostic.

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