Electron density diagnostics for Fe XII in the solar plasma

Details Electron density diagnostics for Fe XII in the solar plasma Electron density diagnostics for Fe XII in the solar plasma

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...343.1004t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 343, Aug. 15, 1989, p. 1004-1006. Research supported by DOE and SERC.

Astronomy and Astrophysics

Astrophysics

17

Electron Density (Concentration), Solar Activity Effects, Solar Flares, Solar Wind, Emission Spectra, Line Spectra, Solar Spectra, Ultraviolet Spectra

Scientific paper

Density-sensitive emission-line ratios R1 = I(338.27 A)/I(364.47 A) and R2 = I(338.27 A)/I(352.10 A) are calculated for Fe XII using new electron collisional excitation rates which are substantially larger than those previously published. Electron densities deduced from the values of R1 and R2 for solar active regions and flares obtained by the NRL S082A slitless spectrograph on Skylab are in good agreement.

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