Transitions between the N = 2 and N = 3 levels of NE VII in the solar spectrum

Details Transitions between the N = 2 and N = 3 levels of NE VII in the solar spectrum Transitions between the N = 2 and N = 3 levels of NE VII in the solar spectrum

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..105..313l&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 105, June 1986, p. 313-322.

Physics

9

Electron States, Electron Transitions, Line Spectra, Neon, Solar Spectra, Electron Density (Concentration), Electron Energy, Population Theory, Temperature Dependence

Scientific paper

Theoretical populations of the 2s3l levels of Ne VII are presented for electron temperatures from 2.5×105K to 4×106K and electron densities from 108cm-3 to 1012cm-3. These, in conjunction with intensities of previously observed solar Ne VII lines and wavelengths and intensities observed in the laboratory, are used to identify further Ne VII lines in the solar spectrum. The dependence on temperature of intensity ratios such as I(2s2p1P-2s3d1D)/I(2s2p3P-2s3d3D) is demonstrated and the advantages of the small wavelength separation of such lines for solar electron temperature diagnostics are discussed.

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