Effect of dielectronic recombination excitation on solar line intensities

Details Effect of dielectronic recombination excitation on solar line intensities Effect of dielectronic recombination excitation on solar line intensities

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jqsrt..23..585c&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 23, June 1980, p. 585-593. Research supported by the Universi

Physics

1

Electron Recombination, Line Spectra, Solar Spectra, Electron Impact, Emission Spectra, Metal Ions, Solar Atmosphere, Tables (Data)

Scientific paper

The intensities of lines emitted from the solar atmosphere and observed on earth are calculated by considering electron-impact excitation followed by radiative emission. In order to determine the contribution of dielectronic-recombination excitation (DRE), the calculations have been repeated with the inclusion of DRE as a process for excitation, along with electron-impact excitation; the excited electron is assumed to deexcite through radiative emission. DRE is found to contribute significantly and the contribution generally increases with a decrease in wavelength and an increase of ionic charge.

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