Line ratios for solar ultra-violet lines of OV

Details Line ratios for solar ultra-violet lines of OV Line ratios for solar ultra-violet lines of OV

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...89..243d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 89, Dec. 1983, p. 243-251. Research supported by the Science and Engineering Research Counc

Astronomy and Astrophysics

Astronomy

16

Line Spectra, Oxygen Spectra, Solar Spectra, Ultraviolet Astronomy, Electron Density (Concentration), Electron Impact, Plasma Temperature, Proton Impact, Satellite-Borne Instruments

Scientific paper

New O V rate coefficients are used to calculate the ratio of the
intensity of the 760 Å multiplet to that of the 630 Å line.
Results are given for a range of electron densities and temperatures.
The theoretical ratios are compared with observed line ratios for
different solar regions.

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