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Line ratios for solar ultra-violet lines of Ov

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Abstract

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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Doyle, J.G., Dufton, P.L., Keenan, F.P. et al. Line ratios for solar ultra-violet lines of Ov . Sol Phys 89, 243–251 (1983). https://doi.org/10.1007/BF00217248

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  • DOI: https://doi.org/10.1007/BF00217248

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