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- W2001063170 abstract "The solar O III spectrum above 900 A is analyzed, including several visible and infrared lines which are important in nebular studies. The dependence of the line intensities on the rate of photoexcitation by He Ly-alpha is determined, and the observability of these lines in the solar spectrum is studied. The impact approximation is employed to calculate the expected line widths of the stronger solar O III lines. The photoexciting field at 304 A calculated from the observed intensities of the O III lines below 900 A (Bhatia et al., 1982) is compared with the field predicted by a recent model (Avrett et al., 1976). It is shown that additional radiation trapping must be present beyond that given by this model." @default.
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- W2001063170 date "1983-09-01" @default.
- W2001063170 modified "2023-09-24" @default.
- W2001063170 title "The solar O III spectrum. II - Longer wavelengths, line widths, and the He II Lyman alpha radiation field" @default.
- W2001063170 doi "https://doi.org/10.1086/190887" @default.
- W2001063170 hasPublicationYear "1983" @default.
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