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- W2964209927 abstract "The line pair He 3888 and H 8 3889 has been observed simultaneously with the Ca + 8498 line in a number of quiescent prominences. The He/H 8 emission ratio R is found to cover defined parts of a general anti-correlation with the total H 8 emission, depending on the kinetic temperature, T kin , of the individual prominence: High H 8 brightness is related to small R and T kin values and preferably occurs in prominences with less significant fine-structure" @default.
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- W2964209927 date "1994-06-01" @default.
- W2964209927 modified "2023-10-18" @default.
- W2964209927 title "Dependence of the He/H_8_ emission ratio on brightness, temperature, and structuring of prominences" @default.
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