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On the line intensity ratios E(Hα)/E(D3) and E(Hβ)/E(D3) in prominences
Authors:G Stellmacher
Institution:(1) Institut d'Astrophysique, Paris, France
Abstract:The intensity ratios E(Hagr)/E(D3) and E(Hbeta)/E(D3) in prominences depend on the total optical thickness in Hagr of the layer. The emission of the He D3 line appears relatively enhanced in thin layers and in outer parts of the prominences.
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