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Auslöschung der koronalen [FeX]3 s2 3 p52P1/2−2P1 1/2-Strahlung (6374 Å) durch Protuberanzen

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Summary

It is shown that the intensity of the red coronal line 6374 Á is diminished in the regions of the stationary solar prominences.

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  1. Astrophysikalisches Observatorium der Eidg. Sternwarte, Arosa

    M. Waldmeier

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  1. M. Waldmeier
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Waldmeier, M. Auslöschung der koronalen [FeX]3 s2 3 p52P1/2−2P1 1/2-Strahlung (6374 Å) durch Protuberanzen. Experientia 2, 220–221 (1946). https://doi.org/10.1007/BF02172772

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  • DOI: https://doi.org/10.1007/BF02172772

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