Protuberanzen über dem Sonnenrand im Licht der roten Wasserstoff-Linie H-alpha mit Messspalt (weiß) und der blauen Emission des Ortho-Heliums, überlagert vom Spektrum des Himmels-Streulichts; darunter das 100-fach abgeschwächte Spektrum der Sonnen-Scheibe, auf der Helium nicht emittiert wird; Fotomontage: Uwe Nolte (GWDG).
Source: Foto: Universität Göttingen
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