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Der Sonnenrand. Chromosphäre, Korona und Protuberanzen. Spektroheliogramme

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Book cover Physik der Sternatmosphären

Zusammenfassung

Wir ergänzen zunächst den einleitenden Abschnitt 132 des vorhergehenden Kapitels durch einige allgemeine Bemerkungen über Art und Technik der Beobachtung totaler Sonnenfinsternisse: Kurz vor Beginn der Totalität strahlt die äußerste Zone der Photosphäre stellenweise durch die Täler des Mondes. Dessen Rand erscheint daher wie von einer Kette leuchtender Perlen umgeben, den sog. Baily-Beads.

The erratum of this chapter is available at http://dx.doi.org/10.1007/978-3-642-47425-5_36

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  1. Universität Kiel, Deutschland

    Dr. A. Unsöld (Professor für Theoretische Physik)

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© 1955 Springer-Verlag Ohg. Berlin · Göttingen · Heidelberg

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Unsöld, A. (1955). Der Sonnenrand. Chromosphäre, Korona und Protuberanzen. Spektroheliogramme. In: Physik der Sternatmosphären. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-47425-5_21

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  • DOI: https://doi.org/10.1007/978-3-642-47425-5_21

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