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Anwendung der Theorie der Fraunhofer-Linien
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Author(s):
A. Unsöld
Publication date
(Print):
1938
Publisher:
Springer Berlin Heidelberg
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Kindheit, Jugend und Entwicklung
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On the Composition of the Sun's Atmosphere
Henry Norris Russell
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Molecules in the Sun and Stars
Henry Norris Russell
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The Spectroscopic Absolute Magnitudes and Parallaxes of 4179 Stars
Walter Adams
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Alfred H. Joy
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Milton Humason
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(1935)
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Book Chapter
Publication date (Print):
1938
Pages
: 331-349
DOI:
10.1007/978-3-642-50754-0_15
SO-VID:
968e1b2a-874c-4caf-aa7a-7b8072b4b0a9
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Book chapters
pp. 1
Strahlungstheorie
pp. 21
Anwendung des Planckschen Gesetzes auf die Strahlung der Sonne. Strahlungsmessungen
pp. 40
Die Strahlung der Sterne
pp. 62
Thermische Ionisation und Anregung
pp. 88
Strahlungsgleichgewicht und kontinuierliches Spektrum der Sternatmosphären
pp. 113
Kontinuierlicher Absorptionskoeffizient und Energieverteilung in den kontinuierlichen Spektren der Sterne
pp. 141
Der Aufbau der Sternatmosphären
pp. 148
Physikalische Grundlagen der Theorie der Fraunhofer-Linien. I.Teil: Klassische Theorie
pp. 169
Physikalische Grundlagen der Theorie der Fraunhofer-Linien. 2. Teil: Quantentheorie
pp. 196
Physikalische Grundlagen der Theorie der Fraunhofer-Linien. 3. Teil. Experimentelle Prüfung der Theorie und Messung von Übergangswahrscheinlichkeiten usw
pp. 208
Messung der Konturen und Gesamtabsorptionen von Fraunhofer-Linien
pp. 226
Strahlungsgleichgewicht und Fraunhofer-Linien
pp. 264
Die Deutung der Fraunhofer-Linien. Beobachtung und Theorie
pp. 316
Beeinflussung der Linienkonturen durch Rotation und Expansion der Sterne
pp. 331
Anwendung der Theorie der Fraunhofer-Linien
pp. 350
Die Struktur der äußeren Schichten der Sonne
pp. 390
Der Sonnenrand. Protuberanzen, Chromosphäre und Korona. Spektroheliogramme
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