Hochschulschrift
Generation and propagation of longitudinal tube waves in late-type stellar atmospheres and the rotation-emission activity relation
- Location
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Deutsche Nationalbibliothek Frankfurt am Main
- Dimensions
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30 cm
- Extent
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III, 127, V S.
- Language
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Englisch
- Notes
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graph. Darst.
Heidelberg, Univ., Diss., 2001
- Keyword
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Späte Spektralklasse
Sternatmosphäre
Longitudinalwelle
Flussschlauch
Sternatmosphäre
Magnetohydrodynamik
Sternrotation
Chromosphäre
- Creator
- Table of contents
- Rights
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Bei diesem Objekt liegt nur das Inhaltsverzeichnis digital vor. Der Zugriff darauf ist unbeschränkt möglich.
- Last update
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11.06.2025, 2:04 PM CEST
Data provider
This object is provided by:
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Deutsche Nationalbibliothek. If you have any questions about the object, please contact the data provider.
Object type
- Hochschulschrift
Associated
Other Objects (12)
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Generation and propagation of longitudinal tube waves in late-type stellar atmospheres and the rotation-emission activity relation
Characterization of stellar and sub-stellar atmospheres
Characterization of stellar and sub-stellar atmospheres
Problems in stellar atmospheres and envelopes
Diffusion processes in white dwarf stellar atmospheres
Non-analytical line profiles in stellar atmospheres : for planetary host star systems
Observational diagnostics of 3D radiation-MHD simulations of solar and stellar atmospheres
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Simulating supernova shock propagation through stellar envelopes in 3D
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Differential rotation and stellar convection : sun and solar-type stars
Generation and propagation of longitudinal tube waves in late-type stellar atmospheres and the rotation-emission activity relation
Characterization of stellar and sub-stellar atmospheres
Characterization of stellar and sub-stellar atmospheres
Problems in stellar atmospheres and envelopes
Diffusion processes in white dwarf stellar atmospheres
Non-analytical line profiles in stellar atmospheres : for planetary host star systems
Observational diagnostics of 3D radiation-MHD simulations of solar and stellar atmospheres
Großbritannien.- London.- Kolloquium Nr. 51 (Turbulence in Stellar Atmospheres) der Internationalen Astronomischen Union
Simulating supernova shock propagation through stellar envelopes in 3D
Atmospheres
Atmosphères