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Stellar turbulence and mode physics

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 01 Jan 2009Embargo end date: 01 Jan 2009 Austria English Publisher:Springer NetherlandsJournal:Astrophysics and Space Science, volume 328, pages 237-244 (issn: 0004-640X, eissn: 1572-946X, Copyright policy )Funded by:FWF | Asteroseismology: sonic p...
Authors: Houdek, Günter;

doi: 10.1007/978-90-481-9198-7_39 , 10.1007/s10509-009-0226-0 , 10.48550/arxiv.0911.4909

arXiv: 0911.4909

Stellar turbulence and mode physics

Abstract

An overview of selected topical problems on modelling oscillation properties in solar-like stars is presented. High-quality oscillation data from both space-borne intensity observations and ground-based spectroscopic measurements provide first tests of the still-ill-understood, superficial layers in distant stars. Emphasis will be given to modelling the pulsation dynamics of the stellar surface layers, the stochastic excitation processes and the associated dynamics of the turbulent fluxes of heat and momentum.

Proc. HELAS Workshop on 'Synergies between solar and stellar modelling', eds M. Marconi, D. Cardini, M. P. Di Mauro, Astrophys. Space Sci., in the press

Country
Austria
Related Organizations
Keywords

Astronomy, FOS: Physical sciences, asteroseismology, Astronomie, pulsation mode physics, stellar structure, Astrophysics - Solar and Stellar Astrophysics, Stability and instability of geophysical and astrophysical flows, 1030 Physics, 1030 Physik, Galactic and stellar structure, Hydrodynamic and hydromagnetic problems in astronomy and astrophysics, convection, Solar and Stellar Astrophysics (astro-ph.SR)

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    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 14
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    		 Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
14
Average
Average
Top 10%
Green
bronze
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