Two-scale mass-flux closure models for turbulence: p-mode amplitudes in 
solar-like stars

Belkacem, K.; Samadi, R.; Goupil, M.-J.; Kupka, F.; Dupret, M.-A.

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Conference Paper

Two-scale mass-flux closure models for turbulence: p-mode amplitudes in solar-like stars

MPS-Authors

/persons/resource/persons20215

Kupka, F.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Belkacem, K., Samadi, R., Goupil, M.-J., Kupka, F., & Dupret, M.-A. (2007). Two-scale mass-flux closure models for turbulence: p-mode amplitudes in solar-like stars. Communications in Asteroseismology, (150), 153-154.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-ACEF-A

Abstract

There is no abstract available