| Issue |
EAS Publications Series
Volume 21, 2006
Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars
|
|
|---|---|---|
| Page(s) | 105 - 126 | |
| DOI | https://doi.org/10.1051/eas:2006108 | |
| Published online | 07 June 2006 | |
Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars
M. Rieutord and B. Dubrulle (eds)
EAS Publications Series, 21 (2006) 105-126
M. Rieutord and B. Dubrulle (eds)
EAS Publications Series, 21 (2006) 105-126
Wave transport in stratified media
Département de Physique, Université de Montréal, CP 6128,
Succursale Centre-Ville, Montréal, Québec, H3C 3J8
In this course, I will review the main properties of internal gravity waves, and examine how they can lead to particle and angular momentum transport in stars. I will then present some recent results that have been obtained for angular momentum transport which show that waves are an important ingrediant of stellar modelling.
© EAS, EDP Sciences, 2006