| Issue |
|
EAS Publications Series
Volume 21,
2006
Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars
|
|
Page(s)
|
|
3 |
| DOI |
|
10.1051/eas:2006103 |
| 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) 3-3DOI: 10.1051/eas:2006103
The foundations of fluid dynamics
M. Rieutord Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées, UMR 5572,
CNRS et Université Paul Sabatier, 14 avenue E. Belin, 31400 Toulouse,
France
Abstract
In this lecture I introduce the basic concepts needed to understand
fluid motions at a macroscopic level. Hence, the idea of a continuous
medium and its kinematical properties are presented. Then the physical
laws governing the motion (mass, momentum and energy equation) are
derived and discussed. The concept of rheological law is introduced and
illustrated. I end this lecture with a discussion of the boundary
conditions that are needed to complete the equations of motion.
© EAS, EDP Sciences 2006
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