Tidal Effects in Stars, Planets and Disks
M.-J. Goupil and J.-P. Zahn (eds)
EAS Publications Series, 29 (2008) 127-147
DOI: 10.1051/eas:0829004
The dynamics of rotating fluids and binary stars
M. RieutordLaboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées, UMR 5572, CNRS et Université Paul Sabatier, 14 avenue E. Belin, 31400 Toulouse, France
Published online: 20 June 2008
Abstract
In this lecture I try to explain the basic concepts related to fluid
motions when a background rotation dominates the flows.
In particular, the notions of geostrophic flow, Ekman layer, Ekman
circulation are explained. However, the main focus of this lecture is on
the eigenmodes which occur in such a context and I emphasize here the
special effects conveyed to inertial and gravito-inertial modes
by the hyperbolic nature of the governing operators. A final section
introduces the case of the elliptic instability which I recently
suggested as one of the processes of binary synchronization.
© EAS, EDP Sciences 2008


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