AUCLAIR-DESROTOUR, P.; MATHIS, Stéphane; LASKAR, Jacques; LECONTE, J.

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Licencia de uso del documento

AUCLAIR-DESROTOUR, P.
ECLIPSE 2018

MATHIS, Stéphane
Maintenance Myélinique et Neuropathies Périphériques [MMNP]

LASKAR, Jacques
Institut de Mécanique Céleste et de Calcul des Ephémérides [IMCCE]

Idioma

Communication dans un congrès

Este ítem está publicado en

Proceedings of the Annual meeting of the Frenh Society of Astronomy and Astrophysics. - 3 au 6 juillet 2018 – Bordeaux-France- SF2A-2018- Eds.: P. Di Matteo, F. Billebaud, F. Herpin, N. Lagarde, J.-B. Marquette, A. Robin, O. Venot, pp.33-35, 2018-07-03, Bordeaux.

Resumen en inglés

Oceanic tides are a major source of tidal dissipation. They are a key actor for the orbital and rotational evolution of planetary systems, and contribute to the heating of icy satellites hosting a subsurface ocean. Oceanic tides are characterized by a highly frequency-resonant behavior, which is mainly due to the propagation of surface gravity waves in the case of thin oceans, and internal waves when they are deeper. In this work, we derive self-consistent ab initio expressions of the oceanic tidal torque as a function of the key physical parameters of the system (the ocean depth, the Brunt-V\"ais\"al\"a stratification frequency, the rotation rate, the tidal frequency, the Rayleigh friction). These solutions include the coupled mechanisms of internal and surface gravito-inertial waves, which allows us to study the case of planets hosting deep oceans and offer interesting prospects for the coupling between subsurface oceans and ice shells in the case of icy satellites.< Leer menos

Palabras clave en inglés

Astrophysics - Earth and Planetary Astrophysics

85-06

Orígen

Importado de Hal

Centros de investigación

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804