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On the computation of resonant tidal dissipation in the liquid layers of planets and stars

Published online by Cambridge University Press:  16 October 2024

Jérémy Rekier Open the ORCID record for Jérémy Rekier [Opens in a new window]  and
Santiago A. Triana
Jérémy Rekier*
Affiliation:
Royal Observatory of Belgium, 3 avenue circulaire, 1180 Brussels, Belgium Dpt. of Earth & Planetary Science, University of California, Berkeley, California 94720, USA
Santiago A. Triana
Affiliation:
Royal Observatory of Belgium, 3 avenue circulaire, 1180 Brussels, Belgium
*
email: jeremy.rekier@observatory.be
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Abstract

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Planets and stars have liquid layers that can support internal gravity waves and inertial waves respectively restored by the buoyancy and Coriolis forces. Both types of waves are excited by tides, leading to resonantly amplified dissipation. We review the theoretical formalism to compute these resonances and present some challenges and methods to overcome them.

Keywords

liquid layersbuoyancyCoriolistidesresonances
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S382: Complex Planetary Systems II: Latest Methods for an Interdisciplinary Approach , December 2022 , pp. 167 - 173
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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