40 citations · 82 across the 4 of their papers we have counts for
4 papers
Tidal dissipation by inertial waves in differentially rotating convective envelopes of low-mass stars
Mathieu Guenel, Stéphane Mathis, Clément Baruteau +1
Tidal interactions in close star-planet or binary star systems may excite inertial waves (their restoring force is the Coriolis force) in the convective region of the stars. The di…
The impact of rotation on turbulent tidal friction in stellar and planetary convective regions
Stéphane Mathis, Pierre Auclair-Desrotour, Mathieu Guenel +2
Turbulent friction in convective regions in stars and planets is one of the key physical mechanisms that drive the dissipation of the kinetic energy of tidal flows in their interio…
Tidal inertial waves in the differentially rotating convective envelopes of low-mass stars - I. Free oscillation modes
M. Guenel, C. Baruteau, S. Mathis +1
Star-planet tidal interactions may result in the excitation of inertial waves in the convective region of stars. In low-mass stars, their dissipation plays a prominent role in the…
Free inertial modes in differentially rotating convective envelopes of low-mass stars : numerical exploration
M. Guenel, C. Baruteau, S. Mathis +1
Tidally-excited inertial waves in stellar convective regions are a key mechanism for tidal dissipation in stars and therefore the evolution of close-in binary or planetary systems.…