22 citations · 43 across the 5 of their papers we have counts for
5 papers
Hydrodynamic modelling of dynamical tides dissipation in Jupiter's interior as revealed by Juno
Hachem Dhouib, Clément Baruteau, Stéphane Mathis +3
The Juno spacecraft has acquired exceptionally precise data on Jupiter's gravity field, offering invaluable insights into Jupiter's tidal response, interior structure, and dynamics…
Hydrodynamical modelling of tidal dissipation in gas giant planets at the time of space missions
Hachem Dhouib, Clément Baruteau, Stéphane Mathis +3
Gas giant planets are differentially rotating magnetic objects that have strong and complex interactions with their environment. In our Solar system, they interact with their numer…
Can we detect deep axisymmetric toroidal magnetic fields in stars?
Hachem Dhouib, Stéphane Mathis, Lisa Bugnet +2
One of the major discoveries of asteroseismology is the signature of a strong extraction of angular momentum (AM) in the radiative zones of stars across the entire Hertzsprung-Russ…
Detecting deep axisymmetric toroidal magnetic fields in stars. The traditional approximation of rotation for differentially rotating deep spherical shells with a general azimuthal magnetic field
Hachem Dhouib, Stéphane Mathis, Lisa Bugnet +2
Asteroseismology has revealed small core-to-surface rotation contrasts in stars in the whole HR diagram. This is the signature of strong transport of angular momentum (AM) in stell…
The traditional approximation of rotation for rapidly rotating stars and planets. I. The impact of strong deformation
Hachem Dhouib, Vincent Prat, Timothy Van Reeth +1
The Traditional Approximation of Rotation (TAR) is a treatment of the hydrodynamic equations of rotating and stably stratified fluids in which the action of the Coriolis accelerati…