activity
20172026
most citedMagnetic signatures on mixed-mode frequencies. I. An axisymmetric fossil field inside the core of red giants

59 citations · 169 across the 19 of their papers we have counts for

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6 papers · 1 filter

astro-ph.EP2026

Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations

Shijun Chu, Zhao Guo, Aurélie Astoul +2

We study tidal flows in the convective envelopes of rotating, magnetised fluid bodies, such as low-mass stars and giant planets. In well-mixed convective regions, (magneto-)inertia…

astro-ph.EP2025

The stability of propagating plane inertial waves in rotating fluids

Valentin Skoutnev, Aurélie Astoul, Adrian J. Barker

Inertial waves transport energy and momentum in rotating fluids and are a major contributor to mixing and tidal dissipation in Earth's oceans, gaseous planets, and stellar interior…

astro-ph.EP2023

Tidal dissipation in rotating and evolving giant planets with application to exoplanet systems

Yaroslav A. Lazovik, Adrian J. Barker, Nils B. de Vries +1

We study tidal dissipation in models of rotating giant planets with masses in the range throughout their evolution. Our models incorporate a frequency-depen…

astro-ph.EP2023★ 1 cited

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…

astro-ph.EP2023

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…

astro-ph.EP2022★ 9 cited

How do tidal waves interact with convective vortices in rapidly-rotating planets and stars?

Virgile Dandoy, Junho Park, Kyle Augustson +2

The dissipation of tidal inertial waves in planetary and stellar convective regions is one of the key mechanisms that drive the evolution of star-planet/planet-moon systems. In thi…