Tidal dissipation in giant planets
Tidal interactions between moons and planets can have major effects on the orbits, spins,
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …
[HTML][HTML] The EU Center of Excellence for Exascale in Solid Earth (ChEESE): Implementation, results, and roadmap for the second phase
Abstract The EU Center of Excellence for Exascale in Solid Earth (ChEESE) develops
exascale transition capabilities in the domain of Solid Earth, an area of geophysics rich in …
exascale transition capabilities in the domain of Solid Earth, an area of geophysics rich in …
The effects of non-linearities on tidal flows in the convective envelopes of rotating stars and planets in exoplanetary systems
In close exoplanetary systems, tidal interactions drive orbital and spin evolution of planets
and stars over long time-scales. Tidally forced inertial waves (restored by the Coriolis …
and stars over long time-scales. Tidally forced inertial waves (restored by the Coriolis …
Vortex cluster arising from an axisymmetric inertial wave attractor
S Boury, I Sibgatullin, E Ermanyuk… - Journal of Fluid …, 2021 - cambridge.org
We present an experimental and numerical study of the nonlinear dynamics of an inertial
wave attractor in an axisymmetric geometrical setting. The rotating ring-shaped fluid domain …
wave attractor in an axisymmetric geometrical setting. The rotating ring-shaped fluid domain …
[PDF][PDF] Tidal Dissipation in Giant Planets
Tidal interactions between moons and planets can have major effects on the orbits, spins,
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …
and thermal evolution of the moons. In the Saturn system, tidal dissipation in the planet …
Precession-driven flows in stress-free ellipsoids
Motivated by modelling rotating turbulence in planetary fluid layers, we investigate
precession-driven flows in ellipsoids subject to stress-free boundary conditions (SF-BC). The …
precession-driven flows in ellipsoids subject to stress-free boundary conditions (SF-BC). The …
[HTML][HTML] Resonant and non-resonant flows in longitudinally and latitudinally librating spheres
Resonant and non-resonant flows in longitudinally and latitudinally librating spheres | Physics of
Fluids | AIP Publishing Skip to Main Content Umbrella Alt Text Umbrella Alt Text Close …
Fluids | AIP Publishing Skip to Main Content Umbrella Alt Text Umbrella Alt Text Close …
Noise induced effects in the axisymmetric spherical Couette flow
O Krivonosova, M Gritsevich… - … Transactions of the …, 2023 - royalsocietypublishing.org
We study the axisymmetric, wide gap, spherical Couette flow in the presence of noise in
numerical simulations and experiments. Such studies are important because most of the …
numerical simulations and experiments. Such studies are important because most of the …
Mean flow induced by longitudinal libration of a fluid-filled rotating container bounded by two conical surfaces
MV Kurgansky - European Journal of Mechanics-B/Fluids, 2024 - Elsevier
The problem of determining a mean flow induced by longitudinal libration of a rapidly
rotating fluid-filled container bounded by the surfaces of two oppositely oriented right circular …
rotating fluid-filled container bounded by the surfaces of two oppositely oriented right circular …
The spectrum of the Poincar {\'e} operator in an ellipsoid
YC de Verdiere, J Vidal - arXiv preprint arXiv:2305.01369, 2023 - arxiv.org
We reprove the fact, due to Backus, that the Poincar {\'e} operator in ellipsoids admits a pure
point spectrum with polynomial eigenfunctions. We then show that the eigenvalues of the …
point spectrum with polynomial eigenfunctions. We then show that the eigenvalues of the …