Understanding fluid flows in planetary cores and subsurface oceans, as well as their signatures in available observational data (gravity, magnetism, rotation, etc.), is a …
A Astoul, AJ Barker - The Astrophysical Journal Letters, 2023 - iopscience.iop.org
We simulate the nonlinear hydrodynamical evolution of tidally excited inertial waves in convective envelopes of rotating stars and giant planets modeled as spherical shells …
A Astoul, AJ Barker - Monthly Notices of the Royal Astronomical …, 2022 - academic.oup.com
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 …
This work is devoted to an experimental study of the stability of a steady flow in a rotating spherical cavity with an oscillating core. The case of circular core oscillations in a plane …
Context. Surface magnetic fields have been detected in 5–10% of isolated massive stars, hosting outer radiative envelopes. They are often thought to have a fossil origin, resulting …
S Subbotin, M Shiryaeva - Physics of Fluids, 2021 - pubs.aip.org
Fluid flow excited by a core oscillating in a rotating spherical cavity is experimentally investigated. Oscillations are set by an external inertial field so that in the reference frame of …
F Garcia, M Seilmayer, A Giesecke… - … Interdisciplinary Journal of …, 2020 - pubs.aip.org
Direct numerical simulations of a liquid metal filling the gap between two concentric spheres are presented. The flow is governed by the interplay between the rotation of the inner sphere …
The occurrence of magnetohydrodynamic quasiperiodic flows with four fundamental frequencies in differentially rotating spherical geometry is understood in terms of a sequence …
K Yoshikawa, T Itano, M Sugihara-Seki - Physics of Fluids, 2023 - pubs.aip.org
Spherical Couette flow experiments were conducted according to the work of Egbers and Rath [Acta Mech. 111, 125–140 (1995)]. While the value of the critical Reynolds number …