Core eigenmodes and their impact on the Earth's rotation
Abstract Changes in the Earth's rotation are deeply connected to fluid dynamical processes
in the outer core. This connection can be explored by studying the associated Earth …
in the outer core. This connection can be explored by studying the associated Earth …
First field application of cyclic soft stimulation at the Pohang Enhanced Geothermal System site in Korea
H Hofmann, G Zimmermann, M Farkas… - Geophysical Journal …, 2019 - academic.oup.com
Precession of planets or moons affects internal liquid layers by driving flows, instabilities and
possibly dynamos. The energy dissipated by these phenomena can influence orbital …
possibly dynamos. The energy dissipated by these phenomena can influence orbital …
Fast quasi‐geostrophic Magneto‐Coriolis modes in the Earth's core
Fast changes of Earth's magnetic field could be explained by inviscid and diffusion‐less
quasi‐geostrophic (QG) Magneto‐Coriolis modes. We present a hybrid QG model with …
quasi‐geostrophic (QG) Magneto‐Coriolis modes. We present a hybrid QG model with …
Precessing spherical shells: flows, dissipation, dynamo and the lunar core
Precession of planets or moons affects internal liquid layers by driving flows, instabilities and
possibly dynamos. The energy dissipated by these phenomena can influence orbital …
possibly dynamos. The energy dissipated by these phenomena can influence orbital …
Turbulent viscosity acting on the equilibrium tidal flow in convective stars
Convection is thought to act as a turbulent viscosity in damping tidal flows and in driving spin
and orbital evolution in close convective binary systems. This turbulent viscosity should be …
and orbital evolution in close convective binary systems. This turbulent viscosity should be …
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 …
Libration‐driven flows in ellipsoidal shells
Planets and satellites can undergo physical librations, which consist of forced periodic
variations in their rotation rate induced by gravitational interactions with nearby bodies. This …
variations in their rotation rate induced by gravitational interactions with nearby bodies. This …
Experimental study of the nonlinear saturation of the elliptical instability: inertial wave turbulence versus geostrophic turbulence
In this paper, we present an experimental investigation of the turbulent saturation of the flow
driven by the parametric resonance of inertial waves in a rotating fluid. In our set-up, a half …
driven by the parametric resonance of inertial waves in a rotating fluid. In our set-up, a half …
Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
Turbulent convection is thought to act as an effective viscosity in damping equilibrium tidal
flows, driving spin and orbital evolution in close convective binary systems. Compared to …
flows, driving spin and orbital evolution in close convective binary systems. Compared to …
Magnetic fields driven by tidal mixing in radiative stars
Stellar magnetism plays an important role in stellar evolution theory. Approximatively 10 per
cent of observed main sequence (MS) and pre-main-sequence (PMS) radiative stars exhibit …
cent of observed main sequence (MS) and pre-main-sequence (PMS) radiative stars exhibit …