Sustaining Earth's magnetic dynamo

M Landeau, A Fournier, HC Nataf, D Cébron… - Nature Reviews Earth & …, 2022 - nature.com
Earth's magnetic field is generated by fluid motions in the outer core. This geodynamo has
operated for over 3.4 billion years. However, the mechanism that has sustained the …

Tidal dissipation in stars and giant planets

GI Ogilvie - Annual Review of Astronomy and Astrophysics, 2014 - annualreviews.org
Astrophysical fluid bodies that orbit close to one another induce tidal distortions and flows
that are subject to dissipative processes. The spin and orbital motions undergo a coupled …

Quasi-periodic eruptions from mildly eccentric unstable mass transfer in galactic nuclei

W Lu, E Quataert - Monthly Notices of the Royal Astronomical …, 2023 - academic.oup.com
We propose that the recently observed quasi-periodic eruptions (QPEs) in galactic nuclei
are produced by unstable mass transfer due to Roche lobe overflow of a low-mass main …

Flows driven by libration, precession, and tides

M Le Bars, D Cébron, P Le Gal - Annual Review of Fluid …, 2015 - annualreviews.org
Because of gravitational interactions with their companions, the rotational dynamics of
planets and stars involve periodic perturbations of their shape, the direction of their …

An impact-driven dynamo for the early Moon

M Le Bars, MA Wieczorek, Ö Karatekin, D Cébron… - Nature, 2011 - nature.com
The origin of lunar magnetic anomalies,,,, remains unresolved after their discovery more
than four decades ago. A commonly invoked hypothesis is that the Moon might once have …

Nonlinear tides in close binary systems

NN Weinberg, P Arras, E Quataert… - The Astrophysical …, 2012 - iopscience.iop.org
We study the excitation and damping of tides in close binary systems, accounting for the
leading-order nonlinear corrections to linear tidal theory. These nonlinear corrections …

The deep Earth may not be cooling down

D Andrault, J Monteux, M Le Bars, H Samuel - Earth and planetary science …, 2016 - Elsevier
The Earth is a thermal engine generating the fundamental processes of geomagnetic field,
plate tectonics and volcanism. Large amounts of heat are permanently lost at the surface …

Non-linear evolution of tidally forced inertial waves in rotating fluid bodies

B Favier, AJ Barker, C Baruteau… - Monthly Notices of the …, 2014 - academic.oup.com
We perform one of the first studies into the non-linear evolution of tidally excited inertial
waves in a uniformly rotating fluid body, exploring a simplified model of the fluid envelope of …

The equilibrium tide in stars and giant planets-I. The coplanar case

F Remus, S Mathis, JP Zahn - Astronomy & Astrophysics, 2012 - aanda.org
Context. Since 1995, more than 500 extrasolar planets have been discovered orbiting very
close to their parent star, where they experience strong tidal interactions. Their orbital …

Inertial wave turbulence driven by elliptical instability

T Le Reun, B Favier, AJ Barker, M Le Bars - Physical Review Letters, 2017 - APS
The combination of elliptical deformation of streamlines and vorticity can lead to the
destabilization of any rotating flow via the elliptical instability. Such a mechanism has been …