150 citations · 286 across the 8 of their papers we have counts for
8 papers
Electric interface condition for sliding and viscous contacts
Jérémy Rekier, Santiago A. Triana, Antony Trinh +1
First principles of electromagnetism impose that the tangential electric field must be continuous at the interface between two media. The definition of the electric field depends o…
Powering the Galilean Satellites with Moon-Moon Tides
Hamish C. F. C. Hay, Antony Trinh, Isamu Matsuyama
There is compelling evidence for subsurface water oceans among the three outer Galilean satellites, and evidence for an internal magma ocean in the innermost moon, Io. Tidal forces…
Inertial modes of a freely rotating ellipsoidal planet and their relation to nutations
Jeremy Rekier, Santiago A. Triana, Antony Trinh +1
We compute the inertial modes of a freely rotating two-layer planetary model with an ellipsoidal inviscid fluid core and a perfectly rigid mantle. We present a method to derive ana…
The formation of the Martian moons
Pascal Rosenblatt, Ryuki Hyodo, Francesco C. Pignatale +5
Almost all the planets of our solar system have moons. Each planetary system has however unique characteristics. The Martian system has not one single big moon like the Earth, not…
The coupling between inertial and rotational eigenmodes in planets with liquid cores
Santiago Andres Triana, Jeremy Rekier, Antony Trinh +1
The Earth is a rapidly rotating body. The centrifugal pull makes its shape resemble a flattened ellipsoid and Coriolis forces support waves in its fluid core, known as inertial wav…
Inertial Modes in Near-Spherical Geometries
J. Rekier, A. Trinh, S. A. Triana +1
We propose a numerical method to compute the inertial modes of a container with near-spherical geometry based on the fully spectral discretisation of the angular and radial directi…
Internal energy dissipation in Enceladus's ocean from tides and libration and the role of inertial waves
J. Rekier, A. Trinh, S. A. Triana +1
Enceladus is characterised by a south polar hot spot associated with a large outflow of heat, the source of which remains unclear. We compute the viscous dissipation resulting from…
Enceladus's and Dione's floating ice shells supported by minimum stress isostasy
Mikael Beuthe, Attilio Rivoldini, Antony Trinh
Enceladus's gravity and shape have been explained in terms of a thick isostatic ice shell floating on a global ocean, in contradiction of the thin shell implied by librations. Here…