Jérémie Vidal (Ph.D.)
CNRS Researcher, LGL-TPE (ENS Lyon - Univ. Lyon 1)
Email: jeremie [dot] vidal [at] ens-lyon [dot] fr
Tutorials - 30 h - Modelling with Ordinary Differential Equations, B.Sc. in Applied Mathematics
Tutorials - 20 h - Calculus and Mathematical Analysis, B.Sc. in Applied Mathematics
Lectures notes - Geophysical Fluid Dynamics, M. Sc. (M2R) in Geophysics & Fuid Dynamics
Tutorials - 30 h - Internal geodynamics & Heat Transferts, M. Sc. (M1) in Geophysics
Tutorials - 30 h - Mathematical Tools for Earth Sciences, B. Sc (L3) in Geosciences
Tutorials - 30 h - Complex Analysis, B. Sc. (L3) in Mechanics
Tutorials - 15 h - Partial Differential Equations, B. Sc. (L3) in Mechanics,
Tutorials - 18 h - Geomagnetism, B. Sc. (L3) in Geosciences
Lab. work - 6 h - Rayleigh-Bénard convection, B. Sc. (L2) in Physics and Geosciences
L2 & L3: Second and third academic years in France. M1: Fourth academic year in France.
M2R: Fifth academic year in France (preparation for Ph.D. fellowships)
June - July 2025: Angèle Bichot (B.Sc, ENS Ulm), Influence de la topographie sur les modes d'oscillation d'un fluide en rotation
Co-supervised with D. Cébron
August 2018: Remy Monville (B.Sc., Univ. Grenoble Alpes), Rotating convection in stably stratified planetary cores
Co-supervised with D. Cébron and Dr N. Schaeffer. One Publication!
January - June 2015: Rizka Zakiah Drajat (M.Sc., Univ. Grenoble Alpes), Alven waves in the Earth’s outer core
Co-supervised with N. Schaeffer and Dr L. Métivier (LJK)
May 2015: Nicolas Durand (B.Sc., Univ. Grenoble Alpes),Visualisations in Geomagnetism using Matplotlib
Co-supervised with D. Jault.
Spring 2015: Yann Alexanian (B.Sc., Univ. Grenoble Alpes), Pedagogical experiment of an MHD propulsion boat
Co-supervised with D. Cébron. One Publication!
Fig. 1: Proof-of-concept MHD boat (built with Y. Alexanian). See the improved version published in Cébron et al. (2017, Plos One).
During my PhD, I was involved in the graduate course (M.Sc.) Geophysical Fluid Dynamics. The course aimed at giving the students the basics to understand the dynamics of planetary and stellar fluids layers (e.g. atmospheres, planetary liquid cores), dealing with rotating flows, hydrodynamic stability theory and wave motions.
Here are the title of chapters to outline the physical content.
Chapter 1 - Rotating fluids
Chapter 2 - Stratified fluids
Chapter 3 - Linear hydrodynamic stability
Chapter 4 - Gravitational effects in rotating fluids
Chapter 5 - Thermal convection I (linear study)
Chapter 6 - Thermal convection II (weakly non-linear analysis)
Chapter 7 - Turbulence