Search Results - "Petitdemange, L."
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Magnetohydrodynamics of stably stratified regions in planets and stars
Published in Geophysical and astrophysical fluid dynamics (03-05-2020)“…Stably stratified layers are present in stellar interiors (radiative zones) as well as planetary interiors - recent observations and theoretical studies of the…”
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2
Dipolar dynamos in stratified systems
Published in Monthly notices of the Royal Astronomical Society (11-04-2015)“…Observations of low-mass stars reveal a variety of magnetic field topologies ranging from large-scale, axial dipoles to more complex magnetic fields. At the…”
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3
Bistability between equatorial and axial dipoles during magnetic field reversals
Published in Physical review letters (08-06-2012)“…Numerical simulations of the geodynamo in the presence of heterogeneous heating are presented. We study the dynamics and the structure of the magnetic field…”
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Coriolis darkening in late-type stars II. Effect of self-sustained magnetic fields in stratified convective envelope
Published 13-03-2024“…Modeling the surface brightness distribution of stars is of prime importance to interpret observations. Nevertheless, this remains quite challenging for cool…”
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5
Magnetohydrodynamics of stably stratified regions in planets and stars
Published 09-10-2019“…Stably stratified layers are present in stellar interiors (radiative zones) as well as planetary interiors - recent observations and theoretical studies of the…”
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Journal Article -
6
Dipolar dynamos in stratified systems
Published 03-03-2015“…2015, MNRAS, 448(3), 2055-2065 Observations of low-mass stars reveal a variety of magnetic field topologies ranging from large-scale, axial dipoles to more…”
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7
Topology and field strength in spherical, anelastic dynamo simulations
Published 02-03-2015“…A&A, 564, A78 (2014) Numerical modelling of convection driven dynamos in the Boussinesq approximation revealed fundamental characteristics of the…”
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Oscillatory dynamos and their induction mechanisms
Published 10-01-2011“…Context: Large-scale magnetic fields resulting from hydromagnetic dynamo action may differ substantially in their time dependence. Cyclic field variations,…”
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