activity
20072022
most citedA 3D kinematic Babcock Leighton solar dynamo model sustained by dynamic magnetic buoyancy and flux transport processes

31 citations · 151 across the 9 of their papers we have counts for

collaborators

14 papers

astro-ph.SR202219 cited

Transition from multipolar to dipolar dynamos in stratified systems

B. Zaire, L. Jouve, T. Gastine +4

Observations of surface magnetic fields of cool stars reveal a large diversity of configurations. Although there is now a consensus that these fields are generated through dynamo p…

astro-ph.IM2022

Well-being in French Astrophysics

N. A. Webb, C. Bot, S. Charpinet +8

It has become clear that early career astrophysics researchers (doctoral researchers, post-docs, etc) have a very diverse appreciation of their career, with some declaring it the b…

astro-ph.SR202213 cited

Angular momentum transport in a contracting stellar radiative zone embedded in a large scale magnetic field

B. Gouhier, L. Jouve, F. Lignières

Some contracting or expanding stars are thought to host a large-scale magnetic field in their radiative interior. By interacting with the contraction-induced flows, such fields may…

astro-ph.SR2020

Axisymmetric investigation of differential rotation in contracting stellar radiative zones

B. Gouhier, F. Lignières, L. Jouve

Context. Stars experience rapid contraction or expansion at different phases of their evolution. Modelling the angular momentum and chemical elements transport occurring during the…

astro-ph.SR202025 cited

Interplay between magnetic fields and differential rotation in a stably stratified stellar radiative zone

L. Jouve, F. Lignières, M. Gaurat

The present study aims at studying the flow and field produced by a stellar radiative zone which is initially made to rotate differentially in the presence of a large-scale poloida…

astro-ph.SR2019

Dipolar stability in spherical simulations: the impact of an inner stable zone

Bonnie Zaire, Laurene Jouve

Magnetic fields vary in complexity for different stars. The stability of dipolar magnetic fields is known to depend on different quantities, e.g., the stellar rotation, the stratif…