most citedSimulations of turbulent convection in rotating young solar-like stars: Differential rotation and meridional circulation

66 citations · 157 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2008

First performances of the GOLF-NG instrumental prototype observing the Sun in Tenerife

D. Salabert, S. Turck-Chieze, J. C. Barriere +14

The primary challenge of GOLF-NG (Global Oscillations at Low Frequency New Generation) is the detection of the low-frequency solar gravity and acoustic modes, as well as the possib…

astro-ph2008

What can we learn on the structure and the dynamics of the solar core with g modes?

S. Mathur, J. Ballot, A Eff-Darwich +4

The detection of the signature of dipole gravity modes has opened the path to study the solar inner radiative zone. Indeed, g modes should be the best probes to infer the propertie…

astro-ph200844 cited

Variations of the solar granulation motions with height using the GOLF/SoHO experiment

S. Lefebvre, R. A. Garcia, S. J. Jimenez-Reyes +2

Below 1 mHz, the power spectrum of helioseismic velocity measurements is dominated by the spectrum of convective motions (granulation and supergranulation) making it difficult to d…

astro-ph200844 cited

Update on g-mode research

R. A. Garcia, A. Jimenez, S. Mathur +6

Since the beginning of this century we have attended a blooming of the gravity-mode research thanks to the unprecedented quality of the data available, either from space with SoHO,…

astro-ph20073 cited

Oscillations in Procyon A: First results from a multi-site campaign

S. Hekker, T. Arentoft, H. Kjeldsen +45

Procyon A is a bright F5IV star in a binary system. Although the distance, mass and angular diameter of this star are all known with high precision, the exact evolutionary state is…

astro-ph200766 cited

Simulations of turbulent convection in rotating young solar-like stars: Differential rotation and meridional circulation

Jérôme Ballot, Allan Sacha Brun, Sylvaine Turck-Chièze

We present the results of three-dimensional simulations of the deep convective envelope of a young (10 Myr) one-solar-mass star, obtained with the Anelastic Spherical Harmonic code…