activity
20042018
most citedSeismic diagnostics for transport of angular momentum in stars 1. Rotational splittings from the PMS to the RGB

310 citations · 615 across the 10 of their papers we have counts for

collaborators

10 papers

physics.acc-ph2018★ 16 cited

Design of a 5 GeV Laser Plasma Accelerating Module in the Quasi-linear Regime

Xiangkun Li, Alban Mosnier, Phu Anh Phi Nghiem

Multi-GeV-class laser plasma accelerating modules are key components of laser plasma accelerators, because they can be used as a booster of an upstream plasma or conventional injec…

astro-ph.SR2012★ 310 cited

Seismic diagnostics for transport of angular momentum in stars 1. Rotational splittings from the PMS to the RGB

J. P. Marques, M. J. Goupil, Y. Lebreton +12

Rotational splittings are currently measured for several main sequence stars and a large number of red giants with the space mission Kepler. This will provide stringent constraints…

astro-ph.SR2010★ 104 cited

Seismic and dynamical solar models i-the impact of the solar rotation history on neutrinos and seismic indicators

Sylvaine Turck-Chieze, Ana Palacios, Joao Marques +1

Solar activity and helioseismology show the limitation of the standard solar model and call for the inclusion of dynamical processes in both convective and radiative zones. We conc…

astro-ph2008★ 19 cited

Impact of a radius and composition variation on the solar subsurface layers stratification

Sandrine Lefebvre, Phu Anh Phi Nghiem, Sylvaine Turck-Chieze

Several works have reported changes of the Sun's subsurface stratification inferred from f-mode or p-mode observations. Recently a non-homologous variation of the subsurface layers…

astro-ph2007★ 3 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-ph2006★ 1 cited

Solar Mean Magnetic Field Near the Surface and its Variation During a Cycle

P. A. P. Nghiem, R. A. Garcia, S. J. Jimenez-Reyes

The unsigned mean magnetic field characterizes the magnetic energy settled in the region near the solar surface. It is one of the determinant ingredients that govern the turbulence…