13 citations · 43 across the 9 of their papers we have counts for
9 papers
A new particle-based code for Lagrangian stochastic models applied to stellar turbulent convection
J. Philidet, K. Belkacem
The inclusion of convection in stellar evolution models lacks realism, especially near convective-radiative interfaces. Furthermore, the interaction of convection with oscillations…
Glitches in solar-like oscillating F-type stars: Possible contribution of non-linear terms
M. Deal, M. -J. Goupil, J. Philidet +3
The glitch signatures in for F-type stars (higher amplitude and period of the oscillatory component) are very different from those of G-type stars. The aim of this work i…
Measuring stellar surface rotation and activity with the PLATO mission -- I. Strategy and application to simulated light curves
S. N. Breton, A. F Lanza, S. Messina +20
The Planetary Transits and Oscillations of stars mission (PLATO) will allow us to measure surface rotation and monitor photometric activity of tens of thousands of main sequence so…
Interaction of solar inertial modes with turbulent convection. A 2D model for the excitation of linearly stable modes
J. Philidet, L. Gizon
Inertial modes have been observed on the Sun at low longitudinal wavenumbers. These modes probe the dynamics and structure of the solar convection zone down to the tachocline. Whil…
Coupling between turbulence and solar-like oscillations: A combined Lagrangian PDF/SPH approach. II - Mode driving, damping and modal surface effect
J. Philidet, K. Belkacem, M. -J. Goupil
The first paper of this series established a linear stochastic wave equation for solar-like p-modes, correctly taking the effect of turbulence thereon into account. In this second…
Coupling between turbulence and solar-like oscillations: a combined Lagrangian PDF/SPH approach. I -- The stochastic wave equation
J. Philidet, K. Belkacem, M. -J. Goupil
Aims. This series of papers aims at building a new formalism specifically tailored to study the impact of turbulence on the global modes of oscillation in solar-like stars. This fi…
Surface effects and turbulent pressure. Assessing the Gas- and Reduced- empirical models
K. Belkacem, F. Kupka, J. Philidet +1
The use of the full potential of stellar seismology is made difficult by the improper modeling of the upper-most layers of solar-like stars and their influence on the modeled frequ…
Velocity-intensity asymmetry reversal of solar radial p-modes
J. Philidet, K. Belkacem, H. -G. Ludwig +2
The development of space-borne missions has significantly improved the quality of the measured spectra of solar-like oscillators. Their -mode line profiles can now be resolved,…
Modelling the asymmetries of the Sun's radial -mode line profiles
J. Philidet, K. Belkacem, R. Samadi +2
In this paper, we aim to develop a predictive model for solar radial -mode line profiles in the velocity spectrum. Unlike the approach favoured by prior studies, this model is n…