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 paper, we aim at deriving simultaneous expressions for the excitation rate, damping rate, and modal surface effect associated with any given p-mode, as an explicit function of the statistical properties of the turbulent velocity field. We reduce the stochastic wave equation to complex amplitude equations for the normal oscillating modes of the system. We then derive the equivalent Fokker-Planck equation for the real amplitudes and phases of all the oscillating modes of the system simultaneously. The effect of the finite-memory time of the turbulent fluctuations (c...
Calculations were carried out in order to probe the influence of turbulence on the solar oscillation...
We investigate the rates at which energy is supplied to individual p-modes as a function of their fr...
We examine the influence of the Reynolds stress as the main contribution of turbulence on the oscill...
International audienceContext. The ever-increasing quality of asteroseismic measurements offers a un...
International audienceContext. The development of space-borne missions such as CoRoT and Kepler now ...
A review on acoustic mode damping and excitation in solar-type stars is presented. Current models fo...
Context. The development of space-borne missions such as CoRoT and Kepler now provides us with numer...
Acoustic power and oscillation amplitudes of radial oscillations computed for a solar model are c...
International audienceContext: Turbulent motions in stellar convection zones generate acoustic energ...
We present a formalism for investigating the interaction between p-mode oscillations and convection ...
We study the excitation of a damped harmonic oscillator by a random force as a model for the stochas...
Context. Detection of solar gravity modes remains a major challenge to our understanding of the in...
Context. Turbulent motions in stellar convection zones generate acoustic energy, part of which is th...
We investigate the frequency dependence of the power spectral density of low-degree solar p modes by...
Aims.We extend semi-analytical computations of excitation rates for solar oscillation modes to thos...
Calculations were carried out in order to probe the influence of turbulence on the solar oscillation...
We investigate the rates at which energy is supplied to individual p-modes as a function of their fr...
We examine the influence of the Reynolds stress as the main contribution of turbulence on the oscill...
International audienceContext. The ever-increasing quality of asteroseismic measurements offers a un...
International audienceContext. The development of space-borne missions such as CoRoT and Kepler now ...
A review on acoustic mode damping and excitation in solar-type stars is presented. Current models fo...
Context. The development of space-borne missions such as CoRoT and Kepler now provides us with numer...
Acoustic power and oscillation amplitudes of radial oscillations computed for a solar model are c...
International audienceContext: Turbulent motions in stellar convection zones generate acoustic energ...
We present a formalism for investigating the interaction between p-mode oscillations and convection ...
We study the excitation of a damped harmonic oscillator by a random force as a model for the stochas...
Context. Detection of solar gravity modes remains a major challenge to our understanding of the in...
Context. Turbulent motions in stellar convection zones generate acoustic energy, part of which is th...
We investigate the frequency dependence of the power spectral density of low-degree solar p modes by...
Aims.We extend semi-analytical computations of excitation rates for solar oscillation modes to thos...
Calculations were carried out in order to probe the influence of turbulence on the solar oscillation...
We investigate the rates at which energy is supplied to individual p-modes as a function of their fr...
We examine the influence of the Reynolds stress as the main contribution of turbulence on the oscill...