2 papers
astro-ph.SR2025
Is convective turbulence the only exciting mechanism of global p modes in the Sun?
E. Panetier, R. A. GarcÃa, S. N. Breton +2
In solar-like oscillators, acoustic waves are excited by turbulent motion in the convective envelope and propagate inward, generating a variety of standing pressure modes. When com…
astro-ph.SR2024
Solar p-modes excitation rate along the magnetic activity cycle
E. Panetier, S. N. Breton, R. A. GarcÃa +2
Magnetic cycles of solar-like stars influence their internal physics. Thus, the frequency, amplitude, excitation rate, and damping of the acoustic oscillation modes (p-modes) vary…