Revisiting the hypothesis of purely stochastic excitation of global p modes in the Sun
Context. 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 (p modes). When combining the power of several solar acoustic modes, some studies have reported an excess that is not compatible with pure stochastic excitation. This
Panetier, E. et al.
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2025