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20242026
most citedSeismic differences between solar magnetic cycles 23 and 24 for low-degree modes

9 citations · 11 across the 9 of their papers we have counts for

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astro-ph.SR2025

Is convective turbulence the only exciting mechanism of global p modes in the Sun?

E. Panetier, R. A. García, 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…