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Cited article:

Structure and Dynamics of the Sun’s Interior Revealed by the Helioseismic and Magnetic Imager

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Global Turbulent Solar Convection: A Numerical Path Investigating Key Force Balances in the Context of the Convective Conundrum

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Assessing the validity of the anelastic and Boussinesq approximations to model solar inertial modes

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Astronomy & Astrophysics 696 A160 (2025)
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Radial Flow Component of Sun’s High-frequency Retrograde Inertial Waves

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Existence of small-scale Rossby waves points to low convective velocity amplitudes in the Sun

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Physics of Fluids 36 (8) (2024)
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Inertial Waves in a Nonlinear Simulation of the Sun's Convection Zone and Radiative Interior

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The Astrophysical Journal 966 (1) 29 (2024)
https://doi.org/10.3847/1538-4357/ad27d1