Turbulence in the Sun is suppressed on large scales and confined to equatorial regions

Consequences of high effective Prandtl number on solar differential rotation and convective velocity

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Global-scale equatorial Rossby waves as an essential component of solar internal dynamics

(2018) Björn Löptien et al.   Nature Astronomy

Asteroseismic detection of latitudinal differential rotation in 13 Sun-like stars

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Sensitivity of helioseismic measurements of normal-mode coupling to flows and sound-speed perturbations

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Seismic Sounding of Convection in the Sun

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Large-scale magnetic fields at high Reynolds numbers in magnetohydrodynamic simulations

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Improved Helioseismic Analysis of Medium- ℓ $\ell$ Data from the Michelson Doppler Imager

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Toroidal and poloidal energy in rotating Rayleigh–Bénard convection

(2014) Susanne Horn et al.   JOURNAL OF FLUID MECHANICS

Detectability of Large-Scale Solar Subsurface Flows

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ON THE AMPLITUDE OF CONVECTIVE VELOCITIES IN THE DEEP SOLAR INTERIOR

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Anomalously weak solar convection

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A UNIFIED APPROACH TO THE HELIOSEISMIC INVERSION PROBLEM OF THE SOLAR MERIDIONAL FLOW FROM GLOBAL OSCILLATIONS

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Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO)

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MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA)

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Penumbral Structure and Outflows in Simulated Sunspots

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Solar Rotation Rate and Its Gradients During Cycle 23

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