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Cited article:

Supergranular-scale solar convection not explained by mixing-length theory

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The Sun’s Magnetic Power Spectra over Two Solar Cycles. I. Calibration between SDO/HMI and SOHO/MDI Magnetograms

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The Impact of Stellar Surface Magnetoconvection and Oscillations on the Detection of Temperate, Earth-Mass Planets Around Sun-Like Stars

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HELIOSEISMIC IMAGING OF SUPERGRANULATION THROUGHOUT THE SUN’S NEAR-SURFACE SHEAR LAYER

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THE ROLE OF SUBSURFACE FLOWS IN SOLAR SURFACE CONVECTION: MODELING THE SPECTRUM OF SUPERGRANULAR AND LARGER SCALE FLOWS

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Specifics of the solar photospheric convection at granulation, mesogranulation, and supergranulation scales

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Analysis of Supergranule Sizes and Velocities Using Solar Dynamics Observatory (SDO)/Helioseismic Magnetic Imager (HMI) and Solar and Heliospheric Observatory (SOHO)/Michelson Doppler Imager (MDI) Dopplergrams

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Solar Cycle Phase Dependence of Supergranular Fractal Dimension

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Observations of Photospheric Dynamics and Magnetic Fields: From Large-Scale to Small-Scale Flows

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Structure and Evolution of Supergranulation from Local Helioseismology

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Helioseismology, Asteroseismology, and MHD Connections

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