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Cited article:

Magnetic Flux in the Sun Emerges Unaffected by Supergranular-scale Surface Flows

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Inflows Towards Bipolar Magnetic Active Regions and Their Nonlinear Impact on a Three-Dimensional Babcock–Leighton Solar Dynamo Model

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Solar convective velocities: Updated helioseismic constraints

A. C. Birch, B. Proxauf, T. L. Duvall, L. Gizon, S. Hanasoge, B. W. Hindman and K. R. Sreenivasan
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Inferring the Solar Meridional Circulation Flow Profile by Applying Bayesian Methods to Time–Distance Helioseismology

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Three-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun

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Study of Global Photospheric and Chromospheric Flows Using Local Correlation Tracking and Machine Learning Methods I: Methodology and Uncertainty Estimates

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Contribution of flows around active regions to the north-south helioseismic travel-time measurements

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Evolution of solar surface inflows around emerging active regions

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Exploring the latitude and depth dependence of solar Rossby waves using ring-diagram analysis

B. Proxauf, L. Gizon, B. Löptien, et al.
Astronomy & Astrophysics 634 A44 (2020)
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Solar meridional circulation from twenty-one years of SOHO/MDI and SDO/HMI observations

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Astronomy & Astrophysics 619 A99 (2018)
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Large-scale photospheric motions determined from granule tracking and helioseismology from SDO/HMI data

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

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