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Cited article:

Inversion for Inferring Solar Meridional Circulation: The Case with Constraints on Angular Momentum Transport inside the Sun

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

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Astronomy & Astrophysics 664 A189 (2022)
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Meridional flow in the Sun’s convection zone is a single cell in each hemisphere

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Properties of Solar Rossby Waves from Normal Mode Coupling and Characterizing Its Systematics

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A coarse-to-fine strategy for the registration of the multi-wavelength high-resolution solar images

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Frequency Dependence of Helioseismic Measurements of the Center-to-Limb Effect and Flow-induced Travel-time Shifts

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On-Orbit Performance of the Helioseismic and Magnetic Imager Instrument onboard the Solar Dynamics Observatory

J. T. Hoeksema, C. S. Baldner, R. I. Bush, J. Schou and P. H. Scherrer
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Large-scale photospheric motions determined from granule tracking and helioseismology from SDO/HMI data

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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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Solar-cycle Variations of Meridional Flows in the Solar Convection Zone Using Helioseismic Methods

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Inversions for Deep Solar Meridional Flow Using Spherical Born Kernels

Vincent G. A. Böning, Markus Roth, Jason Jackiewicz and Shukur Kholikov
The Astrophysical Journal 845 (1) 2 (2017)
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