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Active-region Modulation of Subsurface Meridional Flows and Magnetic Flux Transport on the Sun

  • Authors: Anisha Sen, S.P. Rajaguru, Ruizhu Chen, Junwei Zhao, Shukur Kholikov

Anisha Sen et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 1.

Time–latitude profile of variations in the residual meridional flow at two depths, 0.99R and 0.95R, respectively, are in panels (A) and (B). Positive values correspond to poleward flow in both hemispheres. Corresponding time–latitude variations in the longitudinally averaged signed (i.e., the magnetic butterfly diagram) and unsigned magnetic field are in the lower panels (C) and (D), respectively. The solid line overplotted in panel (D) marks the mean latitude, θm, of peak magnetic flux in each hemisphere, and the dotted–dashed lines in panels (A), (B), and (D) enclose the region 10°– 25° away from θm. The two vertical dotted lines mark epochs of solar cycle 24 maximum (2014) and minimum (2020). Sunspot locations are overplotted as black dots.

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