Solar-cycle variations in meridional flows and rotational shear within the Sun's near-surface shear layer
Anisha Sen, S.P. Rajaguru, Abhinav Govindan Iyer, Ruizhu Chen, Junwei Zhao, Shukur Kholikov

TL;DR
This study investigates how solar-cycle variations influence meridional flows and rotational shear in the Sun's near-surface layer, revealing the role of the Coriolis force and flow patterns related to active regions.
Contribution
It provides new insights into the spatio-temporal variations of flows in the NSSL and their connection to solar activity, highlighting the influence of the Coriolis force on these dynamics.
Findings
Coriolis force affects large-scale flow variations during the solar cycle.
Near-surface inflows towards active regions form a local circulation pattern.
Changes in rotation gradient are linked to flow variations and solar activity.
Abstract
Using solar-cycle long helioseismic measurements of meridional and zonal flows in the near-surface shear layer (NSSL) of the Sun, we study their spatio-temporal variations and connections to active regions. We find that near-surface inflows towards active latitudes are part of a local circulation with an outflow away from them at depths around 0.97 R, which is also the location where the deviations in the radial gradient of rotation change sign. These results, together with opposite-signed changes over latitude and depth in the above quantities observed during the solar minimum period, point to the action of the Coriolis force on large-scale flows as the primary cause of changes in the rotation gradient within the NSSL. We also find that such Coriolis force-mediated changes in near-surface flows towards active latitudes only marginally change the amplitude of zonal flow and hence are…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Oceanographic and Atmospheric Processes
