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Tuesday, October 30 2018

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Uninterrupted observations of solar oscillations from Solar and Heliospheric Observatory and Solar Dynamics Observatory in 1996-2018 provide opportunity to investigate variations of the interior structure and dynamics of the Sun during the last two solar activity cycles, and gain insight into the mechanism of magnetic field generation. In particular, helioseismic measurements of the differential rotation and meridional circulation reveal the spatiotemporal dynamics of the solar convection zone, associated with the dynamo process.