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tokens: This work was supported by NYUAD Institute Grant G1502 “NYUAD Center for Space Science”. RA acknowledges support from the NYUAD Kawadar Research Program. The HMI data is courtesy of NASA/SDO and the HMI Science Team. Computational resources were provided by the German Data Center for SDO funded by the German Aerospace Center. SMH and LG thank the Max Planck partner group program for supporting this work. Author contributions: CSH and LG designed the research goals. RA proposed the machine-learning methodology for predicting flows and performed experimental and computational analysis. CSH prepared data and performed helioseismic analysis. All authors contributed to the final manuscript. We thank Aaron Birch and Bastian Proxauf for helpful insight into the ring-diagram pipeline.