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Abstract: An AI-powered Surface Flux Transport model to measure high-resolution velocity fields and forecast magnetic flux emergence (AGU25)

An AI-powered Surface Flux Transport model to measure high-resolution velocity fields and forecast magnetic flux emergence

Dr. Shea A. Hess Webber, PhD1, Nina Bonaventura2, Nishu Karna3, Spiridon Kasapis4, Plinio Guzmán5, Andrés Muñoz-Jaramillo6, Katherine Keegan7, Bibhuti Kumar Jha6 and Anthony Yeates8, (1)Stanford University, HEPL, Stanford, CA, United States, (2)University of Arizona, Steward Observatory, Tucson, United States, (3)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (4)Princeton University, Department of Astrophysical Sciences, Princeton, United States, (5)Fused Labs, Inc., Brooklyn, United States, (6)Southwest Research Institute Boulder, Boulder, United States, (7)Emory University, Department of Mathematics, Atlanta, United States, (8)University of Durham, Durham, United Kingdom
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