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Abstract: New Models of Jupiter's Magnetopause and Bow Shock: Probabilistic Locations, Shapes, and Internally‐Driven Variation (AGU25)

New Models of Jupiter's Magnetopause and Bow Shock: Probabilistic Locations, Shapes, and Internally‐Driven Variation

Matthew James Rutala1, Caitriona Mary Jackman1, Corentin Louis2, Abigail Azari3, Fran Bagenal4, Steven P Joy5, William S Kurth6, Timothy Benjamin Keebler7, Rohini Giles8, Robert W Ebert8,9, Charles Bowers7 and Marissa F. Vogt10, (1)Dublin Institute for Advanced Studies, School of Cosmic Physics, Dublin, Ireland, (2)LIRA, Observatoire de Paris, Paris, France, (3)University of Alberta, Alberta Machine Intelligence Institute, Edmonton, Canada, (4)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States, (5)University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, CA, United States, (6)University of Iowa, Iowa City, United States, (7)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (8)Southwest Research Institute, San Antonio, United States, (9)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, United States, (10)Planetary Science Institute Tucson, Tucson, United States