A Bayesian fit to Ulysses, Galileo, Cassini and Juno crossing data yields new Jupiter magnetopause and bow shock models that are smaller, polar-flattened, and dawn-dusk asymmetric relative to previous empirical models.
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New Models of Jupiter's Magnetopause and Bow Shock through the Juno Prime Mission: Probabilistic Location, Shape, and Internally-driven Variation
A Bayesian fit to Ulysses, Galileo, Cassini and Juno crossing data yields new Jupiter magnetopause and bow shock models that are smaller, polar-flattened, and dawn-dusk asymmetric relative to previous empirical models.