1D Parker winds work only for weak tides; a simulation-calibrated Mixture Model of spherical plus L1/L2 nozzle escape predicts 3D mass-loss rates better across Roche-filling and thermal regimes.
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Atmospheric Escape Rates of Planets in Stellar Tidal Fields from 3-D Hydrodynamic Simulations
1D Parker winds work only for weak tides; a simulation-calibrated Mixture Model of spherical plus L1/L2 nozzle escape predicts 3D mass-loss rates better across Roche-filling and thermal regimes.