A single time-evolving implicit MHD model from Sun to Earth produces noticeable differences in plasma parameters versus steady-state simulations and supports L5-based solar wind forecasting.
M., Landi, E., Manchester, W
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COCONUT: Toward practical time-evolving Sun-to-Earth magnetohydrodynamic modeling
A single time-evolving implicit MHD model from Sun to Earth produces noticeable differences in plasma parameters versus steady-state simulations and supports L5-based solar wind forecasting.