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.
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COCONUT simulations find open magnetic flux falls by up to 45% within 3 solar radii, matches in-situ observations, and varies by a factor of 1.4 during solar maximum.
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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.
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MHD modeling of magnetic flux evolution around solar maximum by the coronal model COCONUT
COCONUT simulations find open magnetic flux falls by up to 45% within 3 solar radii, matches in-situ observations, and varies by a factor of 1.4 during solar maximum.