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One of the Sun-to-Earth modelling chains implemented in the VSWMC that became operational in 2019 (see Poedts et al., 2020). In this chain EUHFORIA is coupled to models to determine the Kp and Dst indices and the plasma sphere stand-off distance, based on the synthetic wind data at L1 from EUHFORIA. The Kp index and the plasma sphere stand-off distance (Dso) are then used to drive the British Antarctic Survey Radiation Belt Model.
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