Speaker
Jens Pomoell
(University of Helsinki)
Description
In this presentation, novel time-dependent modelling assets recently developed at the University of Helsinki are presented. We focus especially on highlighting two recent developments: 1) physics-based modelling of the large-scale dynamics caused by space-weather relevant magnetized Coronal Mass Ejections (CMEs) starting at 5 solar radii and extending out to the heliosphere and 2) self-consistent data-driven modelling of the formation and eruption of active region magnetic fields. Combining these methods provides a unique capability to efficiently perform data-driven dynamic modelling of CMEs from the low corona to the heliosphere, with a potential to significantly improve upon current space weather modelling paradigms.
| Numerical model | GLOW and EUHFORIA+ |
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Author
Jens Pomoell
(University of Helsinki)