EGU21-8153
https://doi.org/10.5194/egusphere-egu21-8153
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Global 6-dimensional hybrid-Vlasov modelling of the magnetosphere: First Vlasiator results

Minna Palmroth1,2, Urs Ganse1, Markus Battarbee1, Lucile Turc1, Yann Pfau-Kempf1, Maarja Bussov1, Maxime Grandin1, Andreas Johlander1, Jonas Suni1, Maxime Dubart1, Kostis Papadakis1, and Markku Alho1
Minna Palmroth et al.
  • 1University of Helsinki, Helsinki, Finland (minna.palmroth@helsinki.fi)
  • 2Finnish Meteorological Institute, Helsinki, Finland

Numerical simulations are key in modern space physics, as they can be used as 1) context to data, 2) predict future behaviour of the system, 3) understand the system using unforeseen boundary conditions, and increasingly also in 4) discovering new phenomena that are hard to be observed using point-wise satellite measurements. Especially, the discovery of new phenomena pertains to global systems, where phenomena of interest may be initiated far away from the point of observations. The most typical method of simulating the global solar wind - magnetosphere - ionosphere system is based on magnetohydrodynamics (MHD), which is however not representing the actual plasma behaviour in locations where kinetic physics becomes important. Such regions are e.g., the foreshock - magnetosheath interaction, reconnection, and the inner magnetosphere.

Vlasiator is the world’s first and so far the only global simulation based on the hybrid-Vlasov approach that simulates the ion distributions accurately without noise. The simulation has, for computational reasons, been so far executed in 2D real space. Even so, the global 5D Vlasiator results have shown without a doubt that ion-kinetic effects cannot be neglected from the large scales, as small-scale phenomena affect large scales and vice versa. This scale coupling leads to phenomena that are not predicted using local simulations without proper boundary conditions, or with spacecraft measurements lacking the global context.

Here, we present the world’s first global 6-dimensional ion-kinetic global magnetospheric simulation run, accurate both locally and globally. The simulation box extends from the dayside to the nightside, and includes global dynamics and both dayside and nightside reconnection regions. We will investigate unambiguously for the first time the dayside magnetopause reconnection as driven by the kinetic variations in the magnetosheath, and tail reconnection as driven by magnetic flux from the dayside.

How to cite: Palmroth, M., Ganse, U., Battarbee, M., Turc, L., Pfau-Kempf, Y., Bussov, M., Grandin, M., Johlander, A., Suni, J., Dubart, M., Papadakis, K., and Alho, M.: Global 6-dimensional hybrid-Vlasov modelling of the magnetosphere: First Vlasiator results, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-8153, https://doi.org/10.5194/egusphere-egu21-8153, 2021.

Corresponding displays formerly uploaded have been withdrawn.