Observations and models of the Earth's magnetosphere

Responsible person: Johan De Keyser 

Overall description
Science-based prediction of the effects of the solar wind on the Earth's magnetosphere requires both visualization of observations and numerical simulation of magnetospheric dynamics based on a physical model. 

Long Term Goal

  • Maintain and expand data processing and model visualization tools (MIM software)
  • Develop an operational simulation tool, based on a kinetic approach (go beyond the existing huge but not-so-physical MHD simulations used elsewhere).

Short Term Goal

  • Maintain MIM software and distribution
  • Simulation proof of principle. Build and demonstrate a (non-operational) simulation for the acceleration region above aurora.

Travel Info





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