Speaker
Prof.
Joerg Buechner
(Max-Planck-Institute for Solar System Reserach)
Description
We compare observed CME eruptions with the results of GOEMHD3 numerical simulations of the Solar atmosphere based on data obtained by observations of the Sun and taking into account cross-scale coupling effects of turbulence. We compare our findings with those of current laboratory eruption experiments carried out at the Princeton Plasma Physics Laboratory (MRX).
Primary author
Prof.
Joerg Buechner
(Max-Planck-Institute for Solar System Reserach)
