MHD modeling of a geoeffective interplanetary CME with the magnetic
topology informed by in-situ observations
MHD modeling of a geoeffective interplanetary CME with the magnetic
topology informed by in-situ observations
Variations of the magnetic field within solar coronal mass ejections (CMEs) in the heliosphere depend on the CME`s magnetic structure as it leaves the solar corona and its subsequent evolution through interplanetary space. To account for this evolution, we developed a new numerical model of the inner heliosphere that simulates …