ELEvoHI_v2.0.0.0

ELEvoHI relies on heliospheric imagers (HI) observations to obtain the kinematics of a CME. With the newly developed deformable front, the model is able to react to the ambient solar wind conditions during the entire propagation and along the whole front of the CME. To get an estimate of the ambient solar wind conditions, we make us of ambient solar wind models.

ELEvoHI_v1.0.0.0

This is the first release of ELEvoHI.