Analysis of solar eruptions deflecting in the low corona: influence of
the magnetic environment
Analysis of solar eruptions deflecting in the low corona: influence of
the magnetic environment
Coronal mass ejections (CMEs) can exhibit non-radial evolution. The background magnetic field is considered the main driver for the trajectory deviation relative to the source region. The influence of the magnetic environment has been largely attributed to the gradient of the magnetic pressure. In this work, we propose a new …