Numerical model of the coronal mass ejection taking into account the magnetic field of the stellar wind
Abstract
A numerical model of stellar wind flow around a hot jupiter at the moment of passage of a coronal mass ejection from a star is considered in the paper. As an important factor the influence of the stellar wind magnetic field is taken into account in the model.
- Publication:
-
INASAN Science Reports
- Pub Date:
- October 2019
- DOI:
- 10.26087/INASAN.2019.3.1.017
- Bibcode:
- 2019INASR...3..112Z