Ion Escape Processes of Mars with a Weak Intrinsic Magnetic Field
Abstract
The ion tailward flux increases by the magnetization of Mars. Ions escape through four channels in the magnetotail, which are related to the cusp region and the reconnection. This could result in the escape rate from the upper atmosphere enhanced.
- Publication:
-
Fourth International Conference on Early Mars: Geologic, Hydrologic, and Climatic Evolution and the Implications for Life
- Pub Date:
- October 2017
- Bibcode:
- 2017LPICo2014.3034S