Ionospheric Plasma Transported Into the Martian Magnetosheath
Abstract Heavy cold ions at Mars are gravitationally bound to the planet unless some process provides energy to them. Observations show that cold (<20 eV) and dense (∼>1 cm−3) O+/O2+ ions with bulk velocities equal to energies ∼1 keV can reach deep into the nightside Martian magnetosheath. The...
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| Main Authors: | Sergey Shuvalov, Laila Andersson, Jasper S. Halekas, Christopher M. Fowler, Kathleen Gwen Hanley, Gina DiBraccio |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Wiley
2024-03-01
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| Series: | Geophysical Research Letters |
| Subjects: | |
| Online Access: | https://doi.org/10.1029/2023GL107953 |
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