Magnetosheath plasma flow model around Mercury
<p>The magnetosheath is defined as the plasma region between the bow shock, where the super-magnetosonic solar wind plasma is decelerated and heated, and the outer boundary of the intrinsic planetary magnetic field, the so-called magnetopause. Based on the Soucek–Escoubet magnetosheath flow mo...
| Main Authors: | , , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Copernicus Publications
2021-06-01
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| Series: | Annales Geophysicae |
| Online Access: | https://angeo.copernicus.org/articles/39/563/2021/angeo-39-563-2021.pdf |