טוען...
Earth's magnetosphere and outer radiation belt under sub-Alfvénic solar wind
The interaction between Earth's magnetic field and the solar wind results in the formation of a collisionless bow shock 60,000–100,000 km upstream of our planet, as long as the solar wind fast magnetosonic Mach (hereafter Mach) number exceeds unity. Here, we present one of those extremely rare...
שמור ב:
| הוצא לאור ב: | Nat Commun |
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| Main Authors: | , , , , , |
| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
Nature Publishing Group
2016
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| נושאים: | |
| גישה מקוונת: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5063966/ https://ncbi.nlm.nih.gov/pubmed/27694887 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/ncomms13001 |
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