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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...
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| Publicado no: | Nat Commun |
|---|---|
| Main Authors: | , , , , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Nature Publishing Group
2016
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| Assuntos: | |
| Acesso em linha: | 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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