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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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Bibliografske podrobnosti
izdano v:Nat Commun
Main Authors: Lugaz, Noé, Farrugia, Charles J., Huang, Chia-Lin, Winslow, Reka M., Spence, Harlan E., Schwadron, Nathan A.
Format: Artigo
Jezik:Inglês
Izdano: Nature Publishing Group 2016
Teme:
Online dostop: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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