Turbulent mass transfer caused by vortex induced reconnection in collisionless magnetospheric plasmas

Magnetic reconnection is believed to be the main driver to transport solar wind into the Earth’s magnetosphere when the magnetopause features a large magnetic shear. However, even when the magnetic shear is too small for spontaneous reconnection, the Kelvin–Helmholtz instability driven by a super-Al...

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Detalles Bibliográficos
Autores principales: Nakamura, T. K. M., Hasegawa, H., Daughton, W., Eriksson, S., Li, W. Y., Nakamura, R.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2017
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5693928/
https://www.ncbi.nlm.nih.gov/pubmed/29150662
http://dx.doi.org/10.1038/s41467-017-01579-0

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5693928/
https://www.ncbi.nlm.nih.gov/pubmed/29150662
http://dx.doi.org/10.1038/s41467-017-01579-0

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