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The multi-scale nature of the solar wind

The solar wind is a magnetized plasma and as such exhibits collective plasma behavior associated with its characteristic spatial and temporal scales. The characteristic length scales include the size of the heliosphere, the collisional mean free paths of all species, their inertial lengths, their gy...

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Detalles Bibliográficos
Autores principales: Verscharen, Daniel, Klein, Kristopher G., Maruca, Bennett A.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer International Publishing 2019
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6934245/
https://www.ncbi.nlm.nih.gov/pubmed/31929769
http://dx.doi.org/10.1007/s41116-019-0021-0