Cross-scale energy transport in space plasmas

The solar wind is a supersonic magnetized plasma streaming far into the heliosphere. Although cooling as it flows, it is rapidly heated upon encountering planetary obstacles. At Earth, this interaction forms the magnetosphere and its sub-regions. The present paper focuses on particle heating across...

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Veröffentlicht in:	Nature physics 2016-12, Vol.12 (12), p.1164-1169
Hauptverfasser:	Moore, T. W., Nykyri, K., Dimmock, A. P.
Format:	Artikel
Sprache:	eng
Schlagworte:	639/766/1960/1134 639/766/525/869 Atomic Classical and Continuum Physics Complex Systems Condensed Matter Physics Cooling Energy transfer Fluids Heating Magnetospheres Mathematical and Computational Physics Molecular Obstacles Optical and Plasma Physics Physics Plasma physics Shear Solar physics Solar wind Sun Theoretical
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