Self-organization in collisionless, high-$\beta$ turbulence

The MHD equations, as a collisional fluid model that remains in local thermodynamic equilibrium (LTE), have long been used to describe turbulence in myriad space and astrophysical plasmas. Yet, the vast majority of these plasmas, from the solar wind to the intracluster medium (ICM) of galaxy cluster...

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Bibliographische Detailangaben

Hauptverfasser:	Majeski, S, Kunz, M. W, Squire, J
Format:	Artikel
Sprache:	eng
Schlagworte:	Physics - High Energy Astrophysical Phenomena Physics - Plasma Physics Physics - Space Physics
Online-Zugang:	Volltext bestellen
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