2024
DOI: 10.1017/s0022377824001296
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Self-organization in collisionless, high-β turbulence

S. Majeski,
M.W. Kunz,
J. Squire

Abstract: The magnetohydrodynamic (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 clusters, are only weakly collisional at best, meaning that significant deviations from LTE are not only possible but common. Recent studies have demonstrated that the kinetic physics inherent to this… Show more

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