Ion-scale Transition of Plasma Turbulence: Pressure–Strain Effect

نویسندگان

چکیده

We investigate properties of solar wind-like plasma turbulence using direct numerical simulations. analyze the transition from large, magnetohydrodynamic (MHD) scales to ion characteristic ones two-dimensional hybrid (fluid electrons, kinetic ions) To capture and quantify properties, we apply Karman-Howarth-Monin (KHM) equation for compressible Hall MHD (extended by considering pressure as a tensor quantity) results. The KHM analysis indicates that (the so called break in power spectrum) results combination an onset physics effective dissipation owing pressure-strain energy-exchange channel resistivity. discuss simulation context wind.

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2022

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/ac5fad