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.
منابع مشابه
Spatial structure of ion-scale plasma turbulence
1 Space Research Institute, Austrian Academy of Sciences, Graz, Austria 2 Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany 3 Institut für Theoretische Physik, Technische Universität Braunschweig, Braunschweig, Germany 4 Institute for Space Sciences, Bucharest-Măgurele, Romania 5 Institut für Planetenforschung, Deutsches Zentrum für...
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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