Four-thirds law of energy and magnetic helicity in electron and Hall magnetohydrodynamic fluids
arXiv:2303.04290 · doi:10.1016/j.physd.2023.133835
Abstract
In this paper, by exploiting the feature of the Hall term, we establish some local version four-thirds laws for the dissipation rates of energy and magnetic helicity in both electron and Hall magnetohydrodynamic equations in the sense of Duchon-Robert type. New 4/3 laws for the dissipation rates of magnetic helicity in these systems are first observed and four-thirds law involving the dissipation rates of energy for the Hall magnetohydrodynamic equations generalizes the work of Galtier.
19 pages
References in corpus (6)
- Recent progress in astrophysical plasma turbulence from solar wind observations
- Simulations of Electron Magnetohydrodynamic Turbulence
- Magnetic Helicity Conservation and Inverse Energy Cascade in Electron Magnetohydrodynamic Wave Packets
- Exact scaling laws and the local structure of isotropic magnetohydrodynamic turbulence
- Energy transfer, discontinuities and heating in the inner solar wind measured with a weak and local formulation of the Politano-Pouquet law
- Onsager's Conjecture for Subgrid Scale -Models of Turbulence