Self-consistent stationary MHD shear flows in the solar atmosphere as electric field generators
D.H. Nickeler, M. Karlicky, T. Wiegelmann, M. Kraus

TL;DR
This paper models the electric fields generated by shear flows in the solar atmosphere's magnetic structures, revealing filamented fields and energy gains consistent with observations, using exact solutions of MHD equations.
Contribution
It provides a self-consistent analytical framework for calculating electric fields in shear flows within the solar corona, incorporating nonideal MHD effects and resistivity.
Findings
Electric fields are highly filamented and spatially structured.
Parallel electric field component dominates and correlates with resistivity maxima.
Electron energies reach tens of keV, matching observational data.
Abstract
Magnetic fields and flows in coronal structures, for example, in gradual phases in flares, can be described by 2D and 3D magnetohydrostatic (MHS) and steady magnetohydrodynamic (MHD) equilibria. Within a physically simplified, but exact mathematical model, we study the electric currents and corresponding electric fields generated by shear flows. Starting from exact and analytically calculated magnetic potential fields, we solveid the nonlinear MHD equations self-consistently. By applying a magnetic shear flow and assuming a nonideal MHD environment, we calculated an electric field via Faraday's law. The formal solution for the electromagnetic field allowed us to compute an expression of an effective resistivity similar to the collisionless Speiser resistivity. We find that the electric field can be highly spatially structured, or in other words, filamented. The electric field component…
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