Stream-Aligned Magnetohydrodynamics for Solar Wind Simulations
Igor V Sokolov, Lulu Zhao, Tamas I Gombosi

TL;DR
This paper introduces a stream-aligned MHD model for solar wind simulations, simplifying the equations by aligning magnetic and velocity fields, which allows efficient generation of realistic steady-state solar atmosphere solutions.
Contribution
The paper proposes a novel stream-aligned MHD model that simplifies the full MHD equations while accurately capturing steady-state solutions relevant for solar wind modeling.
Findings
Efficient generation of Parker spiral solutions.
The model fully accounts for magnetic forces in plasma dynamics.
Steady-state solutions of the model are valid solutions of full MHD.
Abstract
We present a reduced magnetohydrodynamic (MHD) mathematical model describing the dynamical behavior of highly conducting plasmas with frozen-in magnetic fields, constrained by the assumption that, there exists a frame of reference, where the magnetic field vector, , is aligned with the plasma velocity vector, , at each point. We call this solution "stream-aligned MHD" (SA-MHD). Within the framework of this model, the electric field, , in the induction equation vanishes identically and so does the electromagnetic energy flux (Poynting flux), , in the energy equation. At the same time, the force effect from the magnetic field on the plasma motion (the Ampere force) is fully taken into account in the momentum equation. Any steady-state solution of the proposed model is a…
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