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A Magnetohydrodynamic Relaxation Method for Non-Force-Free Magnetic Field in Magnetohydrostatic Equilibrium View all abstracts by submitter

Takahiro Miyoshi   Submitted: 2019-12-23 20:25

A nonlinear force-free field (NLFFF) extrapolation is widely used to reconstruct the three-dimensional magnetic field in the solar corona from the observed photospheric magnetic field. However, the pressure gradient and gravitational forces are ignored in the NLFFF model, even though the photospheric and chromospheric magnetic fields are not in general force-free. Here we develop a magnetohydrodynamic (MHD) relaxation method that reconstructs the solar atmospheric (chromospheric and coronal) magnetic field as a non-force-free magnetic field (NFFF) in magnetohydrostatic equilibrium where the Lorentz, pressure gradient, and gravitational forces are balanced. The system of basic equations for the MHD relaxation method is derived, and mathematical properties of the system are investigated. A robust numerical solver for the system is constructed based on the modern high-order shock capturing scheme. Two-dimensional numerical experiments that include the pressure gradient and gravitational forces are also demonstrated.

Authors: Takahiro Miyoshi, Kanya Kusano, Satoshi Inoue
Projects: None

Publication Status: Accepted for publication in ApJS
Last Modified: 2019-12-24 10:23
Go to main E-Print page  Quantifying the Toroidal Flux of Pre-existing Flux Ropes of CMEs  Re-analysis of Lepping's Fitting Method for Magnetic Clouds: Lundquist Fit Reloaded  Edit Entry  Download Preprint  Delete Entry 

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