An Evolution and Eruption of the Coronal Magnetic Field through a Data-Driven MHD Simulation

Abstract

We present a newly developed data-driven magnetohydrodynamics (MHD) simulation code under a zero-beta approximation based on a method proposed by Hayashi et al. 2018 and 2019. Although many data-driven MHD simulations have been developed and conducted, there are not many studies on how accurately those simulations can reproduce the phenomena observed in the solar corona. In this study, we investigated the performance of our data-driven simulation quantitatively using ground-truth data. The ground-truth data was produced by an MHD simulation in which the magnetic field is twisted by the sunspot motions. A magnetic flux rope (MFR) is created by the cancellation of the magnetic flux at the polarity inversion line due to the converging flow on the sunspot, which eventually leads the eruption of the MFR. We attempted to reproduce these dynamics using the data-driven MHD simulation. The coronal magnetic fields are driven by the electric fields, which are obtained from a time-series of the photospheric magnetic field that is extracted from the ground-truth data, on the surface. As a result, the data-driven simulation could capture the subsequent MHD processes, the twisted coronal magnetic field and formation of the MFR, and also its eruption. We report these results and compare with the ground-truth data, and discuss how to improve the accuracy and optimize numerical method.

arXiv commentAccepted for publication in ApJ

References in corpus (28)

• The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs -- Space-weather HMI Active Region Patches
• Evolution of Magnetic Field and Energy in A Major Eruptive Active Region Based on SDO/HMI Observation
• Non-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejection
• Flare-productive active regions
• Tracking Vector Magnetograms with the Magnetic Induction Equation
• A Method for Data-Driven Simulations of Evolving Solar Active Regions
• High-resolution observations of flare precursors in the low solar atmosphere
• Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
• Formation and Eruption of an Active Region Sigmoid: I. Study by Nonlinear Force-Free Field Modeling
• Magnetohydrodynamic Simulation of the X2.2 Solar Flare on 2011 February 15: I. Comparison with the Observations
• A Comprehensive Method of Estimating Electric Fields from Vector Magnetic Field and Doppler Measurements
• Solar Magnetic Flux Rope Eruption Simulated by a Data-Driven Magnetohydrodynamic Model
• 3D Prominence-hosting Magnetic Configurations: Creating a Helical Magnetic Flux Rope
• Estimating Electric Fields from Vector Magnetogram Sequences
• Magnetohydrodynamic Simulation of Magnetic Null-point Reconnections and Coronal dimmings during the X2.1 flare in NOAA AR 11283
• The PDFI_SS Electric Field Inversion Software
• Comparative Study of Data-driven Solar Coronal Field Models Using a Flux Emergence Simulation as a Ground-truth Data Set
• Optimization of Photospheric Electric Field Estimates for Accurate Retrieval of Total Magnetic Energy Injection
• Magnetohydrodynamic Simulations for Studying Solar Flare Trigger Mechanism
• Testing the Accuracy of Data Driven MHD Simulations of Active Region Evolution
• Statistical Relation between Solar Flares and Coronal Mass Ejections with Respect to Sigmoidal Structures in Active Regions
• Data-driven MHD simulation of successive solar plasma eruptions
• Reconstruction of a Large-scale Pre-flare Coronal Current Sheet Associated with an Homologous X-shaped Flare
• A Study of Magnetic Field Characteristics of Flaring Active Region Based on Nonlinear Force-free Field Extrapolation
• Chromospheric magnetic field: A comparison of He I 10830 A observations with nonlinear force-free field extrapolation
• Evolution of the Non-potential Magnetic Field in the Solar Active Region 12673 Based on a Nonlinear Force-free Modeling
• Onset Mechanism of M6.5 Solar Flare Observed in Active Region 12371
• Extrapolation of Three-dimensional Magnetic Field Structure in Flare-productive Active Regions with Different Initial Conditions

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