Data-constrained Magnetohydrodynamic Simulation of an Intermediate Solar Filament Eruption
Solar eruptive activities could occur in weak magnetic field environments and over large spatial scales, which are especially relevant to eruptions involving intermediate or quiescent solar filaments. To handle the large scales, we implement and apply a flux rope embedding method using regularized B...
Main Authors: | Yang Guo, Jinhan Guo, Yiwei Ni, M. D. Ding, P. F. Chen, Chun Xia, Rony Keppens, Kai E. Yang |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acf75b |
Similar Items
-
Rotational Flows in Solar Coronal Flux Rope Cavities
by: Valeriia Liakh, et al.
Published: (2023-01-01) -
Nonlinear Fast Magnetosonic Waves in Solar Prominence Pillars
by: Leon Ofman, et al.
Published: (2023-01-01) -
Solar prominences: theory and models
by: Sarah E. Gibson
Published: (2018-10-01) -
Understanding the Lateral Drifting of an Erupting Filament with a Data-constrained Magnetohydrodynamic Simulation
by: J. H. Guo, et al.
Published: (2023-01-01) -
Formation of Polar Crown Filament Magnetic Fields by Supergranular Helicity Injection
by: Huanxin Chen, et al.
Published: (2024-01-01)