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
-
Conditions for Solar Prominence Formation Triggered by Single Localized Heating
by: Takero Yoshihisa, et al.
Published: (2024-01-01) -
Rotational Flows in Solar Coronal Flux Rope Cavities
by: Valeriia Liakh, et al.
Published: (2023-01-01) -
Mass Cycle and Dynamics of a Virtual Quiescent Prominence
by: D. Donné, et al.
Published: (2024-01-01) -
Nonlinear Fast Magnetosonic Waves in Solar Prominence Pillars
by: Leon Ofman, et al.
Published: (2023-01-01) -
Frozen-field Modeling of Coronal Condensations with MPI-AMRVAC. I. Demonstration in Two-dimensional Models
by: Yuhao Zhou, et al.
Published: (2024-01-01)