Data-constrained Magnetohydrodynamic Simulation for Magnetic Flux Rope Eruptions Driven by Magnetic Reconnection
We conducted data-constrained magnetohydrodynamic (MHD) simulations for solar active region (AR) NOAA AR 11429, which produced two X-class flares within a span of 63 minutes. The simulations were performed using the zero- β MHD approximation, with the initial condition derived from the nonlinear for...
Saved in:
| Main Authors: | Nian Liu, Satoshi Inoue, Ying Wang, Haimin Wang |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adba56 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842. I. Dynamics of the Solar Eruption Associated with the X7.1 Solar Flare
by: Keitarou Matsumoto, et al.
Published: (2025-01-01) -
Acceleration of Solar Eruptions via Enhanced Torus Instability Driven by Small-scale Flux Emergence
by: Satoshi Inoue, et al.
Published: (2025-01-01) -
Basic Pattern of Three-dimensional Magnetic Reconnection within Strongly Turbulent Current Sheets
by: Yulei Wang, et al.
Published: (2025-01-01) -
A Successful Sheared-arcade Eruption Triggered by a Failed Erupted Small Filament
by: Wentai Fu, et al.
Published: (2025-01-01) -
The Effect of Plasma-β on the Heating Mechanisms during Magnetic Reconnection in Partially Ionized Low Solar Atmosphere
by: Abdullah Zafar, et al.
Published: (2025-01-01)