SIP-IFVM: A Time-evolving Coronal Model with an Extended Magnetic Field Decomposition Strategy

SIP-IFVM: A Time-evolving Coronal Model with an Extended Magnetic Field Decomposition Strategy

Time-evolving magnetohydrodynamic (MHD) coronal modeling, driven by a series of time-dependent photospheric magnetograms, represents a new generation of coronal simulations. This approach offers more realistic results than traditional steady coronal models constrained by a static magnetogram. Howeve...

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Bibliographic Details
Main Authors: Haopeng Wang, Liping Yang, Stefaan Poedts, Andrea Lani, Yuhao Zhou, Yuhang Gao, Luis Linan, Jiakun Lv, Tinatin Baratashvili, Jinhan Guo, Rong Lin, Zhan Su, Caixia Li, Man Zhang, Wenwen Wei, Yun Yang, Yucong Li, Xinyi Ma, Edin Husidic, Hyun-Jin Jeong, Mahdi Najafi-Ziyazi, Juan Wang, Brigitte Schmieder
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
The Sun
Magnetohydrodynamics
Magnetohydrodynamical simulations
Solar corona
Online Access:https://doi.org/10.3847/1538-4365/add0b1
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