Data-driven modeling of solar coronal magnetic field evolution and eruptions-Reference-Cited by-同舟云学术

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Data-driven modeling of solar coronal magnetic field evolution and eruptions

Published:2022-05 Issue:3 Volume:3 Page:100236
ISSN:2666-6758
Container-title:The Innovation
language:en
Short-container-title:The Innovation

Author:

Jiang Chaowei^ORCID,Feng Xueshang,Guo Yang,Hu Qiang

Publisher

Elsevier BV

Subject

Multidisciplinary

Reference197 articles.

1. Physics of the Solar Corona. An Introduction;Aschwanden,2004

2. Coronal mass ejections: models and their observational basis;Chen;Living Rev. Solar Phys.,2011

3. Solar flares: magnetohydrodynamic processes;Shibata;Living Rev. Solar Phys.,2011

4. The solar magnetic field;Solanki;Rep. Prog. Phys.,2006

Cited by 29 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Magnetic flux rope models and data-driven magnetohydrodynamic simulations of solar eruptions;Reviews of Modern Plasma Physics;2024-09-05

2. Magnetic Eruption from a Three-ribbon Flare;The Astrophysical Journal;2024-08-28

3. Recent advances in solar data-driven MHD simulations of the formation and evolution of CME flux ropes;Reviews of Modern Plasma Physics;2024-08-10

4. Analysis of modeled 3D solar magnetic field during 30 X/M-class solar flares;Frontiers in Astronomy and Space Sciences;2024-05-10

5. Developments of a fundamental mechanism for initiation of solar eruptions;Reviews of Modern Plasma Physics;2024-04-19

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