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Cited article:

Why are non-radial solar eruptions less frequent than radial ones?

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Monthly Notices of the Royal Astronomical Society: Letters 533 (1) L25 (2024)
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Developments of a fundamental mechanism for initiation of solar eruptions

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Reviews of Modern Plasma Physics 8 (1) (2024)
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A model of solar magnetic flux rope eruption initiated primarily by magnetic reconnection

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Monthly Notices of the Royal Astronomical Society 529 (1) 761 (2024)
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MHD Simulations of the Solar Corona to Determine the Conditions for Large Solar Flares and the Acceleration of Cosmic Rays during Them

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Physics 5 (3) 895 (2023)
https://doi.org/10.3390/physics5030058

A model of failed solar eruption initiated and destructed by magnetic reconnection

Chaowei Jiang, Aiying Duan, Peng Zou, Zhenjun Zhou, Xinkai Bian, Xueshang Feng, Pingbing Zuo and Yi Wang
Monthly Notices of the Royal Astronomical Society 525 (4) 5857 (2023)
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A Fundamental Mechanism of Solar Eruption Initiation in a Multipolar Magnetic Field

Xinkai Bian, Chaowei Jiang, Xueshang Feng, Pingbing Zuo and Yi Wang
The Astrophysical Journal 956 (2) 73 (2023)
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A Brief Review of Interplanetary Physics Research Progress in Mainland China during 2020–2022

Xinhua ZHAO, Jiansen HE, Chenglong SHEN, Shiwei FENG, Chaowei JIANG, Huichao LI, Gang QIN and Xi LUO
Chinese Journal of Space Science 42 (4) 612 (2022)
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MHD Simulation of Homologous Eruptions from Solar Active Region 10930 Caused by Sunspot Rotation

Xinyi Wang, Chaowei Jiang, Xueshang Feng, Aiying Duan and Xinkai Bian
The Astrophysical Journal 938 (1) 61 (2022)
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The role of photospheric converging motion in initiation of solar eruptions

Xinkai Bian, Chaowei Jiang and Xueshang Feng
Frontiers in Astronomy and Space Sciences 9 (2022)
https://doi.org/10.3389/fspas.2022.982108