Testing a Solar Coronal Magnetic Field Extrapolation Code with the Titov-Demoulin Magnetic Flux Rope Model by Jiang, Chaowei, Feng, Xueshang

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Why are non-radial solar eruptions less frequent than radial ones? by Liu, Qingjun, Jiang, Chaowei, Feng, Xuesheng, Zuo, Pingbing, Wang, Yi

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The Rotation of Magnetic Flux Rope Formed during Solar Eruption by Zhou, Zhenjun, Jiang, Chaowei, Liu, Rui, Wang, Yuming, Liu, Lijuan, Cui, Jun

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On the Lorentz Force and Torque of Solar Photospheric Emerging Magnetic Fields by Duan, Aiying, Jiang, Chaowei, Toriumi, Shin, Syntelis, Petros

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The role of photospheric converging motion in initiation of solar eruptions by Bian, Xinkai, Jiang, Chaowei, Feng, Xueshang

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Numerical Simulation of a Fundamental Mechanism of Solar Eruption with Different Magnetic Flux Distributions by Bian, Xinkai, Jiang, Chaowei, Feng, Xueshang, Zuo, Pingbing, Wang, Yi, Wang, Xinyi

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A fundamental mechanism of solar eruption initiation in multipolar magnetic field by Bian, Xinkai, Jiang, Chaowei, Feng, Xueshang, Zuo, Pingbing, Wang, Yi

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Diagnosing a Solar Flaring Core with Bidirectional Quasi-Periodic Fast Propagating Magnetoacoustic Waves by Miao, Yuhu, Li, Dong, Ding, Yuan, Jiang, Chaowei, Elmhamdi, Abouazza, Zhao, Mingyu, Anfinogentov, Sergey

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Can Injection Model Replenish the Filaments in Weak Magnetic Environment? by Zou, Peng, Jiang, Chaowei, Fengsi Wei, Cao, Wenda

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Light Bridges Can Suppress the Formation of Coronal Loops by Miao, Yuhu, Fu, Libo, Du, Xian, Ding, Yuan, Jiang, Chaowei, Su, Jiangtao, Zhao, Mingyu, Anfinogentov, Sergey

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Preprocess the Photospheric Vector Magnetograms for NLFFF Extrapolation using a Potential Field Model and an Optimization Method by Jiang, Chaowei, Feng, Xueshang

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Extrapolation of the Solar Coronal Magnetic Field from SDO/HMI Magnetogram by a CESE--MHD--NLFFF Code by Jiang, Chaowei, Feng, Xueshang

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A Model of Solar Magnetic Flux Rope Eruption Initiated Primarily by Magnetic Reconnection by Liu, Qingjun, Jiang, Chaowei, Bian, Xinkai, Feng, Xueshang, Zuo, Pingbing, Wang, Yi

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The Relationship between Chirality, Sense of Rotation, and Hemispheric Preference of Solar Eruptive Filaments by Zhou, Zhenjun, Liu, Rui, Cheng, Xing, Jiang, Chaowei, Wang, Yuming, Liu, Lijuan, Cui, Jun

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Data-driven MHD Simulation of the Formation and Initiation of a Large-scale Pre-flare Magnetic Flux Rope in Solar Active Region 12371 by He, Wen, Jiang, Chaowei, Zou, Peng, Duan, Aiying, Feng, Xueshang, Zuo, Pingbing, Wang, Yi

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Continuous Null-Point Magnetic Reconnection Builds Up a Torus Unstable Magnetic Flux Rope Triggering the X9.3 Flare in Solar Active Region~12673 by Zou, Peng, Jiang, Chaowei, Fengsi Wei, Feng, Xueshang, Zuo, Pingbing, Wang, Yi

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A fundamental mechanism of solar eruption initiation by Jiang, Chaowei, Feng, Xueshang, Liu, Rui, Yan, XiaoLi, Hu, Qiang, Moore, Ronald L, Duan, Aiying, Cui, Jun, Zuo, Pingbing, Wang, Yi, Fengsi Wei

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A Study of Pre-Flare Solar Coronal Magnetic Fields: Magnetic Flux Ropes by Duan, Aiying, Jiang, Chaowei, He, Wen, Feng, Xueshang, Zou, Peng, Cui, Jun

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A Statistical Study of Solar Filament Eruptions That Forms High-Speed Coronal Mass Ejections by Zou, Peng, Jiang, Chaowei, Fengsi Wei, Zuo, Pingbing, Wang, Yi

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A model of failed solar eruption initiated and destructed by magnetic reconnection by Jiang, Chaowei, Duan, Aiying, Zou, Peng, Zhou, Zhenjun, Bian, Xinkai, Feng, Xueshang, Zuo, Pingbing, Wang, Yi

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