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Cited article:

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Understanding the global structure of the September 5, 2022, coronal mass ejection using sunRunner3D

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The reason for the widespread energetic storm particle event of 13 March 2023

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Cross-field Diffusion Effects on Particle Transport in a Solar Coronal Flux Rope

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Modeling Ion Acceleration and Transport in Corotating Interaction Regions: The Mass-to-charge Ratio Dependence of the Particle Spectrum

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Unraveling the Origins of an Extreme Solar Eruptive Event with Hard X-Ray Imaging Spectroscopy

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Effects of adiabatic focusing and free-escape boundaries in coronal shock acceleration

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Journal of Space Weather and Space Climate 14 15 (2024)
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