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Reverse Current Model for Coronal Mass Ejection Cavity Formation

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The Origin, Early Evolution and Predictability of Solar Eruptions

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An Observationally Constrained Model of a Flux Rope that Formed in the Solar Corona

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Successive X-class Flares and Coronal Mass Ejections Driven by Shearing Motion and Sunspot Rotation in Active Region NOAA 12673

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Multi-spacecraft Observations of the Rotation and Nonradial Motion of a CME Flux Rope Causing an Intense Geomagnetic Storm

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