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Laboratory study of the torus instability threshold in solar-relevant, line-tied magnetic flux ropes
Andrew Alt, Clayton E. Myers, Hantao Ji +7
Coronal mass ejections (CME) occur when long-lived magnetic flux ropes (MFR) anchored to the solar surface destabilize and erupt away from the Sun. This destabilization is often de…
Decoding the Pre-Eruptive Magnetic Field Configurations of Coronal Mass Ejections
S. Patsourakos, A. Vourlidas, T. Török +15
A clear understanding of the nature of the pre-eruptive magnetic field configurations of Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting solar…
Coronal Mini-jets in an Activated Solar Tornado-like Prominence
Huadong Chen, Jun Zhang, Bart De Pontieu +3
High-resolution observations from the () reveal the existence of a particular type of small solar jets, which arose singly or in clust…
Initiation and Early Kinematic Evolution of Solar Eruptions
X. Cheng, J. Zhang, B. Kliem +5
We investigate the initiation and early evolution of 12 solar eruptions, including six active region hot channel and six quiescent filament eruptions, which were well observed by t…
Extreme Ultraviolet Late Phase of Solar Flares
Jun Chen, Rui Liu, Kai Liu +4
A second peak in extreme ultraviolet sometimes appears during the gradual phase of solar flares, which is known as EUV late phase (ELP). Stereotypically ELP is associated with two…