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A Two-Step Magnetic Reconnection in a Confined X-class Flare in Solar Active Region 12673
Peng Zou, Chaowei Jiang, Xueshang Feng +3
Solar flares are often associated with coronal eruptions, but there are confined ones without eruption, even for some X-class flares. How such large flares occurred and why they ar…
Magnetohydrodynamic Simulation of the X9.3 Flare on 2017 September 6: Evolving Magnetic Topology
Chaowei Jiang, Peng Zou, Xueshang Feng +7
Three-dimensional magnetic topology is crucial to understanding the explosive release of magnetic energy in the corona during solar flares. Much attention has been given to the pre…
Decipher the Three-Dimensional Magnetic Topology of a Great Solar Flare
Chaowei Jiang, Peng Zou, Xueshang Feng +5
Three-dimensional magnetic topology of solar flare plays a crucial role in understanding its explosive release of magnetic energy in the corona. However, such three-dimensional cor…