Magnetic flux ropes in the solar corona: structure and evolution toward eruption

@article{Liu2020MagneticFR,
  title={Magnetic flux ropes in the solar corona: structure and evolution toward eruption},
  author={Rui Liu},
  journal={Research in Astronomy and Astrophysics},
  year={2020},
  volume={20}
}
  • Rui Liu
  • Published 22 July 2020
  • Physics
  • Research in Astronomy and Astrophysics
Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in the solar atmosphere, flux ropes hold the key to understanding the physical mechanisms of solar eruptions, which impact the heliosphere and planetary atmospheres. The strongést disturbances in the Earth’s space environments are often associated with large-scale flux ropes from the Sun colliding with the Earth’s… 
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