Complete replacement of magnetic flux in a flux rope during a coronal mass ejection
Author:
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
https://www.nature.com/articles/s41550-023-01966-2.pdf
Reference51 articles.
1. Patsourakos, S. et al. Decoding the pre-eruptive magnetic field configurations of coronal mass ejections. Space Sci. Rev. 216, 131 (2020).
2. Liu, R. Magnetic flux ropes in the solar corona: structure and evolution toward eruption. Res. Astron. Astrophys. 20, 165 (2020).
3. Priest, E. R. & Forbes, T. G. The magnetic nature of solar flares. Astron. Astrophys. Rev. 10, 313–377 (2002).
4. Temmer, M. Space weather: the solar perspective. Living Rev. Sol. Phys. 18, 4 (2021).
5. Cheng, X., Guo, Y. & Ding, M. Origin and structures of solar eruptions I: magnetic flux rope. Sci. China Earth Sci. 60, 1383–1407 (2017).
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