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Origin and Structures of Solar Eruptions I: Magnetic Flux Rope
DOI: 10.1007/s11430-017-9074-6 Bibcode: 2017ScChD..60.1383C

Cheng, Xin; Guo, Yang; Ding, MingDe

Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic eruptive phenomena in our solar system and able to release a large quantity of plasma and magnetic flux from the solar atmosphere into the solar wind. When these high-speed magnetized plasmas along with the energetic particles arrive at the Earth, they may intera…

2017 Science China Earth Sciences
IRIS SOHO 116