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Analysis of the Helical Kink Stability of Differently Twisted Magnetic Flux Ropes
Magnetic flux ropes (MFRs) are usually considered to be the magnetic structure that dominates the transport of helicity from the Sun into the heliosphere. They entrain a confined plasma within a helically organized magnetic structure and are able to cause geomagnetic activity. The formation, evolution, and twist distribution of MFRs are issues subject to strong debate. Although different twist profiles have been suggested so far, none of them has been thoroughly explored yet. The aim of this work is to present a theoretic ...
Florido-Llinas, M.; Nieves-Chinchilla, T.; Linton, M.;
Published by: Solar Physics Published on: 09/2020
YEAR: 2020   DOI: 10.1007/s11207-020-01687-z
coronal mass ejections; Flux ropes; Kink instability; magnetic fields; parker solar probe; Solar Probe Plus; Twist distribution