CMEs Driven by Flux Rope Herniation

Details CMEs Driven by Flux Rope Herniation CMEs Driven by Flux Rope Herniation

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.2908r&link_type=abstract

American Astronomical Society Meeting 210, #29.08; Bulletin of the American Astronomical Society, Vol. 39, p.138

Astronomy and Astrophysics

Astronomy

Scientific paper

Much numerical work has been done on the magnetic kink instability as a CME driver, but thus far it is all subject to numerical diffusion which can bias results toward eruption. We present further results on this instability in the absence of reconnection. We have found that a highly twisted metastable magnetic configuration consisting of a fluxrope contained by an arcade is capable of creating an impulsive CME through herniation and without any reconnection.

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