Topological Evolution of a Fast Magnetic Breakout CME in Three Dimensions

By B. Lynch, S. Antiochos, C. R. DeVore, Jan Luhmann, T. Zurbuchen. 2008

226 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/6531d50d38c018459942f8cb04ca0e575bef49d0

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Citations in the corpus

Three-dimensional magnetic reconnection regimes: a review (2011, background): “3D null point reconnection, via the spine-fan reconnection mode, has been proposed as a mechanism for polar jets (Pariat et al., 2009) as well as for CMEs via the ‘magnetic breakout’ model (Antiochos et al., 1999; Lynch et al., 2008).”
The standard flare model in three dimensions II: upper limit on solar flare energy (2012, background): “%) of the total released magnetic energy is converted into the CME kinetic energy (Amari et al. 2003; Jacobs et al. 2006; Lynch et al. 2008; Reeves et al. 2010).”
DIRECT EVIDENCE FOR A FAST CORONAL MASS EJECTION DRIVEN BY THE PRIOR FORMATION AND SUBSEQUENT DESTABILIZATION OF A MAGNETIC FLUX ROPE (2012, background): “S R ] 3 0 N ov 2 & Roumeliotis 1992; Antiochos et al. 1999; Amari et al. 2000; Lynch et al. 2008; Vršnak 2008), or in the photosphere or low chromosphere, photospheric flux rope (e.g., Magara & Longcope 2001; Manchester et al. 2004; Gibson & Fan 2006; Archontis & Hood 2008) after the emergence of…”
The standard flare model in three dimensions - I. Strong-to-weak shear transition in post-flare loops (2012, result): “This ratio is consistent with the values found in other 3D MHD simulations of CME triggering (see e.g. Amari et al. 2003; Lynch et al. 2008).”
How Many CMEs Have Flux Ropes? Deciphering the Signatures of Shocks, Flux Ropes, and Prominences in Coronagraph Observations of CMEs (2012, methodology): “…MHD Solver (ARMS; DeVore and Antiochos, 2008) simulation of the ‘magnetic breakout’ CME initiation mechanism (Antiochos, DeVore, and Klimchuk, 1999; Lynch et al., 2004, 2008) and the subsequent FR-CME propagation in the low corona to construct synthetic coronagraph images we can directly compare…”
The Physical Processes of CME/ICME Evolution (2017, methodology): “In contrast to these simulations, in which the eruption starts from a fully-developed flux rope, Lynch et al. (2009) modeled CME rotation starting from a sheared arcade, using the breakout model (Antiochos et al. 1999; Lynch et al. 2008).”