A Numerical Study of the Breakout Model for Coronal Mass Ejection Initiation

By P. MacNeice, S. Antiochos, A. D. Phillips, D. Spicer, C. R. DeVore, K. Olson. 2004

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View Paper: https://www.semanticscholar.org/paper/a4751af8bd95d440302c8b66b1b30868d9317a74

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In Astronomy and Astrophysics

Citations in the corpus

A MODEL FOR SOLAR POLAR JETS (2009, background): “This type of current structure is common to any low-beta system driven by footpoint motions (e.g. Antiochos & DeVore 1999; MacNeice et al. 2004).”
NEW SOLAR EXTREME-ULTRAVIOLET IRRADIANCE OBSERVATIONS DURING FLARES (2011, background): “While the onset of the eruption may be due to what is known as break-out reconnection (Antiochos et al. 1999), it is the flare reconnection that produces the rapid acceleration (MacNeice et al. 2004).”
Long‐range magnetic couplings between solar flares and coronal mass ejections observed by SDO and STEREO (2011, background): “The third interpretation, in which the changing large‐scale field destabilizes regional field configurations, is one that is, for example, invoked in the breakout model of filament eruptions and CMEs [e.g., Gary and Moore, 2004; MacNeice et al., 2004; DeVore and Antiochos, 2008].”
Homologous Confined Filament Eruptions via Magnetic Breakout (2008, methodology): “Our previous work on axisymmetric breakout configurations (Antiochos et al. 1999; MacNeice et al. 2004) showed analogous features in the acceleration profiles, although (1) the special symmetry in those cases leads to the formation of flux ropes disconnected from the solar surface, rather than…”
The Calm before the Storm: The Link between Quiescent Cavities and Coronal Mass Ejections (2006, background): “The idea of the erupting CME as a magnetic flux rope has gained acceptance over the years (Amari et al. 2003; Chen&Krall 2003; Roussev et al. 2003; MacNeice et al. 2004; Manchester et al. 2004).”
Sixty-five years of solar radioastronomy: flares, coronal mass ejections and Sun–Earth connection (2008, background): “Results of numerical studies of the breakout model show that the plasmoid ejection occurs at the speed of the coronal Alfven speed and that the breakout model can produce fast CMEs (MacNeice et al. 2004).”
Topological Evolution of a Fast Magnetic Breakout CME in Three Dimensions (2008, methodology): “MacNeice et al. (2004) showed that with sufficient resolution, the axisymmetric simulation breakout results were independent of the grid size.”
A Statistical Study of Main and Residual Accelerations of Coronal Mass Ejections (2006, background): “These models usually show a transition from slow to fast motion of the erupting magnetic structure (Mikic & Linker 1994; Lin & Forbes 2000; Chen & Shibata 2000; MacNeice et al. 2004).”