Homologous Confined Filament Eruptions via Magnetic Breakout

By C. R. DeVore, S. Antiochos. 2008

197 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/f8ece6a1cac328beeffc43155aaa64343658d5c8

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. M. Temmer
2. C. Schrijver
3. A. Vourlidas
4. H. Hudson
5. N. Lugaz
6. Etienne Pariat
7. A. Title
8. Yan Li

Citations in the corpus

• Driving major solar flares and eruptions: A review (2008, background): “One recent example of such fields is discussed by DeVore and Antiochos (2008).”
• Topological Evolution of a Fast Magnetic Breakout CME in Three Dimensions (2008, background): “Recent simulations by DeVore & Antiochos (2008) have shown the breakout process works in a true 3D system with four distinct flux systems and a null line that intersects the boundary, yielding homologous eruptions when the system is continually energized.”
• 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 ].”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “…free energy into the system through flux emergence (MacTaggart and Hood, 2009; Chatterjee and Fan, 2013), through continuous shear motions (DeVore and Antiochos, 2008; Soenen et al., 2009), or by the perturbation of previously neighboring eruptions (Török et al., 2011; Bemporad et al.,…”
• THREE-DIMENSIONAL MODELING OF QUASI-HOMOLOGOUS SOLAR JETS (2010, background): “In contrast to DeVore & Antiochos (2008), our free energy Ef does not accumulate secularly, because the magnetic and kinetic energies are free to escape through the top boundary of our open domain.”
• An Observational Overview of Solar Flares (2011, background): “Therefore models which permit the release of stored magnetic energy without field opening are also necessary - such as those proposing internal reconnections in active region core field (Gibson & Fan 2006), or reconnection without full field opening (DeVore & Antiochos 2008; Masson et al. 2009).”
• How Many CMEs Have Flux Ropes? Deciphering the Signatures of Shocks, Flux Ropes, and Prominences in Coronagraph Observations of CMEs (2012, methodology): “We analyze results obtained with an Adaptively Refined 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…”