The Partial Expulsion of a Magnetic Flux Rope

By S. Gibson, Yuhong Fan. 2006

141 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/9fadd6eceb4159eac4a2803534fde61bb8b90eb1

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In Astronomy and Astrophysics

1. M. Temmer
2. S. Gibson
3. Yuhong Fan
4. A. Vourlidas
5. S. Patsourakos
6. H. Hudson
7. Wei Liu
8. L. Green

In Molecular Biology

1. S. Gibson
2. Yuhong Fan
3. M. Temmer
4. Wei Liu
5. B. Kliem
6. L. Green
7. S. Patsourakos
8. G. Toma

Citations in the corpus

• 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).”
• Onset of Coronal Mass Ejections Due to Loss of Confinement of Coronal Flux Ropes (2007, methodology): “As was found in Gibson & Fan (2006a, 2006b), in case K, a flux rope containing dipped helical field lines is left behind in the posteruption state (see the left panels of Fig.”
• Coronal prominence structure and dynamics: A magnetic flux rope interpretation (2006, methodology): “As the rope emerges, the coronal field quasi-statically evolves through increasingly energized equilibria, until a magnetic twist threshold is crossed, leading to loss of equilibrium and eruption [Fan, 2005; Gibson and Fan, 2006].”
• The Calm before the Storm: The Link between Quiescent Cavities and Coronal Mass Ejections (2006, background): “Partially erupting magnetic flux ropes, where a significant portion of the twisted field remains behind after the eruption, have been demonstrated numerically and used to explain partial filament eruptions and the quick reforming of X-ray sigmoids (Gibson & Fan 2006; Gibson et al. 2006).”
• DIRECT EVIDENCE FOR A FAST CORONAL MASS EJECTION DRIVEN BY THE PRIOR FORMATION AND SUBSEQUENT DESTABILIZATION OF A MAGNETIC FLUX ROPE (2012, background): “…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 a twisted flux tube from the convection zone.”
• Eruption of magnetic flux ropes during flux emergence (2008, unknown): “Also, Gibson & Fan (2006) studied the eruption of a rope in the case that sufficient twist had emerged to induce a loss of equilibrium.”
• Photospheric flux cancellation and associated flux rope formation and eruption (2010, background): “This, however, is conclusive only if the sigmoid survives an eruption (Gibson & Fan 2006; Green & Kliem 2009), since S shaped field lines in a sheared arcade (Antiochos et al. 1994)can only then be excluded.”