Slip-Running Reconnection in Quasi-Separatrix Layers

By G. Aulanier, Etienne Pariat, P. Démoulin, C. R. DeVore. 2006

223 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/f16055ba86b0d01597d392a6fa6984c105458543

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In Astronomy and Astrophysics

1. G. Aulanier
2. Etienne Pariat
3. M. Temmer
4. C. Schrijver
5. P. Démoulin
6. M. Janvier
7. Haimin Wang
8. Chang Liu

Citations in the corpus

• Alfvén Waves in the Solar Atmosphere (2012, background): “However, current understanding suggests they can be generated during the reconnection process, when the magnetic field relaxes from its stressed pre-flare state (Aulanier et al. 2006).”
• Three-dimensional magnetic reconnection regimes: a review (2011, background): “The continuous change of connectivity of field lines traced from comoving footpoints has led to such reconnection being termed variously magnetic flipping (Priest and Forbes, 1992) or slip-running reconnection (if the virtual flipping velocity exceeds some threshold, Aulanier et al. (2006)).”
• THE NATURE OF FLARE RIBBONS IN CORONAL NULL-POINT TOPOLOGY (2009, background): “An apparent slippage velocity of reconnecting field lines which is sub-Alfvénic implies slipping reconnection, whereas a super-Alfvénic slippage velocity defines the slip-running reconnection (Aulanier et al. 2006).”
• The standard flare model in three dimensions - III. Slip-running reconnection properties (2013, background): “Since the field lines are slipping from the initial to the final positions within less than one Alfvén time, this motion can be coined a “slip-running” reconnection motion (as defined in Aulanier et al. 2006).”
• CIRCULAR RIBBON FLARES AND HOMOLOGOUS JETS (2012, background): “Second, the clearly observed sequential brightening of the fan ribbon k2 and the elon- gated shape of the inner spine ribbon k1 well resemble the event of M09, and would strongly suggest the existence of extended QSLs, in which the null point and the related fan-spine structure are embedded.”
• An Observational Overview of Solar Flares (2011, background): “This Figure reveals strong resemblances between observed and calculated features; in particular the lower source moves extremely rapidly almost in coincidence with one of the separatrix intersections, in a manner suggesting the “slip-running” reconnection model of Aulanier et al. (2006).”