Extending the concept of separatrices to QSLs for magnetic reconnection

By P. Démoulin. 2006

133 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/bb08547cfb263644ad5a05a9922f7a60af638c8f

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In Astronomy and Astrophysics

1. G. Aulanier
2. Etienne Pariat
3. P. Démoulin
4. J. Thalmann
5. T. Wiegelmann
6. David Pontin
7. S. Solanki
8. C. R. DeVore

Citations in the corpus

• Slip-Running Reconnection in Quasi-Separatrix Layers (2006, background): “In these cases, flare ribbons correspond to the intersection of the QSLs with the chromosphere (see e.g. Démoulin et al., 1997 and the review of Démoulin, 2006), and the diverging motions of flare ribbons there correspond to those of the QSLs during the reconnection (as described in Section 5.4…”
• Three-dimensional magnetic reconnection regimes: a review (2011, background): “For a detailed review of these ideas, see Démoulin (2006).”
• The magnetic field in the solar atmosphere (2014, background): “It is possible to trace the different magnetic flux domains in the corona and their footprint on the solar surface, given that the 3D magnetic field configuration is known (Priest and Démoulin, 1995; Demoulin et al., 1997; Démoulin, 2006; Titov et al., 2002).”