Reconnection of Twisted Flux Tubes as a Function of Contact Angle
By M. Linton, R. Dahlburg, S. Antiochos. 2001
159 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/ade96c00794bd3ed014a9668947eb661857f1fc3
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In Astronomy and Astrophysics
- A. Lazarian
- Gregory L. Eyink
- Ethan Vishniac
- David Pontin
- J. Klimchuk
- Huirong Yan
- Grzegorz Kowal
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In Nuclear and High Energy Physics
Citations in the corpus
- Three-dimensional magnetic reconnection regimes: a review (2011, background): “Notably, Linton et al. (2001) and Linton and Priest (2003) have investigated the interaction of magnetic flux tubes in an otherwise field-free environment, and discovered different possible interactions (‘merge’, ‘bounce’, ‘tunnel’ and ‘slingshot’) depending on the relative orientations of the…”
- FAST MAGNETIC RECONNECTION AND SPONTANEOUS STOCHASTICITY (2011, background): “…could be generalized to allow for compressible plasma and asymmetric field-strengths (Cassak & Shay 2007), flux-tubes intersecting at an angle or with a shared component of magnetic field (guide field) Bz (Linton et al. 2001), twisted flux-tubes with magnetic helicity (Zweibel & Rhoads 1995), etc.”
- On Solving the Coronal Heating Problem (2005, background): “However, tubes with opposite twist and like polarity (having axial fields pointed in the same general direction) are not prone to interact (Linton, Dahlburg, and Antiochos, 2001; case RL0 in their notation).”