The scaling of embedded collisionless reconnection
By M. Shay, J. Drake, M. Swisdak, B. Rogers. 2004
133 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/92f3d52dcd5d849b19bb55c57948e23d453b2dd5
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In Astronomy and Astrophysics
In Nuclear and High Energy Physics
Citations in the corpus
- Magnetic Reconnection in Astrophysical and (2009, background): “However, Shay et al. (1999, 2004) and Huba & Rudakov (2004) argued that the length L of the outflow region always adjusts itself, possibly after a slow development phase (Shay et al. 2004), to about 10 δi.”
- NUMERICAL TESTS OF FAST RECONNECTION IN WEAKLY STOCHASTIC MAGNETIC FIELDS (2009, methodology): “In particular, simulations using Hall MHD have produced stable X-point reconnection (Shay et al. 1998, 2004).”
- Magnetic Fields in Galaxies (2010, background): “This is presently a matter of some controversy, with arguments and numerical evidence for independence (Shay et al. 2004) but also for a linear scaling (Fitzpatrick 2004).”
- A MAGNETIC RECONNECTION MECHANISM FOR ION ACCELERATION AND ABUNDANCE ENHANCEMENTS IN IMPULSIVE FLARES (2009, methodology): “Our simulations are performed with the PIC code p3d (Zeiler et al. 2002) and the Hall MHD code f3d (Shay et al. 2004).”
- Multi-point observations of the Hall electromagnetic field and secondary island formation during magnetic reconnection (2006, result): “tent with results from some simulation studies [Shay et al., 2004].”