Experimental study of two-fluid effects on magnetic reconnection in a laboratory plasma with variable collisionality
By M. Yamada, Yang Ren, H. Ji, J. Breslau, S. Gerhardt, R. Kulsrud, A. Kuritsyn. 2006
146 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/92f53ae1f22d3dcdfa07f2b0a3f0eee424659a42
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In Astronomy and Astrophysics
- U. Colorado
- Boulder
- Cosmology
- Stanford University
- D. Physics
- Center for Nonlinear Studies
- Kavli Institute for Astrophysics
- D. N. B. D. O. Physics
In Nuclear and High Energy Physics
- U. Colorado
- Boulder
- Cosmology
- Center for Nonlinear Studies
- Kavli Institute for Astrophysics
- Stanford University
- D. N. B. D. O. Physics
- D. Physics
Citations in the corpus
- Magnetic Reconnection in Astrophysical and (2009, methodology): “Using Equation 2, we find δSP δi = ( L λmfp )1/2 (me mi )1/4 , (6) where λmfp is the electron mean free path; we have assumed Te = Ti, vA ∼ vthi (β ∼ 1 in the reconnection layer), and η⊥ ∼ 2η‖ owing to the magnetic field (Yamada et al. 2006).”
- A Reconnection Switch to Trigger gamma-Ray Burst Jet Dissipation (2010, background): “Therefore, it is important to determine whether a reconnecting system is collisional or collisionless in order to determine whether current sheets operate in the fast reconnection mode (Cassak et al. 2005; Malyshkin et al. 2005; Yamada et al. 2006; Bessho & Bhattacharjee 2007; Uzdensky 2007a,c).”