Geospace Environmental Modeling (GEM) magnetic reconnection challenge

By Juhani Birn, J. Drake, M. Shay, B. Rogers, R. Denton, M. Hesse, M. Kuznetsova, Zhiwei Ma, Ashis Bhattacharjee, A. Otto and 1 more. 2001

1,119 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/cb11f346bb41adf8c5d89d91ad106beb3091ffb1

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In Astronomy and Astrophysics

1. B. Cerutti
2. E. Zweibel
3. M. Yamada
4. J. Klimchuk
5. B. Lavraud
6. Chang Liu
7. K. Xu
8. M. Begelman

In Molecular Biology

1. J. Klimchuk
2. B. Lavraud
3. M. Yamada
4. E. Zweibel
5. N. Vilmer
6. V. Petrosian
7. L. Fletcher
8. J. Borovsky

Citations in the corpus

• A Reconnection Switch to Trigger gamma-Ray Burst Jet Dissipation (2010, neutral): “The Hall effect involves a two-fluid laminar reconnection configuration with vr ≤ 0.1vA (Mandt, Denton & Drake 1994; Shay et al. 1998; Bhattacharjee, Ma & Wang 2001; Birn et al. 2001; Cassak et al. 2005; Daughton et al. 2006; Yamada et al. 2006).”
• A Unified Gas Kinetic Scheme for Continuum and Rarefied Flows V: Multiscale and Multi-Component Plasma Transport (2016, background): “Magnetic Reconnection Magnetic reconnection is a process in which the topology of the magnetic field lines changes [39].”
• Non-thermal particle acceleration in collisionless relativistic electron-proton reconnection (2016, background): “…is the Hall effect, which has received much attention in nonrelativistic reconnection studies (Sonnerup 1979; Terasawa 1983; Shay et al. 1998; Birn et al. 2001; Rogers et al. 2001; Wang et al. 2000; Ren et al. 2005; Uzdensky & Kulsrud 2006), and has also been observed in relativistic…”
• Magnetic Reconnection in Astrophysical and (2009, background): “We note that even with the presence of the thin electron diffusion region, the reconnection rate is still primarily determined by the Hall electric field, as was concluded by the multicode GEM project (Birn et al. 2001).”
• Impulsive Magnetic Reconnection in the Earth's Magnetotail and the Solar Corona (2004, background): “…22:23 AR AR222-AA42-09.tex AR222-AA42-09.sgm LaTeX2e(2002/01/18) P1: IKH IMPULSIVE MAGNETIC RECONNECTION 373 because Hall MHD effects decouple electron and ion motions in the reconnection layer (Biskamp et al. 1995, Ma & Bhattacharjee 1996, Shay & Drake 1998, Wang et al. 2000, Birn et al. 2001).”
• Particle Acceleration and Magnetic Dissipation in Relativistic Current Sheet of Pair Plasmas (2007, neutral): “It has been believed that the reconnection’s global energy dissipation is controlled by the Hall physics (Birn et al. 2001).”