Collisionless magnetic reconnection: Electron processes and transport modeling
By M. Hesse, Juhani Birn, M. Kuznetsova. 2001
183 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/804f6a885d364e8d3ba72b722a91146b27d523d8
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In Astronomy and Astrophysics
In Nuclear and High Energy Physics
Citations in the corpus
- Current sheet structure near magnetic X‐line observed by Cluster (2003, methodology): “, 1998] and PIC [Hesse et al., 2001; Pritchett, 2001] simulations that a magnetic reconnection produces a quadrupolar out-of-plane component of the magnetic field.”
- Multi-point observations of the Hall electromagnetic field and secondary island formation during magnetic reconnection (2006, background): “significant (20–40%) fraction of the lobe magnetic field strength B0 [Hesse et al., 2001].”
- Dipolarization fronts as a signature of transient reconnection in the magnetotail (2009, background): “[12] Recent particle simulations with open boundaries [Daughton et al., 2006] revealed a number of new effects, such as the elongation of the electron dissipation region and the formation ofthe secondary magnetic islands thatwerenot detected before for the case of antiparallel undriven reconnection ”
- A Unified Gas Kinetic Scheme for Continuum and Rarefied Flows V: Multiscale and Multi-Component Plasma Transport (2016, methodology): “Various models were used to describe this phenomenon, for example the electron MHD [40], MHD and Hall MHD [41, 42], full particle [43], and hybrid model [44].”