Hall magnetohydrodynamic reconnection: The Geospace Environment Modeling challenge

By Zhiwei Ma, Ashis Bhattacharjee. 2001

162 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/5875bd7e801149d2030e666511f5e9a4cb80cc93

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. G. Aulanier
2. Etienne Pariat
3. P. Démoulin
4. C. R. DeVore
5. Chang Liu
6. K. Xu
7. Brigitte Schmieder
8. C. Schrijver

In Nuclear and High Energy Physics

1. G. Aulanier
2. Etienne Pariat
3. P. Démoulin
4. Chang Liu
5. K. Xu

Citations in the corpus

• 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].”
• Slip-Running Reconnection in Quasi-Separatrix Layers (2006, background): “…frame of resistive MHD (see e.g. Petschek, 1964; Strauss, 1986; Priest and Forbes, 1992a; Craig and McClymont, 1993; Baty, Priest, and Forbes, 2006) or of Hall MHD, which supports reconnection through collisionless processes (see e.g. Ma and Bhattacharjee, 2001; Bhattacharjee, Ma, and Wang, 2003).”