Computer Science
Scientific paper
Jan 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19.1797s&link_type=abstract
Advances in Space Research, vol. 19, p. 1797
Computer Science
3
Magnetic Field Reconnection, Current Sheets, Magnetoresistivity, Tearing Modes (Plasmas), Solar Corona, Plasma Dynamics, Transient Response, Magnetic Field Configurations
Scientific paper
After induced tearing and multiple coalescence, the present 2D compressible MHD simulations of current-sheet dynamics influenced by multiple anomalous resistivity areas and slight asymmetries first form, and then accelerate, a plasmoid. X-points drive the dynamical evolution toward transient reconnection geometry. Attention is given to the Lundquist number dependence of current density extrema, plasmoid bulk velocity, and maximum reconnection rate.
Kliem Bernhard
Schumacher Joerg
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