Reconnection in multiple current sheet configurations in the solar corona

Details Reconnection in multiple current sheet configurations in the solar corona Reconnection in multiple current sheet configurations in the solar corona

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19.1879b&link_type=abstract

Advances in Space Research, vol. 19, p. 1879

Computer Science

1

Solar Corona, Magnetic Field Reconnection, Solar Magnetic Field, Current Sheets, Magnetic Field Configurations, Tearing Modes (Plasmas), Three Dimensional Models, Magnetohydrodynamic Stability, Coronal Mass Ejection, Magnetic Flux

Scientific paper

With a view to the study of solar coronal helmet streamers, 3D resistive MHD simulations are conducted of magnetic reconnection in a multiple current magnetic sheet configuration. The simulations of the linear and nonlinear development of the tearing mode instability indicate that reconnection in complex coronal neighboring flux systems converts magnetic field energy into thermal energy and results in small-scale tonge outflows rather than coronal mass ejections on a larger scale.

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