Dynamic development of coronal current sheets

Physics

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Current Sheets, Magnetohydrodynamic Stability, Solar Corona, Stellar Mass Ejection, Magnetic Field Reconnection, Solar Flares, Tearing Modes (Plasmas), Type 4 Bursts

Scientific paper

The possible interplay of tearing, coalescence, and current-driven kinetic instabilities in current sheets is considered on the basis of order of magnitude estimates of instability thresholds and scalings. Arguments are given that favor the development of internal dynamics for current sheets with stationary inflow and appropriate combination of parameters (the impulsive bursty regime of reconnection). The model relates newly emerging flux to flare energy release and provides the basis for an understanding of moving type 4 radio bursts associated with coronal mass ejections.

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