Numerical Simulation of Reconnection Between Emerging Flux and Coronal Field

Details Numerical Simulation of Reconnection Between Emerging Flux and Coronal Field Numerical Simulation of Reconnection Between Emerging Flux and Coronal Field

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..367y&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.367-370.

Physics

3

Scientific paper

Two dimensional resistive MHD numerical simulation is performed for the reconnection between emerging flux and overlying coronal field. Two types of reconnection are investigated. The `two-sided-loop' type occurs when the coronal field is horizontal, and a pair of horizontal hot jets and cool magnetic island ejection is produced. The `anemone-jet' type reconnection occurs when the coronal field is vertical or oblique, and both a vertical hot jet and a cool jet are generated.

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