Dynamics of the physical state during two-current-loop collisions

Details Dynamics of the physical state during two-current-loop collisions Dynamics of the physical state during two-current-loop collisions

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..145..297c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 145, no. 2, p. 297-315.

Physics

18

Coronal Loops, Solar Atmosphere, Solar Flares, Solar Magnetic Field, Electric Fields, Magnetohydrodynamics, Pressure Gradients, Stellar Models

Scientific paper

The time evolution of physical quantities during complete and partial magnetic reconnections was investigated. A model of two-current-loop collisions is presented as an explanation of the impulsive nature of solar flares. Self-consistent expressions and a set of equations governing the behavior of physical properties just after magnetic reconnection were derived from magnetohydrodynamic equations. The model geometry of loop-loop interaction is presented and the theoretical model of loop interaction is developed. The results of numerical simulations are presented and discussed. Results indicate that direct collisions provide a more rapid pinch and stronger enhancement of physical properties but has no influence on jet production.

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