Numerical simulation of the magnetic reconnection in solar flares.

Details Numerical simulation of the magnetic reconnection in solar flares. Numerical simulation of the magnetic reconnection in solar flares.

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ppmto..18..330f&link_type=abstract

Publ. Purple Mt. Obs., Vol. 18, No. 3, p. 330 - 333

Computer Science

Magnetic Reconnection: Solar Flares, Magnetic Reconnection: Solar X-Ray Flares

Scientific paper

2D magnetic reconnection in solar flares is numerically simulated. The results show that when the reconnection occurs at a high altitude, the evolution can reproduce the main characteristics (such as flaring loop motions and footpoints separation, etc.) of two-ribbon flares; while that with a low reconnection X-point shows a large similarity to compact flares. The results also indicate that there is no direct relation between the rises of soft X-ray loops and the X-point.

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