Numerical study on the flaring loop dynamics.

Computer Science

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Solar Flares: Numerical Simulations, Solar Flares: Magnetic Reconnection

Scientific paper

Numerical simulations are performed to study the flaring loop dynamics during magnetic reconnection. Two models are considered with different reconnection point heights. In the model with high reconnection point, the results can reproduce the loop motions in the two-ribbon flares, while in the model with low reconnection point, the evolution shows a large similarity to the compact flares. It implies that the two types of solar flares could be unified into the same model, where the height of the reconnection point leads to the bifurcation.

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