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Fig. 1.

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Evolution of quantities on the equatorial plane throughout the selected flux eruption event. The first column illustrates the ratio of vertical magnetic field strength to gas pressure, the second column the magnetization, and the third column their product, σBz2/Pg, used for the identification of magnetic reconnection sites on the equatorial plane. The white and black contours in the first two columns outline the magnetic reconnection sites illustrated in the third column.

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