A 2.5D radiative MHD simulation produces 41 reversals of the reconnection current sheet over 40 periods, with the first 30-minute period attributed to quasi-periodic convective forcing from below the photosphere.
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Numerical simulation of oscillatory magnetic reconnection modulated by solar convective motions
A 2.5D radiative MHD simulation produces 41 reversals of the reconnection current sheet over 40 periods, with the first 30-minute period attributed to quasi-periodic convective forcing from below the photosphere.