WP1: Modeling interacting magnetic loops in the solar corona
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Set of <strong>3D time-dependent MHD simulations</strong><strong> of interacting magnetic structures</strong> in the solar corona using the PLUTO code (Mignone et al. 2007; Mignone et al. 2012). Simulations were performed with different diffusion thresholds to investigate more and more impulsive evolution and higher and higher heating rates. Results will appear in Petralia et al. 2021, in preparation.
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2021-11-03
