WP1: Modeling interacting magnetic loops in the solar corona
Authors/Creators
- 1. INAF Osservatorio Astronomico di Palermo
- 2. UNIPA Dipartimento Fisica e Chimica
Description
Set of 3D time-dependent MHD simulations of interacting magnetic structures 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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