WP1: Modeling interacting magnetic loops in the solar corona
收藏NIAID Data Ecosystem2026-05-02 收录
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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.
创建时间：
2024-07-17
