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and graduate students each year, including many doctoral students, as well as postdoctoral researchers and visiting scientists. The laboratory covers a wider variety of topics than its name suggests and
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. Their results will be convolved with advanced radiative codes to calculate fluxes and multi-messenger spectra. These simulations will also be supplemented by kinetic simulations of particle acceleration in
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" (ARMS) code, running on high-performance computing centers. The simulation domain will consist of a restricted portion of the solar atmosphere. The doctoral student will have to explore the simulation
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using 3D MHD numerical simulations with the ARMS code. For the first time, such a model will self-consistently generate induced jets in a realistic magnetic topological configuration, including polar