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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
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simulations in 3D MHD of the propagation of solar jets, in close connection with solar and in-situ observations. This should lead to the development of the next generation of solar jet propagation models, from
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exciton transport to the reaction center or to a donor-acceptor interface, respectively. Characterizing, modeling and improving exciton transport properties in molecular materials remain essential tasks in
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