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(MHD) simulations to model the large-scale flow and particle-in-cell (PIC) simulations to study particle kinetics on microscopic plasma scales. In addition, recent detections of electromagnetic flares in
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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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collaboration with Hospices Civils de Lyon, France. Research activities include: Characterization of nanostructured surfaces Simulating biofilm model/host interactions via a flow cell co-culture system with
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different ice sheet models on comparable topographic configurations, in order to identify sources of uncertainty and possible improvements. 2. Contribute to ISMIP7 Antarctica experiments: carry out