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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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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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bench (optical, electronic and mechanical) and multiphysics analysis using high-performance on-site instruments (optical spectrum analyzer, 3D intensity profile, wavefront, RF spectrum, field polarization
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, organization and structural order, as well as the EE transport dimensionality (2D versus 3D) to push beyond state-of-the-art energy transport lengths in synthetic LH systems. In this context we propose a PhD