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the physics of particle acceleration in highly magnetized (relativistic) turbulence under conditions similar to those of the above sources. Particular attention will be paid to the nonlinear back
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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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., providing initial and boundary conditions). In particular, the thesis will benefit from the use of the CNRS-INSU THEMIS telescope, a 1-meter-class optical solar telescope, dedicated to the study of solar
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