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tool to be developed during the project; - Experimentally characterize the performance of the membrane-based reciprocating expander coupled to the linear alternator, using compressed air at various
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. The proposed work is thus mainly oriented towards analytical modeling and numerical simulation. The principal numerical tools, a unidirectional pulse propagator and a Maxwell fluid code, are developed at ILM 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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Lyon Website https://www.cnrs.fr/fr https://lbti.ibcp.fr/ Street 7, Passage du Vercors Postal Code 69007 E-Mail catherine.moali@cnrs.fr STATUS: EXPIRED X (formerly Twitter) Facebook LinkedIn Whatsapp
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charge‑transport properties. • Familiarity with codes such as Gaussian, VASP, CRYSTAL, Quantum ESPRESSO, or equivalent. • Ability to collaborate in an interdisciplinary environment and to communicate
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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