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extended complexes) The application to various models of MHD and flows in porous media The numerical analysis of the schemes The development of the computational kernel of the NEMESIS software library
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of very-high-energy gamma-ray sources, in the context of study of magnetic fields in the Milky Way galaxy and in the intergalactic medium. The work will include development of numerical code for modelling
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will be hosted at LCPMR (Sorbonne Université, Paris), in a dynamic scientific environment internationally recognized for its expertise in attoscience, numerical methods, and modeling. The EPAD project
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understanding its internal structure. Interpreting these geophysical data to model planetary structure and dynamics depends on understanding the physical properties of materials under relevant pressure and
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. This data is crucial for improving the numerical models aimed at simulating crystal morphologies and interfacial dynamics, as well as gaining a better understanding of the solidification mechanisms. Where
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. ISTerre is part of the Observatory of Universe Sciences (OSU) at Grenoble Alpes University (UGA), which is responsible for numerous national observation services. This work will be carried out under
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such as Euclid poses many modeling challenges. The COLIBRI ERC aims precisely to develop new theoretical and numerical tools to overcome one of these challenges: baryon modeling. The CDD will have two
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deformation behaviors. This will be supported by numerical simulations developed by the LEM where nanoindentation simulations at the atomic scale will be performed by Molecular Dynamic (MD) as well as finite
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changeYears of Research Experience1 - 4 Additional Information Eligibility criteria Strong background in atmospheric science, ocean–atmosphere interactions, or environmental modeling. • Knowledge of numerical
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data from numerical geodynamo simulations, and to an intercomparison of the several candidate models in an application to the geomagnetic field as seen from satellite observations. These evaluations will