Bienvenue sur la collection HAL de la Maison de la Simulation, laboratoire commun au CEA, au CNRS, à l'Université Paris-Saclay et à l'Université Versailles Saint-Quentin. Elle est spécialisée dans le calcul haute performance et les simulations numériques en lien étroit avec les applications physiques, le génie logiciel parallèle, les modèles de programmation, les techniques de visualisation, l'intelligence artificielle et l'informatique quantique.

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Pour toute question : hal@cea.fr

Nombre de documents

291

Nombre de notices

116

Indicateur d'Open Access

86 %

Evolution des dépôts

mots clés

Gas dynamics Domain decomposition in space method Bagging ISM structure AMITEXFFTP Ensemble learning ISM clouds Astrophysics - Earth and Planetary Astrophysics MPI Aerodynamics Planets and satellites terrestrial planets Adaptive optics-instrumentation Solvation ISM kinematics and dynamics FFT Brown dwarfs Astrophysics - Solar and Stellar Astrophysics Stars formation Astrometry Techniques spectroscopic ISM molecules Planets and satellites atmospheres Iterative methods Radiative transfer ISM individual objects Orion B Asynchronous communication Calcul haute performance OpenMP Surface tension Efficiency Complex and heterogeneous dynamic system Laser Detection-techniques Plasma physics Turbulence Supercapacitors Conservation laws Epidemic Big data Astrochemistry HPC Big data analysis Gravitational effects Planets and satellites interiors Interferometers-planets and satellites Hyperbolic systems Instrumentation Parallel computing Numerical simulation Sparse matrix Compressible two-phase flow Exoplanet atmospheres Infrared planetary systems Dask Dynamic processes Sharp interface Planets and satellites fundamental parameters Magnetohydrodynamics Convection Planets and satellites formation Methods data analysis High angular resolution CUDA GPU computing Compressible flows Data parallelism Well-balanced property Boosting Cybersecurity Methods numerical Water Exascale Planets and satellites gaseous planets High performance computing Supernovae general High Performance Computing Accretion disks Low-Mach correction Unite and conquer Domain decomposition Hydrodynamics Approximate Riemann solver Accretion Planets and satellites composition HII regions Schrödinger equation Methods statistical Two-phase flows Stars massive Electron Distributed computing Godunov-type scheme Ghost Fluid method Shallow water equations Unite and Conquer Insider threat Geometric multigrid Energy Large time steps Astrophysics - Astrophysics of Galaxies