index - Maison de la Simulation
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.

Dépôts récents

 

 

Pour toute question : hal@cea.fr

Nombre de documents

291

Nombre de notices

117

Indicateur d'Open Access

86 %

Evolution des dépôts

mots clés

Complex and heterogeneous dynamic system Planets and satellites gaseous planets Interferometers-planets and satellites Laser ISM molecules Approximate Riemann solver Distributed computing Dask Astrochemistry Adaptive optics-instrumentation Electron Planets and satellites composition Two-phase flows Godunov-type scheme Plasma physics Cybersecurity Detection-techniques HPC Methods statistical ISM structure ISM kinematics and dynamics OpenMP High angular resolution Techniques spectroscopic Instrumentation Surface tension Supernovae general Planets and satellites atmospheres AMITEXFFTP Exascale Magnetohydrodynamics Aerodynamics Stars massive Well-balanced property Hyperbolic systems High performance computing GPU computing Exoplanet atmospheres Insider threat Astrophysics - Astrophysics of Galaxies Efficiency FFT Planets and satellites formation Ghost Fluid method Hydrodynamics Asynchronous communication Planets and satellites terrestrial planets Astrophysics - Solar and Stellar Astrophysics Brown dwarfs Geometric multigrid Solvation Planets and satellites interiors Accretion disks Large time steps Numerical simulation Unite and Conquer Methods numerical Calcul haute performance Supercapacitors Big data Gravitational effects Data parallelism Conservation laws Iterative methods Domain decomposition CUDA Infrared planetary systems Turbulence Epidemic Convection Stars formation Water Energy HII regions Accretion ISM clouds High Performance Computing Low-Mach correction Boosting Astrometry Bagging Shallow water equations Parallel computing Compressible two-phase flow Radiative transfer Sparse matrix ISM individual objects Orion B Schrödinger equation 65Y05 Sharp interface Dynamic processes Unite and conquer Planets and satellites fundamental parameters Big data analysis Compressible flows Methods data analysis Ensemble learning Gas dynamics Astrophysics - Earth and Planetary Astrophysics MPI