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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.
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