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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
275
Nombre de notices
117
Indicateur d'Open Access
85 %
Evolution des dépôts
mots clés
Asynchronous communication
Techniques spectroscopic
Linear algebra
Large time steps
Conservation laws
Sparse matrix
Astrophysics - Astrophysics of Galaxies
Low-Mach correction
Water
Accretion disks
GPU computing
Infrared planetary systems
HPC
High angular resolution
Adaptive optics-instrumentation
Parallel computing
Calcul haute performance
Planets and satellites composition
ISM clouds
Hyperbolic systems
Sharp interface
Big data
CUDA
Approximate Riemann solver
Planets and satellites atmospheres
Schrödinger equation
Geometric multigrid
Supercapacitors
Astrophysics - Earth and Planetary Astrophysics
Detection-techniques
Epidemic
Astrochemistry
Two-phase flows
Aerodynamics
Gravitational effects
Level-Set
Dask
Planets and satellites interiors
Low Mach correction
FFT
Dynamic processes
Radiative transfer
Insider threat
High performance computing
Shallow water equations
Instrumentation
Plasma physics
Efficiency
Boosting
Surface tension
Complex and heterogeneous dynamic system
Planets and satellites gaseous planets
Data parallelism
ISM structure
Turbulence
Domain decomposition
Ensemble learning
Astrophysics - Solar and Stellar Astrophysics
Compressible two-phase flow
Supernovae general
ISM kinematics and dynamics
Accretion
Unite and Conquer
Gas dynamics
65Y05
Stars massive
Methods numerical
Planets and satellites formation
Electron
Hydrodynamics
ISM molecules
Big data analysis
Astrometry
Brown dwarfs
Low Froude
Godunov-type scheme
Methods data analysis
Well-balanced property
Energy
AMITEXFFTP
Stars formation
Unite and conquer
Ghost Fluid method
Exascale
Iterative methods
Solvation
Interferometers-planets and satellites
HII regions
ISM individual objects Orion B
Cybersecurity
MPI
OpenMP
Laser
Planets and satellites fundamental parameters
Magnetohydrodynamics
Linear systems
Methods statistical
Convection
Bagging
High Performance Computing