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