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