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