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