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