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