MY13 showed the change in the sense of global mean and the subsequent paper, and MY15 clarified the different convection aspects between the main cloud disturbances under the highest resolution simulation only.
ABSTRACT: We present the results from recent ultra-high resolution simulations of star-formation in the early universe.
We have applied ANTARES in order to obtain high resolution simulations of solar granulation which we describe and analyze.
This model allows for high resolution simulations of ion-temperature-gradient-driven turbulence using realistic plasma parameters assuming locality of the turbulent fluctuations.
A massively parallel high performance computational platform (a 1200 processor IBM SP-2) was used to conduct three-dimensional, high resolution simulations to ascertain the spatial variability to be expected during a monitoring period.
Importantly, the AL model is fully coupled to an existing GPU based computational fluid dynamic solver, enabling high resolution simulations in reasonable time frames using desktop size server systems.
Due to the absence of hydrodynamic instabilities behind the main front of regular structure detonations, the results obtained by solving the Euler equations and Navier Stokes equations are similar for detonations with regular structure even in high resolution simulations.
This paper reports high resolution simulations using a fifth-order weighted essentially non-oscillatory (WENO) scheme with a third-order TVD Runge Kutta time stepping method to examine the features of detonation front and physics in square ducts.
