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Cluster IT90_0 data at z=0
3-D distribution of gas density, dark matter density, temperature, and 3-components of velocity field for cluster IT90_0 (relaxed) at z=0, simulated with the ENZO code (Bryan... -
Simulated radio relics
Fits datacube of 256 x 256 pixels and 100 frequency channels, for the simulated synchrotron radio emission from a galaxy cluster at z=0.05. Each pixel is 34 kpc, and has values... -
Initial conditions for pre-merger cluster simulation with ENZO
Initial conditions for ENZO (enzo-project.org) AMR simulations of a pair of massive clusters in an early merger stage. Nested initial conditions are needed to produce 2 sets of... -
Background Data for: UAV Icing: Aerodynamic Degradation Caused by Intercycle ...
This dataset contains geometries, simulations results, and experimental results used in the paper "UAV Icing: Aerodynamic Degradation Caused by Intercycle and Runback Ice Shapes... -
Toward an explanatory parameter space for sediment trapping in estuaries
In the context of the CAPTURE project, idealized numerical simulations have been carried out with the width-averaged modeling framework iFlow v3.0. These numerical simulations... -
COM3D: Turbulent Combustion Code User’s Guides
COM3D is a three-dimensional code for turbulent reactive flow simulations in complex 3D-geometries. The Favre averaged Navier-Stokes equations are solved together with different...
