In this white paper we report our experiences in porting the stellar atmosphere simulation code Bifrost to Intel Xeon Phi - Knights Landing Architecture (KNL). Bifrost is a parallel, Fortran 95/MPI code for solving the 3D radiation magnetohydrodynamic (RMHD) equations on a staggered grid using a high order compact finite difference scheme. The focus is on finding the most performant runtime setup and estimate possible performance gain when compared with Intel Haswell based nodes
With at least 60 processing cores, the Xeon-Phi coprocessor is a truly multicore architecture, which...
The Knights Landing (KNL) release of the Intel Many Integrated Core (MIC) Xeon Phi line of processor...
ii This thesis describes the building of two Beowulf clusters in a grid computing environment and pa...
Context. Numerical simulations of stellar convection and photospheres have been developed to the poi...
Context. Numerical simulations of stellar convection and photospheres have been developed to the poi...
Context. Numerical simulations of stellar convection and photospheres have been developed to the poi...
In this work an astrophysical simulation code, XFLAT, is developed to study neutrino oscillations in...
Three dimensional particle-in-cell laser-plasma simulation is an important area of computational phy...
The subject of this project is the analysis and enabling of the RayBen code, which implements a fini...
We consider an interesting from computational point of view standing wave simulation by solving coup...
This is the final report of our NASA AISRP grant entitled 'High Performance Parallel Methods for Spa...
Partial Differential Equations (PDEs) are widely used to simulate many scenarios in science and engi...
We developed a data parallel code written in High Performance Fortran for simulating magnetized flui...
The whitepaper reports our investigation into the porting, optimization and subsequent performance o...
The Knights Landing (KNL) release of the Intel Many Integrated Core (MIC) Xeon Phi line of processor...
With at least 60 processing cores, the Xeon-Phi coprocessor is a truly multicore architecture, which...
The Knights Landing (KNL) release of the Intel Many Integrated Core (MIC) Xeon Phi line of processor...
ii This thesis describes the building of two Beowulf clusters in a grid computing environment and pa...
Context. Numerical simulations of stellar convection and photospheres have been developed to the poi...
Context. Numerical simulations of stellar convection and photospheres have been developed to the poi...
Context. Numerical simulations of stellar convection and photospheres have been developed to the poi...
In this work an astrophysical simulation code, XFLAT, is developed to study neutrino oscillations in...
Three dimensional particle-in-cell laser-plasma simulation is an important area of computational phy...
The subject of this project is the analysis and enabling of the RayBen code, which implements a fini...
We consider an interesting from computational point of view standing wave simulation by solving coup...
This is the final report of our NASA AISRP grant entitled 'High Performance Parallel Methods for Spa...
Partial Differential Equations (PDEs) are widely used to simulate many scenarios in science and engi...
We developed a data parallel code written in High Performance Fortran for simulating magnetized flui...
The whitepaper reports our investigation into the porting, optimization and subsequent performance o...
The Knights Landing (KNL) release of the Intel Many Integrated Core (MIC) Xeon Phi line of processor...
With at least 60 processing cores, the Xeon-Phi coprocessor is a truly multicore architecture, which...
The Knights Landing (KNL) release of the Intel Many Integrated Core (MIC) Xeon Phi line of processor...
ii This thesis describes the building of two Beowulf clusters in a grid computing environment and pa...