Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8132340 | Advances in Space Research | 2018 | 8 Pages |
Abstract
This paper introduces the Sheffield Magnetohydrodynamics Algorithm Using GPUs (SMAUG+), an advanced numerical code for solving magnetohydrodynamic (MHD) problems, using multi-GPU systems. Multi-GPU systems facilitate the development of accelerated codes and enable us to investigate larger model sizes and/or more detailed computational domain resolutions. This is a significant advancement over the parent single-GPU MHD code, SMAUG (Griffiths et al., 2015). Here, we demonstrate the validity of the SMAUGâ¯+â¯code, describe the parallelisation techniques and investigate performance benchmarks. The initial configuration of the Orszag-Tang vortex simulations are distributed among 4, 16, 64 and 100â¯GPUs. Furthermore, different simulation box resolutions are applied: 1000Ã1000,2044Ã2044,4000Ã4000 and 8000Ã8000. We also tested the code with the Brio-Wu shock tube simulations with model size of 800 employing up to 10â¯GPUs. Based on the test results, we observed speed ups and slow downs, depending on the granularity and the communication overhead of certain parallel tasks. The main aim of the code development is to provide massively parallel code without the memory limitation of a single GPU. By using our code, the applied model size could be significantly increased. We demonstrate that we are able to successfully compute numerically valid and large 2D MHD problems.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
N. Gyenge, M.K. Griffiths, R. Erdélyi,