Abstract
To use the massively parallel scalar type supercomputer for the large scale numerical magnetospheric simulation, we made performance evaluation of a three-dimensional Magnetohydrodynamic (MHD) simulation code for space plasma simulations of planetary magnetosphere on the K computer with 262,144 cores at RIKEN. For parallelization of the MHD code, we use four different methods, i.e., regular one-dimensional, two-dimensional, three-dimensional domain decomposition methods and a cache-hit type of three-dimensional domain decomposition method. We found that the one-dimensional decomposition and cache-hit type of three-dimensional decomposition achieves the best performance and our MHD code can scale over 200,000 processes on the K computer.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
Similar content being viewed by others
References
Chen, F.F.: Introduction to Plasma Physics. Plenum Press, NY (1974)
Top500 Supercomputing Sites, http://www.top500.org/
Fukazawa, K., Umeda, T., Miyoshi, T., Terada, N., Matsumoto, Y., Ogino, T.: Performance measurement of magneto-hydro-dynamic code for space plasma on the various scalar type supercomputer systems. IEEE Trans. Plasma Sci. 38(9), 2254 (2010)
Fukazawa, K., Umeda, T.: Performance measurement of magnetohydrodynamic code for space plasma on the typical scalar type supercomputer systems with the large number of cores. International Journal of High Performance Computing Applications (2012), doi:10.1177/1094342011434813
Oliker, L., Canning, A., Carter, J., Shalf, J., Ethier, S.: Scientific computations on modern parallel vector systems. In: Proc. SC 2004: High Performance Computing, Networking, and Storage Conference (2004)
Ogino, T., Walker, R.J., Ashour-Abdalla, M.: A global magnetohydrodynamic simulation of the magnetopause when the interplanetary magnetic field is northward. IEEE Trans. Plasma Sci. 20, 817–828 (1992)
Fukazawa, K., Ogino, T., Walker, R.J.: A simulation study of dynamics in the distant Jovian magnetotail. J. Geophys. Res. 115, A09219 (2010a), doi:10.1029/2009JA015228
Fukazawa, K., Ogino, T., Walker, R.J.: A Magnetohydrodynamic Simulation Study of Kronian Field-Aligned Currents and Aurora. J. Geophys. Res. (2011) (revised)
Supercomputer K RIKEN Advanced Institute for Computational Science site, http://www.aics.riken.jp/en/
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2013 Springer-Verlag Berlin Heidelberg
About this paper
Cite this paper
Fukazawa, K., Nanri, T., Umeda, T. (2013). Performance Evaluation of Magnetohydrodynamics Simulation for Magnetosphere on K Computer. In: Tan, G., Yeo, G.K., Turner, S.J., Teo, Y.M. (eds) AsiaSim 2013. AsiaSim 2013. Communications in Computer and Information Science, vol 402. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-45037-2_61
Download citation
DOI: https://doi.org/10.1007/978-3-642-45037-2_61
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-45036-5
Online ISBN: 978-3-642-45037-2
eBook Packages: Computer ScienceComputer Science (R0)