抄録
To use the massively parallel scalar type supercomputer for the large scale numerical magnetospheric simulation, the computational performance of magneto-hydro-dynamic (MHD) code is evaluated. We have made performance tuning of a three-dimensional MHD code for space plasma simulations on the HA8000 with 1024 cores at the University of Tokyo. 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 regular two and three-dimensional decompositions are suitable for HA8000 system. In addition we found the three problems to run the large scale simulation, data I/O, storage system and post processing. To improve them, we can simulate the high resolution Saturn's magnetosphere.
| 元の言語 | 英語 |
|---|---|
| ホスト出版物のタイトル | Proceedings of the 14th IEEE International Conference on High Performance Computing and Communications, HPCC-2012 - 9th IEEE International Conference on Embedded Software and Systems, ICESS-2012 |
| ページ | 976-982 |
| ページ数 | 7 |
| DOI | |
| 出版物ステータス | 出版済み - 12 7 2012 |
| イベント | 14th IEEE International Conference on High Performance Computing and Communications, HPCC-2012 - 9th IEEE International Conference on Embedded Software and Systems, ICESS-2012 - Liverpool, 英国 継続期間: 6 25 2012 → 6 27 2012 |
その他
| その他 | 14th IEEE International Conference on High Performance Computing and Communications, HPCC-2012 - 9th IEEE International Conference on Embedded Software and Systems, ICESS-2012 |
|---|---|
| 国 | 英国 |
| 市 | Liverpool |
| 期間 | 6/25/12 → 6/27/12 |
Fingerprint
All Science Journal Classification (ASJC) codes
- Software
これを引用
Performance of large scale MHD simulation of global planetary magnetosphere with massively parallel scalar type supercomputer including post processing. / Fukazawa, Keiichiro; Nanri, Takeshi.
Proceedings of the 14th IEEE International Conference on High Performance Computing and Communications, HPCC-2012 - 9th IEEE International Conference on Embedded Software and Systems, ICESS-2012. 2012. p. 976-982 6332278.研究成果: 著書/レポートタイプへの貢献 › 会議での発言
}
TY - GEN
T1 - Performance of large scale MHD simulation of global planetary magnetosphere with massively parallel scalar type supercomputer including post processing
AU - Fukazawa, Keiichiro
AU - Nanri, Takeshi
PY - 2012/12/7
Y1 - 2012/12/7
N2 - To use the massively parallel scalar type supercomputer for the large scale numerical magnetospheric simulation, the computational performance of magneto-hydro-dynamic (MHD) code is evaluated. We have made performance tuning of a three-dimensional MHD code for space plasma simulations on the HA8000 with 1024 cores at the University of Tokyo. 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 regular two and three-dimensional decompositions are suitable for HA8000 system. In addition we found the three problems to run the large scale simulation, data I/O, storage system and post processing. To improve them, we can simulate the high resolution Saturn's magnetosphere.
AB - To use the massively parallel scalar type supercomputer for the large scale numerical magnetospheric simulation, the computational performance of magneto-hydro-dynamic (MHD) code is evaluated. We have made performance tuning of a three-dimensional MHD code for space plasma simulations on the HA8000 with 1024 cores at the University of Tokyo. 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 regular two and three-dimensional decompositions are suitable for HA8000 system. In addition we found the three problems to run the large scale simulation, data I/O, storage system and post processing. To improve them, we can simulate the high resolution Saturn's magnetosphere.
UR - http://www.scopus.com/inward/record.url?scp=84870424141&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84870424141&partnerID=8YFLogxK
U2 - 10.1109/HPCC.2012.142
DO - 10.1109/HPCC.2012.142
M3 - Conference contribution
AN - SCOPUS:84870424141
SN - 9780769547497
SP - 976
EP - 982
BT - Proceedings of the 14th IEEE International Conference on High Performance Computing and Communications, HPCC-2012 - 9th IEEE International Conference on Embedded Software and Systems, ICESS-2012
ER -