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Extending stability beyond CPU millennium: a micron-scale atomistic simulation of Kelvin-Helmholtz instability
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Conference on High Performance Networking and Computing archive
Proceedings of the 2007 ACM/IEEE conference on Supercomputing - Volume 00 table of contents
Reno, Nevada
SESSION: Gordon Bell prize finalists table of contents
Article No. 58  
Year of Publication: 2007
ISBN:978-1-59593-764-3
Authors
J. N. Glosli  Lawrence Livermore National Laboratory, Livermore, CA
D. F. Richards  Lawrence Livermore National Laboratory, Livermore, CA
K. J. Caspersen  Lawrence Livermore National Laboratory, Livermore, CA
R. E. Rudd  Lawrence Livermore National Laboratory, Livermore, CA
J. A. Gunnels  IBM Corporation, Yorktown Heights, New York
F. H. Streitz  Lawrence Livermore National Laboratory, Livermore, CA
Sponsors
IEEE-CS\DATC : IEEE Computer Society
ACM: Association for Computing Machinery
Publisher
ACM  New York, NY, USA
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ABSTRACT

We report the computational advances that have enabled the first micron-scale simulation of a Kelvin-Helmholtz (KH) instability using molecular dynamics (MD). The advances are in three key areas for massively parallel computation such as on BlueGene/L (BG/L): fault tolerance, application kernel optimization, and highly efficient parallel I/O. In particular, we have developed novel capabilities for handling hardware parity errors and improving the speed of interatomic force calculations, while achieving near optimal I/O speeds on BG/L, allowing us to achieve excellent scalability and improve overall application performance. As a result we have successfully conducted a 2-billion atom KH simulation amounting to 2.8 CPU-millennia of run time, including a single, continuous simulation run in excess of 1.5 CPU-millennia. We have also conducted 9-billion and 62.5-billion atom KH simulations. The current optimized ddcMD code is benchmarked at 115.1 TFlop/s in our scaling study and 103.9 TFlop/s in a sustained science run, with additional improvements ongoing. These improvements enabled us to run the first MD simulations of micron-scale systems developing the KH instability.


REFERENCES

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Collaborative Colleagues:
J. N. Glosli: colleagues
D. F. Richards: colleagues
K. J. Caspersen: colleagues
R. E. Rudd: colleagues
J. A. Gunnels: colleagues
F. H. Streitz: colleagues