An Integrated MPI and OpenMP Approach for Plasma Dynamics Simulations

Plasma dynamics is the behavior exhibited by two or more charged species with respect to electric or magnetic fields. In high-performance computing (HPC) applications, it requires all these factors: the accuracy of parallel implementations, effective inter-process communication, and scalability with...

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Vydané v:2024 International Conference on Computing, Semiconductor, Mechatronics, Intelligent Systems and Communications (COSMIC) s. 42 - 47
Hlavní autori: Prakash, Yellaboina Mani, K, Girish K, Verma, Lalit, Kumar, Shivam, Bhowmik, Biswajit
Médium: Konferenčný príspevok..
Jazyk:English
Vydavateľské údaje: IEEE 22.11.2024
Predmet:
Adaptation models
Computational efficiency
Computational modeling
HCMPI
High performance computing
Load modeling
Mathematical models
MPI
MPI Continuations
MPI_T
OpenMP
Parallel processing
Plasmas
Scalability
TAMPI
Task-based programming models
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Shrnutí:Plasma dynamics is the behavior exhibited by two or more charged species with respect to electric or magnetic fields. In high-performance computing (HPC) applications, it requires all these factors: the accuracy of parallel implementations, effective inter-process communication, and scalability with respect to workload. This paper points out the limitations in the current approaches to the plasma dynamics problems, and discusses the use of MPI continuation tasks and of its performance enhancement with OpenMP methods. Within the framework of the Vlasov-Poisson system, we develop theory of MPI continuation and describe techniques optimal for its use, which allows to efficiently combine communication with computation, which is quite a difficult task in most of the cases, especially in the case of multidimensional simulations. The results allow better insights on how to increase the level of parallelism and reduce the time to compute, which in turn fosters the formulation of more effective high-performance strategies and also the understanding of the parallelism in plasma simulations using the MPI standard.
DOI:10.1109/COSMIC63293.2024.10871490