Abstract
We have developed an astrophysical rotating plasma simulator by which we can simulate global dynamics of magnetized rotating plasmas in 2 and 3 dimensions. One of the major applications of this simulator is a differentially rotating disk around a black hole (accretion disk) which is believed to be the central ‘engine’ of active galactic nuclei(AGN) such as quasars. We incorporated nested-grid scheme in order to simulate spacial scale ranging from the observed 100 pc (∼ 1018 m) torus of AGN to the central region of the accretion disk (∼ 1013 m ). By the calculation of 3 CPU vector-parallelized code we get total CPU time of calculation about 1/2 that of non-parallelized code.
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References
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Norman, M. L., Bryan, G. L.: Cosmological adaptive mesh refinement. numa.conf (1999) 19–28
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© 2000 Springer-Verlag Berlin Heidelberg
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Kuwabara, T., Matsumoto, R., Miyaji, S., Nakamura, K. (2000). Implementation of Nested Grid Scheme for Global Magnetohydrodynamic Simulations of Astrophysical Rotating Plasmas. In: Bubak, M., Afsarmanesh, H., Hertzberger, B., Williams, R. (eds) High Performance Computing and Networking. HPCN-Europe 2000. Lecture Notes in Computer Science, vol 1823. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-45492-6_63
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DOI: https://doi.org/10.1007/3-540-45492-6_63
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Online ISBN: 978-3-540-45492-2
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