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Performance of Adaptive Mesh Refinement Scheme for Hydrodynamics on Simulations of Expanding Supernova Envelope

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Book cover High Performance Computing (ISHPC 2002)

Part of the book series: Lecture Notes in Computer Science ((LNCS,volume 2327))

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Abstract

We present results of performance measurement of our astrophysical fluid dynamics code with Adaptive Mesh Refinement (AMR) scheme. As an example of its application for astrophysical phenomena, we show the results of 3D simulation of Rayleigh-Taylor instability in expanding supernova envelope and the possibility of reconciliation of the present model with observations. The efficiency of memory and CPU-time savings is discussed and measured with this simulation. Its result shows that our code has the ability to simulate phenomena with wide dynamic ranges even in limited computing resources.

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Author information

Authors and Affiliations

  1. Graduate School of Science and Technology, Chiba University, Japan

    Ayato Noro, Tomoya Ogawa & Shigeki Miyaji

  2. Morioka Local Meteorological Observatory, Morioka, Japan

    Takuma Ohta

  3. Institute of Media and Information Technology, Chiba University, Japan

    Kazuyuki Yamashita

  4. Communications Research Laboratory, Japan

    Mitue Den

Authors
  1. Ayato Noro
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  2. Tomoya Ogawa
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  3. Takuma Ohta
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  4. Kazuyuki Yamashita
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  5. Shigeki Miyaji
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  6. Mitue Den
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Editor information

Editors and Affiliations

  1. Institute of Software Science, University of Vienna, Liechtensteinstr. 22, 1090, Vienna, Austria

    Hans P. Zima

  2. Department of Information and Computer Science, Nara Women’s University, Kitauoyanishimachi, Nara City, 630-8506, Japan

    Kazuki Joe

  3. Institute of Information Science and Electronics, University of Tsukuba, Tenno-dai 1-1-1, Tsukuba, Ibaraki, 305-8577, Japan

    Mitsuhisa Sato

  4. Internet Systems Research Laboratories, NEC Corporation, 4-1-1, Miyazaki, Miyamae, Kawasaki, Kanagawa, 216-8555, Japan

    Yoshiki Seo

  5. Kyoto University, Yoshidahonmachi, Sakyo-ku, Kyoto, 606-8501, Japan

    Masaaki Shimasaki

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© 2002 Springer-Verlag Berlin Heidelberg

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Noro, A., Ogawa, T., Ohta, T., Yamashita, K., Miyaji, S., Den, M. (2002). Performance of Adaptive Mesh Refinement Scheme for Hydrodynamics on Simulations of Expanding Supernova Envelope. In: Zima, H.P., Joe, K., Sato, M., Seo, Y., Shimasaki, M. (eds) High Performance Computing. ISHPC 2002. Lecture Notes in Computer Science, vol 2327. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-47847-7_18

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  • DOI: https://doi.org/10.1007/3-540-47847-7_18

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-43674-4

  • Online ISBN: 978-3-540-47847-8

  • eBook Packages: Springer Book Archive

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