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Prediction and Modelling of Turbulence based on Machine Learning

JAXA Supercomputer System Annual Report February 2021-January 2022

Report Number: R21EACA39

Subject Category: JSS Inter-University Research

PDF available here

  • Responsible Representative: Masanobu Inubushi, Associate Professor, Tokyo University of Science
  • Contact Information: Masanobu Inubushi(inubushi@rs.tus.ac.jp)
  • Members: Susumu Goto, Masanobu Inubushi, Kensuke Nakatani

Abstract

Turbulence models play essential roles in aerospace science and technology, such as flows around aircraft and of planetary atmospheres. They are rapidly empowered by machine learning methods (Duraisamy, Iaccarino, and Xiao, 2019) and will be a crucial building block of aerospace science and technology in the near future. The present study aims to integrate physics and data-driven methods for turbulence modeling.

Reference URL

Please refer to https://www.rs.tus.ac.jp/~inubushi/ .

Reasons and benefits of using JAXA Supercomputer System

Machine-learning-based predictions and models of turbulence will be necessary for future aerospace science and technology. The reason to use JAXA Supercomputer System is that we can develop these methods based on training data of turbulent flows with high-resolution, numerical calculations requiring a massively parallel supercomputer.

Achievements of the Year

We study the unpredictability of turbulence based on the orbital instability characterized by the Lyapunov exponent and vector. Fig. 1 shows the vortex tubes in turbulent flows in a periodic box (red) and the unstable mode corresponding to the Lyapunov vector (blue). The unstable mode has dipole structures that are localized at the vortex tubes.

Annual Reoprt Figures for 2021

Fig.1: (a) The vortex tubes in the periodic box (red isosurfaces of the enstrophy) and the unstable mode (blue isosurfaces of the enstrophy of the Lyapunov vector). (b) The enlarged figure of (a) and the cross-section.

 

Publications

N/A

Usage of JSS

Computational Information

  • Process Parallelization Methods: MPI
  • Thread Parallelization Methods: OpenMP
  • Number of Processes: 16 - 64
  • Elapsed Time per Case: 30 Hour(s)

JSS3 Resources Used

 

Fraction of Usage in Total Resources*1(%): 0.00

 

Details

Please refer to System Configuration of JSS3 for the system configuration and major specifications of JSS3.

Computational Resources
System Name CPU Resources Used
(Core x Hours)
Fraction of Usage*2(%)
TOKI-SORA 1038.15 0.00
TOKI-ST 0.00 0.00
TOKI-GP 0.00 0.00
TOKI-XM 0.00 0.00
TOKI-LM 0.00 0.00
TOKI-TST 0.00 0.00
TOKI-TGP 0.00 0.00
TOKI-TLM 0.00 0.00

 

File System Resources
File System Name Storage Assigned
(GiB)
Fraction of Usage*2(%)
/home 49.00 0.05
/data and /data2 5320.00 0.06
/ssd 250.00 0.06

 

Archiver Resources
Archiver Name Storage Used
(TiB)
Fraction of Usage*2(%)
J-SPACE 0.00 0.00

*1: Fraction of Usage in Total Resources: Weighted average of three resource types (Computing, File System, and Archiver).

*2: Fraction of Usage:Percentage of usage relative to each resource used in one year.

 

ISV Software Licenses Used

ISV Software Licenses Resources
ISV Software Licenses Used
(Hours)
Fraction of Usage*2(%)
ISV Software Licenses
(Total)
0.00 0.00

*2: Fraction of Usage:Percentage of usage relative to each resource used in one year.

JAXA Supercomputer System Annual Report February 2021-January 2022


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Language / 言語

"Annual Report" available

How to use JSS3

To use JSS3, please refer to "How to use JSS3" page .

Location

Chofu Aerospace Center
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