Compressing the time series of five dimensional distribution function data from gyrokinetic simulation using principal component analysis

Yuuichi Asahi, Keisuke Fujii, Dennis Manuel Heim, Shinya Maeyama, Xavier Garbet, Virginie Grandgirard, Yanick Sarazin, Guilhem Dif-Pradalier, Yasuhiro Idomura, Masatoshi Yagi

Research output: Contribution to journalArticlepeer-review

6 Scopus citations

Abstract

Phase space structures are extracted from the time series of five dimensional distribution function data computed by the flux-driven full-f gyrokinetic code GT5D. Principal component analysis (PCA) is applied to reduce the dimensionality and the size of the data. Phase space bases in (φ, v ≈, w) and the corresponding spatial coefficients (poloidal cross section) are constructed by PCA, where φ, v ≈, and w, respectively, mean the toroidal angle, the parallel velocity, and the perpendicular velocity. It is shown that 83% of the variance of the original five dimensional distribution function can be expressed with 64 principal components, i.e., the compression of the degrees of freedom from 1.3 × 1 0 12 to 1.4 × 10 9. One of the important findings - resulting from the detailed analysis of the contribution of each principal component to the energy flux - deals with avalanche events, which are found to be mostly driven by coherent structures in the phase space, indicating the key role of resonant particles. Another advantage of the proposed analysis is the decoupling of 6D (1D time and 5D phase space) data into the combinations of 3D data which are visible to the human eye.

Original languageEnglish
Article number012304
JournalPhysics of Plasmas
Volume28
Issue number1
DOIs
StatePublished - Jan 1 2021
Externally publishedYes

Funding

This work has been carried out using the JFRS-1 supercomputer system at the Computational Simulation Centre of International Fusion Energy Research Centre (IFERC-CSC) in Rokkasho Fusion Institute of QST (Aomori, Japan). The author Y.A. thank Dr. T.-H. Watanabe and Dr. N. Aiba for the fruitful discussions about the phase space dynamics. The author Y.A. also thanks the IFERC-CSC support team for the Dask usage and keeping my large amount of simulation data above 5 Peta Byte. This work has been supported by JHPCN project Nos. jh190065-NAHI and jh200053-MDHI, the MEXT Japan (Program for Promoting Researches on the Supercomputer Fugaku “Exploration of Burning Plasma Confinement Physics,” No. hp200127) and MEXT Japan, Grant No. 20K14441. This work has also received funding from NINS program No. 01111905, the grant of Joint Research by the National Institutes of Natural Sciences (NINS). This work has been carried out using the JFRS-1 supercomputer system at the Computational Simulation Centre of International Fusion Energy Research Centre (IFERC-CSC) in Rokkasho Fusion Institute of QST (Aomori, Japan). The author Y.A. thank Dr. T.-H. Watanabe and Dr. N. Aiba for the fruitful discussions about the phase space dynamics. The author Y.A. also thanks the IFERC-CSC support team for the Dask usage and keeping my large amount of simulation data above 5 Peta Byte. This work has been supported by JHPCN project Nos. jh190065-NAHI and jh200053-MDHI, the MEXT Japan (Program for Promoting Researches on the Supercomputer Fugaku "Exploration of Burning Plasma Confinement Physics," No. hp200127) and MEXT Japan, Grant No. 20K14441. This work has also received funding from NINS program No. 01111905, the grant of Joint Research by the National Institutes of Natural Sciences (NINS).

FundersFunder number
Exploration of Burning Plasma Confinement Physics20K14441, hp200127
IFERC-CSC
International Fusion Energy Research Centre
JHPCN
Rokkasho Fusion Institute of QST
Ministry of Education, Culture, Sports, Science and Technology
National Institutes of Natural Sciences01111905

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