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Validation Study On Upwinding Schemes For Core MHD/Turbulent Simulation

https://repo.qst.go.jp/records/54880
https://repo.qst.go.jp/records/54880
4e429189-5dcc-4b8d-9e07-4b485be2c31b
Item type 会議発表論文 / Conference Paper(1)
公開日 2018-04-15
タイトル
タイトル Validation Study On Upwinding Schemes For Core MHD/Turbulent Simulation
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_5794
資源タイプ conference paper
アクセス権
アクセス権 metadata only access
アクセス権URI http://purl.org/coar/access_right/c_14cb
著者 瀬戸, 春樹

× 瀬戸, 春樹

WEKO 561186

瀬戸, 春樹

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矢木, 雅敏

× 矢木, 雅敏

WEKO 561187

矢木, 雅敏

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瀬戸 春樹

× 瀬戸 春樹

WEKO 561188

en 瀬戸 春樹

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矢木 雅敏

× 矢木 雅敏

WEKO 561189

en 矢木 雅敏

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内容記述タイプ Abstract
内容記述 The validity of upwinding schemes for core MHD/turbulent simulation is numerically investigated by the used of a fully linearized 3-field resistive ballooning mode (RBM) model with three different discretiza- tion schemes on a convective derivative, (1) 4th order central differential (C4), (2) 4th order linear upwinding scheme (U4), (3) 3rd order weighted essentially non-oscillatory (WENO) scheme (W3). The simulations reveal that, in the cases with U4 and W3, the temporally varying upwinding direction can be unphysical nonlinear energy channels among toroidal modes and drive unphysical mode transitions even if the equation system is fully linearized theoretically. On the other hand, growth rates and eigen functions of RBM are conserved over the simulation time in the case with C4. These result show that any upwinding scheme should not be employed in the core region where nonlinear wave couplings described by convective derivatives such as the ExB flow term and the magnetic fluttering term are the fundamental nature of plasma instability and turbulence.
書誌情報 International Conference Proceedings of MC2017

発行日 2017-04
出版者
出版者 Korean Nuclear Society
関連サイト
識別子タイプ URI
関連識別子 https://www.kns.org/paper_file/paper/MC2017_2017_11/P384S11-01SetoH.pdf
関連名称 https://www.kns.org/paper_file/paper/MC2017_2017_11/P384S11-01SetoH.pdf
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