Introducing electromagnetic effects in Soledge3X

IF 1.3 4区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS Contributions to Plasma Physics Pub Date : 2024-02-20 DOI:10.1002/ctpp.202300147
Raffael Düll, Hugo Bufferand, Eric Serre, Guido Ciraolo, Virginia Quadri, Nicolas Rivals, Patrick Tamain
{"title":"Introducing electromagnetic effects in Soledge3X","authors":"Raffael Düll, Hugo Bufferand, Eric Serre, Guido Ciraolo, Virginia Quadri, Nicolas Rivals, Patrick Tamain","doi":"10.1002/ctpp.202300147","DOIUrl":null,"url":null,"abstract":"In the pedestal region, electromagnetic effects affect the evolution of micro-instabilities and plasma turbulence. The transport code Soledge3X developed by the CEA offers an efficient framework for turbulent 3D simulation on an electrostatic model with a fixed magnetic field. The physical accuracy of the model is improved with electromagnetic induction, driven by the local value of the parallel component of the electromagnetic vector potential <mjx-container aria-label=\"upper A Subscript parallel to\" ctxtmenu_counter=\"0\" ctxtmenu_oldtabindex=\"1\" jax=\"CHTML\" role=\"application\" sre-explorer- style=\"font-size: 103%; position: relative;\" tabindex=\"0\"><mjx-math aria-hidden=\"true\"><mjx-semantics><mjx-mrow><mjx-msub data-semantic-children=\"0,1\" data-semantic- data-semantic-role=\"latinletter\" data-semantic-speech=\"upper A Subscript parallel to\" data-semantic-type=\"subscript\"><mjx-mi data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"italic\" data-semantic- data-semantic-parent=\"2\" data-semantic-role=\"latinletter\" data-semantic-type=\"identifier\"><mjx-c></mjx-c></mjx-mi><mjx-script style=\"vertical-align: -0.177em;\"><mjx-mo data-semantic- data-semantic-parent=\"2\" data-semantic-role=\"neutral\" data-semantic-type=\"fence\" size=\"s\"><mjx-c></mjx-c></mjx-mo></mjx-script></mjx-msub></mjx-mrow></mjx-semantics></mjx-math><mjx-assistive-mml aria-hidden=\"true\" display=\"inline\" unselectable=\"on\"><math altimg=\"/cms/asset/384147f5-9670-4578-83ff-25b62e3a2f39/ctpp202300147-math-0001.png\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><semantics><mrow><msub data-semantic-=\"\" data-semantic-children=\"0,1\" data-semantic-role=\"latinletter\" data-semantic-speech=\"upper A Subscript parallel to\" data-semantic-type=\"subscript\"><mi data-semantic-=\"\" data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"italic\" data-semantic-parent=\"2\" data-semantic-role=\"latinletter\" data-semantic-type=\"identifier\">A</mi><mo data-semantic-=\"\" data-semantic-parent=\"2\" data-semantic-role=\"neutral\" data-semantic-type=\"fence\">∥</mo></msub></mrow>$$ {A}_{\\parallel } $$</annotation></semantics></math></mjx-assistive-mml></mjx-container>, known from Ampère's law. It is solved implicitly in a coupled system with the vorticity equation on the electric potential <mjx-container aria-label=\"normal upper Phi\" ctxtmenu_counter=\"1\" ctxtmenu_oldtabindex=\"1\" jax=\"CHTML\" role=\"application\" sre-explorer- style=\"font-size: 103%; position: relative;\" tabindex=\"0\"><mjx-math aria-hidden=\"true\"><mjx-semantics><mjx-mrow><mjx-mi data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"normal\" data-semantic- data-semantic-role=\"greekletter\" data-semantic-speech=\"normal upper Phi\" data-semantic-type=\"identifier\"><mjx-c></mjx-c></mjx-mi></mjx-mrow></mjx-semantics></mjx-math><mjx-assistive-mml aria-hidden=\"true\" display=\"inline\" unselectable=\"on\"><math altimg=\"/cms/asset/fb20ad0a-7dc8-4bfb-a2fa-e8ac8f5e6142/ctpp202300147-math-0002.png\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><semantics><mrow><mi data-semantic-=\"\" data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"normal\" data-semantic-role=\"greekletter\" data-semantic-speech=\"normal upper Phi\" data-semantic-type=\"identifier\" mathvariant=\"normal\">Φ</mi></mrow>$$ \\Phi $$</annotation></semantics></math></mjx-assistive-mml></mjx-container>. The consequence is a basic electromagnetic behavior in the form of shear Alfvén waves. A finite electron mass prevents unphysical speeds but requires solving for the time evolution of the parallel current density <mjx-container aria-label=\"j Subscript parallel to\" ctxtmenu_counter=\"2\" ctxtmenu_oldtabindex=\"1\" jax=\"CHTML\" role=\"application\" sre-explorer- style=\"font-size: 103%; position: relative;\" tabindex=\"0\"><mjx-math aria-hidden=\"true\"><mjx-semantics><mjx-mrow><mjx-msub data-semantic-children=\"0,1\" data-semantic- data-semantic-role=\"latinletter\" data-semantic-speech=\"j Subscript parallel to\" data-semantic-type=\"subscript\"><mjx-mi data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"italic\" data-semantic- data-semantic-parent=\"2\" data-semantic-role=\"latinletter\" data-semantic-type=\"identifier\"><mjx-c></mjx-c></mjx-mi><mjx-script style=\"vertical-align: -0.177em;\"><mjx-mo data-semantic- data-semantic-parent=\"2\" data-semantic-role=\"neutral\" data-semantic-type=\"fence\" size=\"s\"><mjx-c></mjx-c></mjx-mo></mjx-script></mjx-msub></mjx-mrow></mjx-semantics></mjx-math><mjx-assistive-mml aria-hidden=\"true\" display=\"inline\" unselectable=\"on\"><math altimg=\"/cms/asset/5933078b-9c9b-455b-b54f-23a1b7e2321a/ctpp202300147-math-0003.png\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><semantics><mrow><msub data-semantic-=\"\" data-semantic-children=\"0,1\" data-semantic-role=\"latinletter\" data-semantic-speech=\"j Subscript parallel to\" data-semantic-type=\"subscript\"><mi data-semantic-=\"\" data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"italic\" data-semantic-parent=\"2\" data-semantic-role=\"latinletter\" data-semantic-type=\"identifier\">j</mi><mo data-semantic-=\"\" data-semantic-parent=\"2\" data-semantic-role=\"neutral\" data-semantic-type=\"fence\">∥</mo></msub></mrow>$$ {j}_{\\parallel } $$</annotation></semantics></math></mjx-assistive-mml></mjx-container> in the generalized Ohm's law. This term can be analytically included with little computational overhead in the system on <mjx-container aria-label=\"normal upper Phi\" ctxtmenu_counter=\"3\" ctxtmenu_oldtabindex=\"1\" jax=\"CHTML\" role=\"application\" sre-explorer- style=\"font-size: 103%; position: relative;\" tabindex=\"0\"><mjx-math aria-hidden=\"true\"><mjx-semantics><mjx-mrow><mjx-mi data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"normal\" data-semantic- data-semantic-role=\"greekletter\" data-semantic-speech=\"normal upper Phi\" data-semantic-type=\"identifier\"><mjx-c></mjx-c></mjx-mi></mjx-mrow></mjx-semantics></mjx-math><mjx-assistive-mml aria-hidden=\"true\" display=\"inline\" unselectable=\"on\"><math altimg=\"/cms/asset/c31a20f6-90f8-4fdd-aa4b-a67405911c28/ctpp202300147-math-0004.png\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><semantics><mrow><mi data-semantic-=\"\" data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"normal\" data-semantic-role=\"greekletter\" data-semantic-speech=\"normal upper Phi\" data-semantic-type=\"identifier\" mathvariant=\"normal\">Φ</mi></mrow>$$ \\Phi $$</annotation></semantics></math></mjx-assistive-mml></mjx-container> and <mjx-container aria-label=\"upper A Subscript parallel to\" ctxtmenu_counter=\"4\" ctxtmenu_oldtabindex=\"1\" jax=\"CHTML\" role=\"application\" sre-explorer- style=\"font-size: 103%; position: relative;\" tabindex=\"0\"><mjx-math aria-hidden=\"true\"><mjx-semantics><mjx-mrow><mjx-msub data-semantic-children=\"0,1\" data-semantic- data-semantic-role=\"latinletter\" data-semantic-speech=\"upper A Subscript parallel to\" data-semantic-type=\"subscript\"><mjx-mi data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"italic\" data-semantic- data-semantic-parent=\"2\" data-semantic-role=\"latinletter\" data-semantic-type=\"identifier\"><mjx-c></mjx-c></mjx-mi><mjx-script style=\"vertical-align: -0.177em;\"><mjx-mo data-semantic- data-semantic-parent=\"2\" data-semantic-role=\"neutral\" data-semantic-type=\"fence\" size=\"s\"><mjx-c></mjx-c></mjx-mo></mjx-script></mjx-msub></mjx-mrow></mjx-semantics></mjx-math><mjx-assistive-mml aria-hidden=\"true\" display=\"inline\" unselectable=\"on\"><math altimg=\"/cms/asset/fd5d01fe-6846-4ea0-8797-7956545850e1/ctpp202300147-math-0005.png\" xmlns=\"http://www.w3.org/1998/Math/MathML\"><semantics><mrow><msub data-semantic-=\"\" data-semantic-children=\"0,1\" data-semantic-role=\"latinletter\" data-semantic-speech=\"upper A Subscript parallel to\" data-semantic-type=\"subscript\"><mi data-semantic-=\"\" data-semantic-annotation=\"clearspeak:simple\" data-semantic-font=\"italic\" data-semantic-parent=\"2\" data-semantic-role=\"latinletter\" data-semantic-type=\"identifier\">A</mi><mo data-semantic-=\"\" data-semantic-parent=\"2\" data-semantic-role=\"neutral\" data-semantic-type=\"fence\">∥</mo></msub></mrow>$$ {A}_{\\parallel } $$</annotation></semantics></math></mjx-assistive-mml></mjx-container> and improves its numerical condition, facilitating the iterative solving procedure. Simulations on a periodic slab case let us observe the predicted bifurcation of the wave propagation speed between the Alfvén wave and the electron thermal wave speeds for varying perpendicular wavenumbers. The first results on a circular geometry with a limiter attest to the feasibility of turbulent electromagnetic scenarios.","PeriodicalId":10700,"journal":{"name":"Contributions to Plasma Physics","volume":null,"pages":null},"PeriodicalIF":1.3000,"publicationDate":"2024-02-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Contributions to Plasma Physics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1002/ctpp.202300147","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, FLUIDS & PLASMAS","Score":null,"Total":0}
引用次数: 0

Abstract

In the pedestal region, electromagnetic effects affect the evolution of micro-instabilities and plasma turbulence. The transport code Soledge3X developed by the CEA offers an efficient framework for turbulent 3D simulation on an electrostatic model with a fixed magnetic field. The physical accuracy of the model is improved with electromagnetic induction, driven by the local value of the parallel component of the electromagnetic vector potential , known from Ampère's law. It is solved implicitly in a coupled system with the vorticity equation on the electric potential . The consequence is a basic electromagnetic behavior in the form of shear Alfvén waves. A finite electron mass prevents unphysical speeds but requires solving for the time evolution of the parallel current density in the generalized Ohm's law. This term can be analytically included with little computational overhead in the system on and and improves its numerical condition, facilitating the iterative solving procedure. Simulations on a periodic slab case let us observe the predicted bifurcation of the wave propagation speed between the Alfvén wave and the electron thermal wave speeds for varying perpendicular wavenumbers. The first results on a circular geometry with a limiter attest to the feasibility of turbulent electromagnetic scenarios.
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在 Soledge3X 中引入电磁效应
在基座区域,电磁效应会影响微不稳定性和等离子体湍流的演变。由 CEA 开发的传输代码 Soledge3X 为固定磁场静电模型的湍流三维模拟提供了一个高效框架。该模型的物理精度通过电磁感应得到了提高,电磁感应由电磁矢量势的平行分量 A∥$$ {A}_{\parallel } $$$(由安培定律得知)的局部值驱动。它与电势 Φ$$ \Phi $$ 上的涡度方程隐含在一个耦合系统中求解。其结果是剪切阿尔芬波形式的基本电磁行为。有限的电子质量可以防止非物理速度,但需要求解广义欧姆定律中平行电流密度 j∥$$ {j}_{\parallel } $$$的时间演化。在 Φ$$ \Phi $$ 和 A∥$$ {A}_\{parallel } $$ 上的系统中,可以用很少的计算开销分析包含这个项,并改善其数值条件,促进迭代求解过程。通过对周期板的模拟,我们可以观察到在不同的垂直波数下,阿尔芬波速和电子热波速之间的波速传播预测分岔。在带有限幅器的圆形几何体上得出的第一个结果证明了湍流电磁场景的可行性。
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来源期刊
Contributions to Plasma Physics
Contributions to Plasma Physics 物理-物理:流体与等离子体
CiteScore
2.90
自引率
12.50%
发文量
110
审稿时长
4-8 weeks
期刊介绍: Aims and Scope of Contributions to Plasma Physics: Basic physics of low-temperature plasmas; Strongly correlated non-ideal plasmas; Dusty Plasmas; Plasma discharges - microplasmas, reactive, and atmospheric pressure plasmas; Plasma diagnostics; Plasma-surface interaction; Plasma technology; Plasma medicine.
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