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Erratum: “RF plugging of multi-mirror machines” [Phys. Plasmas 30, 072510 (2023)] 勘误:"多镜机的射频插接" [Phys. Plasmas 30, 072510 (2023)]
Pub Date : 2024-05-01 DOI: 10.1063/5.0218189
Tal Miller, Ilan Be'ery, Eli Gudinetsky, Ido Barth
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引用次数: 0
Anomalous transport of multi-species edge plasma with the generalized Hasegawa–Wakatani model and the FLR effects 使用广义长谷川-若谷模型和 FLR 效应的多物种边缘等离子体的反常输运
Pub Date : 2024-05-01 DOI: 10.1063/5.0209568
S. Krasheninnikov, R. D. Smirnov
Anomalous transport of multi-species plasma is considered with the generalized Hasegawa–Wakatani model [A. R. Knyazev and S. I. Krasheninnikov, Phys. Plasmas 31, 012502 (2024)] further extended to incorporate the Finite Larmor Radius (FLR) effects. By introducing the “associated” enstrophy, it is shown that with no FLR effects (where anomalous transport of all ion species is described as a transport of passive scalars in the turbulent fields of the electrostatic potential and electron density fluctuations) the fluctuating densities of ion species converge to the state where they are linearly proportional to electron density and vorticity fluctuations, which confirm previous numerical findings of [A. R. Knyazev and S. I. Krasheninnikov, Phys. Plasmas 31, 012502 (2024)]. However, in contrast to the “cold” ion approximation, with the FLR effects included, both the plasma turbulence and the dynamics of all ion species become interconnected. Therefore, for simplicity, the FLR effects in this work were considered only for a small “trace” impurity fraction. It is found that for light (neon) “trace” impurity, the FLR effects reduce both anomalous flux and density fluctuations. However, for heavy (tungsten) “trace” impurity, the FLR effects exhibit non-monotonic impact on anomalous transport.
利用广义长谷川-若谷模型[A. R. Knyazev 和 S. I. Krasheninnikov,Phys. Plasmas 31, 012502 (2024)]考虑了多物种等离子体的反常传输,并进一步扩展以纳入有限拉莫半径(FLR)效应。通过引入 "相关 "熵,结果表明,在没有 FLR 效应的情况下(所有离子种类的反常传输被描述为静电势和电子密度波动湍流场中被动标量的传输),离子种类的波动密度收敛到与电子密度和涡度波动成线性比例的状态,这证实了[A. R. Knyazev 和 S. I. Krasheninnikov,Phys. Plasmas 31, 012502 (2024)]之前的数值发现。然而,与 "冷 "离子近似相反,在包含 FLR 效应的情况下,等离子体湍流和所有离子种类的动力学都变得相互关联。因此,为简单起见,本研究只考虑了 "痕量 "杂质分数较小的 FLR 效应。研究发现,对于轻(氖)"痕量 "杂质,FLR 效应会降低异常通量和密度波动。然而,对于重(钨)"痕量 "杂质,FLR效应对反常传输的影响是非单调的。
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引用次数: 1
On anomalous transport of multi-species plasma associated with the resistive ballooning and resistive drift waves driven turbulence 与阻力气球和阻力漂移波驱动湍流相关的多物种等离子体异常输运问题
Pub Date : 2024-05-01 DOI: 10.1063/5.0209754
S. I. Krasheninnikov
Anomalous transport of multi-species plasma related to the resistive ballooning and resistive drift wave turbulence is considered in a “cold” ion approximation. It is found that similar to the resistive drift wave turbulence [see A. R. Knyazev and S. I. Krasheninnikov, Phys. Plasmas 31, 012502 (2024); and S. I. Krasheninnikov and R. D. Smirnov, Phys. Plasmas (to be published)] the addition of the ballooning drive does not change the main features of anomalous transport of the multi-species plasma: (i) The transport of all ion species is described as a transport of the passive scalars in the turbulent field of the electrostatic potential and electron density perturbation; (ii) the density of ion species with a larger ratio of the mass to charge has the tendency to the accumulation/depletion in the vortices of plasma flow; and (iii) the cross-field transport of all plasma species (including electrons and ions) is described by the same anomalous transport coefficient.
在 "冷 "离子近似中考虑了与电阻气球和电阻漂移波湍流有关的多物种等离子体的异常输运。研究发现,与电阻漂移波湍流类似[见 A. R. Knyazev 和 S. I. Krasheninnikov,Phys. Plasmas 31, 012502 (2024);以及 S. I. Krasheninnikov 和 R. D. Smirnov,Phys.等离子体(待出版)]气球驱动的加入并没有改变多物种等离子体异常输运的主要特征:(i) 所有离子种类的输运都被描述为静电势和电子密度扰动湍流场中被动标量的输运;(ii) 质量与电荷比值较大的离子种类的密度有在等离子体流的漩涡中积累/消耗的趋势;(iii) 所有等离子体种类(包括电子和离子)的跨场输运都用相同的反常输运系数来描述。
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引用次数: 0
Characterization of ECRH plasmas in TOMAS 在 TOMAS 系统中确定 ECRH 等离子体的特征
Pub Date : 2024-05-01 DOI: 10.1063/5.0204690
J. Buermans, A. Adriaens, S. Brezinsek, K. Crombé, N. Desmet, L. Dittrich, A. Goriaev, Y. Kovtun, L. D. López-Rodríguez, P. Petersson, M. Van Schoor
To improve the plasma performance and control the density and plasma quality during the flat top phase, wall conditioning techniques are used in large fusion devices like W7-X and in JT60-SA. To study the performance of electron cyclotron wall conditioning, numerous experiments were performed on the TOroidally MAgnetized System, which is operated by LPP-ERM/KMS at the FZ-Jülich. It is a facility designed to study plasma production, wall conditioning, and plasma–surface interactions. The produced electron cyclotron resonance heating plasmas are characterized in various conditions by density and temperature measurements using a movable triple Langmuir probe in the horizontal and the vertical direction, complemented by video and spectroscopic data, to obtain a 2D extrapolation of the plasma parameters in the machine. A way to calibrate the triple Langmuir probe measurements is also investigated. These data can be used to determine the direction of the plasma drift in the vessel and identify the power absorption mechanisms. This will give more insight in the plasma behavior and improve the efficiency of wall conditioning and sample exposure experiments.
为了提高等离子体性能,控制平顶阶段的密度和等离子体质量,W7-X 和 JT60-SA 等大型聚变装置都采用了壁调节技术。为了研究电子回旋加速器壁调节的性能,在由 LPP-ERM/KMS 在 FZ-Jülich 操作的 TOroidally MAgnetized System 上进行了大量实验。该系统由位于 FZ-Jülich 的 LPP-ERM/KMS 运营,是专为研究等离子体产生、壁调节和等离子体与表面相互作用而设计的设施。通过使用可移动的三朗缪尔探头在水平和垂直方向测量密度和温度,并辅以视频和光谱数据,对产生的电子回旋共振加热等离子体进行各种条件下的表征,从而获得机器中等离子体参数的二维推断。此外,还研究了校准三重朗缪尔探针测量值的方法。这些数据可用于确定容器中等离子体的漂移方向,并确定功率吸收机制。这将使人们对等离子体的行为有更深入的了解,并提高壁调节和样品暴露实验的效率。
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引用次数: 0
Erratum: “Creating and studying a scaled interplanetary coronal mass ejection” [Phys. Plasmas 31, 042901 (2024)] 勘误:"创建并研究按比例的行星际日冕物质抛射" [Phys. Plasmas 31, 042901 (2024)]
Pub Date : 2024-05-01 DOI: 10.1063/5.0213828
K. Bryant, R. P. Young, H. LeFevre, C. Kuranz, J. Olson, K. McCollam, Cameron Kuchta, C. Forest
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引用次数: 0
Directly driven magnetized fast-ignition targets with steep density gradients for inertial fusion energy 用于惯性聚变能的具有陡峭密度梯度的直接驱动磁化快速点火目标
Pub Date : 2024-05-01 DOI: 10.1063/5.0197817
A. B. Sefkow, B. G. Logan, M. Tabak
The development of advanced targets capable of achieving ignition with improved energy gain at lower driver energies is one of four key technical challenges to be solved in order to realize economical inertial fusion energy. We report the minimum energy necessary for a small hemispherical mass of fast-ignited high-density deuterium–tritium fuel to explosively ignite a significantly larger hemispherical mass of assembled cold fuel with much lower mass density, both with and without a flux-compressed magnetic field connecting the two regions. With the magnetic field, the burn rate improves, and lower energy states become more effective. The imploded fuel reservoir available in the lower-density, larger-mass region of the steep density gradient determines whether the fusion yield is several hundred MJ or up to a few GJ. We report a case wherein the cold reservoir ignited and produced high gain with the assistance of only ∼700 kJ of hotspot yield, an amount that has already been demonstrated as feasible in laboratory experiments using indirect-drive targets.
为了实现经济的惯性聚变能,需要解决四个关键技术挑战,其中之一就是开发能够在较低驱动能量下实现点火并获得更高能量的先进靶件。我们报告了一个小半球形的快速点燃高密度氘氚燃料,在连接两个区域的磁通压缩磁场存在和不存在的情况下,爆炸性点燃一个大得多的半球形的质量密度低得多的组装冷燃料所需的最小能量。在有磁场的情况下,燃烧速度会提高,低能量状态也会变得更加有效。在陡峭密度梯度的低密度、大质量区域中可用的内爆燃料库决定了聚变产率是几百兆焦耳还是几千兆焦耳。我们报告了一个案例,在该案例中,冷燃料库仅在 700 kJ 热点产率的帮助下就点燃并产生了高增益,而这一产率已经在使用间接驱动目标的实验室实验中被证明是可行的。
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引用次数: 0
Fluid simulation of atmospheric argon RF dielectric barrier discharges: Role of neutral gas temperature 大气氩射频介质势垒放电的流体模拟:中性气体温度的作用
Pub Date : 2024-05-01 DOI: 10.1063/5.0202078
Ze-Hui Zhang, Ke-Xin Zhong, Yue Liu, Wei Wang, Yi-Nan Wang, De-Zheng Yang
For atmospheric argon RF dielectric barrier discharges, a self-consistent one-dimensional fluid model based on the drift-diffusive approximations of the particles is established to investigate the role of the neutral gas temperature on the discharge process and the plasma characteristics. A finite difference method is used to solve numerically the model, and the numerical results are obtained for the cases that the neutral gas temperature varies from 300 to 600 K. It shows that an increase in the neutral gas temperature causes a decrease in the ionization rate peak and a decrease in the plasma density, but the electric field and the electron temperature do not change very much. Moreover, the discharge mode transition from α mode to α-γ mode occurs because the growing ion flux induces more secondary electron flux, even if the ions entering the sheaths decrease. In addition, the ground state ionization and the ground state excitation are the main collisions in the argon discharges. When metastable atoms are focused on, the three-body quenching is also an important collision progress.
针对大气氩射频介质势垒放电,建立了基于粒子漂移-扩散近似的自洽一维流体模型,以研究中性气体温度对放电过程和等离子体特性的影响。结果表明,中性气体温度升高会导致电离率峰值降低和等离子体密度减小,但电场和电子温度变化不大。此外,放电模式从α模式过渡到α-γ模式的原因是,即使进入鞘的离子减少,但不断增长的离子通量会诱发更多的二次电子通量。此外,基态电离和基态激发是氩放电中的主要碰撞。当聚焦于逸散原子时,三体淬火也是一个重要的碰撞过程。
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引用次数: 0
A numerical study of electron-magnetohydrodynamics tearing modes in parameter ranges of experimental interest 实验参数范围内电子磁流体力学撕裂模式的数值研究
Pub Date : 2024-05-01 DOI: 10.1063/5.0205061
H. Betar, D. Del Sarto, A. Ghizzo, F. Brochard, D. Zarzoso
We perform a numerical study of the linear dynamics of tearing modes in slab incompressible electron-magnetohydrodynamics (EMHD) by considering some parameter ranges, which can be of interest for laboratory plasmas (e.g., helicon devices) or for astrophysics (e.g., solar-wind turbulence). To this purpose, several non-ideal effects are simultaneously retained (finite electron inertia, resistivity, and electron viscosity), and we make distinction between the dissipation coefficients in the direction parallel and perpendicular to the guide field. We thus identify some new reconnection regimes, characterized by a departure from the customary monotonic power-law scalings of the growth rates with respect to the non-ideal parameters. The results here presented can provide a useful indication for future studies of EMHD regimes relevant to experiments and for extensions of the EMHD tearing mode modeling to more complete regimes including kinetic effects (e.g., “electron-only” reconnection in kinetic regimes).
我们通过考虑一些参数范围,对板坯不可压缩电子磁流体力学(EMHD)中撕裂模式的线性动力学进行了数值研究,这些参数范围可能与实验室等离子体(如螺旋装置)或天体物理学(如太阳风湍流)有关。为此,我们同时保留了几种非理想效应(有限电子惯性、电阻率和电子粘性),并区分了平行和垂直于引导场方向的耗散系数。因此,我们发现了一些新的再连接机制,其特点是增长率与非理想参数的关系偏离了习惯的单调幂律标度。这里介绍的结果可以为今后研究与实验相关的电磁流体力学机制以及将电磁流体力学撕裂模式建模扩展到包括动力学效应在内的更完整机制(如动力学机制中的 "纯电子 "再连接)提供有用的指示。
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引用次数: 0
Creating and studying a scaled interplanetary coronal mass ejection 创建和研究按比例的行星际日冕物质抛射
Pub Date : 2024-04-01 DOI: 10.1063/5.0187219
K. Bryant, R. P. Young, H. LeFevre, C. Kuranz, J. Olson, K. McCollam, C. Forest
The Sun, being an active star, undergoes eruptions of magnetized plasma that reach the Earth and cause the aurorae near the poles. These eruptions, called coronal mass ejections (CMEs), send plasma and magnetic fields out into space. CMEs that reach planetary orbits are called interplanetary coronal mass ejections (ICMEs) and are a source of geomagnetic storms, which can cause major damage to our modern electrical systems with limited warning. To study ICME propagation, we devised a scaled experiment using the Big Red Ball (BRB) plasma containment device at the Wisconsin Plasma Physics Laboratory. These experiments inject a compact torus of plasma as an ICME through an ambient plasma inside the BRB, which acts as the interplanetary medium. Magnetic and temperature probes provide three-dimensional magnetic field information in time and space, as well as temperature and density as a function of time. Using this information, we can identify features in the compact torus that are consistent with those in real ICMEs. We also identify the shock, sheath, and ejecta similar to the structure of an ICME event. This experiment acts as a first step to providing information that can inform predictive models, which can give us time to shield our satellites and large electrical systems in the event that a powerful ICME were to strike.
太阳是一颗活跃的恒星,会爆发磁化等离子体,这些等离子体会到达地球,并在两极附近形成极光。这些爆发称为日冕物质抛射(CMEs),将等离子体和磁场送入太空。到达行星轨道的日冕物质抛射被称为行星际日冕物质抛射(ICMEs),它是地磁暴的来源之一,可以在有限的预警下对我们的现代电力系统造成重大破坏。为了研究日冕物质抛射的传播,我们利用威斯康星等离子体物理实验室的大红球(BRB)等离子体遏制装置设计了一个缩放实验。这些实验通过作为行星际介质的大红球内的环境等离子体,注入一个紧凑的等离子体环作为 ICME。磁场和温度探测器提供时间和空间的三维磁场信息,以及温度和密度与时间的函数关系。利用这些信息,我们可以确定紧凑环的特征,这些特征与真实的集成流体动力学事件中的特征一致。我们还确定了与集成流体器事件结构类似的冲击、鞘和喷出物。这项实验是为预测模型提供信息的第一步,它可以让我们有时间在强大的集成流体事件发生时保护我们的卫星和大型电力系统。
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引用次数: 0
Review and meta-analysis of electron temperatures from high-intensity laser–solid interactions 高强度激光与固体相互作用产生的电子温度回顾与荟萃分析
Pub Date : 2024-04-01 DOI: 10.1063/5.0197279
D. Rusby, A. J. Kemp, S. Wilks, K. G. Miller, M. Sherlock, H. Chen, R. Simpson, D. Mariscal, K. Swanson, B. Djordjević, A. J. Link, G. J. Williams, A. J. Mackinnon
The accelerated electron spectrum from high-intensity laser–solid interaction is often conveniently described using a Boltzmann distribution, whose temperature is known within the field as the hot-electron temperature. The importance of the electron temperature is highlighted by the sheer number of experimental and simulation studies on the subject over the past three decades. Recently, multi-kJ, multi-ps pulses have yielded electron spectra with temperatures far beyond the expected ponderomotive result. Expressions that predict the electron temperature considering laser parameters beyond intensity and wavelength have been developed, albeit using small datasets. In this review, we present what is, to the best of our knowledge, the largest dataset of electron temperatures gathered from experimental measurements and particle-in-cell simulations. This dataset allows us to compare existing analytical and empirical hot-electron temperature scaling models over a wide parameter range. We also develop new scaling models that incorporate the laser pulse duration of the laser and the plasma scale length. Three models that include pulse-duration and scale length dependence are especially successful at predicting both simulated and experimental data. The dataset will soon be made publicly available to encourage further investigation.
高强度激光与固体相互作用产生的加速电子能谱通常使用波尔兹曼分布进行描述,其温度在该领域被称为热电子温度。在过去的三十年中,有关这一主题的实验和模拟研究数量之多,凸显了电子温度的重要性。最近,多kJ、多ps脉冲产生的电子能谱温度远远超出了预期的思脉冲结果。尽管使用的数据集较小,但考虑到激光强度和波长之外的参数,预测电子温度的表达式已经被开发出来。在这篇综述中,我们介绍了据我们所知从实验测量和粒子池模拟中收集到的最大电子温度数据集。通过这个数据集,我们可以在很宽的参数范围内比较现有的分析和经验热电子温度比例模型。我们还开发了包含激光脉冲持续时间和等离子体尺度长度的新比例模型。包含脉冲持续时间和尺度长度依赖性的三个模型在预测模拟和实验数据方面都特别成功。数据集不久将公开发布,以鼓励进一步的研究。
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引用次数: 0
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Physics of Plasmas
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