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Global characterization of a laser-generated neutron source 激光产生的中子源的总体特征
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-06-03 DOI: 10.1017/s0022377824000618
D.P. Higginson, R. Lelièvre, L. Vassura, M.M. Gugiu, M. Borghesi, L.A. Bernstein, D. L. Bleuel, B. L. Goldblum, A. Green, F. Hannachi, S. Kar, S. Kisyov, L. Quentin, M. Schroer, M. Tarisien, O. Willi, P. Antici, F. Negoita, A. Allaoua, J. Fuchs

Laser-driven neutron sources are routinely produced by the interaction of laser-accelerated protons with a converter. They present complementary characteristics to those of conventional accelerator-based neutron sources (e.g. short pulse durations, enabling novel applications like radiography). We present here results from an experiment aimed at performing a global characterization of the neutrons produced using the Titan laser at the Jupiter Laser Facility (Livermore, USA), where protons were accelerated from 23 $mathrm {mu }$m thick plastic targets and directed onto a LiF converter to produce neutrons. For this purpose, several diagnostics were used to measure these neutron emissions, such as CR-39, activation foils, time-of-flight detectors and direct measurement of $^7{rm Be}$ residual activity in the LiF converters. The use of these different, independently operating diagnostics enables comparison of the various measurements performed to provide a robust characterization. These measurements led to a neutron yield of $2.0times 10^{9}$ neutrons per shot with a modest angular dependence, close to that simulated.

激光驱动中子源是激光加速质子与转换器相互作用产生的常规中子源。与传统的加速器中子源相比,激光驱动中子源具有互补的特点(如脉冲持续时间短,可用于射线照相等新型应用)。我们在此介绍一项实验的结果,该实验的目的是对木星激光设施(美国利弗莫尔)使用泰坦激光器产生的中子进行全面鉴定,在该实验中,质子从23 $mathrm {mu }$m厚的塑料靶加速,并被引导到LiF转换器上产生中子。为此,使用了几种诊断方法来测量这些中子发射,如 CR-39、活化箔、飞行时间探测器和直接测量 LiF 转换器中的 $^7{rm Be}$ 残余活动。通过使用这些不同的、独立运行的诊断方法,可以对所进行的各种测量进行比较,从而提供可靠的特征描述。这些测量结果表明,每次发射的中子产率为 10^{9}$ 中子的 2.0 倍,角度依赖性不大,接近模拟产率。
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引用次数: 0
Development of a field-reversed configuration device using radio frequency antennas to produce E × B for current-drive 利用射频天线开发场逆配置装置,为电流驱动产生 E × B
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-05-22 DOI: 10.1017/s0022377824000643
Kiyong Lee, Soo Ouk Jang, Seungryul Yoo, Kyu Dong Lee
A unique field-reversed configuration (FRC) experiment is presently being assembled at the Plasma Technology Research Institute, KFE. It is a compact small-scale FRC device, which uses a set of radio frequency (RF) antennas to produce an internal E × B that drives the electrons for current-drive, in which E is the electric field and B is the magnetic field. This is very similar to the rotating magnetic field (RMF) current-drive, where the horizontal and vertical antennas are driven 90° out of phase. For this device, the RF antennas are arranged differently than the RMF. The RF antennas, being two separate sets, are positioned inside the vacuum chamber. Each set consists of 8 coils, for a total of 16 coils, where 80~100 kHz sine and cosine waveform currents are applied. One set of coils generates a radial B-field, while the other set provides an E-field in the z-direction. As the phase changes, the E and B fields are switched by these two sets. Nevertheless, E × B propagates in the same θ-direction so that this allows the electrons to rotate around the circumference of the device. The FRC device will test wave heating by launching 2.45 GHz microwaves. Also, passive stabilizers are positioned at each end to provide extra stability while preventing tilt instability. The experiment is expected to produce its first plasma in 2025.
目前,KFE 等离子体技术研究所正在组装一个独特的场反转配置(FRC)实验。这是一个紧凑的小型 FRC 设备,它使用一组射频(RF)天线产生内部 E × B,驱动电子进行电流驱动,其中 E 是电场,B 是磁场。这与旋转磁场(RMF)电流驱动非常相似,其中水平和垂直天线的驱动相位相差 90°。对于这种装置,射频天线的布置方式与 RMF 不同。射频天线分为两组,分别放置在真空室内。每组由 8 个线圈组成,共 16 个线圈,施加 80~100 kHz 正弦和余弦波形电流。一组线圈产生径向 B 场,另一组提供 Z 方向的 E 场。随着相位的变化,E 场和 B 场由这两组线圈切换。尽管如此,E × B 仍沿相同的 θ 方向传播,从而使电子能够围绕装置的圆周旋转。FRC 设备将通过发射 2.45 GHz 微波来测试波加热。此外,两端还安装了被动稳定器,以提供额外的稳定性,同时防止倾斜不稳定性。该实验预计将于 2025 年产生第一个等离子体。
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引用次数: 0
Coil optimization for quasi-helically symmetric stellarator configurations 准对称恒星器配置的线圈优化
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-05-22 DOI: 10.1017/s0022377824000540
A. Wiedman, S. Buller, M. Landreman
Filament-based coil optimizations are performed for several quasi-helical stellarator configurations, beginning with the one from Landreman & Paul (Phys. Rev. Lett., vol. 128, 2022, 035001), demonstrating that precise quasi-helical symmetry can be achieved with realistic coils. Several constraints are placed on the shape and spacing of the coils, such as low curvature and sufficient plasma–coil distance for neutron shielding. The coils resulting from this optimization have a maximum curvature 0.8 times that of the coils of the Helically Symmetric eXperiment (HSX) and a mean squared curvature 0.4 times that of the HSX coils when scaled to the same plasma minor radius. When scaled up to reactor size and magnetic field strength, no fast particle losses were found in the free-boundary configuration when simulating 5000 alpha particles launched at $3.5,mathrm {MeV}$ on the flux surface with a normalized toroidal flux of $s=0.5$ . An analysis of the tolerance of the coils to manufacturing errors is performed using a Gaussian process model, and the coils are found to maintain low particle losses for smooth, large-scale errors up to amplitudes of approximately $0.15,mathrm {m}$ . Another coil optimization is performed for the Landreman–Paul configuration with the additional constraint that the coils are purely planar. Visual inspection of the Poincaré plot of the resulting magnetic field-lines reveal that the planar modular coils alone do a poor job of reproducing the target equilibrium. Additional non-planar coil optimizations are performed for the quasi-helical configuration with $5,%$ volume-averaged plasma beta from Landreman et al. (Phys. Plasma, vol. 29, issue 8, 2022, 082501), and a similar configuration also optimized to satisfy the Mercier criterion. The finite beta configurations had larger fast-particle losses, with the free-boundary Mercier-optimized configuration performing the worst, losing approxi
从 Landreman & Paul(《物理评论快报》,第 128 卷,2022 年,035001 期)的构型开始,对几种准螺旋恒星器构型进行了基于丝状线圈的优化,证明可以用现实的线圈实现精确的准螺旋对称性。对线圈的形状和间距施加了一些限制,如低曲率和足够的等离子体-线圈距离以屏蔽中子。优化后的线圈的最大曲率是螺旋对称实验(HSX)线圈的 0.8 倍,在等离子体小半径相同的情况下,平均曲率平方是 HSX 线圈的 0.4 倍。当放大到反应堆尺寸和磁场强度时,在自由边界配置中,当模拟在通量表面以 3.5 美元/mathrm {MeV}$ 的速度发射 5000 颗阿尔法粒子时,没有发现快速粒子损失,归一化环形通量为 0.5 美元/mathrm {MeV}$ 。使用高斯过程模型对线圈对制造误差的容限进行了分析,发现线圈能够在振幅约为0.15mathrm {m}$的平滑大尺度误差下保持较低的粒子损耗。针对 Landreman-Paul 配置进行了另一次线圈优化,额外的限制条件是线圈是纯平面的。对所得到的磁场线的波恩卡雷图进行目测后发现,仅凭平面模块线圈并不能很好地再现目标平衡。针对兰德雷曼等人(《物理等离子体》,第 29 卷,第 8 期,2022 年,082501)提出的具有 5 美元(,%$)体积平均等离子体贝塔值的准螺旋配置,以及为满足梅歇准则而优化的类似配置,进行了额外的非平面线圈优化。有限β配置的快速粒子损失较大,自由边界梅西埃优化配置的表现最差,在$s=0.5$时发射的α粒子损失约为$5.5,%$。
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引用次数: 0
Fluid and kinetic studies of tokamak disruptions using Bayesian optimization 利用贝叶斯优化法对托卡马克中断进行流体和动力学研究
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-05-21 DOI: 10.1017/s0022377824000606
I. Ekmark, M. Hoppe, T. Fülöp, P. Jansson, L. Antonsson, O. Vallhagen, I. Pusztai
When simulating runaway electron dynamics in tokamak disruptions, fluid models with lower numerical cost are often preferred to more accurate kinetic models. The aim of this work is to compare fluid and kinetic simulations of a large variety of different disruption scenarios in ITER. We consider both non-activated and activated scenarios; for the latter, we derive and implement kinetic sources for the Compton scattering and tritium beta decay runaway electron generation mechanisms in our simulation tool Dream (Hoppe et al., Comput. Phys. Commun., vol. 268, 2021, 108098). To achieve a diverse set of disruption scenarios, Bayesian optimization is used to explore a range of massive material injection densities for deuterium and neon. The cost function is designed to distinguish between successful and unsuccessful disruption mitigation based on the runaway current, current quench time and transported fraction of the heat loss. In the non-activated scenarios, we find that fluid and kinetic disruption simulations can have significantly different runaway electron dynamics, due to an overestimation of the runaway seed by the fluid model. The primary cause of this is that the fluid hot-tail generation model neglects superthermal electron transport losses during the thermal quench. In the activated scenarios, the fluid and kinetic models give similar predictions, which can be explained by the significant influence of the activated sources on the runaway dynamics and the seed.
在模拟托卡马克中断中的失控电子动力学时,人们通常会选择数值成本较低的流体模型,而不是更精确的动力学模型。这项工作的目的是比较热核实验堆中各种不同中断情况下的流体和动力学模拟。我们考虑了非激活和激活两种情况;对于后者,我们在模拟工具 Dream 中推导并实施了康普顿散射和氚β衰变失控电子生成机制的动力学源(Hoppe 等人,《计算物理通讯》,第 268 卷,2021 年,108098 期)。为了实现多样化的破坏情景,我们使用贝叶斯优化方法探索了一系列氘和氖的大量物质注入密度。成本函数的设计是为了根据失控电流、电流淬火时间和热损失的传输分数来区分成功和不成功的中断缓解。在非激活情景下,我们发现流体和动力学破坏模拟的失控电子动力学会有显著不同,这是由于流体模型高估了失控种子。造成这种情况的主要原因是流体热尾生成模型忽略了热淬期间的超热电子传输损耗。在活化情况下,流体模型和动力学模型给出了相似的预测结果,这可以解释为活化源对失控动力学和种子的重大影响。
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引用次数: 0
Elastic overtaking collisions of large-amplitude ion-acoustic solitons 大振幅离子声孤子的弹性超越碰撞
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-05-17 DOI: 10.1017/s002237782400062x
Carel P. Olivier
Overtaking collisions of large-amplitude solitons are investigated via fluid simulations for a plasma consisting of cold ions and Boltzmann-distributed electrons. To achieve this, a new fluid simulation code is presented. In addition, a novel approach to construct soliton initial conditions is developed. Using these ideas, initial conditions are combined that allows the simulation of overtaking collisions. It is shown that, in the small-amplitude regime, simulation results agree well with the two-soliton solution obtained from reductive perturbation theory. Interestingly, in the large amplitude regime, both the slow and fast solitons re-emerge after the collision with no significant change, showing that the collisions remain elastic. A comparison between reductive perturbation analysis and the simulations show that the only significant effect of higher order nonlinearities on overtaking collisions is a reduction in the magnitude of the phase shifts of both solitons.
通过对由冷离子和玻尔兹曼分布电子组成的等离子体进行流体模拟,研究了大振幅孤子的超越碰撞。为此,介绍了一种新的流体模拟代码。此外,还开发了一种构建孤子初始条件的新方法。利用这些想法,结合初始条件,可以模拟超车碰撞。结果表明,在小振幅范围内,模拟结果与还原扰动理论得到的双孤子解十分吻合。有趣的是,在大振幅条件下,慢速孤子和快速孤子在碰撞后都会重新出现,但没有显著变化,这表明碰撞仍具有弹性。还原扰动分析与模拟的比较表明,高阶非线性对超越碰撞的唯一显著影响是降低了两个孤子的相移幅度。
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引用次数: 0
Parallel expansion of a fuel pellet plasmoid 燃料颗粒质点的平行膨胀
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-05-17 DOI: 10.1017/s0022377824000588
Alistair M. Arnold, Pavel Aleynikov, Boris N. Breizman
The problem of the assimilation of a cryogenic fuel pellet injected into a hot plasma is considered. Due to the transparency to ambient particles of the plasmoid, the localised region of high-density plasma created by ionisation of the ablated pellet material, electrons reach a ‘quasiequilibrium’ (QE) state which is characterised by a steady-state on the fastest collisional time scale. The simplified electron kinetic equation of the QE state is solved. Taking a velocity moment of the higher-order electron kinetic equation, which is valid on the expansion time scale, permits a fluid closure, yielding an evolution equation for the macroscopic parameters describing the QE distribution function. In contrast to the Braginskii equations, the closure does not require that electrons have a short mean free path compared with the size of density perturbations, and permits an anisotropic and highly non-Maxwellian distribution function. As the QE distribution function accounts for both trapped and passing electrons, the self-consistent electric potential that causes the expansion can be properly described, in contrast to earlier models of pellet plasmoid expansion with an unbounded potential. The plasmoid expansion is simulated using both a Vlasov model and a cold-fluid model for the ions. During the expansion plasmoid ions and electrons obtain nearly equal amounts of energy; as hot ambient electrons provide this energy in the form of collisional heating of plasmoid electrons, the expansion of a pellet plasmoid is expected to be a potent mechanism for the transfer of energy from electrons to ions on a time scale shorter than that of ion–electron thermalisation.
研究考虑了注入热等离子体的低温燃料颗粒的同化问题。由于等离子体对环境粒子的透明性,电子达到了 "准平衡"(QE)状态,该状态的特征是在最快碰撞时间尺度上的稳态。我们求解了 QE 状态的简化电子动力学方程。高阶电子动力学方程的速度矩在膨胀时间尺度上有效,它允许流体闭合,产生描述 QE 分布函数的宏观参数演化方程。与布拉金斯基方程不同的是,这种闭合不要求电子的平均自由路径与密度扰动的大小相比很短,而且允许各向异性和高度非麦克斯韦分布函数。由于 QE 分布函数同时考虑了被困电子和通过电子,因此可以正确描述导致膨胀的自洽电势,这与早期使用无约束电势的小球质点膨胀模型截然不同。我们使用 Vlasov 模型和离子冷流体模型模拟了质点膨胀。在质点膨胀过程中,离子和电子获得了几乎等量的能量;由于热环境电子以质点电子碰撞加热的形式提供能量,因此预计小球质点膨胀是一种有效的能量转移机制,其能量从电子转移到离子的时间尺度比离子-电子热化的时间尺度要短。
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引用次数: 0
Direct stellarator coil design using global optimization: application to a comprehensive exploration of quasi-axisymmetric devices 利用全局优化直接设计恒星器线圈:应用于准轴对称器件的全面探索
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-05-16 DOI: 10.1017/s0022377824000412
Andrew Giuliani
Many stellarator coil design problems are plagued by multiple minima, where the locally optimal coil sets can sometimes vary substantially in performance. As a result, solving a coil design problem a single time with a local optimization algorithm is usually insufficient and better optima likely do exist. To address this problem, we propose a global optimization algorithm for the design of stellarator coils and outline how to apply box constraints to the physical positions of the coils. The algorithm has a global exploration phase that searches for interesting regions of design space and is followed by three local optimization algorithms that search in these interesting regions (a ‘global-to-local’ approach). The first local algorithm (phase I), following the globalization phase, is based on near-axis expansions and finds stellarator coils that optimize for quasisymmetry in the neighbourhood of a magnetic axis. The second local algorithm (phase II) takes these coil sets and optimizes them for nested flux surfaces and quasisymmetry on a toroidal volume. The final local algorithm (phase III) polishes these configurations for an accurate approximation of quasisymmetry. Using our global algorithm, we study the trade-off between coil length, aspect ratio, rotational transform and quality of quasi-axisymmetry. The database of stellarators, which comprises approximately 200 000 coil sets, is available online and is called QUASR, for ‘quasi-symmetric stellarator repository’.
许多恒星仪线圈设计问题都存在多重最小值,局部最优线圈组的性能有时会有很大差异。因此,用局部优化算法一次性解决线圈设计问题通常是不够的,更好的最佳值很可能确实存在。为了解决这个问题,我们提出了一种用于设计恒星器线圈的全局优化算法,并概述了如何对线圈的物理位置应用盒式约束。该算法有一个全局探索阶段,用于搜索设计空间中的有趣区域,随后有三个局部优化算法在这些有趣区域中进行搜索(一种 "全局到局部 "的方法)。第一个局部算法(第一阶段)紧随全局化阶段之后,以近轴扩展为基础,寻找在磁轴附近优化准对称性的恒星线圈。第二个局部算法(第二阶段)采用这些线圈组,并针对嵌套磁通量面和环形体积上的准对称性进行优化。最后一种局部算法(第三阶段)对这些配置进行优化,以精确逼近准对称性。利用我们的全局算法,我们研究了线圈长度、长宽比、旋转变换和准轴对称质量之间的权衡。恒星器数据库包括约 200 000 个线圈组,可在线获取,名为 QUASR,意为 "准对称恒星器存储库"。
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引用次数: 0
Towards ion stopping power experiments with the laser-driven LIGHT beamline 利用激光驱动的 LIGHT 光束线进行离子停止力实验
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-05-16 DOI: 10.1017/s0022377824000576
H. Nazary, M. Metternich, D. Schumacher, F. Neufeld, S.J. Grimm, C. Brabetz, F. Kroll, F.-E. Brack, A. Blažević, U. Schramm, V. Bagnoud, M. Roth
The main emphasis of the Laser Ion Generation, Handling and Transport (LIGHT) beamline at GSI Helmholtzzentrum für Schwerionenforschung GmbH are phase-space manipulations of laser-generated ion beams. In recent years, the LIGHT collaboration has successfully generated and focused intense proton bunches with an energy of 8 MeV and a temporal duration shorter than 1 ns (FWHM). An interesting area of application that exploits the short ion bunch properties of LIGHT is the study of ion-stopping power in plasmas, a key process in inertial confinement fusion for understanding energy deposition in dense plasmas. The most challenging regime is found when the projectile velocity closely approaches the thermal plasma electron velocity ( $v_{i}approx v_{e,text {th}}$ ), for which existing theories show high discrepancies. Since conclusive experimental data are scarce in this regime, we plan to conduct experiments on laser-generated plasma probed with ions generated with LIGHT at a higher temporal resolution than previously achievable. The high temporal resolution is important because the parameters of laser-generated plasmas are changing on the nanosecond time scale. To meet this goal, our recent studies have dealt with ions of lower kinetic energies. In 2021, laser accelerated carbon ions were transported with two solenoids and focused temporally with LIGHT's radio frequency cavity. A bunch length of 1.2 ns (FWHM) at an energy of 0.6 MeV u $^{-1}$ was achieved. In 2022, protons with an energy of 0.6 MeV were transported and temporally compressed to a bunch length of 0.8 ns. The proton beam was used to measure the energy loss in a cold foil. Both the ion and proton beams will also be employed for energy loss measurements in a plasma target.
GSI Helmholtzzentrum für Schwerionenforschung GmbH 的激光离子生成、处理和传输(LIGHT)光束线的主要重点是激光生成离子束的相空间处理。近年来,LIGHT 合作项目已成功产生并聚焦了能量为 8 MeV、时间持续时间短于 1 ns (FWHM) 的强质子束。利用 LIGHT 的短离子束特性,一个有趣的应用领域是研究等离子体中的离子停止功率,这是惯性约束聚变中的一个关键过程,用于了解高密度等离子体中的能量沉积。当射弹速度接近热等离子体电子速度($v_{i}approx v_{e,text {th}}$)时,是最具挑战性的阶段,现有理论对此显示出很大差异。由于在这一机制下缺乏确凿的实验数据,我们计划对激光产生的等离子体进行实验,用 LIGHT 产生的离子进行探测,其时间分辨率要比以前更高。高时间分辨率非常重要,因为激光产生的等离子体的参数是在纳秒级的时间尺度上变化的。为了实现这一目标,我们最近的研究涉及动能较低的离子。2021 年,我们用两个螺线管传输激光加速的碳离子,并用 LIGHT 的射频腔进行时间聚焦。在能量为 0.6 MeV u $^{-1}$ 时,实现了 1.2 ns(FWHM)的束长。2022 年,能量为 0.6 MeV 的质子被传输并在时间上压缩到 0.8 ns 的束长。质子束被用来测量冷箔中的能量损失。离子束和质子束还将用于测量等离子体靶的能量损失。
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引用次数: 0
A structure-preserving particle discretisation for the Lenard–Bernstein collision operator 列纳德-伯恩斯坦碰撞算子的结构保留粒子离散化
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-05-14 DOI: 10.1017/s0022377824000564
S. Jeyakumar, M. Kraus, M.J. Hole, D. Pfefferlé

Collisions are an important dissipation mechanism in plasmas. When approximating collision operators numerically, it is important to preserve their mathematical structure in order to retain the laws of thermodynamics at the discrete level. This is particularly challenging when considering particle methods. A simple but commonly used collision operator is the Lenard–Bernstein operator, or its modified energy- and momentum-conserving counterpart. In this work, we present a macro-particle discretisation of this operator that is provably energy and momentum preserving.

碰撞是等离子体中的一种重要耗散机制。在对碰撞算子进行数值逼近时,必须保留其数学结构,以便在离散水平上保留热力学定律。在考虑粒子方法时,这一点尤其具有挑战性。一个简单但常用的碰撞算子是 Lenard-Bernstein 算子或其修正的能量和动量守恒对应算子。在这项工作中,我们提出了这种算子的宏观粒子离散化方法,它可以证明是能量和动量守恒的。
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引用次数: 0
Overview of neutral beam injectors for plasma heating and diagnostics developed at Budker INP 布德克国际物理研究所开发的用于等离子体加热和诊断的中性束注入器概览
IF 2.5 3区 物理与天体物理 Q3 Physics and Astronomy Pub Date : 2024-05-14 DOI: 10.1017/s0022377824000278
I. Shikhovtsev, Alexander Ivanov, V. Davydenko, Yurii I. Belchenko, G. Abdrashitov, Viktor Belov, Timur Akhmetov, V. Amirov, A. Brul, Peter Deichuli, N. Deichuli, A. Donin, A. Dranichnikov, R. Finashin, D. Gavrisenko, A. Gorbovsky, Valerian Kapitonov, V. Kolmogorov, Alexey Kondakov, I. Maslakov, V. Oreshonok, V. Rashchenko, A. Sanin, Alexey Sorokin, O. Sotnikov, N. Stupishin, R. Vakhrushev, V. Vointsev
An overview of the neutral beam injectors developed at the Budker Institute of Nuclear Physics in Novosibirsk during the last 10 years is presented. These neutral injectors are used for plasma diagnostics, heating and current drive in modern fusion devices with magnetic confinement. An arc or a radio-frequency (RF) discharge generates a plasma in the ion sources of the injectors, and a positive hydrogen or deuterium ion beam is extracted and accelerated by a multiaperture ion-optical system (IOS). The accelerated ion beam is converted into a neutral one in a gas target. The precision multiaperture IOS with spherically concave electrodes provides ballistic focusing of the neutral beam. The high-energy, high-power beam injector based on negative ions, which is currently under development, is described as well. It comprises a RF negative ion source and a wide-aperture electrostatic accelerator separated from the source by a low-energy beam transport line, thereby improving the injector reliability.
本文概述了新西伯利亚布德克核物理研究所(Budker Institute of Nuclear Physics in Novosibirsk)在过去十年中开发的中性束注入器。这些中性束注入器用于现代磁约束聚变装置中的等离子体诊断、加热和电流驱动。电弧或射频(RF)放电会在注入器的离子源中产生等离子体,并通过多孔径离子光学系统(IOS)提取和加速正氢或氘离子束。加速后的离子束在气体靶中转化为中性离子束。带有球形凹面电极的精密多孔离子光学系统可对中性离子束进行弹道聚焦。此外,还介绍了目前正在开发的基于负离子的高能量、高功率射束器。它包括一个射频负离子源和一个宽孔径静电加速器,通过一条低能束传输线与负离子源隔开,从而提高了注入器的可靠性。
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Journal of Plasma Physics
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