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First Observation of Heating of the Globus-M2 Tokamak Wall by Fast Ions Using a Two-Color Pyrometer during Excitation of Toroidal Alfvén Eigenmodes 双色高温计首次观测到环面alfv<s:1>本征模激发过程中快速离子对Globus-M2托卡马克壁的加热
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2026-01-18 DOI: 10.1134/S1063780X25603256
N. N. Bakharev, O. M. Skrekel, A. S. Aleksandrov, I. M. Balachenkov, V. I. Varfolomeev, A. V. Voronin, V. K. Gusev, A. A. Kapralov, E. O. Kiselev, V. B. Minaev, Yu. V. Petrov, N. V. Sakharov, G. Yu. Sotnikova, A. Yu. Telnova, V. A. Tokarev, E. M. Khilkevich, A. E. Shevelev, P. B. Shchegolev

The work presents the results of experiments on the study of fast particle losses to the wall in the Globus-M2 tokamak under conditions of excitation of toroidal Alfvén instabilities using a pyrometer developed at the Ioffe Institute. Data on the time evolution of the wall temperature and local heat flux to the wall during the instability development are presented. The origin of the separation of these quantities into coherent and incoherent components is discussed. Experimental dependences of the increase in wall temperature and heat flux on the instability amplitude are considered. The results of the simulation of fast particle losses during the development of Alfvén-type instabilities are analyzed. Based on these results and experimental data, conclusions are drawn regarding the mechanism of fast particle losses during the interaction with an Alfvén wave.

本文介绍了使用Ioffe研究所开发的高温计,在环形alfv不稳定激励条件下,Globus-M2托卡马克中快速粒子壁面损失的实验结果。给出了不稳定发展过程中壁面温度和壁面局部热流的时间演变数据。讨论了这些量分离为相干分量和非相干分量的原因。考虑了壁面温度和热流的增加对不稳定幅值的实验依赖关系。分析了alfv型不稳定性发展过程中快速粒子损失的模拟结果。基于这些结果和实验数据,得出了与alfvsamn波相互作用时粒子快速损失的机理。
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引用次数: 0
Effect of Thermal Spread of Electrons on Stationary States of Vacuum Diode 电子热扩散对真空二极管定态的影响
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2025-12-25 DOI: 10.1134/S1063780X25603918
A. M. Ignatov

Stationary states of electron beam with arbitrary velocity spread in a vacuum diode are studied. The velocity distribution function of beam electrons is assumed to be constant over a certain velocity range. The limiting current as a function of the velocity spread was obtained. It was ascertained that, within a certain range of parameters, stationary states with two types of virtual cathodes can exist.

研究了任意速度电子束在真空二极管中传播的定态。假定束流电子的速度分布函数在一定的速度范围内是恒定的。得到了极限电流随速度扩散的函数。在一定的参数范围内,可以存在两种虚阴极的稳态。
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引用次数: 0
Optimization of Geometric Parameters of the Antenna System for ICR Heating by the Magnetic Beach Method in an Electrodeless Plasma Thruster 磁滩法优化无极等离子体推力器ICR加热天线系统几何参数
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2025-12-25 DOI: 10.1134/S1063780X25603967
I. A. Abramov, E. D. Gospodchikov

Geometric parameters and shape of the RF antenna must be optimized precisely for efficient ion cyclotron resonance (ICR) heating of plasma by the magnetic beach method in electrodeless plasma thrusters (EPT). To this end, in the present work, we carried out full-wave simulation of the excitation of eigenmodes of the magnetized plasma column by ion-cyclotron (IC) antennas taking into account the radial inhomogeneity of the plasma column and spatial dispersion of the electron and ion dielectric response. Both the total energy deposited by the antennas into plasma and its distribution between the Alfvén eigenmodes of the plasma column and the Alfvén continuum were obtained as a result of the simulation. The simulation was performed for three most popular types of antennas used for the ICR plasma heating in the PS-1 setup. The efficiencies of these types of antennas are compared and the optimal length of each of them is determined.

在无极等离子体推力器(EPT)中,为了实现离子回旋共振(ICR)对等离子体的有效加热,必须对射频天线的几何参数和形状进行精确优化。为此,考虑到等离子体柱的径向非均匀性以及电子和离子介电响应的空间色散,我们利用离子回旋加速器(IC)天线对磁化等离子体柱本征模的激发进行了全波模拟。仿真结果得到了天线进入等离子体的总能量及其在等离子体柱和alfv录影带本征模之间的分布。对PS-1装置中用于ICR等离子体加热的三种最常用的天线进行了模拟。比较了这些天线的效率,并确定了每种天线的最佳长度。
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引用次数: 0
Experiments on the Simulation and Visualization of Dusty Plasma in the Vicinity of an Atmosphereless Cosmic Body 无大气天体附近尘埃等离子体的模拟与可视化实验
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2025-12-25 DOI: 10.1134/S1063780X25603797
I. A. Shashkova, I. A. Kuznetsov, Y. Y. Tian, S. I. Popel, A. A. Kartasheva, G. G. Dolnikov, A. N. Lyash, M. E. Abdelaal, A. V. Zakharov

This work presents a laboratory experiment on the formation of dusty plasma and the visualization of flows of charged dust particles ranging in a diameter from 10 to 100 µm. These particles consist of silicon dioxide, a component of lunar regolith. The influence of near-surface plasma simulated using an electrostatic field and ultraviolet radiation (UV) on the dynamics of regolith-analog particles is examined. Particle trajectories and changes in the surface topography of the particles are visualized, and estimates of their takeoff velocities are obtained. It is shown that the pattern of the particle motion in dusty plasma depends on the presence of UV radiation and the size of the particles themselves. The results of this study are of interest for understanding the physical processes occurring near the surface of the Moon and other atmosphereless bodies in the Solar System, such as Mercury, asteroids, and the moons of Mars.

这项工作提出了一个尘埃等离子体形成的实验室实验,以及直径从10到100微米的带电尘埃颗粒流动的可视化。这些微粒由二氧化硅组成,是月球风化层的一种成分。研究了用静电场和紫外线辐射模拟近表面等离子体对模拟风化层粒子动力学的影响。粒子轨迹和粒子表面形貌的变化是可视化的,并估计了它们的起飞速度。结果表明,尘埃等离子体中粒子运动的模式取决于紫外线辐射的存在和粒子本身的大小。这项研究的结果对于理解月球和太阳系中其他无大气天体(如水星、小行星和火星卫星)表面附近发生的物理过程很有意义。
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引用次数: 0
Simulation of the Antenna–Plasma Coupling Efficiency of the Three-Loop ICR Antenna of the T-15MD Tokamak T-15MD托卡马克三环ICR天线-等离子体耦合效率仿真
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2025-12-25 DOI: 10.1134/S1063780X25603372
K. O. Nedbailov, A. I. Meshcheryakov

Currently, the National Research Center “Kurchatov Institute” is developing an ion-cyclotron resonance (ICR) heating system for the T-15MD tokamak. The ICRF (ion cyclotron range of frequency) system is to be used to heat the ion component of the plasma and generate a non-inductive current (drag current). The total power of the system is 6 MW with a pulse duration of up to 30 s. Under these parameters, reflected power could lead to failure of the ion-cyclotron resonance heating (ICRH) of the system. Therefore, matching the load (plasma) to the generator requires special attention. This work presents a numerical study of the antenna–plasma coupling efficiency for a three-loop antenna developed for ICRF plasma heating in the T‑15MD tokamak. The dependence of the antenna impedance on plasma parameters, its position, and the phasing of the antenna excitation currents is studied.

目前,国家研究中心“库尔恰托夫研究所”正在为T-15MD托卡马克开发一种离子回旋共振(ICR)加热系统。ICRF(离子回旋频率范围)系统用于加热等离子体的离子成分并产生非感应电流(阻力电流)。该系统的总功率为6兆瓦,脉冲持续时间长达30秒。在这些参数下,反射功率会导致系统的离子回旋共振加热(ICRH)失效。因此,将负载(等离子体)与发电机匹配需要特别注意。本文对T - 15MD托卡马克中用于ICRF等离子体加热的三环天线的天线-等离子体耦合效率进行了数值研究。研究了天线阻抗与等离子体参数、等离子体位置和天线激励电流相位的关系。
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引用次数: 0
Neutralization of Kiloampere Beams of Relativistic Electrons with Different Durations in a Plasma Column with a Leading Magnetic Field 在具有超前磁场的等离子体柱中,不同持续时间的千安培相对论电子束的中和作用
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2025-12-25 DOI: 10.1134/S1063780X25603657
A. V. Arzhannikov, S. L. Sinitsky, D. A. Samtsov, P. V. Kalinin, K. N. Kuklin

In experiments on plasma heating during the passage of a relativistic electron beam with a current ~10 kA through a plasma column, the electric and magnetic fields of the beam have to be compensated by the current induced in the plasma, i.e., the so-called charge and current neutralizations of the beam have to occur. In the earliest experiments on injection of high-current relativistic electron beams into a plasma with a magnetic field, the effects of plasma neutralization of the electron beam’s internal electromagnetic field were observed. At the same time, the dynamics of these neutralization processes also depends on the ratio between the duration of the leading edge of the beam current and the flight time of its electrons along the plasma column length. This work describes the results of two substantially different series of experiments on the neutralization of an electron beam with a current of about 10 kA in a plasma column under a strong (4 T) leading magnetic field. In the first series of experiments, the leading edge of the beam current was ≈5 ns and its duration was about 50 ns. In the second series of experiments, the leading edge of the current beam was ~0.1 μs and its duration was ≈5 μs.

在电流~ 10ka的相对论性电子束通过等离子体柱时的等离子体加热实验中,电子束的电场和磁场必须由等离子体中感应的电流来补偿,即所谓电子束的电荷和电流中和必须发生。在最早的有磁场的等离子体中注入大电流相对论电子束的实验中,观察到了等离子体中和电子束内部电磁场的效应。同时,这些中和过程的动力学也取决于光束电流前缘的持续时间与其电子沿等离子体柱长度的飞行时间之间的比率。这项工作描述了在强(4 T)超前磁场下等离子体柱中以约10 kA电流中和电子束的两个本质上不同的系列实验的结果。在第一个系列的实验中,光束电流的前缘约为5 ns,持续时间约为50 ns。在第二组实验中,电流束的前缘为~0.1 μs,持续时间为≈5 μs。
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引用次数: 0
Use of the ТМ110 (E110) Mode of a Cylindrical Microwave Resonator for Estimation of Plasma Density in a Gas Discharge Tube 使用圆柱形微波谐振器的ТМ110 (E110)模式估计气体放电管中的等离子体密度
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2025-12-25 DOI: 10.1134/S1063780X25603578
V. P. Stepin, V. I. Zhukov, S. E. Andreev, D. M. Karfidov, M. S. Usachonak, A. S. Gaidash, S. N. Zamuruev, N. N. Bogachev

Traditional microwave resonator methods for plasma diagnostics face fundamental limitations at high plasma densities (ne > 1011 cm–3) due to the response nonlinearity and resonant peak broadening. The search for alternative approaches that provide accurate measurements over a wide range remains a topical issue. In this work, the feasibility of using the TM110 (E110) mode of a cylindrical resonator (radius R = 45 mm, length H = 30 mm) to measure the electron density in a gas-discharge plasma excited by a surface electromagnetic wave is studied experimentally and numerically. It is found that the coupling coefficient Cv for the TM110 mode remains constant in the range ne = 1011–1012 cm–3, ensuring a linear dependence of the resonant frequency shift on the plasma density. The TM110 mode demonstrates resistance to the resonant peak degradation at high plasma densities ne, in contrast to the TM010 mode, where the signal suppression was observed already at ne ≈ 3 × 1011 cm–3. The obtained measurement results are in good agreement with the results of plasma density measurements using the transmitted wave method and the integrated plasma luminosity, as well as with literature data. The proposed modification of the method is suitable for noninvasive diagnostics of the longitudinal electron density distribution of gas discharge plasma, including plasma antennas.

传统的微波谐振器等离子体诊断方法在高等离子体密度(1011 cm-3)下,由于响应非线性和共振峰增宽,面临着基本的局限性。寻找在大范围内提供精确测量的替代方法仍然是一个热门问题。本文通过实验和数值研究,探讨了利用半径R = 45 mm,长度H = 30 mm的圆柱形谐振器的TM110 (E110)模式测量表面电磁波激发的气体放电等离子体中电子密度的可行性。研究发现,TM110模式的耦合系数Cv在ne = 1011-1012 cm-3范围内保持恒定,从而保证了谐振频移与等离子体密度的线性关系。与TM010模式相比,TM110模式在高等离子体密度ne下可以抵抗共振峰衰减,而TM010模式在ne≈3 × 1011 cm-3处已经观察到信号抑制。所得测量结果与透射波法等离子体密度测量结果、等离子体亮度积分测量结果及文献数据吻合较好。提出的改进方法适用于气体放电等离子体(包括等离子体天线)纵向电子密度分布的无创诊断。
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引用次数: 0
Analytical Study of Weakly Damped Shock Structures in the Adlam–Allen Model Adlam-Allen模型中弱阻尼冲击结构的分析研究
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2025-12-25 DOI: 10.1134/S1063780X25603335
S. S. Abbas, G. Abbas, Z. Iqbal, Ch. Rozina

We investigate the formation of damped oscillatory shock structures in a cold, weakly collisional plasma using the hydromagnetic Adlam–Allen (AA) model. By incorporating a small, constant dissipation term (nu ) motivated by effective electron–ion scattering in the transverse direction, we derive a nonlinear second-order differential equation governing the magnetic field evolution. Using the Sagdeev pseudo-potential method and Jacobian linearization, we systematically classify the resulting structures in the phase space, revealing the conditions under which stable spiral and saddle-type solutions arise. Furthermore, by linearizing the governing equation near equilibrium points, we obtain explicit expressions for the field amplitudes, which exhibit damped harmonic behavior. Our analytical results offer a complementary perspective to prior numerical studies and provide deeper insight into the nature of weakly damped hydromagnetic shock waves relevant to space and laboratory plasmas.

我们利用磁Adlam-Allen (AA)模型研究了冷弱碰撞等离子体中阻尼振荡激波结构的形成。通过引入一个小的,恒定的耗散项(nu ),由有效的横向电子-离子散射激发,我们推导出一个非线性二阶微分方程来控制磁场的演化。利用Sagdeev伪势方法和Jacobian线性化方法,系统地对相空间中得到的结构进行了分类,揭示了产生稳定螺旋型解和鞍型解的条件。此外,通过线性化平衡点附近的控制方程,我们得到了具有阻尼谐波特性的场振幅的显式表达式。我们的分析结果为之前的数值研究提供了一个补充的视角,并对与空间和实验室等离子体相关的弱阻尼磁激波的性质提供了更深入的了解。
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引用次数: 0
Coefficient of Thermal Accommodation of O2 Molecules in Pyrex during a DC Discharge in Oxygen 氧直流放电时耐热玻璃中O2分子的热容纳系数
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2025-12-25 DOI: 10.1134/S1063780X25603980
I. I. Ziganshin, D. V. Kiselevich, D. V. Lopaev, K. R. Galliulin, A. T. Rakhimov

The radial distribution of gas temperature in a DC glow discharge in pure oxygen in a Pyrex tube was measured in different discharge regimes in the pressure range 1–5 Torr. Analysis of the obtained results allowed us to determine the thermal accommodation coefficient for oxygen molecules on Pyrex: 0.26 ± 0.02. The thermal accommodation coefficient determines the spatial distribution of temperature in the plasma-chemical reactor, the kinetics of reactions with heavy particles in the discharge, and the rate of plasma-chemical processing of materials.

在1 ~ 5 Torr的压力范围内,测量了高温管中纯氧直流辉光放电中气体温度的径向分布。对所得结果的分析使我们确定了氧分子在Pyrex上的热适应系数:0.26±0.02。热调节系数决定了等离子体化学反应器内温度的空间分布、放电中与重粒子反应的动力学以及材料的等离子体化学处理速率。
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引用次数: 0
Study of the Main Components of Tokamak Plasma Turbulence 托卡马克等离子体湍流的主要成分研究
IF 1.1 4区 物理与天体物理 Q4 PHYSICS, FLUIDS & PLASMAS Pub Date : 2025-12-25 DOI: 10.1134/S1063780X25603505
V. A. Vershkov, A. V. Melnikov, L. G. Eliseev
<p>This work reviews the current state of research on the three main components of the turbulence spectrum observed in modern tokamaks. These components differ in frequency range and correlation properties, have relatively wide frequency intervals, and sizes larger than the ion Larmor radius. These are broadband (BB), quasi-coherent (QC), and stochastic low-frequency (SLF) fluctuations. BB fluctuations have the broadest frequency range, from 0 to 200–400 kHz, and make the main contribution to the total amplitude of density fluctuations. The characteristic BB sizes are close to those predicted by theory for the ion temperature gradient (ITG) and trapped electron mode (TEM) instabilities. BB are the least correlated fluctuations; in the T-10 tokamak plasma (<i>R</i>/<i>a</i> = 1.5/0.3 m), their typical radial and poloidal correlation lengths are approximately 1 and 2 cm, respectively, while the correlation length along the magnetic field line is less than 2.5 m. Quasi-coherent fluctuations (QC) are manifested as local maxima in the frequency spectra of density oscillations; however, they are most clearly visible in the coherence spectra, since they have radial and poloidal correlation lengths significantly longer than BB. In the T-10 tokamak plasma, correlations along the magnetic field line over a length of up to 10 m were observed for QC modes. Two types of such fluctuations were observed at T-10: low-frequency (LFQC) and high-frequency (HFQC). The characteristic poloidal sizes and dependences on discharge parameters in the T-10 experiments show that the properties of LFQC and HFQC are close to those of ITG and TEM, respectively. The poloidal rotation of QC coincides with the drift [<b>E</b> × <b>B</b>] rotation in magnitude and direction. A relation between the characteristics of these modes and the discharge parameters is demonstrated with a change in density. The magnetic component in QC was demonstrated at T-10 and DIII-D. Gyrokinetic simulation of these experiments showed that the properties of QC are close to the micro-tearing mode (MTM). Additional evidence for the MTM nature of QC is the strong dependence of their spectra on the current profile, the discrete mode structure, and the absence of QC in stellarator plasma. Stochastic low-frequency fluctuations (SLF), excited in the range from 0 to 70 kHz, are the least studied. In the T-10 tokamak, plasma on the side of a low magnetic field, these fluctuations can rotate in the direction opposite to QC. SLFs are uncorrelated along the magnetic field line at the LFS, but correlated at the HFS. SLF fluctuations have a magnetic component. Density and potential fluctuations have different radial and poloidal sizes and are uncorrelated with each other. This suggests the existence of two independent types of fluctuations in the SLF frequency domain. Experiments at DIII-D, by comparing spectra in the L, I, and H modes, showed that fluctuations in the SLF region (up to 70 kHz) can be associated with p
本文综述了在现代托卡马克中观测到的湍流谱的三个主要组成部分的研究现状。这些成分在频率范围和相关特性上不同,具有相对较宽的频率间隔,并且尺寸大于离子拉莫尔半径。它们是宽带(BB)、准相干(QC)和随机低频(SLF)波动。BB波动的频率范围最宽,为0 ~ 200 ~ 400 kHz,对密度波动的总幅值贡献最大。特征BB尺寸接近理论预测的离子温度梯度(ITG)和捕获电子模式(TEM)不稳定性。BB是相关性最小的波动;在T-10托卡马克等离子体(R/a = 1.5/0.3 m)中,它们的典型径向和极向相关长度分别约为1 cm和2 cm,而沿磁力线的相关长度小于2.5 m。准相干涨落(QC)表现为密度振荡频谱的局部极大值;然而,它们在相干光谱中是最清晰可见的,因为它们的径向和极向相关长度明显长于BB。在T-10托卡马克等离子体中,在长达10米的长度上观察到QC模式沿磁场线的相关性。在T-10观察到两种类型的波动:低频(LFQC)和高频(HFQC)。T-10实验的特征极向尺寸和对放电参数的依赖关系表明,LFQC和HFQC的性能分别接近ITG和TEM的性能。QC的极向旋转在量级和方向上与漂移[E × B]的旋转一致。这些模式的特性与放电参数之间的关系随着密度的变化而变化。QC中的磁性成分在T-10和DIII-D中得到证实。这些实验的陀螺动力学模拟表明,QC的性能接近微撕裂模式(MTM)。QC的MTM性质的另一个证据是它们的光谱对电流剖面的强烈依赖,离散模式结构,以及仿星器等离子体中QC的缺失。在0 ~ 70khz范围内激发的随机低频波动(SLF)是研究最少的。在T-10托卡马克中,等离子体在低磁场的一侧,这些波动可以在与QC相反的方向上旋转。slf在LFS处沿磁力线不相关,但在HFS处相关。SLF波动有磁性成分。密度和电位波动具有不同的径向和极向大小,彼此不相关。这表明在SLF频域中存在两种独立类型的波动。在DIII-D的实验中,通过比较L、I和H模式的光谱,发现SLF区域(高达70 kHz)的波动与粒子输运有关,而QCM和BB等高频波动与热输运有关。
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引用次数: 0
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Plasma Physics Reports
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