Pub Date : 2026-01-18DOI: 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.
{"title":"First Observation of Heating of the Globus-M2 Tokamak Wall by Fast Ions Using a Two-Color Pyrometer during Excitation of Toroidal Alfvén Eigenmodes","authors":"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","doi":"10.1134/S1063780X25603256","DOIUrl":"10.1134/S1063780X25603256","url":null,"abstract":"<p>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.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 11","pages":"1336 - 1346"},"PeriodicalIF":1.1,"publicationDate":"2026-01-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145993734","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-12-25DOI: 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.
{"title":"Effect of Thermal Spread of Electrons on Stationary States of Vacuum Diode","authors":"A. M. Ignatov","doi":"10.1134/S1063780X25603918","DOIUrl":"10.1134/S1063780X25603918","url":null,"abstract":"<p>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.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 10","pages":"1222 - 1229"},"PeriodicalIF":1.1,"publicationDate":"2025-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145824321","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-12-25DOI: 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.
{"title":"Optimization of Geometric Parameters of the Antenna System for ICR Heating by the Magnetic Beach Method in an Electrodeless Plasma Thruster","authors":"I. A. Abramov, E. D. Gospodchikov","doi":"10.1134/S1063780X25603967","DOIUrl":"10.1134/S1063780X25603967","url":null,"abstract":"<p>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.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 10","pages":"1183 - 1196"},"PeriodicalIF":1.1,"publicationDate":"2025-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1134/S1063780X25603967.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145824324","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-12-25DOI: 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.
{"title":"Experiments on the Simulation and Visualization of Dusty Plasma in the Vicinity of an Atmosphereless Cosmic Body","authors":"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","doi":"10.1134/S1063780X25603797","DOIUrl":"10.1134/S1063780X25603797","url":null,"abstract":"<p>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.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 10","pages":"1230 - 1242"},"PeriodicalIF":1.1,"publicationDate":"2025-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145824325","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-12-25DOI: 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.
{"title":"Simulation of the Antenna–Plasma Coupling Efficiency of the Three-Loop ICR Antenna of the T-15MD Tokamak","authors":"K. O. Nedbailov, A. I. Meshcheryakov","doi":"10.1134/S1063780X25603372","DOIUrl":"10.1134/S1063780X25603372","url":null,"abstract":"<p>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.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 10","pages":"1167 - 1182"},"PeriodicalIF":1.1,"publicationDate":"2025-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145824314","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-12-25DOI: 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.
{"title":"Neutralization of Kiloampere Beams of Relativistic Electrons with Different Durations in a Plasma Column with a Leading Magnetic Field","authors":"A. V. Arzhannikov, S. L. Sinitsky, D. A. Samtsov, P. V. Kalinin, K. N. Kuklin","doi":"10.1134/S1063780X25603657","DOIUrl":"10.1134/S1063780X25603657","url":null,"abstract":"<p>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.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 10","pages":"1197 - 1210"},"PeriodicalIF":1.1,"publicationDate":"2025-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145824392","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-12-25DOI: 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.
{"title":"Use of the ТМ110 (E110) Mode of a Cylindrical Microwave Resonator for Estimation of Plasma Density in a Gas Discharge Tube","authors":"V. P. Stepin, V. I. Zhukov, S. E. Andreev, D. M. Karfidov, M. S. Usachonak, A. S. Gaidash, S. N. Zamuruev, N. N. Bogachev","doi":"10.1134/S1063780X25603578","DOIUrl":"10.1134/S1063780X25603578","url":null,"abstract":"<p>Traditional microwave resonator methods for plasma diagnostics face fundamental limitations at high plasma densities (<i>n</i><sub>e</sub> > 10<sup>11</sup> cm<sup>–3</sup>) 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 TM<sub>110</sub> (E<sub>110</sub>) mode of a cylindrical resonator (radius <i>R</i> = 45 mm, length <i>H</i> = 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 C<sub>v</sub> for the TM<sub>110</sub> mode remains constant in the range <i>n</i><sub>e</sub> = 10<sup>11</sup>–10<sup>12</sup> cm<sup>–3</sup>, ensuring a linear dependence of the resonant frequency shift on the plasma density. The TM<sub>110</sub> mode demonstrates resistance to the resonant peak degradation at high plasma densities <i>n</i><sub>e</sub>, in contrast to the TM<sub>010</sub> mode, where the signal suppression was observed already at <i>n</i><sub>e</sub> ≈ 3 × 10<sup>11</sup> cm<sup>–3</sup>. 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.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 10","pages":"1263 - 1270"},"PeriodicalIF":1.1,"publicationDate":"2025-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145824345","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-12-25DOI: 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.
{"title":"Analytical Study of Weakly Damped Shock Structures in the Adlam–Allen Model","authors":"S. S. Abbas, G. Abbas, Z. Iqbal, Ch. Rozina","doi":"10.1134/S1063780X25603335","DOIUrl":"10.1134/S1063780X25603335","url":null,"abstract":"<p>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 <span>(nu )</span> 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.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 10","pages":"1256 - 1262"},"PeriodicalIF":1.1,"publicationDate":"2025-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145824380","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-12-25DOI: 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.
{"title":"Coefficient of Thermal Accommodation of O2 Molecules in Pyrex during a DC Discharge in Oxygen","authors":"I. I. Ziganshin, D. V. Kiselevich, D. V. Lopaev, K. R. Galliulin, A. T. Rakhimov","doi":"10.1134/S1063780X25603980","DOIUrl":"10.1134/S1063780X25603980","url":null,"abstract":"<p>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.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 10","pages":"1271 - 1275"},"PeriodicalIF":1.1,"publicationDate":"2025-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145824383","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2025-12-25DOI: 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
{"title":"Study of the Main Components of Tokamak Plasma Turbulence","authors":"V. A. Vershkov, A. V. Melnikov, L. G. Eliseev","doi":"10.1134/S1063780X25603505","DOIUrl":"10.1134/S1063780X25603505","url":null,"abstract":"<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","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 10","pages":"1121 - 1153"},"PeriodicalIF":1.1,"publicationDate":"2025-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145824323","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}