A. G. Rousskikh, A. S. Zhigalin, V. I. Oreshkin, N. A. Ratakhin, A. M. Kuzminykh
{"title":"Influence of Initial Density Distribution of a Substance on the Compression Stability and Radiation Characteristics of Metal-Puff Liners","authors":"A. G. Rousskikh, A. S. Zhigalin, V. I. Oreshkin, N. A. Ratakhin, A. M. Kuzminykh","doi":"10.1134/S1063780X26601161","DOIUrl":"10.1134/S1063780X26601161","url":null,"abstract":"<p>The properties of high-temperature plasma formed during compression of metal-puff liners, which are one of the varieties of Z-pinches, were investigated. The main attention was paid to the influence of the initial distribution of the density of the substance on the compression process and on the radiation characteristics of the liners. Before the implosion process began, the liner’s plasma shell was formed through the combustion of a high-current vacuum arc discharge initiated along the dielectric surface. To form the plasma shell, two plasma gun designs with different electrode geometries were used. The experiments were carried out on a pulse power generator IMRI-5 with a current amplitude in the load of 350 kA and a rise time of 600 ns. During the experiments, the following parameters were recorded: X-ray radiation power; optical images of the liner at different points in time; voltage drop on the liner; IMRI-5 generator current and its derivative, as well as plasma generator current and its derivative. The obtained optical images of the compression of metal-puff liners allow us to state that the use of a plasma gun (both in the first and second modifications) makes it possible to form a shell in which, during compression, the development of Rayleigh–Taylor instabilities is significantly suppressed. According to the authors, the main reason for the effective suppression of RT instabilities is the presence of a radial density distribution profile of the substance in the created plasma shell, which is close in shape to a power function with a degree of –3.5. The use of the second modification of the plasma gun allows to increase the power and radiation output by more than 1.5 times.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1321 - 1331"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309540","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}
S. V. Ivanenko, A. L. Solomakhin, P. V. Pershin, P. V. Zubarev, K. D. Shulyatiev, N. N. Bakharev, V. V. Solokha, E. O. Kiselev, E. E. Tkachenko, O. M. Skrekel, Yu. V. Petrov, N. V. Sakharov, V. K. Gusev, S. V. Krikunov, A. N. Novokhatskii, N. S. Zhiltsov, G. S. Kurskiev, P. B. Shchegolev, V. B. Minaev, P. A. Bagryansky
{"title":"Dispersion Interferometer as an Instrument of Plasma Electron Density Control","authors":"S. V. Ivanenko, A. L. Solomakhin, P. V. Pershin, P. V. Zubarev, K. D. Shulyatiev, N. N. Bakharev, V. V. Solokha, E. O. Kiselev, E. E. Tkachenko, O. M. Skrekel, Yu. V. Petrov, N. V. Sakharov, V. K. Gusev, S. V. Krikunov, A. N. Novokhatskii, N. S. Zhiltsov, G. S. Kurskiev, P. B. Shchegolev, V. B. Minaev, P. A. Bagryansky","doi":"10.1134/S1063780X26601215","DOIUrl":"10.1134/S1063780X26601215","url":null,"abstract":"<p>The article describes the possibility of the plasma density control in fusion devices using a dispersion interferometer by example of Globus-M2 tokamak (Saint Petersburg, Russia) experiments. The characteristics of the dispersion interferometer developed at the Budker Institute of Nuclear Physics (Novosibirsk, Russia): measurement error of integral plasma density ≤6 × 10<sup>16</sup> m<sup>–2</sup> and time resolution of 20 μs, made it possible to use its measurements for generating feedback signals in control loops. Plasma density at Globus-M2 discharges was controlled using a piezoelectric voltage-controlled gas valve. The formation of control signals is based on the PID (proportional–integral–derivative) control algorithm implemented in digital part of interferometer signal recording module. During Globus-M2 experiments, the possibility of the plasma electron density control using a dispersion interferometer was demonstrated.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1311 - 1320"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309541","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}
{"title":"A Theoretical Study of Nonlinear Electron Temperature Transport in Inertial Confinement Fusion","authors":"A. Mohammadian Pourtalari","doi":"10.1134/S1063780X26600301","DOIUrl":"10.1134/S1063780X26600301","url":null,"abstract":"<p>This work presents an analytical approach toward in understanding nonlinear electron temperature transport during the hot-spot formation phase of inertial confinement fusion (ICF), and providing exact analytical solutions for the nonlinear heat conduction equation that governs electron thermal transport in fusion plasmas. It is important to emphasize that the present model is a reduced theoretical framework that isolates nonlinear electron temperature transport as a sub-process of hot-spot formation. By employing self-similar solutions, the expressions for the spatiotemporal evolution of electron temperature, the propagation dynamics of the spherical thermal wave front and the waiting-time phenomenon characterizing the initial stationary phase of heat front evolution is derived. The solution incorporates the Spitzer–Harm temperature-dependent conductivity scaling and satisfies energy conservation with finite initial temperature at the boundary, overcoming limitations of previous similarity solutions that predicted unphysical singularities. Key innovations include the derivation of exact expressions for the waiting time (confinement time), the heat front position, and the electron temperature decay in spherical convergence geometry. Our results should be viewed as ideal limiting cases that provide insight into the nonlinear diffusion process in the absence of geometric and material complexities.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1370 - 1380"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309529","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}
{"title":"Spherical Focusing of a Short Dipole Pulse","authors":"I. I. Metelskii, V. F. Kovalev, V. Yu. Bychenkov","doi":"10.1134/S1063780X26601598","DOIUrl":"10.1134/S1063780X26601598","url":null,"abstract":"<p>A theory of compression of an electromagnetic spherically converging dipole pulse of ultrashort duration has been developed. The spatio-temporal distribution of the electromagnetic field in the focal region and the characteristics of electromagnetic energy cumulation depending on the initial phase of the spherical wave have been studied. A theoretical limit for the maximum value of the pulse field strength at the focal point as a function of the total pulse energy and its duration has been established. Dependences of the maximum amplitude of the electric field at the focal point and the characteristic spatial volume of the compressed pulse on the pulse duration have been found. It has been shown that the minimum (limiting) volume of a pulse compressed during cumulation is <span>({V_{min }} approx 0.057{lambda ^3})</span>, where <span>(lambda )</span> is the radiation wavelength.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1332 - 1345"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1134/S1063780X26601598.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309670","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}
{"title":"On Dust Fractions of Various Compositions under the Conditions of Formation of a Dusty Plasma System near the Nucleus of a Comet","authors":"S. I. Popel, A. P. Golub’, L. M. Zelenyi","doi":"10.1134/S1063780X26601653","DOIUrl":"10.1134/S1063780X26601653","url":null,"abstract":"<p>In a situation where dusty plasma can form in the vicinity of a comet’s nucleus, the influence of the dust composition at the surface of the nucleus on the plasma parameters, as well as on the composition of dust in the coma and tail of the comet, is considered. The cases of silicate and ice dust particles are discussed. It is shown that the influence of electrostatic effects in relation to the effects caused by the force of entrainment of a dust particle by a gas flow is weaker for ice particles than for silicate particles. Accordingly, the importance of ice particles in dusty plasma in the vicinity of comets, compared to silicate particles, becomes apparent at greater distances from the Sun. Furthermore, ice particles rising to certain heights are larger than silicate particles rising to the same heights. Accordingly, ice particles accumulate greater charges than silicate particles. For a comet with parameters of the nucleus close to those of comet 67P/Churyumov–Gerasimenko, the proportion of dust particles carried away by the gas flow from the cometary nucleus relative to their number on the surface of the cometary nucleus does not exceed a value of about 10%. In this case, the proportion of carried away ice dust particles relative to the number of ice dust particles on the cometary nucleus, and, accordingly, included in the composition of the comet’s dust coma and cometary tail, turns out to be several times greater than the proportion of carried away silicate dust relative to the number of silicate dust particles on the cometary nucleus.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1352 - 1360"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1134/S1063780X26601653.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309542","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}
Dmitriy Vasilkov, Nina Skvortsova, Nikolay Kharchev
{"title":"Non-Diffusion Transport in Induction-Free Magnetic Traps and Comparison of Approaches to Its Description","authors":"Dmitriy Vasilkov, Nina Skvortsova, Nikolay Kharchev","doi":"10.1134/S1063780X2660074X","DOIUrl":"10.1134/S1063780X2660074X","url":null,"abstract":"<p>The article presents an analysis of particle transport in the magnetically active plasma of stellarators and an open trap. Thermodynamic and statistical approaches to the description of turbulent transport are considered. The structure of the turbulent flow and its relation to the magnetic structure of the periphery of the magnetized plasma and the statistical characteristics of the flow are analyzed. The conditions of the effect of powerful “density pump-out” are considered and the connection with neoclassical and turbulent flows is given. Various factors influencing the formation of a nonmonotonic density profile are considered. The contribution of various kinetic instabilities to the formation of a turbulent flow is considered. The theoretical calculation of the flows and the connection of the statistical characteristics with the various contributions of the diffusive and non-diffusive flow are analyzed. The possibility of direct modeling of non-diffusion processes is evaluated.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1297 - 1310"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309539","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}
Yu. S. Akishev, N. A. Dyatko, I. V. Kochetov, A. V. Petryakov, V. R. Soloviev, Cheng Zhang
{"title":"On the Applicability of the Local Approximation for the EEDF in Modeling Surface Barrier Discharges and Volume Streamers","authors":"Yu. S. Akishev, N. A. Dyatko, I. V. Kochetov, A. V. Petryakov, V. R. Soloviev, Cheng Zhang","doi":"10.1134/S1063780X26601318","DOIUrl":"10.1134/S1063780X26601318","url":null,"abstract":"<p>The applicability of the local approximation for the electron energy distribution function has been investigated by performing comparative calculations of the electron kinetic characteristics in a specified one-dimensional spatially non-uniform electric field using two methods: by solving the local Boltzmann equation and by the Monte Carlo method. Two situations are considered in which the use of the Monte Carlo method is justified by the physical formulation of the problem: simulation of electron motion in the front region of a positive volume streamer in helium, and simulation of electron motion starting from a surface and moving in the high-field region of the near-wall plasma behind the front of a negative barrier surface discharge in nitrogen.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1381 - 1392"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1134/S1063780X26601318.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309532","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}
{"title":"Two Models of Fast Streamer Discharge in a Thundercloud","authors":"I. M. Kutsyk, E. I. Bochkov","doi":"10.1134/S1063780X26600830","DOIUrl":"10.1134/S1063780X26600830","url":null,"abstract":"<p>Two variants of the mechanism of fast streamer discharge in a thundercloud are considered: an avalanche of streamers and a streamerization wave. In both cases, polarization of the medium is assumed as a result of the creation and branching of streamers. In the first case, the discharge speed is determined by the speed of movement of streamers in the field at the front, and in the second case, by the speed of the wave initiating streamer flashes by the electric field of the polarization wave. The second mechanism is based on the assumptions of small-scale inhomogeneity of the field and the initiation of streamers from large hydrometeors by seed electrons arising as a result of plasma-chemical reactions of detachment from negative ions. The analysis conducted showed the irreparable shortcomings of the first mechanism. The proposed wave mechanism allows us to explain the results of observations of a fast streamer discharge under various conditions. This mechanism predicts two types of fast discharges involving streamers, initiated either by seed electrons generated by extensive air showers (EAS) or by changes in the electric field during the movement of the leader in the intracloud discharge.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1408 - 1418"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309672","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}
{"title":"Kinetic Scheme of a Subthreshold Microwave Microsecond Discharge in a Nitrogen–Oxygen Mixture Considering Oscillatory Kinetics","authors":"Z. A. Zakletskii","doi":"10.1134/S1063780X26601045","DOIUrl":"10.1134/S1063780X26601045","url":null,"abstract":"<p>A study was conducted of plasma-chemical kinetics in the spatial diffusion zone of a subthreshold microwave discharge in air at atmospheric pressure, initiated by microwave radiation with a frequency of 75 GHz and a field strength of 2.4 kV/cm. The calculation model is based on an extended kinetic scheme that takes into account in detail the level-by-level VV and VT transitions with nitrogen and oxygen molecules. It is shown that under conditions of room temperature (300 K) and microsecond pulses, the contribution of vibrational excitation to the overall plasma dynamics is negligible. On the contrary, in the high-temperature regime (~5000 K) at an electron density of 8 × 10<sup>13</sup> cm<sup>−3</sup> oscillatory kinetics becomes decisive. It was established that the generation of nitric oxide under these conditions is limited by the Zeldovich mechanism, and the population of the reacting molecules obeys a distribution close to the Boltzmann one. The reliability of the model is confirmed by the coincidence of the calculated NO content in the afterglow (10<sup>18</sup> cm<sup>−3</sup>) with independent experimental data.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1393 - 1407"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1134/S1063780X26601045.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309538","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}
{"title":"On Nonlinear Wave Structures in Plasma Containing Electrons, Ions, Positrons, and Dust Particles with Variable Charges","authors":"Yu. N. Izvekova, S. I. Popel, O. Ya. Izvekov","doi":"10.1134/S1063780X26601239","DOIUrl":"10.1134/S1063780X26601239","url":null,"abstract":"<p>The possibility of the existence of dust ion-acoustic shock-wave structures associated with anomalous dissipation caused, among other things, by variations in the charges of dust particles in dusty plasma containing, along with electrons and ions, also positrons, is shown. It turns out that the presence of positrons in the plasma expands the region of existence of shock waves, and also reduces the amplitude of the shock wave and increases the width of its front. Moreover, even a small fraction of positrons can have a significant impact on the properties of the shock-wave structure, which is significantly weakened in the presence of positrons. The influence of positrons on shock-wave structures in cosmic dusty plasmas may, in certain situations, modify conclusions regarding the role of shock waves in the formation of stars or the nature of the propagation of shock waves generated by supernova explosions.</p>","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"52 10","pages":"1346 - 1351"},"PeriodicalIF":1.0,"publicationDate":"2026-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149309671","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}