Plasma Physics Reports最新文献_第3页

Microwave Discharge Supported by Gyrotron Radiation on a Dielectric Substrate with Silver Particles in Air to Create a Metallized Coating on ABS Plastic 在空气中含有银粒子的介电基片上以回旋辐射支持微波放电制备ABS塑料金属化涂层

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-09-03 DOI: 10.1134/S1063780X25602639

Z. A. Zakletskii, D. V. Malakhov, S. E Andreev

引用次数: 0

Dusty Plasma in the Solar System: Atmospheres of Planets 太阳系中的尘埃等离子体：行星的大气层

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-09-03 DOI: 10.1134/S1063780X25602780

S. I. Popel, Yu. S. Reznichenko, S. I. Kopnin, Yu. N. Izvekova, A. Yu. Dubinskii, L. M. Zelenyi

引用次数: 0

Fully Vaporization of the Electrically Exploding Platinum Wires in Vacuum 电爆炸铂丝在真空中的完全汽化

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-07-30 DOI: 10.1134/S1063780X24601822

Sh. Wang, J. Zhou, H. Yu, N. Li, K. Guo, T. Wang, M. Cheng, S. Zhang, Zh. Li, K. Wang

{"title":"Fully Vaporization of the Electrically Exploding Platinum Wires in Vacuum","authors":"Sh. Wang, J. Zhou, H. Yu, N. Li, K. Guo, T. Wang, M. Cheng, S. Zhang, Zh. Li, K. Wang","doi":"10.1134/S1063780X24601822","DOIUrl":"10.1134/S1063780X24601822","url":null,"abstract":"Experimental results characterizing the dynamics of the electrically exploding platinum wires without and with insulating coatings are presented. The insulating coatings substantially enhance the energy deposition with the overheating coefficients increasing from 0.5 for exploding bare platinum wires to 1.3 for exploding coated platinum wires with 2 cm in length. Although the homogeneous vaporized platinum wires can be realized in the exploding coated platinum wires, the exploding products exhibits a strong stochastic behavior. Most of the electrically exploding platinum wires produce inhomogeneous structures in energy deposition. Shortening the wire length further increases the specific energy deposition. The total deposited energy is high enough to vaporize the entire wire, while only a part of the wire is transformed into gaseous state. The percentage of vaporization increases almost linearly with the axial electrical field. With decrease of the wire length from 2 to 0.5 cm, the specific energy deposition increases from 2.6 to 14.9 eV/atom, and the percentage of vaporization improves from 52 to 92%.","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 4","pages":"496 - 503"},"PeriodicalIF":1.1,"publicationDate":"2025-07-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145170609","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}

引用次数: 0

Generation of Synchrotron Radiation During the Interaction between a Multiterrawatt Laser Pulse and a Transparent Plasma 多太瓦激光脉冲与透明等离子体相互作用时同步辐射的产生

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-07-30 DOI: 10.1134/S1063780X25602597

O. E. Vais, M. G. Lobok, V. Yu. Bychenkov

引用次数: 0

Electromagnetic and Centrifugal Effects on Plasma Acceleration in the Magnetic Nozzle 电磁和离心效应对磁喷嘴内等离子体加速度的影响

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-07-30 DOI: 10.1134/S1063780X25602214

A. I. Smolyakov, A. Sabo, S. I. Krasheninnikov, P. N. Yushmanov

{"title":"Electromagnetic and Centrifugal Effects on Plasma Acceleration in the Magnetic Nozzle","authors":"A. I. Smolyakov, A. Sabo, S. I. Krasheninnikov, P. N. Yushmanov","doi":"10.1134/S1063780X25602214","DOIUrl":"10.1134/S1063780X25602214","url":null,"abstract":"Plasma flow and acceleration in the converging-diverging magnetic field configuration, such as magnetic nozzle in electric propulsion and open magnetic mirrors for fusion applications are considered. This work analyses plasma acceleration in the magnetic nozzle with an emphasis on the electromagnetic effects and centrifugal forces due to plasma rotation. Intrinsic coupling of the azimuthal rotation and azimuthal magnetic field is analyzed, and additional plasma acceleration due to the conversion of the energy of the azimuthal magnetic field and azimuthal rotation is demonstrated. For large expansion in the diverging magnetic field plasma flow velocities may approach and exceed the Alfvén velocity. In these regimes, stationary solutions for the transonic and trans-Alfvénic flows have been obtained that demonstrate the existence of the unique regular solution passing through all critical points within the MHD theory, i.e., the points where the plasma flow is equal to the signal velocities of the MHD modes: slow and fast magnetohydrodynamic waves and Alfvén wave. The time-dependent initial value simulations show that stationary equilibrium flows are robust and stable, so that time-dependent solutions converge toward stationary solutions.","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 4","pages":"427 - 438"},"PeriodicalIF":1.1,"publicationDate":"2025-07-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145170611","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}

引用次数: 0

Numerical Simulation of Expansion of Artificial Plasma Formations in the Geomagnetic Field 人造等离子体在地磁场中膨胀的数值模拟

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-07-30 DOI: 10.1134/S1063780X25602743

E. M. Urvachev, T. V. Losseva, E. S. Goncharov, A. N. Lyakhov

引用次数: 0

Numerical Study for Prediction of Neon Soft X-Ray Yield Emitted from the Plasma Focus Devices Using the Lee Model Code for Different Anode Shapes 不同阳极形状下等离子体聚焦器件氖软x射线产率的Lee模型码预测数值研究

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-07-30 DOI: 10.1134/S1063780X2460169X

R. Albahri, Y. Abou-Ali, M. Akel

{"title":"Numerical Study for Prediction of Neon Soft X-Ray Yield Emitted from the Plasma Focus Devices Using the Lee Model Code for Different Anode Shapes","authors":"R. Albahri, Y. Abou-Ali, M. Akel","doi":"10.1134/S1063780X2460169X","DOIUrl":"10.1134/S1063780X2460169X","url":null,"abstract":"Numerical experiments were performed using the Lee model code to study the soft X-ray characteristics versus pressure at different operating voltages of the NX2 plasma focus device for two types of anodes (cylindrical and tapered). It was observed that the computed yield increased by 5 times when switching from the cylindrical anode to the tapered one, which agreed with the experimental results. Later, numerical experiments were conducted to study the effect of the different tapering conditions (anode radius at the end of the taper and axial distance at the start of the taper) on the soft X-ray yield, interesting results were reached. We found that the yield is not related to the axial distance for the taper start, but is largely related to the end anode radius of the taper, as there is an optimum end anode radius of the taper that gives the highest yield for soft X-ray. The convergence in previous computed and measured results was taken advantage to conduct numerical experiments on the PF-24 device to find the soft X-ray characteristics and the maximum soft X-ray yield corresponding to the optimum pressure for different anode shapes (cylindrical and tapered). In addition, numerical experiments were conducted to find the optimum conditions of geometric dimensions of the cylindrical anode (anode radius, anode length), and tapering conditions (anode radius at the end of the taper and axial distance at the start of the taper) which give the maximum soft X-ray yield for PF-24 device. The results obtained for the PF-24 device behave identically to the behavior of the results obtained for the NX2 device.","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 4","pages":"484 - 495"},"PeriodicalIF":1.1,"publicationDate":"2025-07-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145171626","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}

引用次数: 0

Evolution of High Energy Density in Plasma Formed upon Irradiation of Steel Foils by Ultrarelativistic Femtosecond Laser Pulses 超相对论飞秒激光脉冲辐照钢箔后等离子体高能量密度的演化

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-07-30 DOI: 10.1134/S1063780X25602810

M. V. Sedov, M. A. Alkhimova, S. S. Makarov

{"title":"Evolution of High Energy Density in Plasma Formed upon Irradiation of Steel Foils by Ultrarelativistic Femtosecond Laser Pulses","authors":"M. V. Sedov, M. A. Alkhimova, S. S. Makarov","doi":"10.1134/S1063780X25602810","DOIUrl":"10.1134/S1063780X25602810","url":null,"abstract":"Results of the particle-in-cell simulation that illustrate evolution of parameters of laser-produced plasma formed upon irradiation of steel foils with a thickness of 1–5 µm by femtosecond laser pulses with intensity of ≥5 × 1021 W/cm2 are presented. Analytical estimates for analysis of energy dissipation in a foil of finite thickness are obtained. Numerical simulations are compared with the results of the recent experiment in which diagnostics of plasma parameters was carried out by methods of X-ray spectroscopy. The results of simulation agree with the experimental results and confirm that a microscopic-sized plasma source with energy density exceeding 1 GJ/cm3 and lifetime of about 500 fs can be formed as a result of action of high-contrast femtosecond laser pulses of ultrarelativistic intensity. In addition, simulations demonstrate that a plasma source with a volume of ~1 µm3 and lifetime of ~5 light periods that has parameters close to those existing inside the Sun, i.e., the temperature of ~1–3 keV and energy density of ≥10 GJ/cm3 (pressure of ≥100 Gbar), can be formed under the same parameters of the experiment.","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 4","pages":"451 - 457"},"PeriodicalIF":1.1,"publicationDate":"2025-07-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145171714","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}

引用次数: 0

Methods for Processing Signals of Magnetic Probes at the T-15MD Tokamak T-15MD托卡马克磁探头信号处理方法

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-07-30 DOI: 10.1134/S1063780X25602317

A. D. Izarova, A. M. Belov, L. G. Eliseev, A. V. Sushkov, A. Yu. Balashov, A. V. Stepin, K. A. Rogozin, G. A. Sarancha

引用次数: 0

Nonlinear Dust Acoustic Waves near the Surface of Phobos and Deimos 火卫一和火卫二表面附近的非线性尘埃声波

IF 1.1 4区物理与天体物理

Plasma Physics Reports Pub Date : 2025-07-30 DOI: 10.1134/S1063780X25602767

Yu. N. Izvekova, S. I. Kopnin, S. I. Popel

{"title":"Nonlinear Dust Acoustic Waves near the Surface of Phobos and Deimos","authors":"Yu. N. Izvekova, S. I. Kopnin, S. I. Popel","doi":"10.1134/S1063780X25602767","DOIUrl":"10.1134/S1063780X25602767","url":null,"abstract":"Phobos and Deimos are atmosphereless celestial bodies with a weak gravity. Their surfaces consist of small regolith grains that are not connected to one another and have appeared due to bombardment with micrometeorites. Their weak gravity makes these bodies interesting for piloted flights and increases the role of dust, since even a small perturbation leads to the creation of massive dust clouds above their surfaces. The surfaces of these satellites of Mars are charged by the electromagnetic radiation from the Sun and the plasma of the solar wind. The dust grains located at the surface and in the near-surface layer absorb the photons, photoelectrons, electrons, and ions of the solar wind, and, as a result, they obtain electric charge. The action of the electrostatic force under the weak gravity conditions leads to the detachment of dust grains from the surface and the creation of a dusty plasma system together with the electrons and ions. In the dusty plasma system above the surfaces of Mars’s satellites, dust acoustic waves can propagate. In this work, we consider nonlinear periodic and solitary dust acoustic waves with an arbitrary amplitude, which can propagate near the surface of Phobos and Deimos, and discuss the possibility of observing these structures.","PeriodicalId":735,"journal":{"name":"Plasma Physics Reports","volume":"51 4","pages":"458 - 463"},"PeriodicalIF":1.1,"publicationDate":"2025-07-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145171715","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}

引用次数: 0