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Статті в журналах з теми "Plasma non collisionels"
Zhang, Yanzeng, and Xian-Zhu Tang. "On the collisional damping of plasma velocity space instabilities." Physics of Plasmas 30, no. 3 (March 2023): 030701. http://dx.doi.org/10.1063/5.0136739.
Повний текст джерелаZhang, Yanzeng, Yuzhi Li, Bhuvana Srinivasan, and Xian-Zhu Tang. "Resolving the mystery of electron perpendicular temperature spike in the plasma sheath." Physics of Plasmas 30, no. 3 (March 2023): 033504. http://dx.doi.org/10.1063/5.0132612.
Повний текст джерелаFan, Kaixuan, Xueqiao Xu, Ben Zhu, and Pengfei Li. "Kinetic Landau-fluid closures of non-Maxwellian distributions." Physics of Plasmas 29, no. 4 (April 2022): 042116. http://dx.doi.org/10.1063/5.0083108.
Повний текст джерелаBret, Antoine, and Ramesh Narayan. "Density jump for parallel and perpendicular collisionless shocks." Laser and Particle Beams 38, no. 2 (April 14, 2020): 114–20. http://dx.doi.org/10.1017/s0263034620000117.
Повний текст джерелаYANG, Wei, Fei GAO, and Younian WANG. "Conductivity effects during the transition from collisionless to collisional regimes in cylindrical inductively coupled plasmas." Plasma Science and Technology 24, no. 5 (April 13, 2022): 055401. http://dx.doi.org/10.1088/2058-6272/ac56ce.
Повний текст джерелаMcCubbin, Andrew J., Gregory G. Howes, and Jason M. TenBarge. "Characterizing velocity–space signatures of electron energization in large-guide-field collisionless magnetic reconnection." Physics of Plasmas 29, no. 5 (May 2022): 052105. http://dx.doi.org/10.1063/5.0082213.
Повний текст джерелаHong, Young-Hun, Tae-Woo Kim, Ju-Ho Kim, Yeong-Min Lim, Moo-Young Lee, and Chin-Wook Chung. "Experimental investigation on the hysteresis in low-pressure inductively coupled neon discharge." Physics of Plasmas 29, no. 9 (September 2022): 093506. http://dx.doi.org/10.1063/5.0092091.
Повний текст джерелаKaganovich, I. D., V. I. Demidov, S. F. Adams, and Y. Raitses. "Non-local collisionless and collisional electron transport in low-temperature plasma." Plasma Physics and Controlled Fusion 51, no. 12 (November 10, 2009): 124003. http://dx.doi.org/10.1088/0741-3335/51/12/124003.
Повний текст джерелаAlharbi, A., I. Ballai, V. Fedun, and G. Verth. "Waves in weakly ionized solar plasmas." Monthly Notices of the Royal Astronomical Society 511, no. 4 (February 18, 2022): 5274–86. http://dx.doi.org/10.1093/mnras/stac444.
Повний текст джерелаHaggerty, Colby C., Antoine Bret, and Damiano Caprioli. "Kinetic simulations of strongly magnetized parallel shocks: deviations from MHD jump conditions." Monthly Notices of the Royal Astronomical Society 509, no. 2 (November 1, 2021): 2084–90. http://dx.doi.org/10.1093/mnras/stab3110.
Повний текст джерелаДисертації з теми "Plasma non collisionels"
Granier, Camille. "Nouveaux développements sur la théorie des instabilités des feuilles de courant dans les plasmas non-collisionels." Electronic Thesis or Diss., Université Côte d'Azur, 2022. http://www.theses.fr/2022COAZ4109.
Повний текст джерелаMagnetic reconnection is a change of topology of the magnetic field, responsible for explosive release of magnetic energy in astrophysical plasmas, as in the case of magnetospheric substorms and coronal mass ejections, as well as in laboratory plasmas, which is the case of sawtooth crashes in tokamaks. In collisionless plasmas as, for instance, the magnetosphere and the solar wind, electron inertia becomes particularly relevant to drive reconnection at regions of intense localized current, denoted as current sheets. In these non-collisional environments, the temperature can often be anisotropic and effects at the electron scale on the reconnection process can become non-negligible.In this thesis, the stability of two-dimensional current sheets, with respect to reconnecting perturbations, in collisionless plasmas with a strong guide field is analysed on the basis of gyrofluid models assuming cold ions. These models can take into account an equilibrium temperature anisotropy,and a finite βe, a parameter corresponding to the ratio between equilibrium electron kinetic pressure and magnetic pressure.We derive and analyze a dispersion relation for the growth rate of collisionless tearing modes accounting for equilibrium electron temperature anisotropy. The analytical predictions are tested against numerical simulations, showing a very good quantitative agreement.In the isotropic case, accounting for finite βe effects, we observe a stabilization of the tearing growth rate when electron finite Larmor radius effects become relevant. In the nonlinear phase, stall phases and faster than exponential phases are observed, similarly to what occurs in the presence of ion finite Larmor radius effects.We also investigate the marginal stability conditions of secondary current sheets, for the development of plasmoids, in collisionless plasmas. In the isotropic βe → 0 regime, we analyze the geometry that characterizes the reconnecting current sheet, and identify the conditions for which it is plasmoid unstable. Our study shows that plasmoids can be obtained, in this context, from current sheets with an aspect ratio much smaller than in the collisional regime. Furthermore, we investigate the plasmoid formation comparing gyrofluid and gyrokinetic simulations.This made it possible to show that the effect of finite βe, promotes the plasmoid instability. Finally, we study the impact of the closure applied on the moments, performed during the derivation of the gyrofluid model, on the distribution and conversion of energy during reconnection
La riconnessione magnetica è un cambiamento nella topologia delcampo magnetico, responsabile del rilascio esplosivo di energia magnetica nei plasmiastrofisici, come nelle tempeste magnetosferiche e nelle espulsioni di massa coronale,nonché nei plasmi di laboratorio, come nel caso delle oscillazioni a dente di sega neitokamak. Nei plasmi non-collisionali come, ad esempio, la magnetosfera e il vento solare,l’inerzia elettronica diventa particolarmente efficace nel causare la riconnessionein regioni di corrente intensa e localizzata, detti strati di corrente. In tali plasmi noncollisionali,la temperatura può essere spesso anisotropa e gli effetti su scala elettronicasul processo di riconnessione possono diventare non trascurabili.In questa tesi, viene analizzata la stabilità di strati di corrente bidimensionali inplasmi non-collisionali con un forte campo guida, sulla base di modelli girofluidi cheassumono ioni freddi. Questi modelli possono tenere conto di un’anisotropia di temperaturadi equilibrio e di un βe finito. Quest’ultimo è un parametro corrispondente alrapporto tra la pressione cinetica elettronica di equilibrio e la pressione magnetica.Deriviamo e analizziamo una relazione di dispersione per il tasso di crescita dei moditearing non-collisionali tenendo conto dell’anisotropia della temperatura di equilibriodegli elettroni. Le previsioni analitiche sono verificate mediante simulazioni numeriche,che mostrano un ottimo accordo quantitativo. Nel caso isotropico, tenendoconto degli effetti di βe finito, si osserva una stabilizzazione del tasso di crescita delmodo tearing quando diventano rilevanti gli effetti del raggio finito di Larmor deglielettroni. Nella fase non lineare si osservano fasi di decelerazione e fasi di accelerazione,simili a quanto avviene in presenza di effetti del raggio di Larmor finito ionico.Studiamo anche le condizioni di stabilità marginale degli strati di corrente secondaria,per lo sviluppo di plasmoidi, in plasmi senza collisioni. Nel regime isotropicocon βe → 0, analizziamo la geometria che caratterizza lo strato di corrente e identifichiamole condizioni in cui esso diventa instabile a causa di un’instabilità che generaplasmoidi. Il nostro studio mostra che i plasmoidi possono essere ottenuti, in questocontesto, da strati di corrente aventi un rapporto d’aspetto molto più piccolo rispettoal regime collisionale. Inoltre, studiamo la formazione di plasmoidi confrontando simulazionigirofluidi e girocinetiche. Ciò ha permesso di dimostrare che l’effetto di βe promuove l’instabilità che genera plasmoidi. Infine, si studia l’impatto della chiusuraapplicata ai momenti, eseguita durante la derivazione del modello girofluido, sulla distribuzionee conversione dell’energia durante la riconnessione
Capdessus, Rémi. "Dynamique d'un plasma non collisionnel interagissant avec une impulsion laser ultra-intense." Thesis, Bordeaux 1, 2013. http://www.theses.fr/2013BOR15268/document.
Повний текст джерелаRésumé en anglais
Ruyer, Charles. "Kinetic instabilities in plasmas : from electromagnetic fluctuations to collisionless shocks". Thesis, Paris 11, 2014. http://www.theses.fr/2014PA112370/document.
Повний текст джерелаCollisionless shocks play a major role in powerful astrophysical objects (e.g., gamma-ray bursts, supernova remnants, pulsar winds, etc.), where they are thought to be responsible for non-thermal particle acceleration and radiation. Numerical simulations have shown that, in the absence of an external magnetic field, these self-organizing structures originate from electromagnetic instabilities triggered by high-velocity colliding flows. These Weibel-like instabilities are indeed capable of producing the magnetic turbulence required for both efficient scattering and Fermi-type acceleration. Along with rapid advances in their theoretical understanding, intense effort is now underway to generate collisionless shocks in the laboratory using energetic lasers. In a first part we study the (w,k)-resolved electromagnetic thermal spectrum sustained by a drifting relativistic plasma. In particular, we obtain analytical formulae for the fluctuation spectra, the latter serving as seeds for growing magnetic modes in counterstreaming plasmas. Distinguishing between subluminal and supraluminal thermal fluctuations, we derived analytical formulae of their respective spectral contributions. Comparisons with particle-in-cell (PIC) simulations are made, showing close agreement in the subluminal regime along with some discrepancy in the supraluminal regime. Our formulae are then used to estimate the saturation time of the Weibel instability of relativistic pair plasmas. Our predictions are shown to match 2-D particle-in-cell (PIC) simulations over a three-decade range in flow energyWe then develop a predictive kinetic model of the nonlinear phase of the Weibel instability induced by two counter-streaming, symmetric and non-relativistic ion beams. This self consistent, fully analytical model allows us to follow the evolution of the beams' properties up to a stage close to complete isotropization and thus to shock formation. Its predictions are supported by 2D and 3D particle-in-cell (PIC) simulations of the ion Weibel instability in uniform geometries, as well as shock-relevant non-uniform configurations. Moreover, they are found in correct agreement with a recent laser-driven plasma collision experiment. Along with this comparison, we pinpoint the important role of electron screening on the ion-Weibel dynamics, which may affect the results of simulations with artificially high electron mass. We subsequently address the shock propagation resulting from the magnetic Weibel turbulence generated in the upstream region. Generalizing the previous symmetric-beam model to the upstream region of the shock, the role of the magnetic turbulence in the shock-front has been analytically and self-consistently characterized. Comparison with simulations validates the model. The interaction of high-energy, ultra-high intensity lasers with dense plasmas is known to produce copious amounts of suprathermal particles. Their acceleration and subsequent transport trigger a variety of Weibel-like electromagnetic instabilities, acting as additional sources of slowing down and scattering. Their understanding is important for the many applications based upon the energy deposition and/or field generation of laser-driven particles. We investigate the ability of relativistic-intensity laser pulses to induce Weibel instability-mediated shocks in overdense plasma targets, as first proposed by Fiuza in 2012. By means of both linear theory and 2D PIC simulations, we demonstrated that in contrast to the standard astrophysical scenario previously addressed, the early-time magnetic fluctuations (Weibel instability) generated by the suprathermal electrons (and not ions) are strong enough to isotropize the target ions and, therefore, induce a collisionless electromagnetic shock
Figua, Habiba. "Contribution des codes euleriens en physique des plasmas non collisionnels." Orléans, 1999. http://www.theses.fr/1999ORLE2037.
Повний текст джерелаGrassi, Anna. "Collisionless shocks in the context of Laboratory Astrophysics." Thesis, Paris 6, 2017. http://www.theses.fr/2017PA066483/document.
Повний текст джерелаThe work presented in this thesis belongs to the general framework of Laboratory Astrophysics. We address various aspects of the physics of collisionless shocks developing in the presence of relativistic plasma flows, in configurations of interest for the astrophysical and the laser-plasma interaction (LPI) communities. The approach used throughout this thesis relied on both analytical modeling and high-performance kinetic simulations, a central tool to describe LPI processes as well as the non-linear physics behind shock formation. The PIC code SMILEI has been widely used and developed during this work. Three physical configurations are studied. First we consider the Weibel instability driven by two counter-streaming electron beams aligned with an external magnetic field. The linear and non-linear phases are explained using theoretical models confirmed by simulations.Then the generation of non-collisional shocks during the interaction of two relativistic plasma pairs is studied in the presence of a perpendicular magnetic field. We focus on the comparison of theoretical predictions for macroscopic variables with the simulation results, as well as on the definition and measurement of the shock formation time, all of which are of great importance for future experiments.Finally, we proposed a scheme to produce, in the laboratory, the ion-Weibel-instability with the use of an ultra-high-intensity laser. The produced flows are faster and denser than in current experiments, leading to a larger growth rate and stronger magnetic fields. These results are important for the LPI at very high intensity
Moreno-Gelos, Quentin. "Non-relativistic collisionless shocks in Laboratory Astrophysics." Thesis, Bordeaux, 2018. http://www.theses.fr/2018BORD0427/document.
Повний текст джерелаCollisionless shocks are ubiquitous in the Universe, especially in the supernova remnants, and are formed via various plasma instabilities mainly depending on the speed and magnetization of plasma flows. The description of such shocks requires a kinetic approach, both analytical and numerical.In this thesis, we have studied, through Particle-In-Cell (PIC) simulations, the underlying processes by which instabilities compete with each other.We have shown that the reduction of the ion-to-electron mass ratio, often used in numerical simulations to accelerate the dynamics of shocks, can have strong consequences on the energy transfer between particles during the non-linear phase of instabilities.These instabilities, like the ionic acoustic instability (IAI) lead under certain conditions to the formation of electrostatic shocks, which can give rise to phase space holes formation, propagating in the downstream shock region, and accelerating the shock.The addition of an external magnetic field leads to different shock mediation, which can vary between the IAI to the slow or fast magneto-sonic waves as a function of the obliquity between the magnetic field and the shock normal.Furthermore, we have shown that the orientation of the magnetic field makes it possible to choose between a convex or concave dispersion of the plasma waves leading to the creation of precursor waves in the upstream or downstream shock regions.These magnetized shocks are correctly represented by the magnetohydrodynamic (MHD) model as long as they remain laminar and their potential in the downstream region is not large enough to reflect the particles of the upstream medium.We have shown that even for sub-critical shocks, a fraction of reflected ions, which cannot be modeled by the MHD, is sufficient for the growth of solitary waves upstream of the shock, leading to the acceleration of the latter, but not to a process of 'self-reformation' as for super-critical shocks.Although spatio-temporal scales are very different, scaling laws make possible the study of such phenomena in the laboratory. Our numerical studies have been done in the context of shock tubes that can be experimentally tested.As such, we propose in this thesis an experiment on the creation of magnetic islands, formed by the interaction of plasmas generated by the irradiation of laser targets bathed in an external magnetic field, leading to the formation of such shocks.Finally, we experimentally and numerically demonstrated the formation of collisionless electromagnetic shocks through the Weibel instability stimulated by theBiermann Battery instability, and leading to particle acceleration by the Fermi mechanism.This new type of experiment could explain the origin of cosmic radiation from supernova remnants
Saussede, Florence. "Simulation numérique d'un choc non collisionnel en physique des plasmas." Bordeaux 1, 1993. http://www.theses.fr/1993BOR10546.
Повний текст джерелаMusatenko, Kateryna. "Analyse des caractéristiques d'ondes au voisinage des chocs dans des plasmas spatiaux : observations des satellites CLUSTER, modélisation et interprétation." Phd thesis, Université d'Orléans, 2009. http://tel.archives-ouvertes.fr/tel-00452683.
Повний текст джерелаPantellini, Filippo. "Etude de la structure des chocs non collisionnels dans les plasmas spatiaux." Paris 7, 1992. http://www.theses.fr/1992PA077148.
Повний текст джерелаMelzani, Mickaël. "Reconnexion magnétique non-collisionelle dans les plasmas relativistes et simulations particle-in-cell." Thesis, Lyon, École normale supérieure, 2014. http://www.theses.fr/2014ENSL0946/document.
Повний текст джерелаThe purpose of this thesis is to study magnetic reconnection in collisionless and relativistic plasmas. Such plasmas can be encountered in various astrophysical objects (microquasars, AGNs, GRBs...), where reconnection could explain high-energy particle and photon production, plasma heating, or transient large-scale outflows. However, a first principle understanding of reconnection is still lacking, especially in relativistic ion-electron plasmas. We first present the basis of reconnection physics. We derive results relevant to relativistic plasma physics, including properties of the Maxwell-Jüttner distribution. Then, we provide a detailed study of our numerical tool, particle-in-cell simulations (PIC). The fact that the real plasma contains far less particles than the PIC plasma has important consequences concerning relaxation times or noise, that we describe. Finally, we study relativistic reconnection in ion-electron plasmas with PIC simulations. We stress outstanding properties: Ohm's law (dominated by bulk inertia), structure of the diffusion zone, energy content of the outflows (thermally dominated), reconnection rate (and its relativistic normalization). Ions and electrons produce power law distributions, with indexes that depend on the inflow Alfvén speed and on the magnetization of the corresponding species. They can be harder than those produced by collisionless shocks. Also, ions can get more or less energy than the electrons, depending on the guide field strength. These results provide a solid ground for astrophysical models that, up to now, assumed with no prior justification the existence of such distributions or of such ion/electron energy repartition
Книги з теми "Plasma non collisionels"
Morawetz, Klaus. Deep Impurities with Collision Delay. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198797241.003.0017.
Повний текст джерелаЧастини книг з теми "Plasma non collisionels"
Tsytovich, Vadim N. "Fluctuations and Particle Collisions." In Lectures on Non-linear Plasma Kinetics, 75–106. Berlin, Heidelberg: Springer Berlin Heidelberg, 1995. http://dx.doi.org/10.1007/978-3-642-78902-1_4.
Повний текст джерелаNovikov, Vladimir G. "Average Atom Approximation in Non-LTE Level Kinetics." In Modern Methods in Collisional-Radiative Modeling of Plasmas, 105–26. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-27514-7_5.
Повний текст джерелаFerland, G. J., and R. J. R. Williams. "Spectral Modeling in Astrophysics—The Physics of Non-equilibrium Clouds." In Modern Methods in Collisional-Radiative Modeling of Plasmas, 153–80. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-27514-7_7.
Повний текст джерелаBykov, A. M., M. A. Malkov, J. C. Raymond, A. M. Krassilchtchikov, and A. E. Vladimirov. "Collisionless Shocks in Partly Ionized Plasma with Cosmic Rays: Microphysics of Non-thermal Components." In Microphysics of Cosmic Plasmas, 523–56. Boston, MA: Springer US, 2013. http://dx.doi.org/10.1007/978-1-4899-7413-6_19.
Повний текст джерелаKorol, Andrey V., and Andrey V. Solov’yov. "PBrS in Non-Relativistic Collisions of Structural Particles with Atoms and Ions." In Springer Series on Atomic, Optical, and Plasma Physics, 121–50. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-45224-6_5.
Повний текст джерелаStock, Reinhard. "Relativistic Nucleus-Nucleus Collisions and the QCD Matter Phase Diagram." In Particle Physics Reference Library, 311–453. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-38207-0_7.
Повний текст джерелаWilson, G. R. "Development of non-Maxwellian velocity distributions as a consequence of nonlocal Coulomb collisions." In Cross‐Scale Coupling in Space Plasmas, 47–60. Washington, D. C.: American Geophysical Union, 1995. http://dx.doi.org/10.1029/gm093p0047.
Повний текст джерелаOgoyski, A. I., and A. B. Blagoev. "Diffusion and Depopulation of the Metastable Cd 3 P0,2 States in Collisions with Neon Atoms." In Advanced Technologies Based on Wave and Beam Generated Plasmas, 499–500. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-017-0633-9_35.
Повний текст джерела"Dynamics of Collisionless Plasma." In Field Theory of Non-Equilibrium Systems, 146–63. 2nd ed. Cambridge University Press, 2023. http://dx.doi.org/10.1017/9781108769266.009.
Повний текст джерелаBers, Abraham. "Kinetic theory of collisions and transport—II. Weakly-ionized plasmas." In Plasma Physics and Fusion Plasma Electrodynamics, 2257–305. Oxford University PressOxford, 2016. http://dx.doi.org/10.1093/acprof:oso/9780199295784.003.0031.
Повний текст джерелаТези доповідей конференцій з теми "Plasma non collisionels"
Quraishi, Qudsia. "Classical collisional diffusion in the annular Penning trap." In NON-NEUTRAL PLASMA PHYSICS IV: Workshop on Non-Neutral Plasmas. AIP, 2002. http://dx.doi.org/10.1063/1.1454311.
Повний текст джерелаBertsche, W. "Collisional Cooling of Pure Electron Plasmas Using CO2." In NON-NEUTRAL PLASMA PHYSICS V: Workshop on Non-Neutral Plasmas. AIP, 2003. http://dx.doi.org/10.1063/1.1635180.
Повний текст джерелаZwicknagel, G. "Energy loss of ions by collisions with magnetized electrons." In NON-NEUTRAL PLASMA PHYSICS IV: Workshop on Non-Neutral Plasmas. AIP, 2002. http://dx.doi.org/10.1063/1.1454322.
Повний текст джерелаKabantsev, Andrey A., and C. Fred Driscoll. "Trapped-Particle-Mediated Collisional Damping of Non-Axisymmetric Plasma Waves." In NON-NEUTRAL PLASMA PHYSICS VI: Workshop on Non-Neutral Plasmas 2006. AIP, 2006. http://dx.doi.org/10.1063/1.2387912.
Повний текст джерелаAnderson, M. W., T. M. O’Neil, James R. Danielson, and Thomas Sunn Pedersen. "Collisional Damping Of Plasma Waves On A Pure Electron Plasma Column." In NON-NEUTRAL PLASMA PHYSICS VII: Workshop on Non-Neutral Plasmas 2008. AIP, 2009. http://dx.doi.org/10.1063/1.3122272.
Повний текст джерелаCoppa, Gianni G. M. "Non-collisional kinetic model for non-neutral plasmas in a Penning trap: General properties and stationary solutions." In NON-NEUTRAL PLASMA PHYSICS IV: Workshop on Non-Neutral Plasmas. AIP, 2002. http://dx.doi.org/10.1063/1.1454327.
Повний текст джерелаDriscoll, C. F., A. A. Kabantsev, D. H. E. Dubin, and Y. A. Tsidulko. "Transport, damping, and wave-couplings from chaotic and collisional neoclassical transport." In NON-NEUTRAL PLASMA PHYSICS VIII: 10th International Workshop on Non-Neutral Plasmas. AIP, 2013. http://dx.doi.org/10.1063/1.4796057.
Повний текст джерелаZwicknagel, Günter. "Ion–electron collisions in a homogeneous magnetic field." In Non-neutral plasma physics III. AIP, 1999. http://dx.doi.org/10.1063/1.1302150.
Повний текст джерелаHollmann, E. M., F. Anderegg, and C. F. Driscoll. "Measurement of cross-magnetic-field heat transport due to long range collisions." In Non-neutral plasma physics III. AIP, 1999. http://dx.doi.org/10.1063/1.1303710.
Повний текст джерелаDubin, Daniel H. E., and Dezhe Z. Jin. "2D collisional diffusion of rods in a magnetized plasma column with finite E×B shear." In Non-neutral plasma physics III. AIP, 1999. http://dx.doi.org/10.1063/1.1302123.
Повний текст джерелаЗвіти організацій з теми "Plasma non collisionels"
Rosenberg, M., and Nicholas A. Krall. Collisional Relaxation of Non-Maxwellian Plasma Distribution in a Polywell (Tradename). Fort Belvoir, VA: Defense Technical Information Center, June 1992. http://dx.doi.org/10.21236/ada257651.
Повний текст джерела