Relevant bibliographies by topics / Computational Plasma Physics

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Computational Plasma Physics'

Author: Grafiati
Published: 4 June 2021
Last updated: 16 February 2022

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Journal articles on the topic "Computational Plasma Physics"

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Koren, Barry, Ute Ebert, Tamas Gombosi, Hervé Guillard, Rony Keppens, and Dana Knoll. "Computational plasma physics." Journal of Computational Physics 231, no. 3 (February 2012): 717. http://dx.doi.org/10.1016/j.jcp.2011.11.012.

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Karney, Charles F. F. "Modern computational techniques in plasma physics." Physics of Plasmas 5, no. 5 (May 1998): 1632–35. http://dx.doi.org/10.1063/1.872831.

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Ostrikov, K., I. Levchenko, and S. Xu. "Computational plasma nanoscience: Where plasma physics meets surface science." Computer Physics Communications 177, no. 1-2 (July 2007): 110–13. http://dx.doi.org/10.1016/j.cpc.2007.02.049.

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Schultz, D. R., P. S. Krstic, T. Minami, M. S. Pindzola, F. J. Robicheaux, J. P. Colgan, S. D. Loch, et al. "Computational atomic physics for plasma edge modeling." Contributions to Plasma Physics 44, no. 13 (April 2004): 247–51. http://dx.doi.org/10.1002/ctpp.200410036.

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Phipps, Claude. "Laser Plasma Physics: Forces and the Nonlinearity Principle." Laser and Particle Beams 19, no. 2 (April 2001): 317. http://dx.doi.org/10.1017/s0263034601002221.

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This is a Landau/Lifschitz-class book. It is a critically important reference work for the whole field of high intensity and/or high plasma density laser-plasma interactions for years to come. It covers everything from single particles to dense fluids, from computational physics to the practical results in fusion, accelerators, you name it. It contains excellent and crystal-clear treatments of the theory of electrodynamics, laser-driven hydrodynamics, the Lorentz force, complex refractive index, and relativistic effects in plasmas. Although “the swamp of plasma physics” is mostly a classical place, Hora clearly indicates where quantum effects must be considered.
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Hewett, Dennis W. "Computational Plasma Physics: With Applications of Fusion and Astrophysics." Fusion Technology 17, no. 2 (March 1990): 362–63. http://dx.doi.org/10.13182/fst90-a39908.

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Mense, Allan T., and Jay I. Frankel. "Computational plasma physics with applications to fusion and astrophysics." Annals of Nuclear Energy 16, no. 9 (January 1989): 487. http://dx.doi.org/10.1016/0306-4549(89)90064-9.

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Hromadka, Jakub, Tomas Ibehej, and Rudolf Hrach. "Computational study of plasma sheath interaction." Physica Scripta T161 (May 1, 2014): 014068. http://dx.doi.org/10.1088/0031-8949/2014/t161/014068.

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Snytnikov, A. V., B. M. Glinskiy, G. B. Zagorulko, and Y. A. Zagorulko. "Ontological approach to formalization of knowledge in computational plasma physics." Journal of Physics: Conference Series 1640 (October 2020): 012013. http://dx.doi.org/10.1088/1742-6596/1640/1/012013.

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Cap, F. F. "Toroidal Boundary Problems in Plasma Physics." ZAMM - Journal of Applied Mathematics and Mechanics / Zeitschrift für Angewandte Mathematik und Mechanik 67, no. 1 (1987): 58–60. http://dx.doi.org/10.1002/zamm.19870670115.

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Dissertations / Theses on the topic "Computational Plasma Physics"

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Kim, Hyun Tae. "Physics and computational simulations of plasma burn-through for tokamak start-up." Thesis, Imperial College London, 2013. http://hdl.handle.net/10044/1/18082.

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This thesis will discuss the fundamental process of high temperature plasma formation, consisting of the Townsend avalanche phase and the subsequent plasma burn-through phase. By means of the applied electric field, the gas is partially ionized by the avalanche process. In order for the electron temperature to increase, the remaining neutrals need to be fully ionized in the plasma burn-through phase, as radiation is the main contribution to the electron power loss. The radiated power loss can be significantly affected by impurities resulting from interaction with the plasma facing components. The parallel transport to the surrounding walls is determined by the so called connection length in the plasma. Previously, plasma burn-through was simulated with the assumptions of constant particle confinement time and impurity fraction. In the new plasma burn-through simulator, called the DYON code, the treatment of particle confinement time is improved with a transonic ambipolar model for parallel transport, by using the effective connection length determined by the magnetic field lines, and Bohm diffusion model for perpendicular transport. In addition, the dynamic evolution of impurity content is calculated in a self-consistent way, using plasma wall interaction models. The recycling of the particles at the walls is also modelled. For a specific application, the recent installation of a beryllium wall at Joint European Torus (JET) enabled to investigate the effects of plasma facing components on plasma formation and build-up of plasma current in the device. According to the JET experiments the Townsend avalanche phase was not influenced by the replacement of the wall material. However, failures during the plasma burn-through phase, that could occur with a carbon wall, are not observed with a beryllium wall. In order to obtain a deeper insight in these effects this thesis will present detailed modelling of plasma burn-through. For the first time a quantitative validation of the simulation results to experimental data is documented. The simulation results with the DYON code show consistent good agreement against JET data obtained with the carbon wall as well as the beryllium wall. According to the DYON results, the radiation barrier in a carbon wall is dominated by the carbon radiation. The radiation barrier in the beryllium wall is mainly from the deuterium radiation rather than the beryllium radiation, as far as the radiated power from other impurities (i.e. carbon, nitrogen, etc) is not significant. These issues are of crucial importance for the International Thermonuclear Experimental Reactor (ITER) where the allowable toroidal electric field for plasma formation is limited to 0.35 V/m, which is significantly lower compared to the typical loop voltage ( 1 V/m) used in the current devices. Using the validated DYON code, predictive simulations for ITER are given, showing a need for RF heating to allow reliable plasma burn-through.
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Cochran, Ginevra E. "New Computational and Experimental Approaches for Studying Ion Acceleration and the Intense Laser-Plasma Interaction." The Ohio State University, 2018. http://rave.ohiolink.edu/etdc/view?acc_num=osu1534432188474908.

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Vanderburgh, Richard N. "One-Dimensional Kinetic Particle-In-Cell Simulations of Various Plasma Distributions." Wright State University / OhioLINK, 2020. http://rave.ohiolink.edu/etdc/view?acc_num=wright1610313011646245.

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Godar, Trenton J. "Testing of Two Novel Semi-Implicit Particle-In-Cell Techniques." Wright State University / OhioLINK, 2014. http://rave.ohiolink.edu/etdc/view?acc_num=wright1402492857.

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Fu, Haiyang. "Modeling of Plasma Irregularities Associated with Artificially Created Dusty Plasmas in the Near-Earth Space Environment." Diss., Virginia Tech, 2013. http://hdl.handle.net/10919/19248.

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Plasma turbulence associated with the creation of an artificial dust layer in the earth's ionosphere is investigated. The Charged Aerosol Release Experiment (CARE) aims to understand the mechanisms for enhanced radar scatter from plasma irregularities embedded in dusty plasmas in space. Plasma irregularities embedded in a artificial dusty plasma in space may shed light on understanding the mechanism for enhanced radar scatter in Noctilucent Clouds (NLCs) and Polar Mesospheric Summer Echoes (PMSEs) in the earth's mesosphere. Artificially created, charged-particulate layers also have strong impact on radar scatter as well as radio signal propagation in communication and surveillance systems. The sounding rocket experiment was designed to develop theories of radar scatter from artificially created plasma turbulence in charged dust particle environment. Understanding plasma irregularities embedded in a artificial dusty plasma in space will also contribute to addressing possible effects of combustion products in rocket/space shuttle exhaust in the ionosphere. In dusty space plasmas, plasma irregularities and instabilities can be generated during active dust aerosol release experiments. Small scale irregularities (several tens of centimeter to meters) and low frequency waves (in the ion/dust scale time in the order of second) are studied in this work, which can be measured by High Frequency (HF), Very High Frequency (VHF) and Ultra High Frequency (UHF) radars. The existence of dust aerosol particles makes computational modeling of plasma irregularities extremely challenging not only because of multiple spatial and temporal scale issue but also due to complexity of dust aerosol particles. This work will provide theoretical and computational models to study plasma irregularities driven by dust aerosol release for the purpose of designing future experiments with combined ground radar, optical and in-situ measurement. In accordance with linear analysis, feasible hybrid computational models are developed to study nonlinear evolution of plasma instabilities in artificially created dusty space plasmas. First of all, the ion acoustic (IA) instability and dust acoustic (DA) instability in homogenous unmagnetized plasmas are investigated by a computational model using a Boltzmann electron assumption. Such acoustic-type instabilities are attributed to the charged dust and ion streaming along the geomagnetic field. Secondly, in a homogenous magnetized dusty plasma, lower-hybrid (LH) streaming instability will be generated by dust streaming perpendicular to the background geomagnetic field. The magnetic field effect on lower-hybrid streaming instabilities is investigated by including the ratio of electron plasma frequency and electron gyro frequency in this model. The instability in weakly magnetized circumstances agree well with that for the ion acoustic (IA) instability by a Boltzmann model. Finally, in an inhomogeneous unmagnetized/magnetized dust boundary layer, possible instabilities will be addressed, including dust acoustic (DA) wave due to flow along the boundary and lower-hybrid (LH) sheared instability due to flow cross the boundary. With applications to active rocket experiments, plasma irregularity features in a linear/nonlinear saturated stage are characterized and predicted. Important parameters of the dust aerosol clouds that impact the evolution of waves will be also discussed for upcoming dust payload generator design. These computational models, with the advantage of following nonlinear wave-particle interaction, could be used for space dusty plasmas as well as laboratory dusty plasmas.
Ph. D.
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Hedlof, Ryan. "Artificially Structured Boundary for Control and Confinement of Beams and Plasmas." Thesis, University of North Texas, 2018. https://digital.library.unt.edu/ark:/67531/metadc1157511/.

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An artificially structured boundary (ASB) produces a short-range, static electromagnetic field that can reflect charged particles. In the work presented, an ASB is considered to consist of a spatially periodic arrangement of electrostatically plugged magnetic cusps. When used to create an enclosed volume, an ASB may confine a non-neutral plasma that is effectively free of applied electromagnetic fields, provided the spatial period of the ASB-applied field is much smaller than any one dimension of the confinement volume. As envisioned, a non-neutral positron plasma could be confined by an ASB along its edge, and the space-charge of the positron plasma would serve to confine an antiproton plasma. If the conditions of the two-species plasma are suitable, production of antihydrogen via three-body recombination for antimatter gravity studies may be possible. A classical trajectory Monte Carlo (CTMC) simulation suite has been developed in C++ to efficiently simulate charged particle interactions with user defined electromagnetic fields. The code has been used to explore several ASB configurations, and a concept for a cylindrically symmetric ASB trap that employs a picket-fence magnetic field has been developed. Particle-in-cell (PIC) modeling has been utilized to investigate the confinement of non-neutral and partially neutralized positron plasmas in the trap.
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Rathod, Chirag. "Examining Plasma Instabilities as Ionospheric Turbulence Generation Mechanisms Using Pseudo-Spectral Methods." Diss., Virginia Tech, 2021. http://hdl.handle.net/10919/102892.

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Turbulence in the ionosphere is important to understand because it can negatively affect communication signals. This work examines different scenarios in the ionosphere in which turbulence may develop. The two main causes of turbulence considered in this work are the gradient drift instability (GDI) and the Kelvin-Helmholtz instability (KHI). The likelihood of the development of the GDI during the August 17, 2017 total solar eclipse is studied numerically. This analysis uses the ``Sami3 is Also a Model of the Ionosphere" (SAMI3) model to study the effect of the eclipse on the plasma density. The calculated GDI growth rates are small compared to how quickly the eclipse moves over the Earth. Therefore, the GDI is not expected to occur during the solar eclipse. A novel 2D electrostatic pseudo-spectral fluid model is developed to study the growth of these two instabilities and the problem of ionospheric turbulence in general. To focus on the ionospheric turbulence, a set of perturbed governing equations are derived. The model accurately captures the GDI growth rate in different limits; it is also benchmarked to the evolution of instability development in different collisional regimes of a plasma cloud. The newly developed model is used to study if the GDI is the cause of density irregularities observed in subauroral polarization streams (SAPS). Data from Global Positioning System (GPS) scintillations and the Super Dual Auroral Radar Network (SuperDARN) are used to examine the latitudinal density and velocity profiles of SAPS. It is found that the GDI is stabilized by velocity shear and therefore will only generate density irregularities in regions of low velocity shear. Furthermore, the density irregularities cannot extend through regions of large velocity shear. In certain cases, the turbulence cascade power laws match observation and theory. The transition between the KHI and the GDI is studied by understanding the effect of collisions. In low collisionality regimes, the KHI is the dominant instability. In high collisionality regimes, the GDI is the dominant instability. Using nominal ionospheric parameters, a prediction is provided that suggests that there exists an altitude in the upper textit{F} region ionosphere above which the turbulence is dominated by the KHI.
Doctor of Philosophy
In the modern day, all wireless communication signals use electromagnetic waves that propagate through the atmosphere. In the upper atmosphere, there exists a region called the ionosphere, which consists of plasma (a mixture of ions, electrons, and neutral particles). Because ions and electrons are charged particles, they interact with the electromagnetic communication signals. A better understanding of ionospheric turbulence will allow for aid in forecasting space weather as well as improve future communication equipment. Communication signals become distorted as they pass through turbulent regions of the ionosphere, which negatively affects the signal quality at the receiving end. For a tangible example, when Global Positioning System (GPS) signals pass through turbulent regions of the ionosphere, the resulting position estimate becomes worse. This work looks at two specific causes of ionospheric turbulence: the gradient drift instability (GDI) and the Kelvin-Helmholtz instability (KHI). Under the correct background conditions, these instabilities have the ability to generate ionospheric turbulence. To learn more about the GDI and the KHI, a novel simulation model is developed. The model uses a method of splitting the equations such that the focus is on just the development of the turbulence while considering spatially constant realistic background conditions. The model is shown to accurately represent results from previously studied problems in the ionosphere. This model is applied to an ionospheric phenomenon known as subauroral polarization streams (SAPS) to study the development of the GDI and the KHI. SAPS are regions of the ionosphere with large westward velocity that changes with latitude. The shape of the latitudinal velocity profile depends on many other factors in the ionosphere such as the geomagnetic conditions. It is found that for certain profiles, the GDI will form in SAPS with some of these examples matching observational data. At higher altitudes, the model predicts that the KHI will form instead. While the model is applied to just the development of the GDI and the KHI in this work, it is written in a general manner such that other causes of ionospheric turbulence can be easily studied in the future.
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Mithen, James Patrick. "Molecular dynamics simulations of the equilibrium dynamics of non-ideal plasmas." Thesis, University of Oxford, 2012. http://ora.ox.ac.uk/objects/uuid:3bae84f9-530d-43da-ad7e-bb9a1784cd1d.

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Molecular dynamics (MD) simulations are used to compute the equilibrium dynamics of a single component fluid with Yukawa interaction potential v(r) = (Ze)^2 exp(−r/λs )/4π eps_0 r. This system, which is known as the Yukawa one-component plasma (YOCP), represents a simplified description of a non-ideal plasma consisting of ions, charge Ze, and electrons. For finite screening lengths λs, the MD results are used to investigate the domain of validity of the hydrodynamic description, i.e., the description given by the Navier-Stokes equations. The way in which this domain depends on the thermodynamic conditions of the YOCP, as well as the strength and range of the interactions, is determined. Remarkably, it is found that the domain of validity is completely determined by the range of the interactions (i.e., λs); this alone determines the maximum wave number k_max at which the hydrodynamic description is applicable. The dynamics of the YOCP at wavevectors beyond k_max are then investigated; these are shown to be in striking agreement with a simple and well known generalisation of the Navier-Stokes equations. In the extreme case of the Coulomb interaction potential (λs = ∞), the very existence of a hydrodynamic description is a known but unsolved problem [Baus & Hansen, 1980]. For this important special case, known as the one-component plasma (OCP), it is shown that the ordinary hydrodynamic description is never valid. Since the OCP is the prototypical system representing a non-ideal plasma, a number of different approaches for modelling its dynamics have been formulated previously. By computing the relevant quantities with MD, the applicability of a number of models proposed in the literature is examined for the first time.
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Frerichs, Heinke Gerd [Verfasser]. "Three-dimensional plasma transport in open chaotic magnetic fields : a computational assessment for tokamak edge layers / vorgelegt von Heinke Gerd Frerichs. [Forschungszentrum Jülich, Energieforschung (IEF), Plasma Physics (IEF-4)]." Jülich : Forschungszentrum, Zentralbibliothek, 2010. http://d-nb.info/1009786954/34.

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Nguyen, Tran-Thuat. "Synthèse et contrôle de la taille de nanocristaux de silicium par plasma froid. Application dans les domaines de l'optoélectronique et de la nanoélectronique." Phd thesis, Ecole Polytechnique X, 2008. http://pastel.archives-ouvertes.fr/pastel-00504166/en/.

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Dans cette thèse nous avons montré que l'on peut on peut synthétiser des nanocristaux de silicium en utilisant des plasmas pulsés de silane dilué dans l'hydrogène. Dans nos conditions de dépôt, en changeant le temps de croissance entre 100 msec et 1 seconde, nous avons pu contrôler la taille des nanocristaux (de 4 nm à 12 nm). A partir de la mesure de la taille des nanocristaux sur les images MET, nous avons pu calculer la vitesse de croissance radiale. Cette vitesse est proportionnelle à la pression partielle de silane dans le mélange gazeux. Nous avons également montré le rôle important de l'hydrogène atomique pour le processus de cristallisation des nanoparticules dans le plasma. La maîtrise de la synthèse des nanocristaux de silicium ouvre la voie à deux champs d'applications : (i) la fabrication de diodes électroluminescences et (ii) la réalisation de transistors à un électron. Pour la première application, une étude préalable de photoluminescence a montré un déplacement vers le bleu du pic de photoluminescence lorsque la taille des nanocristaux diminue. Cela est interprété à la fois comme un effet de confinement quantique et de passivation de la surface des nanocristaux par une coquille de SiOx. Nous avons également élaboré des diodes électroluminescence PIN basées sur les nanocristaux de silicium. Après une optimisation de la structure PIN et des conditions de dépôt de la couche intrinsèque, nous avons obtenu une électroluminescence dans la gamme infrarouge-visible à température ambiante. En vue de l'application aux transistors, nous avons fait des expériences préalables d'injection de charge dans les nanocristaux par AFM/KFM. L'observation qualitative des charges injectées a été réalisée. L'estimation quantitative de ces charges ainsi que l'étude de charges résiduelles dans des nanocristaux dopés est un domaine qui mérite d'être exploré dans l'avenir.
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Books on the topic "Computational Plasma Physics"

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Computational methods in plasma physics. Boca Raton, FL: CRC Press/Taylor & Francis, 2010.

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Visual and computational plasma physics. New Jersey: World Scientific, 2015.

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Tajima, T. Computational plasma physics: With applications to fusion andastrophysics. Redwood City, Calif: Addison-Wesley Pub. Co., Advanced Book Program, 1989.

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Tajima, Toshiki. Computational plasma physics: With applications to fusion and astrophysics. Redwood City, Calif: Addison-Wesley Pub. Co., Advanced Book Program, 1989.

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Huo, Winifred M. Computational Methods for Electron--Molecule Collisions. Boston, MA: Springer US, 1995.

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service), SpringerLink (Online, ed. Cosmic Ray Diffusion in the Galaxy and Diffuse Gamma Emission. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012.

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service), SpringerLink (Online, ed. Stability and Transport in Magnetic Confinement Systems. New York, NY: Springer New York, 2012.

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Wong, Silvester Siu Kai. A computational study of the influence of molecular nitrogen and laser absorption on plasma channel formation created by laser resonance saturation of sodium vapor. [Downsview, Ont.]: Institute for Aerospace Studies, 1985.

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Wong, Silvester Siu Kai. A computational study of the influence of molecular nitrogen and laser absorption on plasma channel formation created by laser resonance saturation of sodium vapor. Downsview, Ont: Institute for Aerospace Studies, 1986.

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Brooks, Robert L. The Fundamentals of Atomic and Molecular Physics. New York, NY: Springer New York, 2013.

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Book chapters on the topic "Computational Plasma Physics"

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Graziani, Frank R. "Computational Plasma Physics." In Encyclopedia of Applied and Computational Mathematics, 278–88. Berlin, Heidelberg: Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-540-70529-1_585.

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Bell, A. R. "Computational Simulation of Plasmas." In Plasma Physics, 13–35. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4758-3_2.

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Andersen, Nils, and Klaus Bartschat. "Computational Methods." In Springer Series on Atomic, Optical, and Plasma Physics, 87–109. New York, NY: Springer New York, 2001. http://dx.doi.org/10.1007/978-1-4613-0187-5_6.

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Andersen, Nils, and Klaus Bartschat. "Computational Methods." In Springer Series on Atomic, Optical, and Plasma Physics, 97–124. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-55216-3_6.

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Lavaud, Michel, and Jean-Marc Victor. "Computation of an Improved Integral Equation by Non Linear Resummation of the First Graphs of the Bridge Function." In Strongly Coupled Plasma Physics, 597–601. Boston, MA: Springer US, 1987. http://dx.doi.org/10.1007/978-1-4613-1891-0_53.

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Raschke, Markus B., Samuel Berweger, and Joanna M. Atkin. "Ultrafast and Nonlinear Plasmon Dynamics." In Challenges and Advances in Computational Chemistry and Physics, 237–81. Dordrecht: Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-7805-4_7.

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Tajima, Toshiki. "Information and Computation." In Computational Plasma Physics, 298–332. CRC Press, 2018. http://dx.doi.org/10.1201/9780429501470-11.

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Tajima, Toshiki. "Introduction." In Computational Plasma Physics, 1–36. CRC Press, 2018. http://dx.doi.org/10.1201/9780429501470-1.

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Tajima, Toshiki. "Geometry." In Computational Plasma Physics, 268–97. CRC Press, 2018. http://dx.doi.org/10.1201/9780429501470-10.

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Tajima, Toshiki. "Interaction between Radiation and A Plasma." In Computational Plasma Physics, 333–66. CRC Press, 2018. http://dx.doi.org/10.1201/9780429501470-12.

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Conference papers on the topic "Computational Plasma Physics"

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Correa-Reina, G., F. Casanova, M. Vénere, C. Moreno, H. Bruzzone, and A. Clausse. "Computational simulation of plasma focus." In PLASMA PHYSICS: IX Latin American Workshop. AIP, 2001. http://dx.doi.org/10.1063/1.1374913.

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"Poster Session 5P10-19: Computational Plasma Physics." In IEEE Conference Record - Abstracts. 31st IEEE International Conference On Plasma Science. IEEE, 2004. http://dx.doi.org/10.1109/plasma.2004.1340038.

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Verboncoeur, J. "Oral Session 7C: Computational plasma physics; basic phenomena - II; dusty plasmas - II." In IEEE Conference Record - Abstracts. 31st IEEE International Conference On Plasma Science. IEEE, 2004. http://dx.doi.org/10.1109/plasma.2004.1340198.

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Hutchinson, I. H. "Spherical Particle Interaction with Flowing Plasma: Computational Discoveries." In NEW VISTAS IN DUSTY PLASMAS: Fourth International Conference on the Physics of Dusty Plasmas. AIP, 2005. http://dx.doi.org/10.1063/1.2134571.

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Humphries, Stanley. "Computational Techniques in Xenos - Integrated 3D Software Suite for Electron and X-ray Physics." In 2007 IEEE Pulsed Power Plasma Science Conference. IEEE, 2007. http://dx.doi.org/10.1109/ppps.2007.4346035.

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Chang, C. S., Sanae-I. Itoh, Shigeru Inagaki, Masako Shindo, and Masatoshi Yagi. "Computational Knowledge for Toroidal Confinement Physics: Part I." In 2ND ITER INTERNATIONAL SUMMER SCHOOL: In conjunction with the 47th Summer School of JSPF for Young Plasma Scientists: Confinement. AIP, 2009. http://dx.doi.org/10.1063/1.3097323.

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Ghildina, Anna R., Pavel A. Mikheyev, Aleksandr K. Chernyshov, Nikolai N. Lunev, and Valeriy N. Azyazov. "The measurement of argon metastable atoms in the barrier discharge plasma." In Saratov Fall Meeting 2017: Fifth International Symposium on Optics and Biophotonics: Laser Physics and Photonics XIX; Computational Biophysics and Analysis of Biomedical Data IV, edited by Vladimir L. Derbov and Dmitry E. Postnov. SPIE, 2018. http://dx.doi.org/10.1117/12.2315232.

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Dietrich, M. R., A. Avril, R. Bowler, N. Kurz, J. S. Salacka, G. Shu, B. B. Blinov, James R. Danielson, and Thomas Sunn Pedersen. "Barium Ions for Quantum Computation." In NON-NEUTRAL PLASMA PHYSICS VII: Workshop on Non-Neutral Plasmas 2008. AIP, 2009. http://dx.doi.org/10.1063/1.3122286.

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Xu, Xiaofei, Huu Duc Vo, Njuki Mureithi, and Xue Feng Zhang. "Turbulent Boundary Layer Separation Control by Using DBD Plasma Actuators: Part II—Numerical Model Validation and Parametric Study." In ASME 2010 International Mechanical Engineering Congress and Exposition. ASMEDC, 2010. http://dx.doi.org/10.1115/imece2010-37325.

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Following an experimental investigation into suppression of a 2-D turbulent boundary layer separation with dielectric barrier discharge (DBD) plasma actuators, the present work investigates the concept numerically. The purpose is to develop and validate a simulation tool that captures the flow physics and carry out a parametric study of the concept at flow regimes beyond the current flow control capability of plasma actuators of conventional strength. First, a plasma actuator model is integrated into the commercial computational fluid dynamics (CFD) code ANSYS CFX to simulate the effects of plasma actuation. This computational tool is validated through comparison of results with the experimental results for pulsed actuation in quiescent air and for the control of a turbulent boundary layer separation at low flow velocities. It is shown that CFX with an integrated plasma model can capture the main experimentally observed effects of DBD actuators on turbulent boundary layer separation. Subsequently, this numerical approach is used, with increased plasma actuator strength, to study the influence of different actuation parameters (e.g., actuation location, direction and frequency) on suppression of turbulent boundary layer separation at higher flow velocities.
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Krzhizhanovskaya, V. V., M. A. Zatevakhin, A. A. Ignatiev, Yu E. Gorbachev, W. J. Goedheer, and P. M. A. Sloot. "A 3D Virtual Reactor for Simulation of Silicon-Based Film Production." In ASME/JSME 2004 Pressure Vessels and Piping Conference. ASMEDC, 2004. http://dx.doi.org/10.1115/pvp2004-3120.

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In this paper we introduce a Grid-based Virtual Reactor, a problem-solving environment that supports detailed numerical study of industrial thin film production in Plasma Enhanced Chemical Vapor Deposition (PECVD) reactors. We describe the physics and chemistry underpinning the deposition process, the numerical approach to simulate these processes on advanced computer architectures as well as the associated software environment supporting computational experiments. In the developed 3D model we took into account all relevant chemical kinetics, plasma physics and transport processes that occur in PECVD reactors. We built an efficient problem-solving environment for scientists studying PECVD processes and end-users working in chemical industry and validated the resulting Virtual Reactor against real experiments.
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Reports on the topic "Computational Plasma Physics"

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Lasinski, B., D. Larson, D. Hewett, A. Langdon, and C. Still. Computational Methods for Collisional Plasma Physics. Office of Scientific and Technical Information (OSTI), February 2004. http://dx.doi.org/10.2172/15009790.

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2

Hewett, D. W. Simulation models for computational plasma physics: Concluding report. Office of Scientific and Technical Information (OSTI), March 1994. http://dx.doi.org/10.2172/10142303.

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3

Shumlak, Uri. Physics-Based Computational Algorithm for the Multi-Fluid Plasma Model. Fort Belvoir, VA: Defense Technical Information Center, June 2014. http://dx.doi.org/10.21236/ada614448.

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