Relevant bibliographies by topics / Weakly ionized plasma

Academic literature on the topic 'Weakly ionized plasma'

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Published: 10 December 2022
Last updated: 28 January 2023

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Journal articles on the topic "Weakly ionized plasma"

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Kiss'ovski, Zh, and A. Shivarova. "Plasma permittivity of weakly ionized inhomogeneous magnetized plasmas." Plasma Physics and Controlled Fusion 37, no. 10 (October 1, 1995): 1119–32. http://dx.doi.org/10.1088/0741-3335/37/10/004.

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Sudan, R. N., A. V. Gruzinov, W. Horton, and N. Kukharkin. "Convective turbulence in weakly ionized plasma." Physics Reports 283, no. 1-4 (April 1997): 95–119. http://dx.doi.org/10.1016/s0370-1573(96)00055-5.

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Lee, Myoung-Jae, and Young-Dae Jung. "Symmetric and Anti-Symmetric Damping Modes of Trivelpiece–Gould Waves in Weakly and Completely Ionized Plasma Waveguides." Symmetry 13, no. 4 (April 16, 2021): 699. http://dx.doi.org/10.3390/sym13040699.

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The collision effects on the low-frequency ion-acoustic Trivelpiece–Gould wave are investigated in weakly and completely ionized plasma waveguides by using the normal mode analysis. In weakly ionized plasma waveguides, it is found that the dependence of the harmonic mode on the absolute value of the scaled damping rate shows the opposite tendency for large and small radii of the cylindrical waveguide. It is also is found that the scaled damping rates for both weakly and completely ionized plasma waveguides decrease with an increase of the electron temperature. It is interesting to note that the scaled damping rate for weakly ionized plasma waveguides shows anti-symmetric behavior when the Trivelpiece–Gould wave propagates in the negative-z direction. However, it is found that the scaled damping rate for completely ionized plasma waveguides shows the symmetric behavior when the Trivelpiece–Gould wave propagates in the negative-z direction.
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Pavlov, V. A. "Weakly ionized plasma in a supersonic plasma flow." Plasma Physics Reports 28, no. 6 (June 2002): 479–83. http://dx.doi.org/10.1134/1.1485651.

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DAS, CHANDRA. "Evolution of magnetic moment in the interaction of waves with kinetically described plasmas." Journal of Plasma Physics 57, no. 2 (February 1997): 343–48. http://dx.doi.org/10.1017/s002237789600493x.

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The non-oscillating part of the magnetic moment field (called the inverse Faraday effect (IFE) for this field from a circularly polarized wave in a medium) is calculated for the interaction of an elliptically polarized wave with a weakly ionized magnetized plasma in a kinetic theory model and with unmagnetized Vlasov plasmas. For a weakly ionized magnetized plasma, the induced field increases with both temperature and ambient magnetic field. For an unmagnetized plasma, it increases parabolically with temperature. The induced magnetic field is found to vary parabolically with temperature in the case of an unmagnetized Vlasov plasma.
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Alharbi, 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.

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ABSTRACT Here, we study the nature and characteristics of waves propagating in partially ionized plasmas in the weakly ionized limit, typical for the lower part of the solar atmosphere. The framework in which the properties of waves are discussed depends on the relative magnitude of collisions between particles, but also on the relative magnitude of the collisional frequencies compared to the gyro-frequency of charged particles. Our investigation shows that the weakly ionized solar atmospheric plasma can be divided into two regions, and this division occurs, roughly, at the base of the chromosphere. In the solar photosphere, the plasma is non-magnetized and the dynamics can described within the three-fluid framework, where acoustic waves associated to each species can propagate. Due to the very high concentration of neutrals, the neutral sound waves propagates with no damping, while for the other two modes the damping rate is determined by collisions with neutrals. The ion- and electron-related acoustic modes propagate with a cut-off determined by the collisional frequency of these species with neutrals. In the weakly ionized chromosphere, only electrons are magnetized, however, the strong coupling of charged particles reduces the working framework to a two-fluid model. The disassociation of charged particles creates electric currents that can influence the characteristic of waves. The propagation properties of waves with respect to the angle of propagation are studied with the help of polar diagrams.
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Graves, David B., and Richard A. Gottscho. "Computer Applications in Plasma Materials Processing." MRS Bulletin 16, no. 2 (February 1991): 16–22. http://dx.doi.org/10.1557/s0883769400057602.

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In manufacturing microelectronic and optoelectronic devices, thin solid films of various sorts are routinely deposited and etched using low pressure, weakly ionized plasmas. The term “plasma” in this context implies an ionized gas with nearly equal numbers of positive and negative charges. This definition is not very restrictive, so. there are an enormous number of phenomena that are termed plasmas. For example, very hot, magnetized, fully ionized plasmas exist in stellar environments and thermonuclear fusion experiments. High temperature electric arcs are a form of plasma as well. In contrast, the plasmas used in electronic materials processing are near room temperature and the gas is usually weakly ionized. Indeed, due to the sensitivity of electronic devices to high temperatures, their low operating temperature is one of the major advantages of plasma processes.Plasma processing is attractive because of two important physiochemical effects: energetic free electrons in the plasma (heated by applied electric fields) dissociate the neutral gas in the plasma to create chemically reactive species; and free positive ions are accelerated by the plasma electric fields to surfaces bounding the plasma. Reactive species created in the plasma diffuse to surfaces and adsorb; wafers to be processed are typically placed on one of these surfaces.The combination of neutral species adsorption and positive ion bombardment results in surface chemical reaction. If the products of the surface reaction are volatile, they leave the surface and etching results. If the products are involatile, a surface film grows.
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Leake, James E., Vyacheslav S. Lukin, and Mark G. Linton. "Magnetic reconnection in a weakly ionized plasma." Physics of Plasmas 20, no. 6 (June 2013): 061202. http://dx.doi.org/10.1063/1.4811140.

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Zagorodny, A. G., A. V. Filippov, A. F. Pal', A. N. Starostin, and A. I. Momot. "Macroparticle screening in a weakly ionized plasma." Journal of Physical Studies 11, no. 2 (2007): 158–64. http://dx.doi.org/10.30970/jps.11.158.

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Stiele, H., H. Lesch, and F. Heitsch. "Thermal instability in a weakly ionized plasma." Monthly Notices of the Royal Astronomical Society 372, no. 2 (October 21, 2006): 862–68. http://dx.doi.org/10.1111/j.1365-2966.2006.10909.x.

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Dissertations / Theses on the topic "Weakly ionized plasma"

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Menzel, Raymond. "Multifluid magnetohydrodynamics of weakly ionized plasmas." Thesis, Rensselaer Polytechnic Institute, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=3630022.

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The process of star formation is an integral part of the new field of astrobiology, which studies the origins of life. Since the gas that collapses to form stars and their resulting protoplanetary disks is known to be weakly ionized and contain magnetic fields, star formation is governed by multifluid magnetohydrodynamics. In this thesis we consider two important problems involved in the process of star formation that may have strongly affected the origins of life, with the goal of determining the thermal effects of these flows and modeling the physical conditions of these environments.

We first considered the outstanding problem of how primitive bodies, specifically asteroids, were heated in protoplanetary disks early in their lifetime. Reexamining asteroid heating due to the classic unipolar induction heating mechanism described by Sonett et al. (1970), we find that this mechanism contains a subtle conceptual error. As original conceived, heating due to this mechanism is driven by a uniform, supersonic, fully-ionized, magnetized, T Tauri solar wind, which sweeps past an asteroid and causes the asteroid to experience a motional electric field in its rest frame. We point out that this mechanism ignores the interaction between the body surface and the flow, and thus only correctly describes the electric field far away from the asteroid where the plasma streams freely. In a realistic protoplanetary disk environment, we show that the interaction due to friction between the asteroid surface and the flow causes a shear layer to form close to the body, wherein the motional electric field predicted by Sonett et al. decreases and tends to zero at the asteroid surface. We correct this error by using the equations of multifluid magnetohydrodynamics to explicitly treat the shear layer. We calculate the velocity field in the plasma, and the magnetic and electric fields everywhere for two flows over an idealized infinite asteroid with varying magnetic field orientations. We show that the total electric field in the asteroid may either be of comparable strength to the electric field predicted by Sonett et al. or vanish depending on the magnetic field geometry. We include the effects of dust grains in the gas and calculate the heating rates in the plasma flow due to ion-neutral scattering and viscous dissipation. We term this newly discovered heating mechanism “electrodynamic heating”, use measurements of asteroid electrical conductivities to estimate the upper limits of the possible heating rates and amount of thermal energy that can be deposited in the solid body, and compare these to the heating produced by the decay of radioactive nuclei like Al26.

For the second problem we modeled molecular line emission from time-dependent multifluid MHD shock waves in star-forming regions. By incorporating realistic radiative cooling by CO and H2 into the numerical method developed by Ciolek & Roberge (2013), we present the only current models of truly time-dependent multifluid MHD shock waves in weakly-ionized plasmas. Using the physical conditions determined by our models, we present predictions of molecular emission in the form of excitation diagrams, which can be compared to observations of protostellar outflows in order to trace the physical conditions of these environments. Current work focuses on creating models for varying initial conditions and shock ages, which are and will be the subject of several in progress studies of observed molecular outflows and will provide further insight into the physics and chemistry of these flows.

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Li, Huayu. "Lattice Boltzmann simulation of laser interaction with weakly ionized plasmas." Diss., Connect to online resource - MSU authorized users, 2008.

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Fourkal, Eugene S. "Nonequilibrium transport processes in weakly ionized plasmas." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1999. http://www.collectionscanada.ca/obj/s4/f2/dsk1/tape9/PQDD_0018/NQ37883.pdf.

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Benyo, Theresa L. "Analytical and Computational Investigations of a Magnetohydrodynamic (MHD) Energy-Bypass System for Supersonic Turbojet Engines to Enable Hypersonic Flight." Kent State University / OhioLINK, 2013. http://rave.ohiolink.edu/etdc/view?acc_num=kent1369153719.

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Du, Ji-Bin, and 杜志彬. "Pattern formation in weakly ionized plasma." Thesis, 1994. http://ndltd.ncl.edu.tw/handle/35200634258491187529.

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Chu, Kuo-Yuan, and 朱國源. "An Aerodynamic Analysis on Cone Body in Weakly Ionized Plasma Flow." Thesis, 2005. http://ndltd.ncl.edu.tw/handle/62099624385690160012.

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碩士
國立成功大學
航空太空工程學系碩博士班
93
According to the increasing requirements of global transportation, the applications in supersonic flight are getting more and more important. Due to the increased drag of supersonic flight, the economic benefits of the higher speed would be reduced. There are many studies are introduced. Joining energy in and ionize the gas is one of the methods to solve the problem. After the gas is ionized, the ions could decrease the aerodynamic drag, but the physical mechanism is very complicated. 　This study utilizes CFD-FASTRAN software. The software calculates Navier-Stokes equations, includes kinetic theory, thermal non-equilibrium, mass diffusivity, source term, and turbulence models. The weakly ionized plasma flow field is calculated by the species of the gas, which is based on the assumption of a fixed ionized degree. 　It is found that the molecular internal temperatures and the ionized degrees are changed in this study. The results show that the drag coefficient of the flying body is decreased by 2~4% when the molecular internal temperature and the ionized degree become higher.
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Chu, Jen-Hung, and 朱仁弘. "The Study of Formation and Collective Behaviors of Fine Silicon -oxide Particles in RF Weakly Ionized Plasmas." Thesis, 1994. http://ndltd.ncl.edu.tw/handle/34094478998016282107.

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博士
國立中央大學
物理與天文學研究所
82
Fine SiO2 paricles are fabricated through gas phase homogeneous chemical reactions and nucleations in rf magnetron discharge in SiH4/O2/Ar gas mixtures. For P>30 mTorr, primary fine particles (PFPs) with diameter about 20 nm can be formed and their diameter increases with the system pressure. They can aggregate with other PFPs to form larger aggregated fine particles (AFPs) with nearly spherical shape. The size of the AFP depends on the duration of the rf power. The homogeneous process creates oxide particles with more relaxed Si-O bonding than the surface- process-dominated counterpart. The plasma-generated fine particles are negatively charged and suspended in the plasma. The accumulation of fine particles causes low-frequency (about 10 Hz) spatiotemporal oscillation of the discharge. At high pressure (>200 mTorr), the random fluctuations of the discharge and the particle motions are suppressed. The Coulomb solids and liquids are directly observed for the first time using an optical microscope in the rf weakly ionized plasma. By properly controlling the system parameters, 3-d hexagonal, face-centered cubic (fcc), body-centered cubic (bcc) and hexagonal close- packed (hcp) crystal structures and solids with coexisting different crystal structures can be obtained. The defects and the growth of the 3-d hexagonal crystal are also observed. Increasing the rf power causes the transtion to the more disorder liquid state and it exhibits a first-order phase transition.
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Books on the topic "Weakly ionized plasma"

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Hillard, G. Barry. Enhanced plasma current collection from weakly conducting solar array blankets. [Washington, DC: National Aeronautics and Space Administration, 1993.

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Rubinstein, Robert. Relaxation from steady states far from equilibrium and the persistence of anomalous shock behavior in weakly ionized gases. Hampton, VA: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, 1999.

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Günther, Klaus, and Rainer Radtke. Electric Properties of Weakly Nonideal Plasmas. de Gruyter GmbH, Walter, 2022.

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Gunther, Klaus, and Rainer Radtke. Electric Properties of Weakly Nonideal Plasmas (Exs (Experientia Supplementum)). Birkhauser, 1985.

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Matsumoto, Michio. Cross-Magnetic Turbulent Diffusion of Charged Particles in a Weakly Ionized Plasma. VS Verlag fur Sozialwissenschaften GmbH, 2012.

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Baer, Tomas. Relaxation of photon echoes in weakly ionized noble-gas plasmas. 1991.

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Columb, Malachy O. Local anaesthetic agents. Edited by Michel M. R. F. Struys. Oxford University Press, 2017. http://dx.doi.org/10.1093/med/9780199642045.003.0017.

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Local anaesthetic agents cause a pharmacologically induced reversible neuropathy characterized by axonal conduction blockade. They act by blocking the sodium ionophore and exhibit membrane stabilizing activity by inhibiting initiation and propagation of action potentials. They are weak bases consisting of three components: a lipophilic aromatic ring, a link, and a hydrophilic amine. The chemical link classifies them as esters or amides. Local anaesthetics diffuse through the axolemma as unionized free-base and block the ionophore in the quaternary ammonium ionized form. The speed of onset of block is therefore dependent on the pKa of the agent and the ambient tissue pH. Esters undergo hydrolysis by plasma esterases and amides are metabolized by hepatic microsomal mixed-function oxidases. Local anaesthetics are bound in the blood to α‎1-acid glycoproteins. Pharmacological potency is dependent on the lipid solubility of the drug as is the potential for systemic toxicity. The blood concentrations required to cause cardiovascular system (CVS) collapse and early central nervous system (CNS) toxicity are used to quantify the CVS:CNS toxicity ratio. Local anaesthetics also have the potential to induce direct neuronal damage. Intravenous lipid emulsion is used for the treatment of systemic toxicity but the scientific evidence is inconsistent. With regard to the pipecoloxylidine local anaesthetics, early evidence indicated that the S- was less toxic than the R-enantiomer. However, clinical research using minimum local analgesic concentration designs suggests that reduced systemic toxicity and motor block sparing is mainly explained by potency rather than enantiomerism.
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Book chapters on the topic "Weakly ionized plasma"

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Somov, Boris V. "Reconnection in Weakly-Ionized Plasma." In Astrophysics and Space Science Library, 397–414. New York, NY: Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-4295-0_15.

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Wiechen, H., G. T. Birk, and H. Lesch. "Self-Generation Of Magnetic Fields In Weakly Ionized Astrophysical Plasmas." In Plasma Astrophysics And Space Physics, 347–56. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4203-8_26.

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Sakai, J. I., M. Suzuki, and T. Fushiki. "Formation and Emergence of Current Loops in Weakly Ionized Plasmas." In Magnetodynamic Phenomena in the Solar Atmosphere, 599–600. Dordrecht: Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0315-9_158.

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Jones, Aoife C., Mohsen Shadmehri, and Turlough P. Downes. "Multifluid Simulations of the Kelvin-Helmholtz Instability in a Weakly Ionised Plasma." In Protostellar Jets in Context, 547–49. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-00576-3_73.

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Bers, 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.

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Abstract This chapter turns to weakly-ionized plasmas. It describes electron-neutral collisions and some of the resulting transport in applied EM fields. The simplified Lorentz model/operator, and the solution of the electron distribution function using an expansion in spherical harmonics analyzed here allows for rigorously defining various relaxation frequencies that were introduced in earlier chapters in an ad-hoc manner. The chapter then pays attention on finding the electrical conductivity in a weakly-ionized plasma in applied EM fields, and addresses diffusion and thermal conductivity and the important case of “intermediate plasmas.” The results of this chapter should be useful, notably in the following domains of study: gas discharges at low power; ionosphere up to an altitude of about 250 km; and dense and not too hot plasmas such as flames and magnetohydrodynamic energy converters.
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"Reconnection in Weakly-Ionized Plasma." In Astrophysics and Space Science Library, 705–23. New York, NY: Springer New York, 2006. http://dx.doi.org/10.1007/978-0-387-68894-7_35.

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Bers, Abraham. "Collisions and collisional transport—III. Weakly-ionized plasmas—Unmagnetized." In Plasma Physics and Fusion Plasma Electrodynamics, 399–437. Oxford University Press, 2016. http://dx.doi.org/10.1093/acprof:oso/9780199295784.003.0007.

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"Diffusion of a Bounded Weakly Ionized Magnetized Plasma." In Transport Phenomena in Partially Ionized Plasma, 225–56. CRC Press, 2001. http://dx.doi.org/10.1201/9781482288094-12.

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"Elastic and Inelastic Collision Processes in Weakly Ionized Gases." In Introduction to Plasma Technology, 15–27. Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, 2010. http://dx.doi.org/10.1002/9783527632169.ch2.

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Fortov, V. E., I. T. Iakubov, and A. G. Khrapak. "IONIZATION EQUILIBRIUM AND THERMODYNAMIC PROPERTIES OF WEAKLY IONIZED PLASMAS." In Physics of Strongly Coupled Plasma, 125–68. Oxford University Press, 2006. http://dx.doi.org/10.1093/acprof:oso/9780199299805.003.0004.

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Conference papers on the topic "Weakly ionized plasma"

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Sato, Eiichi, Yasuomi Hayasi, Rudolf Germer, Yoshitake Koorikawa, Kazunori Murakami, Etsuro Tanaka, Hidezo Mori, et al. "Weakly ionized cerium plasma radiography." In Optical Science and Technology, SPIE's 48th Annual Meeting, edited by Donald R. Snyder. SPIE, 2004. http://dx.doi.org/10.1117/12.506563.

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Loverich, John, and Ammar Hakim. "Modeling weakly ionized gases using TxFluids." In 2010 IEEE 37th International Conference on Plasma Sciences (ICOPS). IEEE, 2010. http://dx.doi.org/10.1109/plasma.2010.5534357.

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Hoyos, Jaime H., Andreas Reisenegger, and Juan A. Valdivia. "Ambipolar diffusion in weakly ionized plasmas." In 2011 IEEE 38th International Conference on Plasma Sciences (ICOPS). IEEE, 2011. http://dx.doi.org/10.1109/plasma.2011.5993219.

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Hou, Lei, and Wei Shi. "Detecting Terahertz Continuous Wave Using Weakly Ionized Plasma." In International Symposium on Ultrafast Phenomena and Terahertz Waves. Washington, D.C.: OSA, 2018. http://dx.doi.org/10.1364/isuptw.2018.tuk35.

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Wirz, Richard, Samuel Araki, and Ben Dankongkakul. "Near-Surface Cusp Confinement for Weakly Ionized Plasma." In 48th AIAA/ASME/SAE/ASEE Joint Propulsion Conference & Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2012. http://dx.doi.org/10.2514/6.2012-3948.

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Hou, Lei, Wei Shi, Yu Wu, Hong Liu, and Yi Ding. "Mechanism of weakly ionized plasma terahertz wave detector." In 2013 38th International Conference on Infrared, Millimeter, and Terahertz Waves (IRMMW-THz 2013). IEEE, 2013. http://dx.doi.org/10.1109/irmmw-thz.2013.6665748.

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Meyer, R., A. Bezant, P. Palm, and I. Adamovich. "MHD Control of Weakly Ionized Supersonic Plasma Flows." In 33rd Plasmadynamics and Lasers Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2002. http://dx.doi.org/10.2514/6.2002-2246.

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Mishin, G. "Frame-skeleton of weakly ionized gas-discharge plasma." In 9th International Space Planes and Hypersonic Systems and Technologies Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1999. http://dx.doi.org/10.2514/6.1999-4906.

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Malmuth, Norman, Anatoly Maslov, A. Sidorenko, V. Fomichev, and T. Korotaeva. "ITAM Study of Aerodynamics in Weakly Ionized Plasma." In 5th AIAA Theoretical Fluid Mechanics Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2008. http://dx.doi.org/10.2514/6.2008-4336.

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Huo, Winifred. "Stark Line Shapes In A Weakly Ionized Plasma." In 43rd AIAA Thermophysics Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2012. http://dx.doi.org/10.2514/6.2012-2740.

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