Добірка наукової літератури з теми "Weakly ionized plasma"
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Статті в журналах з теми "Weakly ionized plasma"
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.
Повний текст джерелаSudan, 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.
Повний текст джерелаLee, 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.
Повний текст джерелаPavlov, 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.
Повний текст джерелаDAS, 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.
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 джерелаGraves, 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.
Повний текст джерелаLeake, 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.
Повний текст джерелаZagorodny, 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.
Повний текст джерелаStiele, 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.
Повний текст джерелаДисертації з теми "Weakly ionized plasma"
Menzel, Raymond. "Multifluid magnetohydrodynamics of weakly ionized plasmas." Thesis, Rensselaer Polytechnic Institute, 2014. http://pqdtopen.proquest.com/#viewpdf?dispub=3630022.
Повний текст джерелаThe 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.
Li, Huayu. "Lattice Boltzmann simulation of laser interaction with weakly ionized plasmas." Diss., Connect to online resource - MSU authorized users, 2008.
Знайти повний текст джерелаFourkal, 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.
Повний текст джерелаBenyo, 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.
Повний текст джерелаDu, Ji-Bin, and 杜志彬. "Pattern formation in weakly ionized plasma." Thesis, 1994. http://ndltd.ncl.edu.tw/handle/35200634258491187529.
Повний текст джерелаChu, 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.
Повний текст джерела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.
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.
Повний текст джерела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.
Книги з теми "Weakly ionized plasma"
Hillard, G. Barry. Enhanced plasma current collection from weakly conducting solar array blankets. [Washington, DC: National Aeronautics and Space Administration, 1993.
Знайти повний текст джерелаRubinstein, 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.
Знайти повний текст джерелаGünther, Klaus, and Rainer Radtke. Electric Properties of Weakly Nonideal Plasmas. de Gruyter GmbH, Walter, 2022.
Знайти повний текст джерелаGunther, Klaus, and Rainer Radtke. Electric Properties of Weakly Nonideal Plasmas (Exs (Experientia Supplementum)). Birkhauser, 1985.
Знайти повний текст джерелаMatsumoto, Michio. Cross-Magnetic Turbulent Diffusion of Charged Particles in a Weakly Ionized Plasma. VS Verlag fur Sozialwissenschaften GmbH, 2012.
Знайти повний текст джерелаBaer, Tomas. Relaxation of photon echoes in weakly ionized noble-gas plasmas. 1991.
Знайти повний текст джерелаColumb, 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.
Повний текст джерелаЧастини книг з теми "Weakly ionized plasma"
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.
Повний текст джерелаWiechen, 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.
Повний текст джерелаSakai, 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.
Повний текст джерелаJones, 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.
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 джерела"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.
Повний текст джерелаBers, 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.
Повний текст джерела"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.
Повний текст джерела"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.
Повний текст джерелаFortov, 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.
Повний текст джерелаТези доповідей конференцій з теми "Weakly ionized plasma"
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.
Повний текст джерелаLoverich, 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.
Повний текст джерелаHoyos, 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.
Повний текст джерелаHou, 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.
Повний текст джерелаWirz, 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.
Повний текст джерелаHou, 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.
Повний текст джерелаMeyer, 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.
Повний текст джерелаMishin, 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.
Повний текст джерелаMalmuth, 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.
Повний текст джерелаHuo, 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.
Повний текст джерела