Log in

Relevant bibliographies by topics / Plasma flow in magnetic field

Contents

Journal articles
Dissertations / Theses
Books
Book chapters
Conference papers
Reports

Academic literature on the topic 'Plasma flow in magnetic field'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'Plasma flow in magnetic field.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "Plasma flow in magnetic field"

1

Ho, Ching Yen, Yu Hsiang Tsai, and Chung Ma. "Effects of External Magnetic Field on Intensity of Plasma Flow." Applied Mechanics and Materials 597 (July 2014): 272–75. http://dx.doi.org/10.4028/www.scientific.net/amm.597.272.

Full text

Abstract:

This paper investigates the intensity distribution along the radial direction for plasma flow subject to external magnetic Field. The toroidal external magnetism is applied in the transverse direction of plasma flow. Considering the steady-state continuity and momentum of the plasma flow subject to external magnetic field, the intensity profile of the plasma is obtained. The results quantitatively verify the intensity enhancement of the plasma with the increasing external magnetic field.

APA, Harvard, Vancouver, ISO, and other styles

2

Nickeler, D. H., and T. Wiegelmann. "Thin current sheets caused by plasma flow gradients in space and astrophysical plasma." Annales Geophysicae 28, no. 8 (2010): 1523–32. http://dx.doi.org/10.5194/angeo-28-1523-2010.

Full text

Abstract:

Abstract. Strong gradients in plasma flows play a major role in space and astrophysical plasmas. A typical situation is that a static plasma equilibrium is surrounded by a plasma flow, which can lead to strong plasma flow gradients at the separatrices between field lines with different magnetic topologies, e.g., planetary magnetospheres, helmet streamers in the solar corona, or at the boundary between the heliosphere and interstellar medium. Within this work we make a first step to understand the influence of these flows towards the occurrence of current sheets in a stationary state situation. We concentrate here on incompressible plasma flows and 2-D equilibria, which allow us to find analytic solutions of the stationary magnetohydrodynamics equations (SMHD). First we solve the magnetohydrostatic (MHS) equations with the help of a Grad-Shafranov equation and then we transform these static equilibria into a stationary state with plasma flow. We are in particular interested to study SMHD-equilibria with strong plasma flow gradients perpendicular to separatrices. We find that induced thin current sheets occur naturally in such situations. The strength of the induced currents depend on the Alfvén Mach number and its gradient, and on the magnetic field.

APA, Harvard, Vancouver, ISO, and other styles

3

MOHAPATRA, RANJITA K., P. S. SAUMIA, and AJIT M. SRIVASTAVA. "ENHANCEMENT OF FLOW ANISOTROPIES DUE TO MAGNETIC FIELD IN RELATIVISTIC HEAVY-ION COLLISIONS." Modern Physics Letters A 26, no. 33 (2011): 2477–86. http://dx.doi.org/10.1142/s0217732311036711.

Full text

Abstract:

It is known that the presence of background magnetic field in cosmic plasma distorts the acoustic peaks in CMBR. This primarily results from different types of waves in the plasma with velocities depending on the angle between the magnetic field and the wave vector. We consider the consequences of these effects in relativistic heavy-ion collisions where very strong magnetic fields arise during early stages of the plasma evolution. We show that flow coefficients can be significantly affected by these effects when the magnetic field remains strong during early stages due to strong induced fields in the conducting plasma. In particular, the presence of magnetic field can lead to enhancement in the elliptic flow coefficient v2.

APA, Harvard, Vancouver, ISO, and other styles

4

Alexeev, I. I., and V. V. Kalegaev. "Magnetic field and plasma flow structure near the magnetopause." Journal of Geophysical Research 100, A10 (1995): 19267. http://dx.doi.org/10.1029/95ja01345.

Full text

APA, Harvard, Vancouver, ISO, and other styles

5

Korobkin, Yu V., N. V. Lebedev, and V. L. Paperny. "Charge separation of plasma flow in curvilinear magnetic field." Technical Physics Letters 38, no. 3 (2012): 254–57. http://dx.doi.org/10.1134/s1063785012030248.

Full text

APA, Harvard, Vancouver, ISO, and other styles

6

Kotalik, P., and H. Nishiyama. "An effect of magnetic field on arc plasma flow." IEEE Transactions on Plasma Science 30, no. 1 (2002): 160–61. http://dx.doi.org/10.1109/tps.2002.1003973.

Full text

APA, Harvard, Vancouver, ISO, and other styles

7

Juusola, Liisa, Sanni Hoilijoki, Yann Pfau-Kempf, et al. "Fast plasma sheet flows and X line motion in the Earth's magnetotail: results from a global hybrid-Vlasov simulation." Annales Geophysicae 36, no. 5 (2018): 1183–99. http://dx.doi.org/10.5194/angeo-36-1183-2018.

Full text

Abstract:

Abstract. Fast plasma flows produced as outflow jets from reconnection sites or X lines are a key feature of the dynamics in the Earth's magnetosphere. We have used a polar plane simulation of the hybrid-Vlasov model Vlasiator, driven by steady southward interplanetary magnetic field and fast solar wind, to study fast plasma sheet ion flows and related magnetic field structures in the Earth's magnetotail. In the simulation, lobe reconnection starts to produce fast flows after the increasing pressure in the lobes has caused the plasma sheet to thin sufficiently. The characteristics of the earthward and tailward fast flows and embedded magnetic field structures produced by multi-point tail reconnection are in general agreement with spacecraft measurements reported in the literature. The structuring of the flows is caused by internal processes: interactions between major X points determine the earthward or tailward direction of the flow, while interactions between minor X points, associated with leading edges of magnetic islands carried by the flow, induce local minima and maxima in the flow speed. Earthward moving flows are stopped and diverted duskward in an oscillatory (bouncing) manner at the transition region between tail-like and dipolar magnetic fields. Increasing and decreasing dynamic pressure of the flows causes the transition region to shift earthward and tailward, respectively. The leading edge of the train of earthward flow bursts is associated with an earthward propagating dipolarization front, while the leading edge of the train of tailward flow bursts is associated with a tailward propagating plasmoid. The impact of the dipolarization front with the dipole field causes magnetic field variations in the Pi2 range. Major X points can move either earthward or tailward, although tailward motion is more common. They are generally not advected by the ambient flow. Instead, their velocity is better described by local parameters, such that an X point moves in the direction of increasing reconnection electric field strength. Our results indicate that ion kinetics might be sufficient to describe the behavior of plasma sheet bulk ion flows produced by tail reconnection in global near-Earth simulations. Keywords. Magnetospheric physics (magnetospheric configuration and dynamics; plasma sheet) – space plasma physics (numerical simulation studies)

APA, Harvard, Vancouver, ISO, and other styles

8

Rincon, François, Francesco Califano, Alexander A. Schekochihin, and Francesco Valentini. "Turbulent dynamo in a collisionless plasma." Proceedings of the National Academy of Sciences 113, no. 15 (2016): 3950–53. http://dx.doi.org/10.1073/pnas.1525194113.

Full text

Abstract:

Magnetic fields pervade the entire universe and affect the formation and evolution of astrophysical systems from cosmological to planetary scales. The generation and dynamical amplification of extragalactic magnetic fields through cosmic times (up to microgauss levels reported in nearby galaxy clusters, near equipartition with kinetic energy of plasma motions, and on scales of at least tens of kiloparsecs) are major puzzles largely unconstrained by observations. A dynamo effect converting kinetic flow energy into magnetic energy is often invoked in that context; however, extragalactic plasmas are weakly collisional (as opposed to magnetohydrodynamic fluids), and whether magnetic field growth and sustainment through an efficient turbulent dynamo instability are possible in such plasmas is not established. Fully kinetic numerical simulations of the Vlasov equation in a 6D-phase space necessary to answer this question have, until recently, remained beyond computational capabilities. Here, we show by means of such simulations that magnetic field amplification by dynamo instability does occur in a stochastically driven, nonrelativistic subsonic flow of initially unmagnetized collisionless plasma. We also find that the dynamo self-accelerates and becomes entangled with kinetic instabilities as magnetization increases. The results suggest that such a plasma dynamo may be realizable in laboratory experiments, support the idea that intracluster medium turbulence may have significantly contributed to the amplification of cluster magnetic fields up to near-equipartition levels on a timescale shorter than the Hubble time, and emphasize the crucial role of multiscale kinetic physics in high-energy astrophysical plasmas.

APA, Harvard, Vancouver, ISO, and other styles

9

Petralia, A., F. Reale, and P. Testa. "Guided flows in coronal magnetic flux tubes." Astronomy & Astrophysics 609 (December 22, 2017): A18. http://dx.doi.org/10.1051/0004-6361/201731827.

Full text

Abstract:

Context. There is evidence that coronal plasma flows break down into fragments and become laminar. Aims. We investigate this effect by modelling flows confined along magnetic channels. Methods. We consider a full magnetohydrodynamic (MHD) model of a solar atmosphere box with a dipole magnetic field. We compare the propagation of a cylindrical flow perfectly aligned with the field to that of another flow with a slight misalignment. We assume a flow speed of 200 km s-1 and an ambient magnetic field of 30 G. Results. We find that although the aligned flow maintains its cylindrical symmetry while it travels along the magnetic tube, the misaligned one is rapidly squashed on one side, becoming laminar and eventually fragmented because of the interaction and back-reaction of the magnetic field. This model could explain an observation made by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory of erupted fragments that fall back onto the solar surface as thin and elongated strands and end up in a hedge-like configuration. Conclusions. The initial alignment of plasma flow plays an important role in determining the possible laminar structure and fragmentation of flows while they travel along magnetic channels.

APA, Harvard, Vancouver, ISO, and other styles

10

Alekseeva, Liliya M. "Instabilities of a Hall plasma flowing across a magnetic field." Laser and Particle Beams 15, no. 1 (1997): 65–72. http://dx.doi.org/10.1017/s0263034600010752.

Full text

Abstract:

Under certain restrictions imposed on the plasma parameters, an analytical 2D solution to the magnetohydrodynamic equations, taking into account the Hall effect [of the HMHD (Hall magnetohydrodynamic) equations], is found for the case when plasma flows across a magnetic field. This solution has the form of the sum of a rather arbitrary steady flow and a small time-dependent disturbance. We show that waves of a purely acoustic nature can propagate against the background of the flow. The magnetic field manifests itself in this process only in that it produces an effective gravity force, the “gravitational” acceleration being proportional ωeτe. Like acoustic-gravity waves in the atmosphere, such quasiacoustic-gravity (QAG) waves in a plasma increase greatly in their amplitude as they propagate “upward,” that is, in this case, to the anode of an accelerating plasma channel. The existence of a rather general dimensionless similarity criterion is also shown. It can be found directly from the structure of the HMHD equations without any restrictions as to the plasma parameters.

APA, Harvard, Vancouver, ISO, and other styles

More sources

Dissertations / Theses on the topic "Plasma flow in magnetic field"

1

Bissell, R. C. "Steady, collisionless plasma flow along a magnetic field." Thesis, University of Oxford, 1986. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.379920.

Full text

APA, Harvard, Vancouver, ISO, and other styles

2

Plechaty, Christopher Ryan. "Penetration of conductive plasma flows across a magnetic field." abstract and full text PDF (free order & download UNR users only), 2008. http://0-gateway.proquest.com.innopac.library.unr.edu/openurl?url_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&res_dat=xri:pqdiss&rft_dat=xri:pqdiss:1453608.

Full text

APA, Harvard, Vancouver, ISO, and other styles

3

Lee, Hyunyong. "Study on Effect of Magnetic Field Configuration on Parallel Plasma Flow during Neutral Beam Injection in Heliotron J." Kyoto University, 2013. http://hdl.handle.net/2433/174742.

Full text

APA, Harvard, Vancouver, ISO, and other styles

4

Sato, Kunihiro. "Kinetic Analyses of Potential Formation in Plasma Flow along Open Magnetic Fields to a Wall." Kyoto University, 1993. http://hdl.handle.net/2433/154656.

Full text

Abstract:

本文データは平成22年度国立国会図書館の学位論文(博士)のデジタル化実施により作成された画像ファイルを基にpdf変換したものである<br>Kyoto University (京都大学)<br>0048<br>新制・論文博士<br>博士(工学)<br>乙第8140号<br>論工博第2669号<br>新制||工||906(附属図書館)<br>UT51-93-F240<br>(主査)教授板谷良平, 教授秋宗秀夫, 教授大引得弘<br>学位規則第4条第2項該当

APA, Harvard, Vancouver, ISO, and other styles

5

Kevin, Obrejan. "Study of magnetic shaping effects on plasma flows and micro-instabilities in tokamak plasmas using the full-f gyrokinetic code based on a real space field solver." Kyoto University, 2017. http://hdl.handle.net/2433/227650.

Full text

APA, Harvard, Vancouver, ISO, and other styles

6

Margetis, Alexander. "Beltrami Flows." Kent State University Honors College / OhioLINK, 2018. http://rave.ohiolink.edu/etdc/view?acc_num=ksuhonors1525299172164402.

Full text

APA, Harvard, Vancouver, ISO, and other styles

7

Viré, Axelle. "Study of the dynamics of conductive fluids in the presence of localised magnetic fields: application to the Lorentz force flowmeter." Doctoral thesis, Universite Libre de Bruxelles, 2010. http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/210062.

Full text

Abstract:

When an electrically conducting fluid moves through a magnetic field, fluid mechanics and electromagnetism are coupled.<p>This interaction is the object of magnetohydrodynamics, a discipline which covers a wide range of applications, from electromagnetic processing to plasma- and astro-physics.<p><p>In this dissertation, the attention is restricted to turbulent liquid metal flows, typically encountered in steel and aluminium industries. Velocity measurements in such flows are extremely challenging because liquid metals are opaque, hot and often corrosive. Therefore, non-intrusive measurement devices are essential. One of them is the Lorentz force flowmeter. Its working principle is based on the generation of a force acting on a charge, which moves in a magnetic field. Recent studies have demonstrated that this technique can measure efficiently the mean velocity of a liquid metal. In the existing devices, however, the measurement depends on the electrical conductivity of the fluid. <p><p>In this work, a novel version of this technique is developed in order to obtain measurements that are independent of the electrical conductivity. This is particularly appealing for metallurgical applications, where the conductivity often fluctuates in time and space. The study is entirely numerical and uses a flexible computational method, suitable for industrial flows. In this framework, the cost of numerical simulations increases drastically with the level of turbulence and the geometry complexity. Therefore, the simulations are commonly unresolved. Large eddy simulations are then very promising, since they introduce a subgrid model to mimic the dynamics of the unresolved turbulent eddies. <p><p>The first part of this dissertation focuses on the quality and reliability of unresolved numerical simulations. The attention is drawn on the ambiguity that may arise when interpretating the results. Owing to coarse resolutions, numerical errors affect the performances of the discrete model, which in turn looses its physical meaning. In this work, a novel implementation of the turbulent strain rate appearing in the models is proposed. As opposed to its usual discretisation, the present strain rate is in accordance with the discrete equations of motion. Two types of flow are considered: decaying turbulence located far from boundaries, and turbulent flows between two parallel and infinite walls. Particular attention is given to the balance of resolved kinetic energy, in order to assess the role of the model.<p><p>The second part of this dissertation deals with a novel version of Lorentz force flowmeters, consisting in one or two coils placed around a circular pipe. The forces acting on each coil are recorded in time as the liquid metal flows through the pipe. It is highlighted that the auto- or cross-correlation of these forces can be used to determine the flowrate. The reliability of the flowmeter is first investigated with a synthetic velocity profile associated to a single vortex ring, which is convected at a constant speed. This configuration is similar to the movement of a solid rod and enables a simple analysis of the flowmeter. Then, the flowmeter is applied to a realistic three-dimensional turbulent flow. In both cases, the influence of the geometrical parameters of the coils is systematically assessed.<br>Doctorat en Sciences<br>info:eu-repo/semantics/nonPublished

APA, Harvard, Vancouver, ISO, and other styles

8

Langlois, Yilin. "Modélisation de l’arc électrique dans un disjoncteur à vide." Thesis, Vandoeuvre-les-Nancy, INPL, 2010. http://www.theses.fr/2010INPL062N/document.

Full text

Abstract:

Un modèle numérique d’un arc électrique diffus dans un disjoncteur à vide à champ magnétique axial (AMF) a été développé dans le but de mieux comprendre à terme la transition d’un mode de fonctionnement diffus de l’arc vers un mode plus concentré. Le comportement du plasma d’arc a été simulé depuis la sortie de la zone de mélange cathodique jusqu’à l’entrée de la gaine anodique. Le modèle bidimensionnel est basé sur un système d’équations hydrodynamiques à deux fluides non magnétisés (ions et électrons), incluant les équations de conservation d’énergie ionique et électronique. Il est démontré que les processus d’ionisation et de recombinaison et les effets visqueux sont négligeables. Les transferts radiatifs ne sont pas considérés en première approximation. Outre les forces dues au champ AMF, le modèle inclut les forces dues aux trois composantes du champ magnétique induit par l’arc. Deux régimes d’écoulement des ions, supersonique (aux faibles densités de courant) et subsonique (aux fortes densités de courant), sont considérés. Près de la cathode, les conditions aux limites sont spécifiées à partir de résultats de la littérature. A proximité de l’anode, elles sont basées sur une description simplifiée de la gaine anodique. Les résultats de simulation présentés mettent en évidence une constriction du courant et un comportement différent des ions aux faibles et aux fortes densités de courant, et renseignent sur l’influence de divers paramètres (intensité du courant, distance interélectrode). Ce travail présente également une étude expérimentale, basée sur des visualisations par vidéo rapide de l’arc et des mesures pyrométriques de la température de la surface de l’anode<br>A model of a diffuse arc in a vacuum circuit breaker with an axial magnetic field (AMF) has been developed with the ultimate aim to better understand the transition of the arc from a diffuse mode to a more confined mode. The interelectrode plasma is simulated from the exit of the mixing region on the cathode side to the entrance of the anode sheath. The two-dimensional model is based on the solution of a system of two-fluid (ions and electrons) hydrodynamic equations, including in particular the energy balance equations relative to both the ions and the electrons, which are treated as non-magnetized particles. It is demonstrated that ionisation and recombination processes, as well as viscous effects, can be neglected. Radiation losses are not taken into account in a first approximation. In addition to the forces due to the AMF, the model considers the forces created by the three components of the magnetic field induced by the arc current. The possibility of both supersonic (at low current density) and subsonic (at high current density) ionic flow regimes is considered. On the cathode side, the boundary conditions are specified using results from the literature. On the anode side, they are based on a simplified description of the anode sheath. The simulation results presented show a constriction of the current lines, emphasize the differences in the behaviour of the ions at low and high current densities, and provide some insight on the influence of various operating parameters (arc current, gap length). The present work comprises also an experimental study, based on high-speed camera visualisations of the arc and measurements of the temperature at the anode surface

APA, Harvard, Vancouver, ISO, and other styles

9

Garren, David Alan. "Magnetic field strength of toroidal plasma equilibria." W&M ScholarWorks, 1991. https://scholarworks.wm.edu/etd/1539623809.

Full text

Abstract:

The goal of nuclear fusion research is to confine a deuterium-tritium plasma at a sufficiently high temperature (15 keV) and density (3 $\times$ 10$\sp{20}$ m$\sp{-3}$) for a sufficient length of time (1 sec) to produce net fusion power. One means to attain the required plasma confinement is to embed the plasma within a magnetic field. The global structure of this magnetic field determines the variation of magnetic field strength within the surfaces of constant plasma pressure. This field strength variation in turn determines many of the stability and confinement properties of the plasma. This dissertation gives the first detailed exposition of the spectrum of possible forms for magnetic field strength corresponding to toroidal plasma equilibria, both within any three-dimensional volume and within any two-dimensional surface of constant plasma pressure. Constraints due to the toroidicity of the configuration and the divergence-free property of the magnetic field are found to limit the form of the field strength. Three-dimensional stellarator equilibria corresponding to a particular form of the magnetic field strength are especially interesting. These "quasi-helically symmetric" equilibria are non-axisymmetric, toroidal configurations in which the magnetic field strength depends on only one angular coordinate, instead of two, within the constant plasma pressure surfaces. Unlike conventional stellarator equilibria, these quasi-helically symmetric equilibria exhibit the favorable confinement properties of axisymmetric tokamak equilibria. We show that stellarators with exact quasi-helical symmetry do not to exist, but that good approximations can be found.

APA, Harvard, Vancouver, ISO, and other styles

10

Simakov, Andrei N. 1974. "Plasma stability in a dipole magnetic field." Thesis, Massachusetts Institute of Technology, 2001. http://hdl.handle.net/1721.1/60756.

Full text

Abstract:

Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2001.<br>Includes bibliographical references (p. 137-141).<br>The MHD and kinetic stability of an axially symmetric plasma, confined by a poloidal magnetic field with closed lines, is considered. In such a system the stabilizing effects of plasma compression and magnetic field compression counteract the unfavorable field line curvature and can stabilize pressure gradient driven magnetohydrodynamic modes provided the pressure gradient is not too steep. Isotropic pressure, ideal MHD stability is studied first and a general interchange stability condition and an integro-differential eigenmode equation for ballooning modes are derived, using the MHD energy principle. The existence of plasma equilibria which are both interchange and ballooning stable for arbitrarily large beta = plasma pressure / magnetic pressure, is demonstrated. The MHD analysis is then generalized to the anisotropic plasma pressure case. Using the Kruskal-Oberman form of the energy principle, and a Schwarz inequality, to bound the complicated kinetic compression term from below by a simpler fluid expression, a general anisotropic pressure interchange stability condition, and a ballooning equation, are derived. These reduce to the usual ideal MHD forms in the isotropic limit. It is typically found that the beta limit for ballooning modes is at or just below that for either the mirror mode or the firehose.<br>(cont.) Finally, kinetic theory is used to describe drift frequency modes and finite Larmor radius corrections to MHD modes. An intermediate collisionality ordering in which the collision frequency is smaller than the transit or bounce frequency, but larger than the mode, magnetic drift, and diamagnetic frequencies, is used for solving the full electromagnetic problem. An integro-differential eigenmode equation with the finite Larmor radius corrections is derived for ballooning modes. It reduces to the ideal MHD ballooning equation when the mode frequency exceeds the drift frequencies. In addition to the MHD mode, this ballooning equation permits an entropy mode solution whose frequency is of the order of the ion magnetic drift frequency. The entropy mode is an electrostatic flute mode, even in equilibrium of arbitrary beta. Stability boundaries for both modes, and the influence of collisional effects on these boundaries has also been investigated.<br>by Andrei N. Simakov.<br>Ph.D.

APA, Harvard, Vancouver, ISO, and other styles

More sources

Books on the topic "Plasma flow in magnetic field"

1

Stangeby, P. C. Comments on "A fluid theory of ion collection by probes in strong magnetic fields with plasma flow" [Phys. Fluids 30, 3777 (1987)]. [s.n.], 1988.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

2

York, Thomas M. The effects of magnetic nozzle configurations on plasma thrusters: Semi-annual progress report. National Aeronautics and Space Administration, Lewis Research Center, 1990.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

3

Hamilton, Russell J. Cyclotron maser and plasma wave growth in magnetic loops. National Aeronautics and Space Administration, 1990.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

4

Brosius, Jeffrey W. Plasma properties and magnetic field structure of the solar corona, based on coordinated Max '91 observations fron SERTS, the VLA, and magnetographs. National Aeronautics and Space Administration, 1995.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

5

Voorhies, Coerte V. Simultaneous solution for core magnetic field and fluid flow beneath an electrically conducting mantle. National Aeronautics and Space Administration, Goddard Space Flight Center, 1993.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

6

Voorhies, Coerte V. Simultaneous solution for core magnetic field and fluid flow beneath an electrically conducting mantle. National Aeronautics and Space Administration, Goddard Space Flight Center, 1993.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

7

Brosius, Jeffrey W. Plasma properties and magnetic field structure of the solar corona, based on coordinated Max '91 observations from SERTS, the VLA, and magnetographs: Final report of work on NASA grant NASW-4933, covering the period 12 July 1994 - 11 July 1996. National Aeronautics and Space Administration, 1996.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

8

Brosius, Jeffrey W. "Plasma properties and magnetic field structure of the solar corona, based on coordinated Max '91 observations fron SERTS, the VLA, and magnetographs": Annual report of work progress on NASA grant NASW-4933 covering the period 12 July 1994 - 11 July 1995. National Aeronautics and Space Administration, 1995.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

9

Manzella, David. High voltage SPT performance. National Aeronautics and Space Administration, Glenn Research Center, 2001.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

10

Moore, T. E. The geopause. National Aeronautics and Space Administration, 1995.

Find full text

APA, Harvard, Vancouver, ISO, and other styles

More sources

Book chapters on the topic "Plasma flow in magnetic field"

1

Somov, Boris V. "Stationary Plasma Flows in a Magnetic Field." In Fundamentals of Cosmic Electrodynamics. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1184-3_12.

Full text

APA, Harvard, Vancouver, ISO, and other styles

2

Somov, Boris V. "Plasma Flows in a Strong Magnetic Field." In Fundamentals of Cosmic Electrodynamics. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1184-3_8.

Full text

APA, Harvard, Vancouver, ISO, and other styles

3

Somov, Boris V. "Plasma Flows in a Strong Magnetic Field." In Astrophysics and Space Science Library. Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4614-4283-7_14.

Full text

APA, Harvard, Vancouver, ISO, and other styles

4

Somov, Boris V. "Cosmic Plasma Flows in a Strong Magnetic Field." In Astrophysics and Space Science Library. Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-015-9592-6_10.

Full text

APA, Harvard, Vancouver, ISO, and other styles

5

Nishida, Hiroyuki, Hiroyuki Ogawa, and Yoshifumi Inatani. "MHD Analysis of Force Acting on Dipole Magnetic Field in Magnetized Plasma Flow." In Computational Fluid Dynamics 2006. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-92779-2_120.

Full text

APA, Harvard, Vancouver, ISO, and other styles

6

Kervalishvili, Guram N., and Hermann Lühr. "Climatology of Air Upwelling and Vertical Plasma Flow in the Terrestrial Cusp Region: Seasonal and IMF-Dependent Processes." In Magnetic Fields in the Solar System. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-64292-5_11.

Full text

APA, Harvard, Vancouver, ISO, and other styles

7

Somov, Boris V. "Plasma Equilibrium in Magnetic Field." In Astrophysics and Space Science Library. Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4614-4283-7_19.

Full text

APA, Harvard, Vancouver, ISO, and other styles

8

Parker, E. N. "Magnetic Discontinuities From Field Topology." In Plasma Astrophysics And Space Physics. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4203-8_1.

Full text

APA, Harvard, Vancouver, ISO, and other styles

9

Clemente, Roberto Antonio. "Anisotropic Magnetic Confinement. Applications to Field-Reversed Configurations." In Plasma Physics. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4758-3_16.

Full text

APA, Harvard, Vancouver, ISO, and other styles

10

Yokoyama, Tatsuhiro, and Claudia Stolle. "Low and Midlatitude Ionospheric Plasma Density Irregularities and Their Effects on Geomagnetic Field." In Earth's Magnetic Field. Springer Netherlands, 2017. http://dx.doi.org/10.1007/978-94-024-1225-3_17.

Full text

APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "Plasma flow in magnetic field"

1

Zimmerman, Joseph W., David L. Carroll, Georgi Hristov, and Phillip J. Ansell. "Configuration Studies for a Plasma Actuator Technique using Arc Breakdown in a Magnetic Field." In 2018 Flow Control Conference. American Institute of Aeronautics and Astronautics, 2018. http://dx.doi.org/10.2514/6.2018-3758.

Full text

APA, Harvard, Vancouver, ISO, and other styles

2

Bobashev, Sergey, Yurii Golovachov, and David VanWie. "Deceleration of Supersonic Plasma Flow by an Applied Magnetic Field." In 33rd Plasmadynamics and Lasers Conference. American Institute of Aeronautics and Astronautics, 2002. http://dx.doi.org/10.2514/6.2002-2247.

Full text

APA, Harvard, Vancouver, ISO, and other styles

3

Kozlov, Andrey. "Plasma Flow Peculiarities in Accelerator Channel with Longitudinal Magnetic Field." In 37th AIAA Plasmadynamics and Lasers Conference. American Institute of Aeronautics and Astronautics, 2006. http://dx.doi.org/10.2514/6.2006-3564.

Full text

APA, Harvard, Vancouver, ISO, and other styles

4

Bobashev, S., Yu Golovachov, V. Maslennikov, et al. "Interaction of supersonic flow of xenon plasma with magnetic field." In 32nd AIAA Plasmadynamics and Lasers Conference. American Institute of Aeronautics and Astronautics, 2001. http://dx.doi.org/10.2514/6.2001-2879.

Full text

APA, Harvard, Vancouver, ISO, and other styles

5

Plechaty, C., R. Presura, S. Stein, L. O'Brien, S. Haque, and M. Tooth. "Investigation of plasma flow redirection by an externally applied magnetic field." In 2011 IEEE 38th International Conference on Plasma Sciences (ICOPS). IEEE, 2011. http://dx.doi.org/10.1109/plasma.2011.5992890.

Full text

APA, Harvard, Vancouver, ISO, and other styles

6

Chernyshev, Alexander, Yurii Golovachov, Yurii Kurakin, Alexander Schmidt, and David Van Wie. "Effect of an Applied Magnetic Field on Blunt Body Plasma Flow." In 44th AIAA Aerospace Sciences Meeting and Exhibit. American Institute of Aeronautics and Astronautics, 2006. http://dx.doi.org/10.2514/6.2006-1002.

Full text

APA, Harvard, Vancouver, ISO, and other styles

7

Bandyopadhyay, P., U. Konopka, K. Jiang, et al. "Magnetic Field Induced Shear Flow in a Strongly Coupled Complex Plasma." In DUSTY∕COMPLEX PLASMAS: BASIC AND INTERDISCIPLINARY RESEARCH: Sixth International Conference on the Physics of Dusty Plasmas. AIP, 2011. http://dx.doi.org/10.1063/1.3659857.

Full text

APA, Harvard, Vancouver, ISO, and other styles

8

Stein, Sandra, Radu Presura, Andrey Esaulov, Stephan Neff, David Martinez, and Christopher Plechaty. "Kelvin-Helmholtz instability in a sheared flow actuated by a magnetic field." In 2010 IEEE 37th International Conference on Plasma Sciences (ICOPS). IEEE, 2010. http://dx.doi.org/10.1109/plasma.2010.5534118.

Full text

APA, Harvard, Vancouver, ISO, and other styles

9

Den Hartog, D. J., A. F. Almagri, J. T. Chapman, et al. "Plasma flow and magnetic mode rotation in the MST reversed-field pinch." In International Conference on Plasma Science (papers in summary form only received). IEEE, 1995. http://dx.doi.org/10.1109/plasma.1995.531702.

Full text

APA, Harvard, Vancouver, ISO, and other styles

10

Domonkos, M. T., J. H. Degnan, P. E. Adamson, et al. "Adventures in the experimental development of an ultrahigh speed plasma flow." In 2012 14th International Conference on Megagauss Magnetic Field Generation and Related Topics (MEGAGAUSS). IEEE, 2012. http://dx.doi.org/10.1109/megagauss.2012.6781456.

Full text

APA, Harvard, Vancouver, ISO, and other styles

Reports on the topic "Plasma flow in magnetic field"

1

Gerwin, R. A., G. J. Marklin, A. G. Sgro, and A. H. Glasser. Characterization of Plasma Flow Through Magnetic Nozzles. Office of Scientific and Technical Information (OSTI), 1990. http://dx.doi.org/10.2172/763033.

Full text

APA, Harvard, Vancouver, ISO, and other styles

2

Fisch, Nathaniel J. Ultra-High Intensity Magnetic Field Generation in Dense Plasma. Office of Scientific and Technical Information (OSTI), 2014. http://dx.doi.org/10.2172/1115189.

Full text

APA, Harvard, Vancouver, ISO, and other styles

3

J.A. Krommes and Allan H. Reiman. Plasma Equilibrium in a Magnetic Field with Stochastic Regions. Office of Scientific and Technical Information (OSTI), 2009. http://dx.doi.org/10.2172/953207.

Full text

APA, Harvard, Vancouver, ISO, and other styles

4

Okuda, H., and S. Hiroe. Neutral beam injection and plasma convection in a magnetic field. Office of Scientific and Technical Information (OSTI), 1988. http://dx.doi.org/10.2172/7108894.

Full text

APA, Harvard, Vancouver, ISO, and other styles

5

J.A. Krommes. Statistical Plasma Physics in a Strong Magnetic Field: Paradigms and Problems. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/827685.

Full text

APA, Harvard, Vancouver, ISO, and other styles

6

Okuda, H., M. Ono, and R. J. Armstrong. Anomalous electron diffusion across a magnetic field in a beam-plasma system. Office of Scientific and Technical Information (OSTI), 1987. http://dx.doi.org/10.2172/5757792.

Full text

APA, Harvard, Vancouver, ISO, and other styles

7

Brooks, J. N. Near-surface sputtered particle transport for an oblique incidence magnetic field plasma. Office of Scientific and Technical Information (OSTI), 1989. http://dx.doi.org/10.2172/5343157.

Full text

APA, Harvard, Vancouver, ISO, and other styles

8

A. Reiman, M. Zarnstorff, D. Mikkelsen, et al. Interaction of Ambipolar Plasma Flow with Magnetic Islands in a Quasi-axisymmetric Stellarator. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/836570.

Full text

APA, Harvard, Vancouver, ISO, and other styles

9

Okuda, H., R. Horton, M. Ono, and M. Ashour-Abdalla. Propagation of a nonrelativistic electron beam in a plasma in a magnetic field. Office of Scientific and Technical Information (OSTI), 1986. http://dx.doi.org/10.2172/6979454.

Full text

APA, Harvard, Vancouver, ISO, and other styles

10

Reed, C. B., and S. Molokov. Flow of two-dimensional liquid metal jet in a strong magnetic field. Office of Scientific and Technical Information (OSTI), 2002. http://dx.doi.org/10.2172/821667.

Full text

APA, Harvard, Vancouver, ISO, and other styles

We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!