Numerical modeling of space plasma flows

ASTRONUM-2006, proceedings of the 1st IGPP-CalSpace International Conference held at Palm Springs, California, USA, 26-30 March 2006 by ASTRONUM-2006 (2006 Palm Springs, Calif.)

Publisher: Astronomical Society of the Pacific Conference Series ASPCS in San Francisco, CA

Written in English
Cover of: Numerical modeling of space plasma flows | ASTRONUM-2006 (2006 Palm Springs, Calif.)
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Subjects:

  • Space plasmas -- Congresses,
  • Plasma turbulence -- Congresses

Edition Notes

Includes bibliographical references.

Statementedited by Nikolai V. Pogorelov and Gary P. Zank.
GenreCongresses.
SeriesAstronomical Society of the Pacific conference series ; v. 359
ContributionsPogorelov, Nikolai V., Zank, G. P.
Classifications
LC ClassificationsQC809.P5 A77 2006
The Physical Object
Paginationxii, 312 p. :
Number of Pages312
ID Numbers
Open LibraryOL17926066M
ISBN 10158381227X
ISBN 109781583812273
LC Control Number2006938400

Numerical modeling of space plasma flows (astronum ). Proceedings of a 6th internation conference held at Velancia, Spain June , ASP Conference Series, Vol. 8th International Conference of Numerical Modeling of Space Plasma Flows (ASTRONUM ) Pogorelov, N. V.; Audit, E.; Zank, G. P. Abstract. Not Available. Publication: 8th International Conference of Numerical Modeling of Space Plasma Flows (ASTRONUM ) Pub Date: Author: N. V. Pogorelov, E. Audit, G. P. Zank. To study this problem, we present a numerical model that simulates the coupling of a Bingham plastic mudslide on a gentle uniform slope with the surface waves which it generates. A formulation of the dynamics of the problem is presented, where the landslide is treated as an incompressible Bingham plastic flow and the water motion is assumed Cited by: Fully kinetic numerical modeling of a plasma thruster in velocity space. Ion-electron recombination was modeled at the boundaries, and neutrals were recycled into the flow. including the.

Several numerical models representing the void space geometries at different shear displacements, as listed in Table , were constructed to investigate the fluid flow characteristics during coupled shear–flow g 3D Navier–Stokes equations is very time-consuming, therefore, the mesh size in the x–y plane of numerical models was simplified to × mm 2, which was. Note that as a consequence of the plasma flow reduction, the reconnected lines are pulled away from the planet by the ML effects Murawski and R. S. Steinolfson: Numerical modeling of the solar wind interaction th Venus Fig. 3. A summary of the field line behaviors in the NL (a) and ML (b) by: Plasma Modeling: Methods and Applications presents and discusses the different approaches that can be adopted for plasma modeling, giving details about theoretical and numerical methods. In geology, numerical modeling is a widely applied technique to tackle complex geological problems by computational simulation of geological scenarios.. Numerical modeling uses mathematical models to describe the physical conditions of geological scenarios using numbers and equations. Nevertheless, some of their equations are difficult to solve directly, such as partial differential equations.

Workshop on Numerical Modeling in MHD and Plasma Physics: methods, tools, and outcomes. The position of the phase boundary depends on discontinuous time- and space-nonlinear coefficients and boundary conditions. The aim of the study is to provide a detailed resolution of the heat flow deep into the material with a fine spatial grid step. Mary Hudson studies space weather patterns that originate from solar eruptions following energy and mass transfers through the interplanetary medium all the way the the Earth's ionosphere. Current investigations focus on the evolution of the Van Allen radiation belts. Barrett Rogers's space physics research focuses on the physics of magnetic reconnection, particle acceleration, global. Issue 10 - Decemer - Dielectric Barrier Discharge Based Plasma Actuators for Flow Control AL Plasmas for Aeronautics Numerical Modeling of Dielectric Barrier Discharge Based Plasma Actuators for Flow Control: the COPAIER/CEDRE Example G. Dufour, F. Rogier (ONERA) E-mail: @ DOI: /AL   Numerical Investigation of Nonequilibrium Plasma Flows in Constrictor- and Segmented-Type Arc Heaters. JOURNAL OF THE JAPAN SOCIETY FOR AERONAUTICAL AND SPACE SCIENCES, Vol. 67, No. 2 Plasma flow modeling for Huels-type arc heater with turbulent diffusion. Physics of Plasmas, Vol. 24, No. 12 Cited by:

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Pogorelov and Gary P. Zank Reconnection-generated Plasma Flows Interacting with the Near-Earth Plasma Sheet P. Pritchett. NUMERICAL MODELING OF SPACE PLASMA FLOWS ASTRONUM Proceedings of the 4th International Conference held at Chamonix, France June 29 - July 3, Edited by:_ Nikolai V.

Pogorelov 'Department of Physics and Center for Space Plasma and Aeronomic Research, Unversity of Alabama in Huntsville Edouard Audit. Physics of Space Plasmas: An Introduction 2nd Edition In its inaugural edition, Physics of Space Plasmas was the most widely used textbook for courses in space plasma physics, and included up-to-date observations from space available at the time.

Throughout universities in the United States and abroad-it has proven itself by: BibTeX @MISC{Pogorelov06in“numerical, author = {N. Pogorelov and J. Raeder and H. Yee and G. Zank and Alexei G. Kritsuk and Rick Wagner and Michael L.

Norman and Paolo Padoan}, title = {In “Numerical Modeling of Space Plasma Flows” ASP Conference Series, Vol. XXX, }, year =. Numerical Modeling of Space Plasma Flows ASTRONUM, ASP Volume Proceedings of a 9th International Conference Held Jun, in Long Beach, by N.V. Pogorelov et al. San Francisco: Astronomical Society of the Pacidic, (1) Advanced numerical methods for space and astrophysical flows; (2) Large-scale fluid-based, kinetic, and hybrid simulations; (3) Turbulence and cosmic ray transport; (4) Magnetohydrodynamics (5) Software packages for modeling and analyzing plasma flows / Visualisation with the application to.

A two-dimensional air plasma modeling including complex air kinetic and flow motion is proposed to describe the plasma creation. The net force exerted by the plasma on the flow is introduced in a Navier–Stokes solver to evaluate the modifications of the flow. This model is able to compute pin plate coronas discharges as well as wire to : François Rogier, Jean-Charles Mateo-Velez, Géraldine Quinio.

Plasma Modeling: Methods and Applications presents and discusses the different approaches that can be adopted for plasma modeling, giving details about theoretical and numerical methods.

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Genre/Form: Conference papers and proceedings Congresses: Additional Physical Format: Online version: ASTRONUM ( San Diego, Calif.). Numerical modeling of space plasma flows. 12th International Conference on Numerical Modeling of Space Plasma Flows: ASTRONUM To cite this article: J.

Phys.: Conf. Ser. View the article online for updates and enhancements. Related content 11th International Conference on Numerical Modeling of Space Plasma Flows: ASTRONUMASTRONUM In the frame of the internal project PUMA (Plasma Used to Master Aerodynamics), ONERA is conducting fundamental studies of plasma-flow interactions.

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Model assumptions (a) The plasma flow is two-dimensional and axisymmetric. (b) The plasma is considered as a Newtonian fluid following the Navier-Stokes. 5th international conference of numerical modeling of space plasma flows (astronum ).

Proceedings of a 5th international conference held at San Diego, California, USA June Edited by Nikolai V. Pogorelov. Get this from a library. Numerical modeling of space plasma flows: ASTRONUM proceedings of the 1st IGPP-CalSpace International Conference held at Palm Springs, California, USA, March [Nikolai V Pogorelov; G P Zank;].

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Two-dimensional numerical model of plasma flow in a Hall thruster. Journal of the Japan Society for Aeronautical and Space Sciences, Vol. 65, No. 2. One-dimensional model of the plasma flow in a Hall thruster.

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