1 S. CHABLE a F. ROGIER b a - ONERA, 2 av. Ed. Belin, 31055 TOULOUSE Cedex 4 b - MIP, Université Paul Sabatier, 118, route de Narbonne, 31062 TOULOUSE.

Slides:



Advertisements
Similar presentations
X X X X X10 14.
Advertisements

Numerical investigations of a cylindrical Hall thruster K. Matyash, R. Schneider, O. Kalentev Greifswald University, Greifswald, D-17487, Germany Y. Raitses,
Chapter 4 Waves in Plasmas 4.1 Representation of Waves 4.2 Group velocity 4.3 Plasma Oscillations 4.4 Electron Plasma Waves 4.5 Sound Waves 4.6 Ion Waves.
INTRODUCTION OF WAVE-PARTICLE RESONANCE IN TOKAMAKS J.Q. Dong Southwestern Institute of Physics Chengdu, China International School on Plasma Turbulence.
6. Wave Phenomena 6.1 General Wave Properties(1) Following Schunk’s notation, we use index 1 to indicate the electric and magnetic wave fields, E 1 and.
F. Cheung, A. Samarian, B. James School of Physics, University of Sydney, NSW 2006, Australia.
Modeling Generation and Nonlinear Evolution of VLF Waves for Space Applications W.A. Scales Center of Space Science and Engineering Research Virginia Tech.
Modeling Generation and Nonlinear Evolution of Plasma Turbulence for Radiation Belt Remediation Center for Space Science & Engineering Research Virginia.
Generation of intense quasistatic fields at high altitudes by the Ionospheric Alfvén Resonator Bill Lotko, Jon Watts, Anatoly Streltsov Thayer School of.
F. Nabais - Vilamoura - November 2004 Internal kink mode stability in the presence of ICRH driven fast ions populations F. Nabais, D. Borba, M. Mantsinen,
NUMERICAL INVESTIGATION OF WAVE EFFECTS IN HIGH-FREQUENCY CAPACITIVELY COUPLED PLASMAS* Yang Yang and Mark J. Kushner Department of Electrical and Computer.
Damping of Whistler Waves through Mode Conversion to Lower Hybrid Waves in the Ionosphere X. Shao, Bengt Eliasson, A. S. Sharma, K. Papadopoulos, G. Milikh.
Hybrid Simulation of Ion-Cyclotron Turbulence Induced by Artificial Plasma Cloud in the Magnetosphere W. Scales, J. Wang, C. Chang Center for Space Science.
Francesco Valentini, Pierluigi Veltri Dipartimento di Fisica, Università degli Studi della Calabria (Italy) Dipartimento di Fisica, Università degli Studi.
Collisional ionization in the beam body  Just behind the front, by continuity  →0 and the three body recombination  (T e,E) is negligible.
Convection in Neutron Stars Department of Physics National Tsing Hua University G.T. Chen 2004/5/20 Convection in the surface layers of neutron stars Juan.
INVESTIGATIONS OF MAGNETICALLY ENHANCED RIE REACTORS WITH ROTATING (NON-UNIFORM) MAGNETIC FIELDS Natalia Yu. Babaeva and Mark J. Kushner University of.
Physics of fusion power Lecture 10 : Running a discharge / diagnostics.
5. Simplified Transport Equations We want to derive two fundamental transport properties, diffusion and viscosity. Unable to handle the 13-moment system.
Computationally efficient description of relativistic electron beam transport in dense plasma Oleg Polomarov*, Adam Sefkov**, Igor Kaganovich** and Gennady.
Effects of Magnetic Field on Two-Plasmon Decay Instability in Homogeneous Plasma Xinfeng Sun ( 孙新锋 ), Zhonghe Jiang ( 江中和 ), Xiwei Hu ( 胡希伟 ) School of.
Physics of Fusion power Lecture4 : Quasi-neutrality Force on the plasma.
F.M.H. Cheung School of Physics, University of Sydney, NSW 2006, Australia.
Tangential discontinuities as “roots” of auroral arcs: an electrostatic magnetosphere-ionosphere coupling mode M. Echim (1,2), M. Roth (1), J.de Keyser.
Wave induced supersonic rotation in mirrors Abraham Fetterman and Nathaniel Fisch Princeton University.
Large-amplitude oscillations in a Townsend discharge in low- current limit Vladimir Khudik, Alex Shvydky (Plasma Dynamics Corp., MI) Abstract We have developed.
Overview of equations and assumptions Elena Khomenko, Manuel Collados, Antonio Díaz Departamento de Astrofísica, Universidad de La Laguna and Instituto.
Interplay of the Turbulence and Strong Coulomb’s Coupling in the Formation of the Anomalous Plasma Resistance Yurii V. Dumin Institute of Ionosphere and.
Microstability analysis of e-ITBs in high density FTU plasmas 1)Associazione EURATOM-ENEA sulla fusione, C.R. Frascati, C.P , Frascati, Italy.
ACKNOWLEDGMENTS This research was supported by the National Science Foundation of China (NSFC) under grants , , , the Specialized.
What are helicons? Helicons are partially ionized RF discharges in a magnetic field. They are basically whistler modes confined to a cylinder. They are.
1 SIMULATION OF VIBROACOUSTIC PROBLEM USING COUPLED FE / FE FORMULATION AND MODAL ANALYSIS Ahlem ALIA presented by Nicolas AQUELET Laboratoire de Mécanique.
Why plasma processing? (1) UCLA Accurate etching of fine features.
Stability Properties of Field-Reversed Configurations (FRC) E. V. Belova PPPL 2003 International Sherwood Fusion Theory Conference Corpus Christi, TX,
L4 ECE-ENGR 4243/ FJain 1 Derivation of current-voltage relation in 1-D wires/nanotubes (pp A) Ballistic, quasi-ballistic transport—elastic.
The Propagation of Electromagnetic Wave in Atmospheric Pressure Plasma Zhonghe Jiang XiWei Hu Shu Zhang Minghai Liu Huazhong University of Science & Technology.
1 Three views on Landau damping A. Burov AD Talk, July 27, 2010.
Nonlinear interactions between micro-turbulence and macro-scale MHD A. Ishizawa, N. Nakajima, M. Okamoto, J. Ramos* National Institute for Fusion Science.
Two problems with gas discharges 1.Anomalous skin depth in ICPs 2.Electron diffusion across magnetic fields Problem 1: Density does not peak near the.
Computational Modeling of Hall Thrusters Justin W. Koo Department of Aerospace Engineering University of Michigan Ann Arbor, Michigan
Electron inertial effects & particle acceleration at magnetic X-points Presented by K G McClements 1 Other contributors: A Thyagaraja 1, B Hamilton 2,
M. Onofri, F. Malara, P. Veltri Compressible magnetohydrodynamics simulations of the RFP with anisotropic thermal conductivity Dipartimento di Fisica,
Quality of model and Error Analysis in Variational Data Assimilation François-Xavier LE DIMET Victor SHUTYAEV Université Joseph Fourier+INRIA Projet IDOPT,
Physics of fusion power Lecture 12: Diagnostics / heating.
17th Cluster Workshop May 2009 R. Maggiolo 1, M. Echim 1,2, M. Roth 1, J. De Keyser 1 1 BIRA-IASB Brussels, Belgium 2 ISS Bucharest, Romania Quasi-stationary.
Radiation spectra from relativistic electrons moving in turbulent magnetic fields Yuto Teraki & Fumio Takahara Theoretical Astrophysics Group Osaka Univ.,
A. Vaivads, M. André, S. Buchert, N. Cornilleau-Wehrlin, A. Eriksson, A. Fazakerley, Y. Khotyaintsev, B. Lavraud, C. Mouikis, T. Phan, B. N. Rogers, J.-E.
Weakly Collisional Landau Damping and BGK Modes: New Results on Old Problems A. Bhattacharjee, C. S. Ng, and F. Skiff Space Science Center University of.
Session SA33A : Anomalous ionospheric conductances caused by plasma turbulence in high-latitude E-region electrojets Wednesday, December 15, :40PM.
Chernoshtanov I.S., Tsidulko Yu.A.
Simulations of NBI-driven Global Alfven Eigenmodes in NSTX E. V. Belova, N. N. Gorelenkov, C. Z. Cheng (PPPL) NSTX Results Forum, PPPL July 2006 Motivation:
of magnetized discharge plasmas: fluid electrons + particle ions
1 Magnetic components existing in geodesic acoustic modes Deng Zhou Institute of Plasma Physics, Chinese Academy of Sciences.
Simulations of turbulent plasma heating by powerful electron beams Timofeev I.V., Terekhov A.V.
21st IAEA Fusion Energy Conf. Chengdu, China, Oct.16-21, /17 Gyrokinetic Theory and Simulation of Zonal Flows and Turbulence in Helical Systems T.-H.
1 ASIPP Sawtooth Stabilization by Barely Trapped Energetic Electrons Produced by ECRH Zhou Deng, Wang Shaojie, Zhang Cheng Institute of Plasma Physics,
Generation of anomalously energetic suprathermal electrons by an electron beam interacting with a nonuniform plasma Dmytro Sydorenko University of Alberta,
Energetic ion excited long-lasting “sword” modes in tokamak plasmas with low magnetic shear Speaker:RuiBin Zhang Advisor:Xiaogang Wang School of Physics,
“Harris” Equilibrium: Initial State for a Broad Class of
Fluid simulation of instabilities in partially magnetized plasmas
ICPs show anomalous skin depth
Nonequilibrium statistical mechanics of electrons in a diode
Experiment Experiment: thing ferromagnetic films
Non-Invasive Characterization of the Hall Thruster Breathing Mode
Coronal Loop Oscillations observed by TRACE
Study of Fast Ions in CESR
2. Crosschecking computer codes for AWAKE
Accelerator Physics G. A. Krafft, A. Bogacz, and H. Sayed
D. V. Rose, T. C. Genoni, and D. R. Welch Mission Research Corp.
Accelerator Physics G. A. Krafft, A. Bogacz, and H. Sayed
Presentation transcript:

1 S. CHABLE a F. ROGIER b a - ONERA, 2 av. Ed. Belin, TOULOUSE Cedex 4 b - MIP, Université Paul Sabatier, 118, route de Narbonne, TOULOUSE Cedex Numerical Investigation and Modeling of Stationary Plasma Thruster Low Frequency Oscillations

2 Scheme of a SPT Magnetic field  Electrons confined in the channel Electric field  Ions accelerated

3 è Advantages : thrusters lower and more accurate than chemical conventional systems (thrust of some mN). è Development since three decades by the Russians. è Development nowadays in U.SA. (M.I.T.), in Russia, in Japan and in France (LPMI, CPAT, CNES, ONERA, LPGP, SNECMA, Astrium...). è Research axes : - clarifications of the mechanisms responsible for the plasma conductivity - reduction of the divergence of the plume - reduction of the low frequency oscillations è Numerical simulations Context

4 1. Introduction 2. Physical model 3. Study of the linear instability modes 4. A simplified model 5. Control of the instabilities 6. Conclusion Plan

5 Bibliography Classification of the low frequency oscillations (Choueri) : è 1-20 kHz band : « loop » axial oscillations, sensitive to the magnetic field and the applied voltage, related to a predator prey model or a depletion of the neutrals - Garrigues and Bœuf (1998), Chesta et al. (2001), Litvak and Fisch (2001). è 5-25 kHz band : rotating spoke related to the ionization process – Janes and Lowder (1966). è kHz band : azimuthal oscillations associated with the gradient of density – Esipchuck and Tilinin (1976). è kHz : oscillations due to the the low ionization of the plasma – Popovic and Melchior (1968).

6 Physical model : Modelization Assumptions : è Ions transport scale time. è è Strong electron-neutral elastic collision rate : Maxwellian fluid for the electrons. è Ballistic neutrals and ions. è Magnetic field not sensitive to the plasma. è Ions not sensitive to the magnetic field. è Monokinetic neutral distribution è Quasineutrality è Inclusion of an electron-wall collision frequency (Bœuf-Garrigues model)

7 Physical model Avec et 1D model and neutral and ion distribution functions,, and are the neutral, ion and electron densities. is the electron mean energy. is the electric potential, the magnetic field. and the ionization rate, the elastic collision rate and the inelastic collision rate. the electron-wall collision frequency and the electron mobility.

8 Linearization Remark : the non local terms don’t allow us to conclude to the dissipation of the perturbed solution. Friedrichs system

9 Link linear – non linear Discretization : the problem is unstable if the positive real part of the eigenvalues is positive Discretized system : Observation : linear instability è The link between the ion Vlasov equation and the electric potential is the mechanism responsible for the instabilities.

10 Link linear – non linear Link between the growth rate and the amplitude of the non linear oscillations. Amplitude of the non linear oscillations obtained from the transient model Growth rate obtained from the linear model. Variation function of

11 Simplified model Assumptions : è Electron mean energy given and constant. è Neutral density given and constant. è Source term neglected. è Linear model : with :

12 Theorical instability Theorem : The problem is bivalued. If is solution so is solution too. è Unstable problem è Relationship with Buneman instability è Control of the instabilities : topology of B, electron-wall collision frequency.

13 Conclusion Treated points : è Spectral study of the linear instability with a stationary quasineutral hybrid model  relationship between the growth rate and the amplitude of the non linear model. è Simplified model to explain the instabilities  relationship with the Buneman instabilities. è Control of the instabilities by modifying the magnetic field of the electron-wall collision frequency. è Predictive model

14