Self-Organization of Plasmas with Flows

Size: px
Start display at page:

Download "Self-Organization of Plasmas with Flows"

Transcription

1 Self-Organization of Plasmas with Flows ICNSP 2003/ 9/10 Graduate School of Frontier Sciences,, National Institute for Fusion Science R. NUMATA, Z. YOSHIDA, T. HAYASHI ICNSP 2003/ 9/10 p.1/14

2 Abstract We have developed a three dimensional nonlinear Hall-Magnetohydrodynamics (Hall-MHD) code, and obtained the double Beltrami Equilibrium, which is a theoretically predicted structure in the Hall-MHD plasma. ICNSP 2003/ 9/10 p.2/14

3 !! & % $ # # " ' Double Beltrami Equilibrium Incompressible two-fluid MHD equations can be cast into coupled vortex equations (electron inertia, displacement current are neglected) (1) where are the generalized vorticities and are the corresponding flows, (2) ). Combining two Beltrami conditions yield ( : ion collisionless skin depth, : speed of light, : ion plasma frequency, : system size). A simplest equilibrium solution is given by the Beltrami conditions ( 2nd-order equation for and, " % ',/. + *) (,- + *) ( (3) where, ICNSP 2003/ 9/10 p.3/14

4 0 0 0, ( Double Beltrami Equilibrium The general solution is described by a linear combination of eigenfunctions of the curl operator ( ) :, ,..(4) The Beltrami conditions give a special class of solution of the general steady state solution such that (5) where is a certain scalar field corresponding the energy density. The latter equality, called the generalized Bernoulli condition, demands the energy density is uniform in space. From the original electron and ion momentum equations, we find that the generalized Bernoulli condition is given by the relation, (6) ICNSP 2003/ 9/10 p.4/14

5 (7) (8) + ( (9) (10) (11) (12) ICNSP 2003/ 9/10 p.5/14 Relaxation Process Global Invariants * + ( * + ( Variational Principle Z.Yoshida and S.M.Mahajan, Phys. Rev. Lett., 88, (2002) are Lagrange multipliers.

6 3 8 Simulation Model We consider compressible Hall-MHD equations (13) (14) (15) 9 (16) (17) : where : density, : number density, : ion pressure, : Reynolds number, magnetic Reynolds number, : ratio of specific heat. We have assumed the quasi-neutrality, and. ICNSP 2003/ 9/10 p.6/14

7 Simulation Model Simulation Domain 3 dimensional rectangular domain Boundary Condition Periodic in direction Rigid perfect conducting wall in 5 5 direction 5 5 (18) (19) where is a unit normal vector, is a normal derivative, and and tangential component of the magnetic field, respectively. To assure tangential components of the electric field vanish, we set is the normal at the wall. Numerical Method 2nd order central difference in space, the Runge-Kutta-Gill method for time integration 2nd order smoothing to suppress short wave length mode add a diffusion in the equation of continuity to keep density positive ICNSP 2003/ 9/10 p.7/14

8 Dispersion Relation In order to check the validity of the code, we have solved the dispersion relation of purely transversal wave in a periodic domain. In an ideal limit, the dispersion relation for small perturbations around a uniform equilibrium, are constants, is given by 7 9 (20) which describes the Alfvén whistler wave. ω numerical ε=0 ε=0.1 (+) ε=0.1 (-) ε=0.05 (+) ε=0.05 (-) analitical ε=0 ε=0.1 (+) ε=0.1 (-) ε=0.05 (+) ε=0.05 (-) k ICNSP 2003/ 9/10 p.8/14

9 (21) (22) (23) ICNSP 2003/ 9/10 p.9/14 Initial Condition 2D force free equilibrium ( ) R.Horiuchi and T.Sato, Phys. Rev. Lett., 55, 211 (1985) ( ( ( ( ( ( ( ( t/ta= Flow (24) Density and Pressure are uniform Bz isosurface

10 ICNSP 2003/ 9/10 p.10/14 Equilibrium State 5 Aspect Ratio : Grid :,

11 5 4 Beltrami Conditions (25) (a) distribution of a (b) distribution of b (26) (27) Beltrami Parameters a b σ t/τa (c) distribution of σ (d) temporal behavior of a,b,σ ICNSP 2003/ 9/10 p.11/14

12 ( Bernoulli Conditions (28) (a) V (b) p ICNSP 2003/ 9/10 p.12/14

13 Variational Principles Energy Electron Helicity Ion Helicity Enstrophy t/τa ICNSP 2003/ 9/10 p.13/14

14 Summary We have developed a nonlinear 3D Hall-MHD simulation code. Flow with perpendicular components remains in the two-fluid relaxed state, while it disappears in the single-fluid MHD model relaxed state. Beltrami & Bernoulli conditions are investigated for two-fluid relaxed state. High resolution simulation is necessary to see the scale separation. Further investigation of parameter dependence, compressibility effect, etc. ICNSP 2003/ 9/10 p.14/14

Macroscopic plasma description

Macroscopic plasma description Macroscopic plasma description Macroscopic plasma theories are fluid theories at different levels single fluid (magnetohydrodynamics MHD) two-fluid (multifluid, separate equations for electron and ion

More information

A Comparison between the Two-fluid Plasma Model and Hall-MHD for Captured Physics and Computational Effort 1

A Comparison between the Two-fluid Plasma Model and Hall-MHD for Captured Physics and Computational Effort 1 A Comparison between the Two-fluid Plasma Model and Hall-MHD for Captured Physics and Computational Effort 1 B. Srinivasan 2, U. Shumlak Aerospace and Energetics Research Program University of Washington,

More information

Two Fluid Dynamo and Edge-Resonant m=0 Tearing Instability in Reversed Field Pinch

Two Fluid Dynamo and Edge-Resonant m=0 Tearing Instability in Reversed Field Pinch 1 Two Fluid Dynamo and Edge-Resonant m= Tearing Instability in Reversed Field Pinch V.V. Mirnov 1), C.C.Hegna 1), S.C. Prager 1), C.R.Sovinec 1), and H.Tian 1) 1) The University of Wisconsin-Madison, Madison,

More information

Transition From Single Fluid To Pure Electron MHD Regime Of Tearing Instability

Transition From Single Fluid To Pure Electron MHD Regime Of Tearing Instability Transition From Single Fluid To Pure Electron MHD Regime Of Tearing Instability V.V.Mirnov, C.C.Hegna, S.C.Prager APS DPP Meeting, October 27-31, 2003, Albuquerque NM Abstract In the most general case,

More information

Formation and Long Term Evolution of an Externally Driven Magnetic Island in Rotating Plasmas )

Formation and Long Term Evolution of an Externally Driven Magnetic Island in Rotating Plasmas ) Formation and Long Term Evolution of an Externally Driven Magnetic Island in Rotating Plasmas ) Yasutomo ISHII and Andrei SMOLYAKOV 1) Japan Atomic Energy Agency, Ibaraki 311-0102, Japan 1) University

More information

Extended MHD simulation of Rayleigh-Taylor/Kelvin-Helmholtz instability

Extended MHD simulation of Rayleigh-Taylor/Kelvin-Helmholtz instability Extended MHD simulation of Rayleigh-Taylor/Kelvin-Helmholtz instability R. Goto (a), T. Hatori (a), H. Miura (a, b), A. Ito (a, b) and M. Sato (b) (a) The Graduate University for Advanced Studies (Sokendai)

More information

Fluid equations, magnetohydrodynamics

Fluid equations, magnetohydrodynamics Fluid equations, magnetohydrodynamics Multi-fluid theory Equation of state Single-fluid theory Generalised Ohm s law Magnetic tension and plasma beta Stationarity and equilibria Validity of magnetohydrodynamics

More information

Nonlinear Processes in Two-Fluid Plasmas

Nonlinear Processes in Two-Fluid Plasmas Nonlinear Processes in Two-Fluid Plasmas Ryusuke Numata December, 2003 Graduate School of Frontier Sciences, The University of Tokyo Contents 1 Introduction 1 2 Hall Magnetohydrodynamics and Equilibrium

More information

A Study of 3-Dimensional Plasma Configurations using the Two-Fluid Plasma Model

A Study of 3-Dimensional Plasma Configurations using the Two-Fluid Plasma Model A Study of 3-Dimensional Plasma Configurations using the Two-Fluid Plasma Model B. Srinivasan, U. Shumlak Aerospace and Energetics Research Program University of Washington IEEE International Conference

More information

The Physics of Fluids and Plasmas

The Physics of Fluids and Plasmas The Physics of Fluids and Plasmas An Introduction for Astrophysicists ARNAB RAI CHOUDHURI CAMBRIDGE UNIVERSITY PRESS Preface Acknowledgements xiii xvii Introduction 1 1. 3 1.1 Fluids and plasmas in the

More information

Magneto-Fluid Coupling in Dynamic Finely Structured Solar Atmosphere Theory and Simulation

Magneto-Fluid Coupling in Dynamic Finely Structured Solar Atmosphere Theory and Simulation Magneto-Fluid Coupling in Dynamic Finely Structured Solar Atmosphere Theory and Simulation Nana L. Shatashvili 1,2, In collaboration with S. M. Mahajan 2, Z. Yoshida 3 R. Miklaszewski 4 & K.I. Nikol skaya

More information

Applying Asymptotic Approximations to the Full Two-Fluid Plasma System to Study Reduced Fluid Models

Applying Asymptotic Approximations to the Full Two-Fluid Plasma System to Study Reduced Fluid Models 0-0 Applying Asymptotic Approximations to the Full Two-Fluid Plasma System to Study Reduced Fluid Models B. Srinivasan, U. Shumlak Aerospace and Energetics Research Program, University of Washington, Seattle,

More information

Reduced MHD. Nick Murphy. Harvard-Smithsonian Center for Astrophysics. Astronomy 253: Plasma Astrophysics. February 19, 2014

Reduced MHD. Nick Murphy. Harvard-Smithsonian Center for Astrophysics. Astronomy 253: Plasma Astrophysics. February 19, 2014 Reduced MHD Nick Murphy Harvard-Smithsonian Center for Astrophysics Astronomy 253: Plasma Astrophysics February 19, 2014 These lecture notes are largely based on Lectures in Magnetohydrodynamics by Dalton

More information

Waves in plasma. Denis Gialis

Waves in plasma. Denis Gialis Waves in plasma Denis Gialis This is a short introduction on waves in a non-relativistic plasma. We will consider a plasma of electrons and protons which is fully ionized, nonrelativistic and homogeneous.

More information

Chapter 1. Introduction to Nonlinear Space Plasma Physics

Chapter 1. Introduction to Nonlinear Space Plasma Physics Chapter 1. Introduction to Nonlinear Space Plasma Physics The goal of this course, Nonlinear Space Plasma Physics, is to explore the formation, evolution, propagation, and characteristics of the large

More information

20. Alfven waves. ([3], p ; [1], p ; Chen, Sec.4.18, p ) We have considered two types of waves in plasma:

20. Alfven waves. ([3], p ; [1], p ; Chen, Sec.4.18, p ) We have considered two types of waves in plasma: Phys780: Plasma Physics Lecture 20. Alfven Waves. 1 20. Alfven waves ([3], p.233-239; [1], p.202-237; Chen, Sec.4.18, p.136-144) We have considered two types of waves in plasma: 1. electrostatic Langmuir

More information

CHAPTER 7 SEVERAL FORMS OF THE EQUATIONS OF MOTION

CHAPTER 7 SEVERAL FORMS OF THE EQUATIONS OF MOTION CHAPTER 7 SEVERAL FORMS OF THE EQUATIONS OF MOTION 7.1 THE NAVIER-STOKES EQUATIONS Under the assumption of a Newtonian stress-rate-of-strain constitutive equation and a linear, thermally conductive medium,

More information

SW103: Lecture 2. Magnetohydrodynamics and MHD models

SW103: Lecture 2. Magnetohydrodynamics and MHD models SW103: Lecture 2 Magnetohydrodynamics and MHD models Scale sizes in the Solar Terrestrial System: or why we use MagnetoHydroDynamics Sun-Earth distance = 1 Astronomical Unit (AU) 200 R Sun 20,000 R E 1

More information

Simple examples of MHD equilibria

Simple examples of MHD equilibria Department of Physics Seminar. grade: Nuclear engineering Simple examples of MHD equilibria Author: Ingrid Vavtar Mentor: prof. ddr. Tomaž Gyergyek Ljubljana, 017 Summary: In this seminar paper I will

More information

MHD Simulation of High Wavenumber Ballooning-like Modes in LHD

MHD Simulation of High Wavenumber Ballooning-like Modes in LHD 1 TH/P9-16 MHD Simulation of High Wavenumber Ballooning-like Modes in LHD H. Miura and N. Nakajima National Institute for Fusion Science, 322-6 Oroshi, Toki, Gifu 509-5292, JAPAN e-mail contact of main

More information

Anisotropic electron distribution functions and the transition between the Weibel and the whistler instabilities

Anisotropic electron distribution functions and the transition between the Weibel and the whistler instabilities Anisotropic electron distribution functions and the transition between the Weibel and the whistler instabilities F. Pegoraro, L. Palodhi, F. Califano 5 th INTERNATIONAL CONFERENCE ON THE FRONTIERS OF PLASMA

More information

Fundamentals of Magnetic Island Theory in Tokamaks

Fundamentals of Magnetic Island Theory in Tokamaks Fundamentals of Magnetic Island Theory in Tokamaks Richard Fitzpatrick Institute for Fusion Studies University of Texas at Austin Austin, TX, USA Talk available at http://farside.ph.utexas.edu/talks/talks.html

More information

SMR/ Summer College on Plasma Physics. 30 July - 24 August, Introduction to Magnetic Island Theory.

SMR/ Summer College on Plasma Physics. 30 July - 24 August, Introduction to Magnetic Island Theory. SMR/1856-1 2007 Summer College on Plasma Physics 30 July - 24 August, 2007 Introduction to Magnetic Island Theory. R. Fitzpatrick Inst. for Fusion Studies University of Texas at Austin USA Introduction

More information

Magnetohydrodynamic waves in a plasma

Magnetohydrodynamic waves in a plasma Department of Physics Seminar 1b Magnetohydrodynamic waves in a plasma Author: Janez Kokalj Advisor: prof. dr. Tomaž Gyergyek Petelinje, April 2016 Abstract Plasma can sustain different wave phenomena.

More information

Toroidal flow stablization of disruptive high tokamaks

Toroidal flow stablization of disruptive high tokamaks PHYSICS OF PLASMAS VOLUME 9, NUMBER 6 JUNE 2002 Robert G. Kleva and Parvez N. Guzdar Institute for Plasma Research, University of Maryland, College Park, Maryland 20742-3511 Received 4 February 2002; accepted

More information

PROBLEM SET. Heliophysics Summer School. July, 2013

PROBLEM SET. Heliophysics Summer School. July, 2013 PROBLEM SET Heliophysics Summer School July, 2013 Problem Set for Shocks and Particle Acceleration There is probably only time to attempt one or two of these questions. In the tutorial session discussion

More information

MHD Modes of Solar Plasma Structures

MHD Modes of Solar Plasma Structures PX420 Solar MHD 2013-2014 MHD Modes of Solar Plasma Structures Centre for Fusion, Space & Astrophysics Wave and oscillatory processes in the solar corona: Possible relevance to coronal heating and solar

More information

Stabilization of sawteeth in tokamaks with toroidal flows

Stabilization of sawteeth in tokamaks with toroidal flows PHYSICS OF PLASMAS VOLUME 9, NUMBER 7 JULY 2002 Stabilization of sawteeth in tokamaks with toroidal flows Robert G. Kleva and Parvez N. Guzdar Institute for Plasma Research, University of Maryland, College

More information

Francesco Califano. Physics Department, University of Pisa. The role of the magnetic field in the interaction of the solar wind with a magnetosphere

Francesco Califano. Physics Department, University of Pisa. The role of the magnetic field in the interaction of the solar wind with a magnetosphere Francesco Califano Physics Department, University of Pisa The role of the magnetic field in the interaction of the solar wind with a magnetosphere Collaboration with M. Faganello & F. Pegoraro Vien na,

More information

Analysis of the flow and heat transfer characteristics for MHD free convection in an enclosure with a heated obstacle

Analysis of the flow and heat transfer characteristics for MHD free convection in an enclosure with a heated obstacle Nonlinear Analysis: Modelling and Control, 2011, Vol. 16, No. 1, 89 99 89 Analysis of the flow and heat transfer characteristics for MHD free convection in an enclosure with a heated obstacle S. Parvin,

More information

arxiv:physics/ v1 [physics.plasm-ph] 7 Jun 1999

arxiv:physics/ v1 [physics.plasm-ph] 7 Jun 1999 Theory of Two Dimensional Mean Field Electron Magnetohydrodynamics arxiv:physics/9906014v1 [physics.plasm-ph] 7 Jun 1999 Amita Das and P. H. Diamond University of California San Diego, La Jolla Abstract

More information

Problem C3.5 Direct Numerical Simulation of the Taylor-Green Vortex at Re = 1600

Problem C3.5 Direct Numerical Simulation of the Taylor-Green Vortex at Re = 1600 Problem C3.5 Direct Numerical Simulation of the Taylor-Green Vortex at Re = 6 Overview This problem is aimed at testing the accuracy and the performance of high-order methods on the direct numerical simulation

More information

Fundamentals of Fluid Dynamics: Elementary Viscous Flow

Fundamentals of Fluid Dynamics: Elementary Viscous Flow Fundamentals of Fluid Dynamics: Elementary Viscous Flow Introductory Course on Multiphysics Modelling TOMASZ G. ZIELIŃSKI bluebox.ippt.pan.pl/ tzielins/ Institute of Fundamental Technological Research

More information

Laminar Boundary Layer Flow on a Flate in a rotating system with Magnetic Field

Laminar Boundary Layer Flow on a Flate in a rotating system with Magnetic Field Laminar Boundary Layer Flow on a Flate in a rotating system with Magnetic Field Dinesh kumar Sharma 1 and Pawan Saxena 2 1 Department of Applied Sciences IIMT College of Engineering Greater Noida -201308

More information

CIMPA/ICTP Geometric Structures and Theory of Control October Acceleration of Plasma Flows Theory and Simulation

CIMPA/ICTP Geometric Structures and Theory of Control October Acceleration of Plasma Flows Theory and Simulation 2369-11 CIMPA/ICTP Geometric Structures and Theory of Control 1-12 October 2012 Acceleration of Plasma Flows Theory and Simulation Nana L. Shatashvili Faculty of Exact & Natural Sciences and Andronikashvili

More information

Dispersive Media, Lecture 7 - Thomas Johnson 1. Waves in plasmas. T. Johnson

Dispersive Media, Lecture 7 - Thomas Johnson 1. Waves in plasmas. T. Johnson 2017-02-14 Dispersive Media, Lecture 7 - Thomas Johnson 1 Waves in plasmas T. Johnson Introduction to plasmas as a coupled system Magneto-Hydro Dynamics, MHD Plasmas without magnetic fields Cold plasmas

More information

6.1. Linearized Wave Equations in a Uniform Isotropic MHD Plasma. = 0 into Ohm s law yields E 0

6.1. Linearized Wave Equations in a Uniform Isotropic MHD Plasma. = 0 into Ohm s law yields E 0 Chapter 6. Linear Waves in the MHD Plasma 85 Chapter 6. Linear Waves in the MHD Plasma Topics or concepts to learn in Chapter 6:. Linearize the MHD equations. The eigen-mode solutions of the MHD waves

More information

Plasma waves in the fluid picture I

Plasma waves in the fluid picture I Plasma waves in the fluid picture I Langmuir oscillations and waves Ion-acoustic waves Debye length Ordinary electromagnetic waves General wave equation General dispersion equation Dielectric response

More information

Hamiltonian and Non-Hamiltonian Reductions of Charged Particle Dynamics: Diffusion and Self-Organization

Hamiltonian and Non-Hamiltonian Reductions of Charged Particle Dynamics: Diffusion and Self-Organization NNP2017 11 th July 2017 Lawrence University Hamiltonian and Non-Hamiltonian Reductions of Charged Particle Dynamics: Diffusion and Self-Organization N. Sato and Z. Yoshida Graduate School of Frontier Sciences

More information

Calculation of alpha particle redistribution in sawteeth using experimentally reconstructed displacement eigenfunctions

Calculation of alpha particle redistribution in sawteeth using experimentally reconstructed displacement eigenfunctions Calculation of alpha particle redistribution in sawteeth using experimentally reconstructed displacement eigenfunctions R. Farengo, H. E. Ferrari,2, M.-C. Firpo 3, P. L. Garcia-Martinez 2,3, A. F. Lifschitz

More information

Chapter 5. The Differential Forms of the Fundamental Laws

Chapter 5. The Differential Forms of the Fundamental Laws Chapter 5 The Differential Forms of the Fundamental Laws 1 5.1 Introduction Two primary methods in deriving the differential forms of fundamental laws: Gauss s Theorem: Allows area integrals of the equations

More information

Collisionless magnetic reconnection with arbitrary guide-field

Collisionless magnetic reconnection with arbitrary guide-field Collisionless magnetic reconnection with arbitrary guide-field Richard Fitzpatrick Center for Magnetic Reconnection Studies Institute for Fusion Studies Department of Physics University of Texas at Austin

More information

Effect of magnetic reconnection on CT penetration into magnetized plasmas

Effect of magnetic reconnection on CT penetration into magnetized plasmas Earth Planets Space, 53, 547 55, 200 Effect of magnetic reconnection on CT penetration into magnetized plasmas Yoshio Suzuki, Takaya Hayashi 2, and Yasuaki Kishimoto Naka Fusion esearch Establishment,

More information

Non-disruptive MHD Dynamics in Inward-shifted LHD Configurations

Non-disruptive MHD Dynamics in Inward-shifted LHD Configurations Non-disrutive MHD Dynamics in Inward-shifted LHD Configurations.Introduction.MHD simulation 3.DNS of full 3D MHD 4. Summary MIUA H. ICHIGUCHI K. NAKAJIMA N. HAYASHI T. (National Institute for Fusion Science)

More information

The Euler Equation of Gas-Dynamics

The Euler Equation of Gas-Dynamics The Euler Equation of Gas-Dynamics A. Mignone October 24, 217 In this lecture we study some properties of the Euler equations of gasdynamics, + (u) = ( ) u + u u + p = a p + u p + γp u = where, p and u

More information

where the index 2 indicates the particle species (electrons and different ion species if present). With

where the index 2 indicates the particle species (electrons and different ion species if present). With hapter 3 Magnetohydrodynamics luid equations are probably the most widely used equations for the description of inhomogeneous plasmas. While the phase fluid which is governed by the Boltzmann equation

More information

Point Vortex Dynamics in Two Dimensions

Point Vortex Dynamics in Two Dimensions Spring School on Fluid Mechanics and Geophysics of Environmental Hazards 9 April to May, 9 Point Vortex Dynamics in Two Dimensions Ruth Musgrave, Mostafa Moghaddami, Victor Avsarkisov, Ruoqian Wang, Wei

More information

NIMROD simulations of dynamo experiments in cylindrical and spherical geometries. Dalton Schnack, Ivan Khalzov, Fatima Ebrahimi, Cary Forest,

NIMROD simulations of dynamo experiments in cylindrical and spherical geometries. Dalton Schnack, Ivan Khalzov, Fatima Ebrahimi, Cary Forest, NIMROD simulations of dynamo experiments in cylindrical and spherical geometries Dalton Schnack, Ivan Khalzov, Fatima Ebrahimi, Cary Forest, 1 Introduction Two experiments, Madison Plasma Couette Experiment

More information

High-m Multiple Tearing Modes in Tokamaks: MHD Turbulence Generation, Interaction with the Internal Kink and Sheared Flows

High-m Multiple Tearing Modes in Tokamaks: MHD Turbulence Generation, Interaction with the Internal Kink and Sheared Flows TH/P3-3 High-m Multiple Tearing Modes in Tokamaks: MHD Turbulence Generation, Interaction with the Internal Kink and Sheared Flows A. Bierwage 1), S. Benkadda 2), M. Wakatani 1), S. Hamaguchi 3), Q. Yu

More information

MAGNETOHYDRODYNAMIC FLOW OF VISCOUS ELECTRICALLY CONDUCTING INCOMPRESSIBLE FLUID THROUGH VERTICAL PLATES SUBJECTED TO INCLINED MAGNETIC FIELD.

MAGNETOHYDRODYNAMIC FLOW OF VISCOUS ELECTRICALLY CONDUCTING INCOMPRESSIBLE FLUID THROUGH VERTICAL PLATES SUBJECTED TO INCLINED MAGNETIC FIELD. International Journal of Scientific and Technical Research in Engineering (IJSTRE) www.ijstre.com Volume 3 Issue 6 ǁ August 2018. MAGNETOHYROYNAMIC FLOW OF VISCOUS ELECTRICALLY CONUCTING INCOMPRESSIBLE

More information

Intermittency of quasi-static magnetohydrodynamic turbulence: A wavelet viewpoint

Intermittency of quasi-static magnetohydrodynamic turbulence: A wavelet viewpoint Intermittency of quasi-static magnetohydrodynamic turbulence: A wavelet viewpoint Naoya Okamoto 1, Katsunori Yoshimatsu 2, Kai Schneider 3 and Marie Farge 4 1 Center for Computational Science, Nagoya University,

More information

Fluctuation dynamo amplified by intermittent shear bursts

Fluctuation dynamo amplified by intermittent shear bursts by intermittent Thanks to my collaborators: A. Busse (U. Glasgow), W.-C. Müller (TU Berlin) Dynamics Days Europe 8-12 September 2014 Mini-symposium on Nonlinear Problems in Plasma Astrophysics Introduction

More information

Control of Neo-classical tearing mode (NTM) in advanced scenarios

Control of Neo-classical tearing mode (NTM) in advanced scenarios FIRST CHENGDU THEORY FESTIVAL Control of Neo-classical tearing mode (NTM) in advanced scenarios Zheng-Xiong Wang Dalian University of Technology (DLUT) Dalian, China Chengdu, China, 28 Aug, 2018 Outline

More information

School and Conference on Analytical and Computational Astrophysics November, Angular momentum transport in accretion disks

School and Conference on Analytical and Computational Astrophysics November, Angular momentum transport in accretion disks 2292-13 School and Conference on Analytical and Computational Astrophysics 14-25 November, 2011 Angular momentum transport in accretion disks Gianluigi Bodo Osservatorio Astronomico, Torino Italy Angular

More information

Jet Stability: A computational survey

Jet Stability: A computational survey Jet Stability Galway 2008-1 Jet Stability: A computational survey Rony Keppens Centre for Plasma-Astrophysics, K.U.Leuven (Belgium) & FOM-Institute for Plasma Physics Rijnhuizen & Astronomical Institute,

More information

Natalia Tronko S.V.Nazarenko S. Galtier

Natalia Tronko S.V.Nazarenko S. Galtier IPP Garching, ESF Exploratory Workshop Natalia Tronko University of York, York Plasma Institute In collaboration with S.V.Nazarenko University of Warwick S. Galtier University of Paris XI Outline Motivations:

More information

On a variational principle for Beltrami flows

On a variational principle for Beltrami flows On a variational principle for Beltrami flows Rafael González, Andrea Costa, and E. Sergio Santini Citation: Physics of Fluids 22, 074102 (2010); doi: 10.1063/1.3460297 View online: http://dx.doi.org/10.1063/1.3460297

More information

Overview of FRC-related modeling (July 2014-present)

Overview of FRC-related modeling (July 2014-present) Overview of FRC-related modeling (July 2014-present) Artan Qerushi AFRL-UCLA Basic Research Collaboration Workshop January 20th, 2015 AFTC PA Release# 15009, 16 Jan 2015 Artan Qerushi (AFRL) FRC modeling

More information

Steady-state Force Balance in the DEBS Code

Steady-state Force Balance in the DEBS Code Steady-state Force Balance in the DEBS Code D. D. Schnack Department of Physics University of Wisconsin - Madison Madison, WI 53706 November 10, 2013 The DEBS code advances the induction equation, the

More information

Collisionless nonideal ballooning modes

Collisionless nonideal ballooning modes PHYSICS OF PLASMAS VOLUME 6, NUMBER 1 JANUARY 1999 Collisionless nonideal ballooning modes Robert G. Kleva and Parvez N. Guzdar Institute for Plasma Research, University of Maryland, College Park, Maryland

More information

INDEX 363. Cartesian coordinates 19,20,42, 67, 83 Cartesian tensors 84, 87, 226

INDEX 363. Cartesian coordinates 19,20,42, 67, 83 Cartesian tensors 84, 87, 226 INDEX 363 A Absolute differentiation 120 Absolute scalar field 43 Absolute tensor 45,46,47,48 Acceleration 121, 190, 192 Action integral 198 Addition of systems 6, 51 Addition of tensors 6, 51 Adherence

More information

1. Introduction, tensors, kinematics

1. Introduction, tensors, kinematics 1. Introduction, tensors, kinematics Content: Introduction to fluids, Cartesian tensors, vector algebra using tensor notation, operators in tensor form, Eulerian and Lagrangian description of scalar and

More information

Vlasov-Maxwell Equations and Cold Plasma Waves

Vlasov-Maxwell Equations and Cold Plasma Waves Astronomy 53 Spring 016) uening Bai Mar.,, 016 Vlasov-Maxwell Equations and Cold Plasma Waves The Vlasov-Maxwell equations Consider a plasma as a collection of N charged particles, each particle i has

More information

The Field-Reversed Configuration (FRC) is a high-beta compact toroidal in which the external field is reversed on axis by azimuthal plasma The FRC is

The Field-Reversed Configuration (FRC) is a high-beta compact toroidal in which the external field is reversed on axis by azimuthal plasma The FRC is and Stability of Field-Reversed Equilibrium with Toroidal Field Configurations Atomics General Box 85608, San Diego, California 92186-5608 P.O. APS Annual APS Meeting of the Division of Plasma Physics

More information

Measurement of magnetic eld line stochasticity in nonlinearly evolving, Department of Engineering Physics,

Measurement of magnetic eld line stochasticity in nonlinearly evolving, Department of Engineering Physics, Measurement of magnetic eld line stochasticity in nonlinearly evolving, nonequilibrium plasmas Y. Nishimura, J. D. Callen, and C. C. Hegna Department of Engineering Physics, University of Wisconsin-Madison,

More information

PLASMA ASTROPHYSICS. ElisaBete M. de Gouveia Dal Pino IAG-USP. NOTES: (references therein)

PLASMA ASTROPHYSICS. ElisaBete M. de Gouveia Dal Pino IAG-USP. NOTES:  (references therein) PLASMA ASTROPHYSICS ElisaBete M. de Gouveia Dal Pino IAG-USP NOTES:http://www.astro.iag.usp.br/~dalpino (references therein) ICTP-SAIFR, October 7-18, 2013 Contents What is plasma? Why plasmas in astrophysics?

More information

Nonequilibrium Dynamics in Astrophysics and Material Science YITP, Kyoto

Nonequilibrium Dynamics in Astrophysics and Material Science YITP, Kyoto Nonequilibrium Dynamics in Astrophysics and Material Science 2011-11-02 @ YITP, Kyoto Multi-scale coherent structures and their role in the Richardson cascade of turbulence Susumu Goto (Okayama Univ.)

More information

Gyrokinetic simulations of magnetic fusion plasmas

Gyrokinetic simulations of magnetic fusion plasmas Gyrokinetic simulations of magnetic fusion plasmas Tutorial 2 Virginie Grandgirard CEA/DSM/IRFM, Association Euratom-CEA, Cadarache, 13108 St Paul-lez-Durance, France. email: virginie.grandgirard@cea.fr

More information

Lecture 15 Strain and stress in beams

Lecture 15 Strain and stress in beams Spring, 2019 ME 323 Mechanics of Materials Lecture 15 Strain and stress in beams Reading assignment: 6.1 6.2 News: Instructor: Prof. Marcial Gonzalez Last modified: 1/6/19 9:42:38 PM Beam theory (@ ME

More information

Heat and Mass Transfer

Heat and Mass Transfer 1 Comments on six papers published by S.P. Anjali Devi and R. Kandasamy in Heat and Mass Transfer, ZAMM, Mechanics Research Communications, International Communications in Heat and Mass Transfer, Communications

More information

THE INTERACTION OF TURBULENCE WITH THE HELIOSPHERIC SHOCK

THE INTERACTION OF TURBULENCE WITH THE HELIOSPHERIC SHOCK THE INTERACTION OF TURBULENCE WITH THE HELIOSPHERIC SHOCK G.P. Zank, I. Kryukov, N. Pogorelov, S. Borovikov, Dastgeer Shaikh, and X. Ao CSPAR, University of Alabama in Huntsville Heliospheric observations

More information

Parash Moni Thakur. Gopal Ch. Hazarika

Parash Moni Thakur. Gopal Ch. Hazarika International Journal of Scientific and Innovative Mathematical Research (IJSIMR) Volume 2, Issue 6, June 2014, PP 554-566 ISSN 2347-307X (Print) & ISSN 2347-3142 (Online) www.arcjournals.org Effects of

More information

Magnetohydrodynamic Waves

Magnetohydrodynamic Waves Magnetohydrodynamic Waves Nick Murphy Harvard-Smithsonian Center for Astrophysics Astronomy 253: Plasma Astrophysics February 17, 2016 These slides are largely based off of 4.5 and 4.8 of The Physics of

More information

Electron magnetohydrodynamic turbulence

Electron magnetohydrodynamic turbulence PHYSICS OF PLASMAS VOLUME 6, NUMBER 3 MARCH 1999 Electron magnetohydrodynamic turbulence D. Biskamp, E. Schwarz, and A. Zeiler Max-Planck-Institut für Plasmaphysik, D-85748 Garching, Germany A. Celani

More information

Analysis of Jeans Instability of Partially-Ionized. Molecular Cloud under Influence of Radiative. Effect and Electron Inertia

Analysis of Jeans Instability of Partially-Ionized. Molecular Cloud under Influence of Radiative. Effect and Electron Inertia Adv. Studies Theor. Phys., Vol. 5, 2011, no. 16, 755-764 Analysis of Jeans Instability of Partially-Ionized Molecular Cloud under Influence of Radiative Effect and Electron Inertia B. K. Dangarh Department

More information

V (r,t) = i ˆ u( x, y,z,t) + ˆ j v( x, y,z,t) + k ˆ w( x, y, z,t)

V (r,t) = i ˆ u( x, y,z,t) + ˆ j v( x, y,z,t) + k ˆ w( x, y, z,t) IV. DIFFERENTIAL RELATIONS FOR A FLUID PARTICLE This chapter presents the development and application of the basic differential equations of fluid motion. Simplifications in the general equations and common

More information

Lecture 3: The Navier-Stokes Equations: Topological aspects

Lecture 3: The Navier-Stokes Equations: Topological aspects Lecture 3: The Navier-Stokes Equations: Topological aspects September 9, 2015 1 Goal Topology is the branch of math wich studies shape-changing objects; objects which can transform one into another without

More information

Application of Reconstruction of Variational Iteration Method on the Laminar Flow in a Porous Cylinder with Regressing Walls

Application of Reconstruction of Variational Iteration Method on the Laminar Flow in a Porous Cylinder with Regressing Walls Mechanics and Mechanical Engineering Vol. 21, No. 2 (2017) 379 387 c Lodz University of Technology Application of Reconstruction of Variational Iteration Method on the Laminar Flow in a Porous Cylinder

More information

Heating and current drive: Radio Frequency

Heating and current drive: Radio Frequency Heating and current drive: Radio Frequency Dr Ben Dudson Department of Physics, University of York Heslington, York YO10 5DD, UK 13 th February 2012 Dr Ben Dudson Magnetic Confinement Fusion (1 of 26)

More information

Sensors Plasma Diagnostics

Sensors Plasma Diagnostics Sensors Plasma Diagnostics Ken Gentle Physics Department Kenneth Gentle RLM 12.330 k.gentle@mail.utexas.edu NRL Formulary MIT Formulary www.psfc.mit.edu/library1/catalog/ reports/2010/11rr/11rr013/11rr013_full.pdf

More information

Fundamentals of Turbulence

Fundamentals of Turbulence Fundamentals of Turbulence Stanislav Boldyrev (University of Wisconsin - Madison) Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas What is turbulence? No exact definition.

More information

Confinement of toroidal non-neutral plasma in Proto-RT

Confinement of toroidal non-neutral plasma in Proto-RT Workshop on Physics with Ultra Slow Antiproton Beams, RIKEN, March 15, 2005 Confinement of toroidal non-neutral plasma in Proto-RT H. Saitoh, Z. Yoshida, and S. Watanabe Graduate School of Frontier Sciences,

More information

Confinement of toroidal non-neutral plasma in Proto-RT

Confinement of toroidal non-neutral plasma in Proto-RT Workshop on Physics with Ultra Slow Antiproton Beams, RIKEN, March 15, 2005 Confinement of toroidal non-neutral plasma in Proto-RT H. Saitoh, Z. Yoshida, and S. Watanabe Graduate School of Frontier Sciences,

More information

Studies of Turbulence-driven FLOWs:

Studies of Turbulence-driven FLOWs: Studies of Turbulence-driven FLOWs: a) V ", V Competition in a Tube b) Revisiting Zonal Flow Saturation J.C. Li, P.H. Diamond, R. Hong, G. Tynan University of California San Diego, USA This material is

More information

Special topic JPFR article Prospects of Research on Innovative Concepts in ITER Era contribution by M. Brown Section 5.2.2

Special topic JPFR article Prospects of Research on Innovative Concepts in ITER Era contribution by M. Brown Section 5.2.2 Special topic JPFR article Prospects of Research on Innovative Concepts in ITER Era contribution by M. Brown Section 5.2.2 5.2.2 Dynamo and Reconnection Research: Overview: Spheromaks undergo a relaxation

More information

Two-fluid theory of collisionless magnetic reconnection

Two-fluid theory of collisionless magnetic reconnection Two-fluid theory of collisionless magnetic reconnection D. Biskamp and E. Schwarz Max-Planck-Institut für Plasmaphysik, 85748 Garching, Germany J. F. Drake Institute for Plasma Research, University of

More information

Electromagneic Waves in a non- Maxwellian Dusty Plasma

Electromagneic Waves in a non- Maxwellian Dusty Plasma Electromagneic Waves in a non- Maxwellian Dusty Plasma Nazish Rubab PhD student, KF University Graz IWF-OEAW Graz 26 January, 2011 Layout Dusty Plasma Non-Maxwellian Plasma Kinetic Alfven Waves Instability

More information

Momentum transport from magnetic reconnection in laboratory an. plasmas. Fatima Ebrahimi

Momentum transport from magnetic reconnection in laboratory an. plasmas. Fatima Ebrahimi Momentum transport from magnetic reconnection in laboratory and astrophysical plasmas Space Science Center - University of New Hampshire collaborators : V. Mirnov, S. Prager, D. Schnack, C. Sovinec Center

More information

Basic plasma physics

Basic plasma physics Basic plasma physics SPAT PG Lectures Jonathan Eastwood 10-14 October 2016 Aims Provide new PhD students in SPAT and the SPC section with an overview of the most important principles in space plasma physics,

More information

INTERACTION OF DRIFT WAVE TURBULENCE AND MAGNETIC ISLANDS

INTERACTION OF DRIFT WAVE TURBULENCE AND MAGNETIC ISLANDS INTERACTION OF DRIFT WAVE TURBULENCE AND MAGNETIC ISLANDS A. Ishizawa and N. Nakajima National Institute for Fusion Science F. L. Waelbroeck, R. Fitzpatrick, W. Horton Institute for Fusion Studies, University

More information

Magnetohydrodynamic Flow of a Liquid Metal in a Curved Circular Duct subject to the Effect of an External Magnetic Field

Magnetohydrodynamic Flow of a Liquid Metal in a Curved Circular Duct subject to the Effect of an External Magnetic Field Paper 85 Civil-Comp Press, 2012 Proceedings of the Eighth International Conference on Engineering Computational Technology, B.H.V. Topping, (Editor), Civil-Comp Press, Stirlingshire, Scotland Magnetohydrodynamic

More information

Hybrid Simulation Method ISSS-10 Banff 2011

Hybrid Simulation Method ISSS-10 Banff 2011 Hybrid Simulation Method ISSS-10 Banff 2011 David Burgess Astronomy Unit Queen Mary University of London With thanks to Dietmar Krauss-Varban Space Plasmas: From Sun to Earth Space Plasma Plasma is (mostly)

More information

Plasma instabilities. Dr Ben Dudson, University of York 1 / 37

Plasma instabilities. Dr Ben Dudson, University of York 1 / 37 Plasma instabilities Dr Ben Dudson, University of York 1 / 37 Previously... Plasma configurations and equilibrium Linear machines, and Stellarators Ideal MHD and the Grad-Shafranov equation Collisional

More information

MHD-particle simulations and collective alpha-particle transport: analysis of ITER scenarios and perspectives for integrated modelling

MHD-particle simulations and collective alpha-particle transport: analysis of ITER scenarios and perspectives for integrated modelling MHD-particle simulations and collective alpha-particle transport: analysis of ITER scenarios and perspectives for integrated modelling G. Vlad, S. Briguglio, G. Fogaccia, F. Zonca Associazione Euratom-ENEA

More information

Project 4: Navier-Stokes Solution to Driven Cavity and Channel Flow Conditions

Project 4: Navier-Stokes Solution to Driven Cavity and Channel Flow Conditions Project 4: Navier-Stokes Solution to Driven Cavity and Channel Flow Conditions R. S. Sellers MAE 5440, Computational Fluid Dynamics Utah State University, Department of Mechanical and Aerospace Engineering

More information

Fluid Mechanics Prof. S. K. Som Department of Mechanical Engineering Indian Institute of Technology, Kharagpur

Fluid Mechanics Prof. S. K. Som Department of Mechanical Engineering Indian Institute of Technology, Kharagpur Fluid Mechanics Prof. S. K. Som Department of Mechanical Engineering Indian Institute of Technology, Kharagpur Lecture - 15 Conservation Equations in Fluid Flow Part III Good afternoon. I welcome you all

More information

Webster s horn model on Bernoulli flow

Webster s horn model on Bernoulli flow Webster s horn model on Bernoulli flow Aalto University, Dept. Mathematics and Systems Analysis January 5th, 2018 Incompressible, steady Bernoulli principle Consider a straight tube Ω R 3 havin circular

More information

Plasma Physics for Astrophysics

Plasma Physics for Astrophysics - ' ' * ' Plasma Physics for Astrophysics RUSSELL M. KULSRUD PRINCETON UNIVERSITY E;RESS '. ' PRINCETON AND OXFORD,, ', V. List of Figures Foreword by John N. Bahcall Preface Chapter 1. Introduction 1

More information

3D MHD Free Surface Fluid Flow Simulation Based on. Magnetic-Field Induction Equations

3D MHD Free Surface Fluid Flow Simulation Based on. Magnetic-Field Induction Equations 3D MHD Free Surface Fluid Flow Simulation Based on Magnetic-Field Induction Equations H.L. HUANG, A. YING, M. A. ABDOU Mechanical and Aerospace Engineering Department, UCLA, Los Angeles, CA, 90095 Huang@fusion.ucla.edu

More information

Analogue non-riemannian black holes in vortical moving plasmas

Analogue non-riemannian black holes in vortical moving plasmas Analogue non-riemannian black holes in vortical moving plasmas arxiv:gr-qc/0509034v1 11 Sep 2005 L.C. Garcia de Andrade 1 Abstract Analogue black holes in non-riemannian effective spacetime of moving vortical

More information