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1 magnetosphere magnetosphere - - like plasma experiment like plasma experiment (RT (RT - - 1 project) 1 project) Zensho YOSHIDA Zensho YOSHIDA the the RT1 RT1 project project University of Tokyo University of Tokyo Graduate School of Frontier Sciences Graduate School of Frontier Sciences

magnetosphere-like plasma experiment (RT-1 project)indico.ictp.it/event/a05217/session/23/contribution/16/material/0/0.pdf · magnetosphere-like plasma experiment (RT-1 project) Zensho

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    magnetospheremagnetosphere--like plasma experimentlike plasma experiment(RT(RT--1 project)1 project)

    Zensho YOSHIDAZensho YOSHIDA  the the RT1RT1 projectproject

    University of TokyoUniversity of TokyoGraduate School of Frontier SciencesGraduate School of Frontier Sciences

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    A Frontier of Plasma PhysicsA Frontier of Plasma Physics

    Interesting “structures” remain unknown in the universe.

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    A Frontier of Plasma PhysicsA Frontier of Plasma Physics

    Interesting “structures” remain unknown in the universe.

    high-beta advanced-fuelfusionFUSION

    high-efficiencyanti-mater plasmaANTIMATER

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    Guidelines to analyze/synthesize plasma Guidelines to analyze/synthesize plasma structuresstructures

    How can plasmas have “diversity” of structures?- compared with a linear system (ex. heat diffusion eq.)- nonlinearity → bifurcation- hyperbolicity, singularity (non-canonical nature) → characteristics

    What is the measure of plasma’s “preference” ?- target functional → variational principle- conservation laws, Casimirs→ constraints

    How can we organize a preferable structure?- relaxation  → self-organization

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    SelfSelf--Organization of Structures Organization of Structures

    Relaxationa natural process of chaos escape from restrictions → homogenize

    How can “structures” emerge and sustain?   co-existence of order and disorder

    ← creation of scale hierarchy (multi-scale)

    Order  ← “symmetry” (conservation laws):    diversity of structures, stability (Lyapunov functions)

    Dynamic (non-conservative) degree of freedom:   entropy vs. dynamics

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    Plasma = coPlasma = co--existence of order and disorderexistence of order and disorder

    Interactions of different scale hierarchyAnalysis of singularities (singular perturbation theory)

    macro microby Biskamp

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    FlowFlow--field couplingfield coupling

    Self-organization of “twists”

    S.M. Mahajan and Z.Yoshida, Phys. Rev. Lett. 81 (1998) 4863.Z. Yoshida and S.M. Mahajan, Phys. Rev. Lett. 88 (2002) 095001.

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    Symmetry and diversitySymmetry and diversity

    equilibrium = critical point of the “Hamiltonian”δH = 0 → “trivial state”

    Non-Canonical system : Casimir invariants (constant of motion) → restriction{C, G} = 0 (for every G)

    Non-trivial (structured) equilibriumH’ = H + µC + µ’C’ + ・・・

      δH’ = 0  → “non-trivial states”  H’→ Lyapunov function

    Z. Yoshida, S. Ohsaki, A. Ito and S.M. Mahajan, J. Math. Phys. 44 (2003) 2168.

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    ““BeltramiBeltrami””--class of equilibriaclass of equilibria

    Vortex dynamics system:

    Casimirs = Helicities → topological constraints

    Structured equiliria:

    Beltrami vortex solutions

    ( ) 0)()()( =+= ∑ uuu jjCHF αδδ

    ( ) ( )L,2,10 ==××∇−∂ nnnnt wvw

    ( )dxC nnn ∫ ×∇⋅= − ww 1

    ( ) ( ) 0curlcurl 1 =−− uNλλ LZ. Yoshida and Y. Giga, Math. Z. 204 (1990), 235-245.Z. Yoshida and S,M, Mahajan, J. Math. Phys. 40 (1999), 5080.

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    Double Beltrami field in HMHD plasmaDouble Beltrami field in HMHD plasma

    u = c1G1 + c2G2

    curl u = c1λ1G1 + c2λ2G2

    ← multi-scaleλ1 = O(1), λ2 = O(ε-1)

    Z. Yoshida, S.M. Mahajan, S. Ohsaki, Phys. Plasmas 11 (2004), 3660.

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    Singular perturbation healing singularitiesSingular perturbation healing singularities

    The Alfven singularity is unfolded by the Hall effect:

    ideal limit (ε→ 0) :

    1±=⋅⋅

    =BvBvforder parameter

    Hall effect (singular perturbation)

    smoothly connect two different phases:

    11 +≤≤− f

    J. Shiraishi, S. Ohsaki, Z. Yoshida, Phys. Plasmas 12 (2005), 092308.

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    RTRT--11devicedevice

    Magnetosphere-like plasma confinement

    basic structure

    flow, waves, pressure, ・・・

    diversity

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    RT1 engineeringRT1 engineering

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    Challenges using RT1Challenges using RT1

    Advanced-fuel fusionhigh-beta confinement

    New method of trapping particlesmagnetic-surface configuration

    Plasma-astrophysicsexperimental simulation of magnetosphere

    Basic plasma physicsflow, relaxed state, wave propagation,particle-orbit (neo-classical) effects, boundary layer, shocks and singularities, etc.

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    SummarySummary

    The RT1 device: magnetosphere-like configurationhigh-temperature super-conducting magnet

    RT1 can host a variety of new-type plasma states.high-beta rotating plasma (Jupiter’s magnetosphere)Double Beltrami states (Hall-MHD), dipole (mirror-like),non-neutral (single-species) plasma, ・・・

    Flow-field coupling produces diverse structures.multi-scale structures, singular perturbations, topological constraints, Lyapunov stability,・・・

    magnetosphere-like plasma experiment(RT-1 project)A Frontier of Plasma PhysicsA Frontier of Plasma PhysicsGuidelines to analyze/synthesize plasma structuresSelf-Organization of StructuresPlasma = co-existence of order and disorderFlow-field couplingSymmetry and diversity“Beltrami”-class of equilibriaDouble Beltrami field in HMHD plasmaSingular perturbation healing singularitiesRT-1deviceRT1 engineeringChallenges using RT1Summary