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PU AST558, 4/25/05 ST Science & Fusion Energy Martin Peng NSTX Program Director Oak Ridge National Laboratory @ Princeton Plasma Physics Laboratory PU Graduate Seminar in Plasma Physics AST558 April 25, 2005 PPPL Spherical Tokamak Plasma Science & Fusion Energy Development Supported by Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics NYU ORNL PPPL PSI SNL UC Davis UC Irvine UCLA UCSD U Maryland U Rochester U Washington U Wisconsin Culham Sci Ctr Hiroshima U HIST Kyushu Tokai U Niigata U Tsukuba U U Tokyo JAERI Ioffe Inst TRINITI KBSI KAIST ENEA, Frascati CEA, Cadarache IPP, Jülich IPP, Garching U Quebec

Columbia U Spherical Tokamak Plasma ScienceSUNIST (PRC) Globus-M (RF) PU AST558, 4/25/05 ST Science & Fusion Energy ST Is Closest to Tokamak; Operates with High Safety Factor and More

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  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Martin PengNSTX Program Director

    Oak Ridge National Laboratory@ Princeton Plasma Physics Laboratory

    PU Graduate Seminar in Plasma PhysicsAST558

    April 25, 2005

    PPPL

    Spherical Tokamak Plasma Science & Fusion Energy Development

    Supported by

    Columbia UComp-X

    General AtomicsINEL

    Johns Hopkins ULANLLLNL

    LodestarMIT

    Nova PhotonicsNYU

    ORNLPPPL

    PSISNL

    UC DavisUC Irvine

    UCLAUCSD

    U MarylandU Rochester

    U WashingtonU Wisconsin

    Culham Sci CtrHiroshima U

    HISTKyushu Tokai U

    Niigata UTsukuba U

    U TokyoJAERI

    Ioffe InstTRINITI

    KBSIKAIST

    ENEA, FrascatiCEA, Cadarache

    IPP, JülichIPP, Garching

    U Quebec

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Spherical Tokamak (ST) Offers Rich Plasma Science Opportunities and High Fusion Energy Potential

    • What is ST and why?• World ST community• Cost-effective steps to fusion energy• Scientific opportunities of ST

    • How does shape (κ, δ, A …) determine pressure? • How does turbulence enhance transport?• How do plasma particles and waves interact?• How do hot plasmas interact with walls?• How to supply magnetic flux without solenoid?

    • Wrap-up

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Tokamak Theory in Early 1980’s Showed Maximum Stable βT Increased with Lowered Aspect Ratio (A)

    • A. Sykes et al. (1983); F. Troyon et al. (1984) on maximum stable toroidal beta βT:

    βTmax = C Ip / a 〈B〉 ≈ 5 C κ / A qj; 〈B〉 ≈ BT at standard AC ≈ constant (~ 3 %m·T/MA) ⇒ βN〈B〉 = volume average B ⇒ BTκ = b/a = elongationA = R0/a = aspect ratioqI ≈ average safety factor Ip = toroidal plasma currentBT ≈ applied toroidal field at R0

    • Peng & Strickler (1986): What would happen to tokamak as A → 1?

    − How would βN, κ, qj, change as functions of A?

    Z

    a ab

    0 RR0

    PlasmaCross

    Section

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Minimizing Tokamak Aspect Ratio Maximizes Field Line Length in Good Curvature ⇒ High β Stability

    Tokamak Compact Toroid (CT)

    Spherical Tokamak (ST)

    Bad CurvatureGood Curvature

    Magnetic Field LineMagnetic Surface

    Small-R close to Tokamak & large-R close to CT.

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    • Naturally increased κ ~ 2; ITF < Ip, IPF < Ip ⇒ higher Ip; lower device cost• Increased Ip/aBT ~ 7 MA/m·T ⇒ βTmax ~ 20%, if βN ~ 3• Increased Ip qedge /aBT ~ 20 MA/m·T ⇒ improved confinement?

    ST Tokamak

    ITF / Ip(~aBT / Ip)

    ΣIPF / Ip

    κ

    Natural Elongation, κ Small Coil Currents/Ip (qedge~2.5)

    R R A

    Z

    0

    A = 2.5κ ≈ 1.4

    A = 1.5κ ≈ 2.0

    ST Plasma Elongates Naturally, Needs Less TF & PF Coil Currents, Increases Ip/aBT ⇒ Higher βTmax

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    ST Research Is Growing WorldwideProof of Principle (~MA)Concept Exploration (~0.3 MA)

    HIT-II (US) Pegasus (US)

    HIST (J) TST-2 (J) TS-3 (J)TS-4 (J)

    CDX-U (US)

    NSTX (US)MAST (UK)

    ETE (B)

    SUNIST (PRC)

    Globus-M (RF)

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    ST Is Closest to Tokamak; Operates with High Safety Factor and More Comparable Self & Applied Fields

    Field Reversed Configuration

    Reversed Field PinchDipole

    Spheromak

    Impr

    ove

    Plas

    ma

    Stab

    ility

    at H

    igh

    β→

    0A

    vera

    ge S

    afet

    y fa

    ctor

    , qav

    g5

    ExampleExampleFusion ConfigurationsFusion Configurations

    Spherical Tokamak(Spherical Torus)

    (NSTX, MAST, TST-2,TS-3,4, HIST, LATE, etc.)

    Tokamak &Advanced Tokamak

    (DIII-D, C-Mod,K-Star, JT60-U, etc.)

    Stellarators(QPS)In Design

    (NCSX)Being Built

    0.5 (Applied Field)/(Applied + Plasma-Produced Field) 1(Self-Organized) Increase Controllability → (Externally Controlled)

    (SSPX, etc.)

    (MST, etc.)

    (LDX, etc.)(LDX, etc.)

    LHD

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Very Low Aspect Ratio (A) Introduces New Opportunities to Broaden Toroidal Plasma Science

    ST Plasmas ExtendsST Plasmas ExtendsToroidal ParametersToroidal Parameters

    A = R/a can be ≥ 1.1

    START – UKAEA Fusion

    How does shape determine pressure?• Strong plasma shaping & self fields

    (vertical elongation ≤ 3, Bp/Bt ~ 1)• Very high βT (~ 40%), βN & fBootstrapHow does turbulence enhance transport?• Small plasma size relative to gyro-radius

    (a/ρi~30–50)• Large plasma flow (MA = Vrotation/VA ≤ 0.3)• Large flow shearing rate (γExB ≤ 106/s)How do plasma particles and waves interact?• Supra-Alfvénic fast ions (Vfast/VA ~ 4–5) • High dielectric constant (ε = ωpe2/ωce2 ~ 50)How do plasmas interact with walls?• Large B mirror ratio in edge (MB ≤ 4, fT → 1)• Strong field line expansion (> factor of 10)How to supply mag flux without solenoid?• Small magnetic flux content (~ liR0Ip)

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Answering the Plasma Science Questions Also Enable Cost-Effective Steps toward Fusion Energy

    Plasma Science Questions in Extended ST Parameter Space

    ⇒ Optimize Fusion DEMO & Development Steps

    How does shape determine pressure?

    ⇒ Lowered magnetic field and device costs

    How does turbulence enhance transport?

    ⇒ Smaller unit size for sustained fusion burn

    How does plasma particles and waves interact?

    ⇒ Efficient fusion α particle, neutral beam, & RF heating

    How to supply magnetic flux without solenoid?

    ⇒ Simplified smaller design, reduced operating cost

    How do hot plasmas interact with wall?

    ⇒ Survivable plasma facing components

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Single-turn demountable center leg for toroidal field coil required to achieve small size and simplified design.Fast remote replacement of all fusion nuclear test components (blanket, FW, PFC) & center post required to permit high duty factor & neutron fluence.Large blanket test areas ∝ (R+a)κa.Adequate tritium breeding ratio & small fusion power from low Arequired for long term fuel sufficiency.High heat fluxes on PFC.Initial core components could use DEMO-relevant technologies (such as from ITER and long-pulse tokamaks).12-MA power supply – Single-turn TF.

    Features Required by High DutyFactor & Neutron Fluence

    Optimized Device Configuration Features of ST Also Fulfill the CTF Mission Effectively

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Mid-Plane Test Modules, Neutral Beam Injection, RF, Diagnostics Are Arranged for Fast Removal & Insert

    • 8 mid-plane blanket test modules provides ~ 15 m2 at maximum flux• Additional cylindrical blanket test area > 50 m2 at reduced flux

    • 3 m2 mid-plane access for neutral beam injection of 30 MW• 2 m2 mid-plane access for RF (10 MW) and diagnostics• All modules accessible through remote handling casks (~ITER)

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    • ITER approach for mid-plane test modules and neutral beam systems

    • Full-remote vertical access

    CTF Requires Remote Accessto All Fusion Core Components

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    • Disconnect upper piping • Remove sliding electrical joint• Remove top hatch

    • Remove upper PF coil • Remove upper divertor• Remove lower divertor• Remove lower PF coil

    • Extract NBI liner• Extract test modules• Remove upper blanket assembly • Remove lower blanket assembly

    • Remove centerstack assembly • Remove shield assembly

    Machine Assembly/Disassembly Sequence Are Made Manageable

    Upper Piping Electrical Joint

    Top Hatch

    Upper PF coil Upper DivertorLower DivertorLower PF coil

    Test Module

    NBI Liner

    Upper Blanket AssyLower Blanket Assy

    Centerstack Assembly Shield

    Assembly

    • Hands-on connect and disconnect service lines outside of shielding and vacuum boundaries

    • Divertor, cylindrical blanket, TF center leg, and shield assembly removed/installed vertically

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Future ST Steps Are Estimated to Require Moderate Sizes to Make Key Advances toward DEMO

    Device NSTX NSST CTF DEMO

    Mission Proof of Principle Performance Extension

    Energy Development, Component Testing

    Practicality of Fusion Electricity

    R (m) 0.85 ~1.5 ~1.2 ~3

    a (m) 0.65 ~0.9 ~0.8 ~2

    κ, δ 2.5, 0.8 ~2.7, ~0.7 ~3, ~0.5 ~3.2, ~0.5

    Ip (MA) 1.5 1 ~5 ~10 ~12

    ~2.6 ~2.1

    Duty factor (%) ~0.01 ~0.01 ~15 30 60

    ~5

    ~50 ~300

    ~4

    0.3

    ~9 ~25

    BT (T) 0.6 ~1.1 ~1.8

    Pulse (s) 1 5 ~50 Steady state Steady state

    Pfusion (MW) − ~10 ~77 ~3100

    WL (MW/m2) − − ~1 ~4

    TFC; Solenoid Multi-turn; Solenoid Multi-turn; Solenoid Single-turn; No-solen. Single-turn; No-solen.

  • PU AST558, 4/25/05 ST Science & Fusion Energy

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    New PF1A-L8 Ch MSE-CIF for j(r)

    Tangential MicrowaveHigh-k Scattering

    UCD

    Nova Photonics Inc.

    Major Exciting New Tools for FY 05 Run

    EF/RWM Coils

    Columbia

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    NSTX Exceeded Standard Scaling & Reached Higher Ip/aBT, Indicating Better Field and Size Utilization

    • Verified very high beta prediction ⇒ new physics:βT = 2μ0〈p〉 / BT02 ≤ 38%βN = βT / (Ip/aBT0) ≤ 6.4〈β〉 = 2μ0〈p〉 / 〈B2〉 ≤ 20%

    • Obtained nearly sustained plasmas with neutral beam and bootstrap current alone– Basis for neutral beam

    sustained ST CTF at Q~2 – Relevant to ITER hybrid mode

    optimization

    • To produce and study full non-inductive sustained plasmas– Relevant to DEMO

    Columbia U, LANL, PPPL

    CTF β requirement well within stabilityLimits, without using active control

    CTF

    βN = 6DEMO

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Strong Plasma Flow (MA=Vφ/VAlfvén~0.3) Has Large Effects on Equilibrium and Stability

    • Internal MHD modes stops growing

    • Pressure axis shifts out by ~10% of outer minor radius

    • Density axis shifts by ~20%

    0.4 0.6 0.8 1.0 1.2 1.4R(m)

    0.0

    0.2

    0.4

    0.6

    0.8

    1.0

    1.2

    1.4 107540 330ms

    MA

    Te(keV)

    ne (m-3)4x1019

    0.5 2.01.0 1.5

    -2

    -1

    1

    2

    0

    R(m)

    Z(m

    )

    pressure surfacesmagnetic surfaces

    Equilibrium Reconstruction with Flow

    Columbia U, GA, PPPL, U Rochester

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Global and Thermal τE’s Compare Favorably with Higher A Database

    • TRANSP analysis for thermal confinement

    τ E

    (ms)

    τE (ms)12080400

    120

    80

    40

    00.00 0.01 0.02 0.03 0.04 0.05

    0.00

    0.05

    0.10

    τ E [

    s]

    τE [s]

    H-modeL-mode

    x2.5

    x1.5

    • Compare with ITER scaling for total confinement, including fast ions

    L-modes have higher non-thermal component and comparable τE! Why?Bell, Kaye, PPPL

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Ion Internal Transport Barrier in Beam-Heated H-Mode Contrasts Improved Electron Confinement in L-Mode

    Magnetic Axis

    Kinetic Profile Local Error Sampling

    Axis Edge

    Regionsrequiringimproved

    dataresolution

    TransportBarrierregionwhere

    χi ~ χiNC

    andχe >> χi

    Columbia U, Culham, ORNL, PPPL

    But L-mode plasmas show improved electron confinement! Why?

    L-mode H-mode

    H-modeL-mode

    T e(k

    eV)

    n e(1

    013 /c

    m3 )

    iITB?

    iITB?

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Analysis Shows Stability to Modes at Ion Gyro-Scale & Strong Instability at Electron Gyro-Scale (H-Mode)

    Em

    issi

    vity

    (mW

    /cm

    3 )

    Ne 8,9+

    MHD event

    Ne puff

    t (ms)

    R (cm)

    Core Transport Physics

    In ion confinement zone

    Thermal Conductivity

    • χion ~ χneoclassical• χelec >> χion

    Impurity Diffusivity

    • Dimp ~ Dneoclassical

    Micro-instability

    calculations

    • Driven by T and n gradients

    • kθρi < 1 (ion gyro-scale) stable or suppressed by Vφshear

    • kθρi >> 1 (electron gyro-scale) strongly unstable

    Cadarache, JHU, PPPL, U. Maryland

    iITB?

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Detailed Diagnosis and Gyrokinetic Analysis of β ~ 1 Turbulence Has Broad Scientific Importance

    Can k¦ρι ≥ 1 turbulence at β ~ 1 be understood?

    Region to be tested

    Armitage (U. Colorado)

    • Astrophysics turbulence dynamics: cascading of MHD turbulence to ion scales is of fundamental importance at β > 1

    • Fusion’s gyrokinetic formalism apply to astrophysical turbulence, covering shocks, solar wind, accretion disks

    • Laboratory ST plasmas provide validation of formulism

    Gyrokinetic turbulence simulation in accretion disk of supermassive black hole at galactic center, assuming damping of turbulence by plasma ions vs. electrons

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Kinetic instabilities are an important issue for Spherical Tori and ITER

    • Energetic particle modes are most ubiquitous, cause most losses– Chirping, lower frequency

    – Better overlap precession, bounce

    and MHD frequencies at low A.

    • Toroidal Alfvén Eigenmodes common – Fewer induced losses

    – more important at high A

    • Compressional Alfvén Eigenmodes and

    Global Alfvén Eigenmodes are common, but apparently benign.

    • Development of M3D,HYM,NOVA codes for prediction/analysis.

    NATIONAL FUSION FACILITYS A N D I E G O

    DIII-D

    0

    1

    2

    3

    4

    5

    6

    βfast(0) / βtot(0)V

    fast

    /VA

    lfvén

    0.0 0.2 0.4 0.6

    ITER NSTX

    ARIES-ST (design)

    0.8

    CTF

    DIII-D

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    A Broad Spectrum of Energetic Particle Driven Modes is Seen on NSTX

    10

    100

    1000

    0.1 0.2 0.3TIME (s)

    FRE

    QU

    EN

    CY

    (kH

    z)

    “Fish-Bones”

    TAE

    CAE/GAE

    108170

    Do these Alfvén Eigenmodes (AEs) and fish-bones (f.b.s) Interact to expel energetic particles?

    PPPL

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    • Off-axis EBWCD may be critical for sustained, solenoid-free, high β ST operation

    • Local EBWCD may provide an effective tool for tearing mode stabilization

    • EBWCD & heating can assist plasma current startup & ramp-up

    • NSTX provides an excellent testbedfor evaluating EBW coupling, heating and CD physics at megawatt rf power levels

    EBW Heating & CD Applied to ST Plasmas Present Unique Opportunities for Scientific & Fusion Energy Research

    Charles Kessel (PPPL) Tokamak Simulation Code

    Total

    Bootstrap

    NBCD

    EBWCD

    J//(A/Wb)

    0

    106

    0 10.5ρ

    NSTX, βt = 42%, βpol = 1.6 Bt = 0.34 T , Ip = 1 MA

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Frequency = 28 GHzEBW Power = 3 MWTotal Driven Current = 135 kA

    30

    15

    0 0.2 0.80.60.4

    1.5

    Z(m)

    -1.5R(m)

    1.40.4

    EBWLauncher

    Modeling Predicts Efficient Local Electron Heating & Off-Axis Ohkawa EBWCD in β ~ 40% NSTX Plasmas

    GENRAY/CQL3D

    β = 41%

    • Strong diffusion near trapped-passing boundary enables efficient Ohkawa EBWCD

    • EBWCD-Bootstrap current synergy may provide ~10% enhancement

    ElectronElectronDiffusionDiffusion

    G. Taylor, et al ., Phys. Plasmas 11, 4733 (2004)R.W. Harvey & G. Taylor, to be published in Phys. Plasmas 12 (May 2005)

    CurrentDensity(A/cm2)

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Full Wave Coupling Code Predicts Efficient O-X-B Coupling at ~ 28 GHz into β = 40% NSTX Plasma

    • Steerable mirror launcher aligns 1 MW rfpower with high O-X-B coupling “window”(Two launchers for 2 MW)

    • Switching between mirrors above and below midplane changes direction of EBW-driven current

    AORSA-1D

    ORNL

    NSTXPlasma

    Low-lossCorrugatedWaveguide

    SteerableMirror

    Launcher

    NSTX Vacuum Vessel

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    ST Plasma Edge Possesses Large Mirror Ratio &Geometric Expansion of Scrape-Off Layer (SOL)

    0

    10

    20

    30

    1.55 1.60 1.65 1.70R (m) in SOL

    A B

    Are

    a Ex

    pans

    ion

    Rat

    io Larger GeometricExpansion

    0

    0.50

    0.75

    1.00

    0 2 4 6 8

    Distance Along SOL Field Line (m)

    inboardoutboard

    |B| (

    T)

    Larger Mirror Ratio (MR)→ More Instabilities→ Larger ⊥ Loss→ Thicker SOL

    Scrape-Off Layer Geometryof Inboard Limited ST Plasma

    0.25 0.5 0.75 1 1.25 1.5

    -1

    -0.5

    0.5

    1

    1.5

    R(m)

    Z(m)

    0

    APlasmaFlux toLimiter

    Divertor

    Limiter

    SOL FluxSurface

    PlasmaEdge

    B:PlasmaFlux ToDivertor

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Increased SOL Mirror Ratio (MR) ⇒ Increased Footprint & Decreased Peak of Divertor Heat Flux

    High & Low δ Divertor Bolometer Measurements

    Rdiv (m) 0.36 0.75

    SOL MR ~ 3 ~ 1.5

    Δdiv (m) ~ 0.3 ~ 0.12

    Factor of ~2 in Rdiv and MR⇓

    Factor of ~3 in Δdiv

    Why?

    SOL MR ≈ 3 SOL MR ≈ 1.5

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Plasma Edge Studies Reveal Turbulence and“Blobs” Important to Divertor Flux Scaling Studies

    He manifold

    Side-viewingreentrant window

    H-mode

    L-mode

    Broadly Based Study:• Gas Puff Imaging

    views along field lines (PPPL, LANL)

    • Very fast camera, 105/s (PSI)

    • Reflectometers and edge (UCLA, ORNL)

    • Reciprocating probe(UCSD)

    • Divertor fast camera(Hiroshima U)

    • IR Cameras (ORNL), Filterscope (PPPL)

    • Modeling (PPPL, UCSD, LLNL, Lodestar)

    105710

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    CHI + OH

    OH only

    HIT-II Experiment

    Culham, KAIST, Kyushu-Tokai U, PPPL, U Tokyo, U Washington

    New absorber insulator installed

    Capacitor bank to be installed

    Three Outer Poloidal Field Startup Scenarios, e.g.:

    Outboard Field Null

    Flux contours 20 kA

    - 20 kA

    2.8 kA

    Coaxial Helicity Injection Tests

    Solenoid Free Start-Up via Coaxial Helicity Injection & Outer Poloidal Field Coil Are Being Tested

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Future ST Steps Are Estimated to Require Moderate Sizes to Make Key Advances toward DEMO

    Device NSTX NSST CTF DEMO

    Mission Proof of Principle Performance Extension

    Energy Development, Component Testing

    Practicality of Fusion Electricity

    R (m) 0.85 ~1.5 ~1.2 ~3

    a (m) 0.65 ~0.9 ~0.8 ~2

    κ, δ 2.5, 0.8 ~2.7, ~0.7 ~3, ~0.5 ~3.2, ~0.5

    Ip (MA) 1.5 1 ~5 ~10 ~12

    ~2.6 ~2.1

    Duty factor (%) ~0.01 ~0.01 ~15 30 60

    ~5

    ~50 ~300

    ~4

    0.3

    ~9 ~25

    BT (T) 0.6 ~1.1 ~1.8

    Pulse (s) 1 5 ~50 Steady state Steady state

    Pfusion (MW) − ~10 ~77 ~3100

    WL (MW/m2) − − ~1 ~4

    TFC; Solenoid Multi-turn; Solenoid Multi-turn; Solenoid Single-turn; No-solen. Single-turn; No-solen.

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    NSTX Made Large Progress in Producing and Studying the Science of Attractive Sustained Plasmas

    • EFIT02• Peak βT• All shapes

    2001-3

    2004

    Frac

    tion

    of S

    elf-D

    riven

    Cur

    rent

    f B

    S~

    0.5

    ×ε½

    β P

    CTF

    DEMO

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Long-Pulse H-Mode Plasmas Made Large Progress in Physics Basis for Next-Term ST Science Facilities

    Well positioned to address the science of sustained high-performance plasmas.

    ARIES-AT (4MW/m2)

    CTF-ST}

    τpulse/τE Normalized pulse length

    Nor

    mal

    ized

    bet

    a x

    norm

    aliz

    ed c

    onfin

    emen

    t NSTX OperationARIES-ST (4WM/m2)

    4

    2

    1MW/m2

    NSST

  • PU AST558, 4/25/05 ST Science & Fusion Energy

    Spherical Tokamak (ST) Offers Rich Plasma Science Opportunities and High Fusion Energy Potential

    • Early MHD theory suggested ST could permit high β, confirmed recently by experiments

    • ST research is highly collaborative worldwide• ST enables cost-effective steps toward practical

    fusion energy• Recent research identified new opportunities for

    addressing key plasma science issues using ST• Results have been very encouraging in many scientific

    topical areas

    We welcome opportunities to answer questions, more show and tell

    Spherical Tokamak Plasma Science & Fusion Energy Development Spherical Tokamak (ST) Offers Rich Plasma Science Opportunities and High Fusion Energy PotentialTokamak Theory in Early 1980’s Showed Maximum Stable bT Increased with Lowered Aspect Ratio (A)Minimizing Tokamak Aspect Ratio Maximizes Field Line Length in Good Curvature High b StabilityST Plasma Elongates Naturally, Needs Less TF & PF Coil Currents, Increases Ip/aBT Higher bTmax Answering the Plasma Science Questions Also Enable Cost-Effective Steps toward Fusion EnergyOptimized Device Configuration Features of ST Also Fulfill the CTF Mission Effectively Strong Plasma Flow (MA=V/VAlfvén~0.3) Has Large Effects on Equilibrium and StabilityIon Internal Transport Barrier in Beam-Heated H-Mode Contrasts Improved Electron Confinement in L-ModeAnalysis Shows Stability to Modes at Ion Gyro-Scale & Strong Instability at Electron Gyro-Scale (H-Mode)Detailed Diagnosis and Gyrokinetic Analysis of b ~ 1 Turbulence Has Broad Scientific ImportanceKinetic instabilities are an important issue for Spherical Tori and ITERA Broad Spectrum of Energetic Particle Driven Modes is Seen on NSTXST Plasma Edge Possesses Large Mirror Ratio &�Geometric Expansion of Scrape-Off Layer (SOL)Increased SOL Mirror Ratio (MR) Increased Footprint & Decreased Peak of Divertor Heat FluxPlasma Edge Studies Reveal Turbulence and�“Blobs” Important to Divertor Flux Scaling StudiesLong-Pulse H-Mode Plasmas Made Large Progress in Physics Basis for Next-Term ST Science FacilitiesSpherical Tokamak (ST) Offers Rich Plasma Science Opportunities and High Fusion Energy Potential