Progressing Performance Tokamak Core Physics Marco Wischmeier - - PowerPoint PPT Presentation

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Progressing Performance Tokamak Core Physics Marco Wischmeier - - PowerPoint PPT Presentation

Progressing Performance Tokamak Core Physics Marco Wischmeier Max-Planck-Institut fr Plasmaphysik 85748 Garching marco.wischmeier at ipp.mpg.de Joint ICTP-IAEA College on Advanced Plasma Physics, Triest, Italy, 2016 Specific Fusion


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Progressing Performance – Tokamak Core Physics

Joint ICTP-IAEA College on Advanced Plasma Physics, Triest, Italy, 2016

Marco Wischmeier Max-Planck-Institut für Plasmaphysik 85748 Garching marco.wischmeier at ipp.mpg.de

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Ø heat insulation (energy transport) Ø magnetohydrodynamic (MHD) stability Ø tokamak operational scenarios Ø exhaust of heat and particles (tomorrow, Wednesday) Specific Fusion Plasma Physics

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Ø heat insulation (energy transport) Ø magnetohydrodynamic (MHD) stability Ø tokamak operational scenarios Specific Fusion Plasma Physics

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α-heating compensates losses:

  • radiative losses (Bremsstrahlung)
  • heat conduction and convection

τE = Wplasma/Ploss (‘energy confinement time’) leads to which has a minimum for nτΕ = 2 x 1020 m-3 s at T = 20 keV

Reactor energetics: the ‚Lawson‘ criterion for nτΕ

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Power Ploss needed to sustain plasma

  • determined by thermal insulation:

τE = Wplasma/Ploss (‘energy confinement time’) Fusion power increases with Wplasma

  • Pfus ~ nDnT<σv> ~ ne

2T2 ~ Wplasma 2

Present day experiments: Ploss compensated by external heating

  • Q = Pfus/Pext ≈ Pfus/Ploss ~ nTτE

Reactor: Ploss compensated by α-(self)heating

  • Q = Pfus/Pext =Pfus/(Ploss-Pα) → ∞ (ignited plasma)

Figure of merit for fusion performance nTτ

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How is heat transported across field lines?

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R Energy confinement time determined by transport

collision Transport to the edge B

  • Experimental finding:
  • ‚Anomalous‘ transport, much larger

heat losses

  • Tokamaks: Ignition expected for R ~ 8 m

Simplest ansatz for heat transport:

  • Diffusion due to binary collisions

χ ≈ rL

2 / τc ≈ 0.005 m2/s

τE ≈ a2/(4 χ)

  • table top device (R ≈ 0.6 m)

should ignite! Important transport regime for tokamaks and stellarators:

  • Diffusion of trapped particles on banana
  • rbits due to binary collisions
  • neo-classical transport (important for

impurities)

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Energy confinement: empirical scaling laws

In lack of a first principles physics model, ITER has been designed

  • n the basis of an empirical scaling law
  • very limited predictive capability, need first principles model
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From empirical scaling laws to physics understanding

First principle based understanding of temperature (density, …) profiles

Pheat

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Anomalous transport due to turbulence Simplest estimation for heat transport due to turbulence: D ≈ (Δreddy)2/τtear ≈ 2 m2/s

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Global turbulence simulations

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Energy Transport in Fusion Plasmas

Anomalous transport determined by gradient driven turbulence

  • temperature profiles show a certain ‘stiffness’
  • ‘critical gradient’ phenomenon – χ increases with Pheat (!)

⇒ increasing machine size will increase central T as well as τE N.B.: steep gradient region in the edge governed by different physics! T(0.4) T(0.8)

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Energy Transport in Fusion Plasmas

Locally, critical gradients can be exceeded (‘Transport Barrier’)

  • sheared rotation can suppress turbulent eddies
  • works at the edge (H-mode, see later) and internally (‘ITB’)

ASDEX Upgrade

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Anomalous transport determines machine size

ITER (Q=10) DEMO (ignited)

  • ignition (self-heated plasma) predicted at R = 7.5 m
  • at this machine size, the fusion power will be of the order of 1 GW

ITER (βN=1.8) DEMO (βN=3)

Major radius R0 [m] Major radius R0 [m] Fusion Power [MW]

1 5 5

7 . 3 7 . 2 1 . 23 . 3 53 . 3 1 . 3 1 2

− = B R H A q c c Q

N

β

4 2 95 3 4 2 1

A q R B c P

N fus

β =

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Ø heat insulation (energy transport) Ø magnetohydrodynamic (MHD) stability Ø tokamak operational scenarios

Specific Fusion Plasma Physics

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Plasma discharges can be subject to instabilities

Desaster β-limit, disruption Self-organisation sationarity of profiles j(r), p(r)

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Plasma discharges can be subject to instabilities

Equilibrium ∇p = j x B means force balance, but not necessarily stability Stability against perturbation has to be evaluated by stability analysis Mathematically: solve time dependent MHD equations

  • linear stability: small perturbation, equilibrium unperturbed,

exponentially growing eigenmodes

  • nonlinear stability: finite peturbation, back reaction on equilibrium,

final state can also be saturated instability

linearly stable linearly unstable

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current driven instabilities pressure driven instabilities Ex.: kink mode Ex.: interchange mode (only tokamaks) (tokamak and stellarator) N.B.: also fast particle pressure (usually kinetic effects)!

Free energies to drive MHD modes

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Ideal MHD: η = 0

  • flux conservation
  • topology unchanged

Resistive MHD: η ≠ 0

  • reconnection of field lines
  • topology changes

Ideal and resistive MHD instabilities

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coupling between island chains (possibly stochastic regions) ⇒ sudden loss of heat insulation ('disruptive instability')

Magnetic islands impact tokamak discharges

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High density clamps current profile and leads to island chains excessive cooling, current can no longer be sustained disruptions lead to high thermal and mechanical loads!

Disruptive instability limits achievable density

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Removal of magnetic islands by microwaves

Electron Cyclotron Resonance at ν = n 28 GHz B [T] Plasma is optically thick at ECR frequency Deposition controlled by local B-field ⇒ very good localisation

n νECR = νwave – k|| v||

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Optimising nT means high pressure and, for given magnetic field, high dimensionless pressure β = 2µ0 <p> / B2 This quantity is ultimately limited by ideal instabilities ‘Ideal’ MHD limit (ultimate limit, plasma unstable on Alfvén time scale ~ 10 µs,

  • nly limited by inertia)
  • ‘Troyon’ limit βmax ~ Ip/(aB), leads to

definition of βN = β/(Ip/(aB))

  • at fixed aB, shaping of plasma cross-

section allows higher Ip → higher β

Ideal MHD instabilities limit achievable pressure

βN=β/(I/aB)=3.5 β [%]

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Ø heat insulation (energy transport) Ø magnetohydrodynamic (MHD) stability Ø tokamak operational scenarios

Specific Fusion Plasma Physics

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What is a ‚tokamak scenario‘?

βp = 1 Ip = 800 kA fNI = 37% βp = 1 Ip = 800 kA fNI = 14%

A tokamak (operational) scenario is a recipe to run a tokamak discharge Plasma discharge characterised by

  • external control parameters: Bt, R0, a, κ, δ, Pheat, ΦD…
  • integral plasma parameters: β = 2µ0<p>/B2, Ip = 2π ∫ j(r) r dr…
  • plasma profiles: pressure p(r) = n(r)*T(r), current density j(r)

→ operational scenario best characterised by shape of p(r), j(r)

current density (a.u.) current density (a.u.)

total j(r) noninductive j(r) total j(r) noninductive j(r)

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Control of the profiles j(r)and p(r) is limited

Pressure profile determined by combination of heating / fuelling profile and radial transport coefficients

  • ohmic heating coupled to temperature profile via σ ~T3/2
  • external heating methods allow for some variation – ICRH/ECRH

deposition determined by B-field, NBI has usually broad profile

  • gas puff is peripheral source of particles, pellets further inside

but: under reactor-like conditions, dominant α-heating ~ (nT)2

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Standard scenario without special tailoring of geometry or profiles

  • central current density usually limited by sawteeth
  • temperature gradient sits at critical value over most of profile
  • extrapolates to very large (R > 10 m, Ip > 30 MA) pulsed reactor

The (low confinement) L-mode scenario

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The (high confinement) H-mode scenario

With hot (low collisionality) conditions, edge transport barrier develops

  • gives higher boundary condition for ‘stiff’ temperature profiles
  • global confinement τE roughly factor 2 better than L-mode
  • extrapolates to more attractive (R ~ 8 m, Ip ~ 20 MA) pulsed reactor
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Quality of heat insulation

Turbulent transport limits (on a logarithmic scale) the gradient of the temperature profile Analogy of a sand pile: limited gradient

But total height is variable by barriers

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Turbulent transport strongly increases with logarithmic temperature gradient

Existence of a critical logarithmic temperature gradient (nearly independent on heating power)

∇T T 1 LT,cr = = - d ln T dr T(a) = T(b) exp b - a LT,cr ⎛ ⎝ ⎛ ⎝ “stiff” temperature profiles

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Core temperature determined by temperature at the edge… Transport barrier at the edge (“high” confinement mode) in divertor geometry … nearly independent of heating power

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Energy Transport in Fusion Plasmas

Anomalous transport determined by gradient driven turbulence

  • linear: main microinstabilities giving rise to turbulence identified
  • nonlinear: turbulence generates ‘zonal flow’ acting back on eddy size
  • (eddy size)2 / (eddy lifetime) is of the order of experimental χ-values
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Macroscopic sheared rotation deforms eddies and tears them

Radial transport increases with eddy size

Sheared flows – the most important saturation mechanism

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Stationary H-modes usually accompanied by ELMs

Edge Localised Modes (ELMs) regulate edge plasma pressure

  • without ELMs, particle confinement ‚too good‘ – impurity accumulation
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Cross section of the spherical tokamak MAST MAST, CCFE, UK

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Plasma discharges can be subject to instabilities MAST, CCFE, UK

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Instability also measured in total radiation

ASDEX Upgrade – tomographic reconstruction of AXUV diods By M. Bernert on youtube

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Stationary H-modes usually accompanied by ELMs

But: ELMs may pose a serious threat to the ITER divertor

  • large ‘type I ELMs’ may lead to too high divertor erosion

acceptable lifetime for 1st ITER divertor

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Progress…

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Tokamaks have made Tremendous Progress

  • figure of merit nTτE doubles

every 1.8 years

  • JET tokamak in Culham (UK) has produced 16 MW of fusion power
  • present knowledge has allowed to design a next step tokamak

to demonstrate large scale fusion power production: ITER