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The Physics Base for ITER and DEMO

This presentation covers key topics in fusion plasma physics, the requirements for ITER and DEMO, the present research status, and an outlook on the field. It delves into core plasma dynamics, transport mechanisms, stability considerations, and the challenges in achieving fusion power. The talk discusses the role of H and bN parameters in determining reactor size, the importance of noninductive current drive for sustaining fusion reactions, and the need for high plasma performance for efficient fusion power generation. It also explores experimental data comparison, current drive methods, and potential scenarios for enhancing plasma confinement and fusion power output. Overall, the presentation offers insights into the physics behind fusion reactors and the advancements required for future fusion energy production.

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The Physics Base for ITER and DEMO

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  1. The Physics Base for ITER and DEMO Hartmut Zohm Max-Planck-Institut für Plasmaphysik, Garching, Germany EURATOM Association • main topics in fusion plasma physics • requirements for ITER and DEMO • present status of physics research • summary and outlook Hauptvortrag given at AKE DPG Spring Meeting, Bonn, 15.03.2010

  2. Fusion Reactor in a Nutshell Core plasma @ T=25 keV, n=1020 m-3 produces Pfus: D+T = He + n + 17.6 MeV Plasma physics – this talk 4/5*Pfus escape as neutrons and hit the first wall (Blanket = tritium production and energy conversion) Neutronics – talk by A. Klix 1/5*Pfus + Pext escape in charged particles along B-field lines and hit the wall in a narrow band Plasma wall interaction – talk by B. Unterberg

  3. Main Areas of Fusion Plasma Physics Transport determines amount of heating needed to obtain required T tE = Wkin/Ploss (Ploss is the power needed to sustain the plasma) experiments measured relative to multi-machine scaling: H=tE,exp/tE,scal Stability determines the limits to kinetic pressure (Pfus ~ n2T2 = p2) b = pkin/pmag = 2m0 pkin / B2 (dimensionless pressure) experimental progress measured relative to ideal MHD limit bN=b/(I/(aB)) a-heating should largely compensate Ploss in a reactor Q=Pfus/Pext, since Pa = Pfus/5, the fraction of a-heating is Pa/Ploss=Q/(Q+5) Exhaust characterised by the ratio of power in charged particles to the major radius, P/R (since the power deposition width is roughly constant)

  4. main topics in fusion plasma physics • requirements for ITER and DEMO • present status of physics research • summary and outlook

  5. H and bN determine machine size Fusion Power [MW] ITER (bN=1.8) DEMO (bN=3) ITER (Q=10) DEMO (ignited) Major radius R0 [m] Major radius R0 [m] • bNdoes almost not enter into Q, but strongly into fusion power • high H helps to achieve ignition, but does not enter in fusion power.

  6. DEMO should have reasonable pulse length Tokamak (ASDEX Upgrade, JET, ITER) Stellarator (Wendelstein 7-X) • Tokamak: poloidal field from plasma current sustained by transfomer: • intrinsically pulsed unless clever tricks are played • Stellarator: all fields from external coils, intrinsically steady state • (but at least 1.5 steps behind in evolution)

  7. bN=3 fCD=0.0 fCD=0.1 fCD=0.2 fCD=0.3 fCD=0.3 bN=4 fCD=0.2 fCD=0.1 fCD=0 Noninductive current drive in a tokamak DEMO Net el. power [MW] Recirculating power fraction Fusion power [MW] Pulse length [s] • Intrinsic thermoelectric current (‚bootstrap current‘) – needs high b • External current drive (e.g. by RF waves) consumes additional power • ‚offset‘ generated by external current drive calls for large unit size • this in turn aggravates the exhaust problem in terms of P/R

  8. Summary: what is required for ITER / DEMO Reality check: how does this compare to present experimental data base?

  9. main topics in fusion plasma physics • requirements for ITER and DEMO • present status of physics research • summary and outlook

  10.    collision Transport to the edge Confinement of plasma core - transport • Simplest ansatz for heat transport: • Diffusion due to collisions • c rL2 / tc 0.005 m2/s • tE a2/(4c) • table top device (a 0.2 m, R  0.6 m) • should ignite! • Experimental result: • • Anomalous transport by turbulence: • c, D a few m2/s • Tokamaks: Ignition expected for • R = 7.5 m for H~1

  11. The H-mode: a transport barrier in the edge discharges with turbulence Suppression • H-mode edge: turbulence • suppressed by sheared rotation • steep edge gradients of T and n • T higher in whole plasma core • (‘profile stiffness’) • H-Mode is standard operational scenario foreseen for ITER (H=1)

  12. Scenarios with improved confinement (H>1) • Improved H-mode = optimised • H-mode scenario (H = 1.2-1.5) • potential for very long pulses • (‘hybrid scenario’) • ITB (Internal Transport Barrier) • scenario (H 1.5) • potential for steady state • (‘advanced tokamak scenario’)

  13. The next step: studying a-heating • Core plasma parameters sufficient to generate significant fusion power • study plasmas with significant self-heating by a-particles in ITER • needs Pa = 1/5 Pfus >> Pext, so it necessarily is closer to a reactor • We expect to see qualitative new physics: • self-heating nonlinear - interesting dynamics • suprathermal a-particles population can interact with plasma waves • We can have a ‘preview’ in machines of the present generation • pilot D-T experiments (JET (EU), TFTR (US)) • suprathermal ions generated by heating systems simulate a-particles

  14. Previous D-T experiments JET, P. Thomas et al., Phys. Rev. Lett. 1998 ITER • First D-T experiments at low Pa/Ptot have demonstrated a-heating • ‚classical‘ (=collisiional) slowing down would guarantee efficient a-heating • question: can we expect this also when Pa is the dominant heating?

  15. Excitation of Alfven waves by Fast Particles Magnetic perturbation Fast ion loss probe • Suprathermal ions with can excite Alfven waves which expel them • in present day experiments, these ions come from heating systems • in future reactors, this could expel a-particles that should heat the plasma!

  16. N=/(I/aB)=3.5  [%] Stability: ideal pressure limit • Ideal instabilities lead to fast large scale deformation of plasma - disruption • ultimate stability limit, usually around bN 4 • Active control possible: nearby conducting structures + internal coils • may help to extend bN above the ideal ‘no-wall’ limit

  17. Wall erosion strongly depends on edge Te • Acceptable erosion rates only if edge plasma Te is in the 10 eV range • plasma in front of wall has to be 1000 x colder than core plasma (!)

  18. From Limiters to Divertors • plasma wall interaction in well defined zone further away from core plasma • possibility to decrease T, increase n along field lines (p=const.)

  19. Additional cooling by impurity seeding Bolometry of total radiated power Discharge with P/R = 13 MW/m (ASDEX Upgrade) 19 No impurity seeding With N2 seeding • Injecting adequate impurities can significantly reduce divertor heat load • impurity species has to be ‘tailored’ according to edge temperature • edge radiation beneficial, but core radiation (and dilution) must be avoided

  20. Edge Localised Modes (ELMs) in the H-mode edge Thermography of divertor target plates (ASDEX Upgrade) • Steep edge pressure gradient in H-mode drives periodic relaxation instability • Edge Localised Modes (ELMs) lead to burst-like energy pulses on first wall • simple extrapolation indicates that ELMs are not acceptable in ITER

  21. ELM mitigation needed for ITER DIII-D Tokamak, USA, Helical perturbation coils (ASDEX Upgrade) • Several techniques have been developed to tailor ELMs • injection of frozen hydrogen pellets increases repetition frequency • application of helical fields supresses ELMs completely • Have to understand physics better to extrapolate to ITER

  22. main topics in fusion plasma physics • requirements for ITER and DEMO • present status of physics research • summary and outlook

  23. Summary: what is required for ITER / DEMO • Main ITER Q=10 requirements demonstrated today (exception: a-heating) • An attractive DEMO will need substantial progress in plasma physics: • higher b to increase fusion power and approach long pulse/steady state • exhaust of power will be a central point for the success of DEMO • Note: another important area (limitation of plasma density) not covered here

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