ReNeW
Developing Predictive Capability for
High Performance Steady State
Plasmas
P. Snyder, A. Kritz, R. Budny, C.S. Chang, M. Greenwald, T. Carter, J. Wright, G.R. Tynan
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Primary Goal
Reduce Time to and Cost & Risk Of 1) ITER-experiments
ReNeW
Secondary Goals: Make Nearer
Term Contributions
• Provide Deeper Physics Insights to
Experiments
• Test Theory using Numerical Experiment
• Help Resolve Serious Performance Issues
• Scenario Modeling for ITER
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Approach:
• Identify Key Issues w/ Existing Theory,
Modeling & Experiment
• Develop Suitable Numerical Models
Capturing Essential Physics
• Scientifically Validate Simulations Across
Range of Experiments
• Use Validated Models to Attempt Prediction
of New Experiments
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Caveat Emptor:
• Recognize we will be extrapolating, not
merely interpolating
• May require new theoretical insights e.g. to
couple disparate spatiotemporal scales & physics => Not just bigger, faster codes
• Will still require reduced models for some
problem elements
– Particularly for incorporation into real-time
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Approach:
• Develop Case Studies
• Sort Based Upon Impact on DEMO Device
• Hear ReNeW workshop presentations &
read whitepapers
• Develop outlines of Predictive Modeling
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Sorting Methodology: What is
Impact of the Prediction?
• Critical Impact: Results influence machine
health and/or safety issues
• Performance Impact: Results influence
HPSS plasma performance
• Ancillary Impact: Results influence non
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Case Studies put forward by Panel
• Pedestal & ELMs
• Edge/SOL/PWI
• Disruptions
• Core Transport & MHD
• RF CD & Heating
• Energetic Particles
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Case Study Organization
• Scientific & Technical Issues
• Challenges
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Pedestal & ELMs: S&T Issues
• Physics of L-H, H-L transitions; threshold
physics
• Pedestal structure mechanisms
• Particle & Power loading to PFCs w/ ELMs,
between ELMs
• ELM Control or Mitigation Scheme
Development
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Pedestal & ELMs: Challenges
• L-H transition trigger, quantitative PLH
predictions
• Pedestal growth to ELM onset
• Inter-ELM simulations w/ realistic
integrated elements (sources, PMI,…)
• ELM Mitigation Physics (pellet pacing,
RMP, …)
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Pedestals & ELMs: Research
Program Elements
• Theory: Possible new approaches that side-step scale
separation assumptions?
• Computation: Need models for complex edge/SOL
geometry, linking w/ PMI, Neoclassical, MHD &
Turbulence. Is GK sufficient? Full Vlasov Required? How to evolve mean profiles w/ these physics included? Push simulations towards low collisionality, high
Greenwald fraction, opaque to neutrals, small rho-star, high beta-N
• Experiments: Improve diagnostics on existing devices
(e.g. fueling sources, Bdot, J|| , high res profiles,
transport fluxes); pedestal studies on new long –pulse devices; Adequate run-time & data analysis coverage
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Edge-SOL: S&T Issues
• Steady-state physics affecting PMI
– Parallel, Perpendicular transport physics – Recycling, First wall condi7oning, High‐T saturated walls – Impurity Genera7on and Transport & Radia7on power losses – PMI & PFC Matl’s Choices – Intrinsic flow genera7on – Tri7um & dust inventory predic7on and control
• Transient heat load effects
• Core Interactions
– Boundary condi7on for Ne, Te, Ti, Vplasma profiles
– Turbulence spreading into core
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Edge-SOL: Challenges
• Significant power loading, pulse length extrapolations for ITER; similar scale extrapolations from ITER to DEMO
• Cannot simultaneously match ALL relevant dimensionless core & edge parameters in
existing experiments => validated predictive modeling essential to fill in gaps
• Quantitative first principles predictions of all key Edge-SOL profiles, dynamics do not exist
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Edge-SOL: Research Program
Elements
• Theory: Fluid & GK comparisons; RF sheath,
kinetic effects; PMI models to incorporate into
plasma simulations; self-consistent flow generation
• Modeling: Integration of parallel & perpendicular
transport & atomic physics; integrate pedestal, SOL, and divertor simulations with PMI & PFC interactions in Steady-state & transient plasmas
• Experiment: Existing devices: Better profile, flow &
turbulence diagnostics including better 2d/3d
coverage; RF sheath measurements, Fueling, in-situ real-time PFC, PMI measurements; Adequate run-time & data analysis coverage
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Energetic Particles: S&T Issues
• Energetic ion driven instabilities
– Stability of energeAc parAcle driven modes – Nonlinear saturaAon, mode‐mode coupling – Longer Ame scale simulaAons (slowing down Ame) requiring parAcle sources and sinks – KineAc effects (moving beyond ideal MHD models of bulk plasma) – Impact of energeAc ion driven instabiliAes on current drive and bulk plasma heat, parAcle, and momentum transport – Effect of background turbulence on energeAc parAcle driven modes
• Energetic ion transport and losses
– AE induced transport and loss
– EnergeAc ion interacAon with background turbulence
– Impact of alpha transport in burning plasma
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Energetic Particles: Challenges
• Significant extrapolation in the physics of AEs to ITER (presence of many of modes, alpha
particle drive rather than beams/ICRF)
• Linear stability predictions OK but predictive capability for nonlinear saturation and induced energetic ion transport and loss needs
development.
• Develop appropriate models for the synthetic diagnostics in simulations for code validation against measurements of certain observable quantities.
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Energetic Particles: Research
Program Elements
• Theory – EnergeAc ion transport by AEs. Current models dramaAcally underpredict energeAc ion loss using experimentally measured mode amplitude and structure (DIII‐D beam ion redistribuAon experiments and NSTX – TAE induced avalanches are examples). – Need to develop reduced theories to understand/explore this problem. – Nonlinear saturaAon of AEs, mode‐mode coupling – ConAnued strong role of analyAc theory in energeAc parAcle physics – New methods for long term simulaAons may be required and tested • Modeling – Nonlinear MHD codes + KineAcs (e.g. M3D extension) – EnergeAc parAcle transport in the presence of mulAple AE modes – KineAc/GyrokineAc simulaAon of energeAc parAcle modes – Comprehensive verificaAon of computaAonal models and soluAons – Sources and sinks for long term simulaAon of the energy confinement Ame scale • Experiment – Expanded energeAc ion distribuAon (e.g. FIDA) and loss diagnosAcs – Direct measurements of energeAc‐ion driven modes: enhanced density and temperature fluctuaAon measurements (e.g. reflectometry, CECE) – Development of local magneAc field fluctuaAon measurements for determining amplitude and mode structure – UAlize basic plasma physics devicesReNeW
Disruptions: S&T Issues
• Disruption probability away from hard
limits
• Detecting disruption with adequate warning
to take action
• Developing and demonstrating workable
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Disruptions: Challenges
• Can we predict operational boundaries including non-ideal (e.g. error fields) w/o empirical testing at performance limit?
• Can we detect & avoid oncoming disruptions via real-time control?
• Can we predict performance of mitigation schemes with sufficient confidence for e.g. DEMO licensing?
• Can we demonstrate that mitigation scheme works as advertised?
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Disruptions: Research Program
Elements
• High fidelity modeling of disruptions including whole plasma non-linear MHD, RE production & transport, mitigation scheme performance
• Dedicated experiments on detection, avoidance and mitigation
• Reduced modeling for incorporation into real-time control schemes
• Key Goals: Reduce disruption probability to acceptable levels, demonstrate mitigation
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RF Heating & CD: S&T Issues
– Alpha physics issues. What is the degree of LH and ICRF parasiAc absorpAon on alpha parAcles. What possible transport effects from RF on alphas may be expected (i.e. “alpha channeling”) – Flow drive. Desirable for suppression of turbulence. Both LH and ICRF waves have created significant toroidal and poloidal flows. The mechanisms are not well understood or predicted by exisAng theory or models. – Current drive. Current profile control is necessary to control locaAon of reversed shear surface and to maintain a non‐inducAve steady state plasma. What are the power requirements and degree of locaAon control? – Nonlinear wave‐par7cle interac7on. Wave parAcle interacAon has been dealt with in the quasilinear framework. What is the effect of nonlinear wave‐ parAcle interacAon and under what condiAons are these effects important? This is a general issue but for burning plasmas may be necessary for accurate calculaAon of RF‐alpha interacAons. – Hea7ng. What are the power requirements and coupling efficiency – relevant for both LH and ICRF.
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RF Heating & CD: Challenges
• Validity of geometric opAcs for LHRF in core – Develop & Compare against full wave soluAons • RF propagaAon/absorpAon in edge/sol region; interacAon with PFCs; RF Sheaths & PMI on antenna &magneAcally connected structures • Nonlinear wave‐parAcle effects on absorpAon • PredicAve antenna coupling • RF flow drive: basic physics not understood
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RF Heating & CD: Research
Program Elements
• Key missing piece: IntegraAng RF w/ other physics (e.g. RF/MHD for predicAve NTM control; RF/turbulence for flow control & impurity control) • New numerical approaches e.g. for complex edge region problems (coupling, RF‐PMI, etc…) • ConAnue syntheAc diagnosAc development; new diagnosAcs for edge/sol physics • Adequate personnel for analysis & verificaAonReNeW
Integrated Modeling: S&T Issues
• Multiple time-space scales (e.g. turbulence
vs. profile evolution scales)
• Strongly coupled phenomena challenge
traditional categorization (e.g. MHD, Turbulence, RF, etc…)
• Integrated models require very high
reliability – failure in place brings down model
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Integrated Modeling: Challenges
• Startup modeling
• L-H and H-L transitions, ELM & sawtooth
cycles
• Pedestal physics integrated w/ core model
• MHD effects in steady-state
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Integrated Modeling: Research
Program Elements
• Improved reduced models needed
• Incorporate higher fidelity (“first
principles”) models into Integrated models
• Better numerical techniques and algorithms
to span wide spatio-temporal scales
• New frameworks (e.g. 3D for islands, ripple,
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Predictive HPSS Plasma Modeling
Will Require
• New Theoretical Approaches Needed – particularly for multiple
physics and/or multiscale problems
• Key aspect of Computational Challenges: Integration of multiple
sets of physics (e.g. RF, MHD and fast particles) into single
model
• Some requirements for new experimental capabilities – new
diagnostics in new confinement regimes,
• There is a role for selected dedicated subscale experiments
• New Class of Researcher who cuts across Expts/Theory/
Modeling to rigorously validate predictive models
• Need to develop user base for existing and emerging “first
principles” simulations & integrated modeling tools