prospects for a next-step st - fusion.wisc.edufusion.wisc.edu/istw/papers/menard2.pdf · prospects...
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Prospects for a nextProspects for a next--step STstep ST
Jon Menard (PPPL)
with contributions from:Ray Fonck (UW Madison)
Stan Kaye (PPPL)Dick Majeski (PPPL)
Masa Ono (PPPL)Steve Sabbagh (Columbia U.)
October 24, 2009
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 2October 24, 2009
Comprehensive assessment of ST issues, gaps, needshas been performed within U.S. during last two years
• FESAC Toroidal Alternates Panel (2008)
• OFES Research Needs Workshop (ReNeW) (2009)
• Ongoing: ST community, PPPL strategic planning
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 3October 24, 2009
FESAC Toroidal Alternates Panel (TAP) recently prioritized issues and gaps for the Spherical Torus (ST) for the ITER era
“Tier 1” issues and key questions from TAP, and NSTX goals:1. Startup and Ramp-Up: Is it possible to start-up and ramp-up the plasma current to
multi-MA levels using non-inductive current drive w/ minimal or no central solenoid?– NSTX goal: demonstrate non-inductive ramp-up and sustainment
2. First-Wall Heat Flux: What strategies can be employed for handling normal and off normal heat flux consistent with core and scrape-off-layer operating conditions?– NSTX goal: assess high flux expansion, detached divertors, liquid metals
3. Electron Transport: What governs electron transport at low-A & low collisionality?– NSTX goal: determine modes responsible for electron turbulent transport and
assess the importance of electromagnetic (high β) and collisional effects
4. Magnets: Can we develop reliable center-post magnets and current feeds to operate reliably under substantial fluence of fusion neutrons?– NSTX goal: develop and utilize higher performance toroidal field magnet
ST ITERST ITER--era goal:era goal: “Establish the ST knowledge base to be ready to construct a low aspect-ratio fusion component testing facility …. to inform the design of a demonstration fusion power plant”
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 4October 24, 2009
ReNeW ST Thrust 16 Identified 7 actions for ST research:
1. Develop MA-level plasma current formation and ramp-up
2. Advance innovative magnetic geometries, first wall solutions (liquid metals)
3. Understand ST confinement/stability at fusion-relevant parameters
4. Develop stability control techniques for long-pulse disruption-free operation
5. Employ energetic particle beams, plasma waves, particle control, and core fueling techniques to maintain the current, control plasma profiles
6. Develop normally-conducting radiation-tolerant magnets for ST applications
7. Extend ST performance to near-burning-plasma conditions
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 5October 24, 2009
ST community formulated preliminary development path timeline during ReNeW
• Much discussion revolved around appropriately colored “grey” box• Near-term ST community goal is to better define next-step options
ITER era
NSTX NSTX-U
Lower ν, ρ∗, Sustained plasma
MAST MAST-U
High Ip Startup, GrowthPegasus Peg-HIRF
ST-CTF, Hybrid
ST Physics Validation at Long-Pulse and
High-Field
LowRecycling Alternative
non-SolenoidalFormationCore fueling, Low-ν
LTX LTX-NBI
TF, Magnet DevelopIntegrated power supply
Fusion Nuclear Science
ITER era
NSTX NSTX-U
Lower ν, ρ∗, Sustained plasma
MAST MAST-U
High Ip Startup, GrowthPegasus Peg-HIRF
ST-CTF, Hybrid
ST Physics Validation at Long-Pulse and
High-Field
LowRecycling Alternative
non-SolenoidalFormationCore fueling, Low-ν
LTX LTX-NBI
TF, Magnet DevelopIntegrated power supplyTF, Magnet DevelopIntegrated power supply
Fusion Nuclear Science
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 6October 24, 2009
ST facilities proposed to follow NSTX/NSTX-U emphasize preparation for fusion Demo
• ST Plasma Material Interface Facility (ST-PMIF)– Develop PMI solutions for FNSF/Demo (low and high-A)– Advance start-up, confinement, sustainment for ST– High Pheat/S ~1MW/m2, high Twall, τpulse ~ 103s
• Fusion Nuclear Science Facility ST (FNST)– Develop/test nuclear components for Demo– Sustain Wneutron ~ 0.2-0.4 1-2MW/m2, τpulse = 103 106s
• Burning Plasma ST (BPST)– Burning plasma science for ST-Demo, high Wneutron FNST– Advance start-up, confinement, PMI for FNST/ST-Demo– High βT=20-40%, high vfast/vAlfven, τpulse=102-103s ?
NHTX
FNSF/ST-CTF
NSST
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 7October 24, 2009
Next STs progress from plasma currentIP~4-6MA up to 10-15MA at toroidal field BT = 2-3T
Device Field and Current
FNST (I) / ST-PMIF
FNST (II)
FNST (IV)BPST (II)
ARIES-ST
ITER
JT-60SA
DIII-D
BPST (III)
BPST (I)
NSTXNSTX-U
FNST (III) ITER-SS
JET (DT)
KSTAREAST
ARIES-AT
0
5
10
15
20
25
30
0 1 2 3 4 5 6Toroidal magnetic field BT [T]
Plas
ma
curr
ent I
P [M
A] Plasma current =1/3 to
1/2 of ST reactor value
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 8October 24, 2009
Next STs remain modest in size: R0 ≤ 1.5m, a < 1m
• FNST/BPST would be ~1/3 to 1/2 size scale of ST reactor–Similar size extrapolation from JET/JT-60SA to ITER
Device Major and Minor Radii
JT-60SA
KSTARDIII-D
ARIES-AT
NSTXNSTX-U
FNST (I) / ST-PMIFFNST (II, III, IV)
BPST
ARIES-ST
ITERITER-SS
JET (DT)
EAST
0.0
1.0
2.0
0 1 2 3 4 5 6Major Radius R0 [m]
Min
or R
adiu
s a
[m]
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 9October 24, 2009
Next major ST facilities target baselinefusion performance at or above JET/JT60-SA levels
Fusion Triple Product
NSTX-U
ITER
KSTAREAST
DIII-D
ARIES-ST
FNST (IV)ITER-SS
BPST (III)
BPST (I)FNST (I)ST-PMIF
FNST (II)FNST (III)
JET (DT)JT-60SA
BPST (II)
ARIES-AT
0.1
1
10
100
0 5 10 15 20⟨Ti ⟩ [keV]
n e-b
ar 2
0 ⟨T i⟩ τ
E-th
[m-3
keV
s]
Relative fusion performance:FNST approaches ITER steady-state (SS)BPST approaches ITER inductive
NSTX-U will increase ST fusion performance 10-fold to near EAST/KSTAR/DIII-D
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 10October 24, 2009
Next major DT ST facilities extend fusion gain from JET levels toward ITER levels
DT Fusion Gain
FNST (I) / ST-PMIF
FNST (II)
JET (DT)
FNST (IV)
ITER-SS
BPST (III)
ARIES-AT
BPST (I)
FNST (III)
ITER
ARIES-ST
BPST (II)
0.1
1.0
10.0
100.0
0 5 10 15 20⟨Ti⟩ [keV]
QDT
FNST QDT = 0.4 3BPST QDT = 0.4 10
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 11October 24, 2009
FNST progressively accesses wall loading and pulse-durations approaching Demo values
• BPST would access ITER Demo wall loading for ITER-level pulse durations
Peak outboard DT neutron wall loading
FNST (I) / ST-PMIF
FNST (II)
FNST (IV)
BPST (III)
BPST (I)
FNST (III)
ITER
ARIES-ST
ITER-SS
BPST (II)
ARIES-AT
0.1
1.0
10.0
1.E+02 1.E+03 1.E+04 1.E+05 1.E+06 1.E+07 1.E+08Pulse duration [s]
MW
/m2
Parallel path to high Parallel path to high fluencefluence??
BPST pulse duration 20-30 current redistribution times(4-6 current redistribution times at ne / nGreenwald ~ 0.5)
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 12October 24, 2009
Potential Risks
• ST Plasma Material Interface Facility (ST-PMIF)–Unclear what parameters/criteria to use for designing and
operating “scale-model” of FNSF/Demo divertor• Unclear matching P/R and P/S of Demo is sufficient• What SOL/divertor physics is most important? role of turbulence?
• Fusion Nuclear Science Facility ST (FNST)–Inadequate knowledge-base for ~10MA start-up/ramp-up–No high-power/long-pulse power/particle exhaust solution–Confinement understanding inadequate (impacts size, power)–High-current radiation-tolerant magnets undeveloped
• Burning Plasma ST (BPST)–Confinement understanding inadequate (impacts size, power)–High-power power/particle exhaust solutions not mature –Advanced performance for high QDT inaccessible–Limited auxiliary current-drive options
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 13October 24, 2009
Prospects for start-up/ramp-up and PMI solutions
• Start-up and ramp-up– Pegasus, NSTX, DIII-D have demonstrated ~150-200kA non-OH start-up– Aim to achieve ≥ 0.5MA start-up in NSTX-U project to ≥ 1MA in FNST– Need non-inductive ramp-up from ~1MA to ~10MA in FNST– NSTX-U will provide first (critical) test of NBI ramp-up in ST– If ramp-up behaves as predicted (or better), could take “leap” to FNST
• This is high-risk approach given present knowledge base/environment• Substantial predictive capability for thermal, fast-ion confinement needed
– Non-inductive ramp-up test to ~1/3-1/2 FNST current would reduce risk
• PMI– Partial divertor detachment has reduced peak heat flux factor of 2-5– NSTX will test LLD particle pumping - first liquid metal tests with divertor– MAST-U will test Super-X, NSTX/NSTX-U will test high flux expansion– NSTX-U plausibly upgradable to “warm” (~350C) walls
• Test hydrogenic retention with high-Z wall + low-recycling Li-wall concept– Dedicated PMI facility would strongly benefit ST, especially if low-A
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 14October 24, 2009
Prospects for transport and stability
• Transport– Next STs (& ATs) require confinement well above ITER H-mode scaling– NSTX-U will improve understanding of transport causes and scalings
• Will extend ν* scaling factor of 3-6 lower• The ν* scaling most important for FNST, β and ρ* scalings for BPST• Electron transport most important given high χe observed in STs
– Need tools to improve confinement motivation for Li research• Primary goal of LTX program
• Stability– Increased CD and profile control capability of NSTX/MAST-U expected
to provide access to high-β regimes w/ full non-inductive current drive• Need to characterize trade-offs between high βN and low disruptivity
– NSTX-U/MAST-U Normalized pulse-lengths limited to ~3-10τCR
– ST has unique β, ρ*, ν*, parameter regime, profile/control requirements• No other long-pulse/steady-state high-performance ST devices are planned• Long-pulse high-performance ST PE or BP would substantially lower risk
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 15October 24, 2009
Prospects for plasma sustainment and magnet development
• Sustainment and profiles– NBI-CD will be utilized/exploited on NSTX/MAST, HHFW on NSTX– EC/EBW should be developed for ramp-up/sustainment: MAST, QUEST?– Core fueling development also needed if Li-wall concept is successful
• Magnets– Requirements will depend on scale of next-step
• ST-PMIF, BPST (initially) could use OH (BPST ½ swing OH 10MA)• FNST nuclear phase must operate w/o OH – ut what about initial phase?
– CS (and other) shielding requirements for BPST must be determined• Will depend on fluence goal of device
– Could develop single-turn TF in ST-PMIF/BPST if FNST is not next step
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 16October 24, 2009
Other risks and considerations for ST development path
• There is risk in having too narrow a range of operating scenarios for fusion nuclear science/burning plasma goals
• There is risk in designing a device which cannot study or exploit scenarios with very high performance, even if the base device mission does not depend on high performance.
• Above risks motivate re-examination of device optimization– Example: Modest increase in size and/or current could significantly
enhance fusion performance• Might reduce risks in achieving nuclear testing mission of FNSF/CTF• But would increase cost
– Need to explore broader range of operating scenarios• Higher density and higher bootstrap fraction scenarios• What do scenarios with reduced confinement look like?• High confinement likely essential for compact/efficient device
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 17October 24, 2009
0D (XL spreadsheet) model of operating points developed(Similar to C. Neumeyer version developed for ST-CTF/NHTX, but simpler)
• NBI CD efficiency estimated including all trapping and slowing-down effects
– D.F.H. Start et al., Plasma physics, Vol. 22, pp. 303 to 316
• NBI and alpha pressure derived from energy moment of slowing-down f(E)
– T.H. Stix, Plasma Physics, Vol. 14, pp. 367 to 384
e-collisionsi-collisionsEnergy loss rateNormalized current drive efficiency
• Special attention given to NBI-CD and fast-ion (NBI + alpha) pressure contribution
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 18October 24, 2009
Confinement well above ITER scaling very important to achieve attractive FNST with acceptable auxiliary power
Required auxiliary power vs. density, H98
0
10
20
30
40
50
60
70
80
90
100
0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 1.1
Greenwald fraction
NB
I Pow
er [M
W] H98=1
H98=1.3H98=1.5H98=1.8
A=1.7, κ=3.3, R0 = 1.5m, BT=2.4T, IP=9-12MA, ENBI=0.5MeV, ITER-98 H-mode scaling
Peak outboard neutron wall loading = 1MW/m2
Required power not strongly dependent on density for H98 = 1.3-1.5Required power lowest for high H98 = 1.5-1.8 (and achieves high fusion gain)
DT fusion gain vs. density, H98
0
5
10
15
0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 1.1Greenwald fraction
QDT
H98=1H98=1.3H98=1.5H98=1.8
PNBI = 60-90MW required for H98=1 QDT ~ 1 – lower ne requires lowest PNBI
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 19October 24, 2009
Total plasma beta depends weakly on density, but bootstrap fraction and fast-ion content depend strongly on density
Bootstrap and Wfast fractions vs. density, H98
0.00.10.20.30.40.50.60.70.80.91.0
0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 1.1
Greenwald fraction
Frac
tions
H98=1H98=1.3H98=1.5H98=1.8
Peak outboard neutron wall loading = 1MW/m2
Low ne: Good NBI profile control, but strong *AE activity?
A=1.7, κ=3.3, R0 = 1.5m, BT=2.4T, IP=9-12MA, ENBI=0.5MeV, ITER-98 H-mode scaling
High ne: lower *AE activity?, but challenging plasma control (like ST-Demo)?Moderate ne: Acceptable (perhaps optimal) *AE activity + control?
Normalized β vs. density, H98
3.0
3.2
3.4
3.6
3.8
4.0
4.2
4.4
0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 1.1
Greenwald fraction
βNH98=1H98=1.3H98=1.5H98=1.8
Less than 15% variation in total βN with density for H98 > 1.3
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 20October 24, 2009
Higher normalized beta operation enables enhancedneutron wall loading for fusion nuclear science/technology
Current and normalized beta vs. density, Wn
0
5
10
15
20
0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 1.1
Greenwald fraction
I P [M
A] a
nd β
N
Wn = 1MW/m^2Wn = 2MW/m^2Wn = 4MW/m^2
βN depends weakly on density, increases from 4 5 6 for higher wall loading
A=1.7, κ=3.3, R0 = 1.5m, BT=2.4T, ENBI=0.5MeV, ITER-98 H-mode scaling, H98=1.5
Aux power required increases with wall loading at low density, decreases at higher density
Plasma current increases at lower density and higher wall loading
q* ~ 2
Required auxiliary power vs. density, Wn
0
10
20
30
40
50
60
70
0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 1.1
Greenwald fraction
NB
I Pow
er [M
W]
Wn = 1MW/m^2Wn = 2MW/m^2Wn = 4MW/m^2
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 21October 24, 2009
Summary
• Issues, gaps, needs, goals for ST are clearly defined– Major upgrades + world program will narrow many gaps
• Next-step ST should have range of operating scenarios to achieve fusion nuclear science missions– Essential to access and understand very high confinement
•Is high-recycling wall good enough, or will a low recycling be needed?
– Plasma density likely critical parameter in scenario physics•Will impact CD and J(r) control, Alfvénic instabilities, divertor regime•0D studies suggest Greenwald fraction ~0.5-0.6 could be attractive
– High βN = 4 6 could increase neutron wall loading 4-fold•But must be weighed against increased control demands, disruptivity
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 22October 24, 2009
Backup
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 23October 24, 2009
Next STs push well beyond divertor and first-wall heat-loads accessible in present fusion devices
Device heat-flux parameters
BPST (II)
ARIES-ST
DIII-DBPST (I)
NSTX
NSTX-U
FNST (I) / ST-PMIFFNST (II)
ITER
JET (DT)JT-60SA
KSTAR
EAST
ARIES-ATFNST (III)
FNST (IV)
BPST (III)
0.0
0.2
0.4
0.6
0.8
1.0
1.2
1.4
0 50 100 150 200
Pheat / R [MW/m]
Pheat /S[MW/m2]
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 24October 24, 2009
FNST scenarios optimize at high normalized H-mode confinement and reduced density (for NBI-CD)
• BPST/reactor scenarios optimize at somewhat lower H98 and higher densityDevice Density and Confinement
BPST (II)ARIES-ST
JT-60SANSTX
NSTX-U
FNST (I) / ST-PMIFFNST (II)
ITER
ITER-SS
JET (DT)
KSTAR
EAST DIII-D
ARIES-AT
FNST (III)
FNST (IV)
BPST (III)
BPST (I)
0.8
1.0
1.2
1.4
1.6
1.8
0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1.0 1.1Greenwald density fraction
H98(y,2)
H98(y,2)=1
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 25October 24, 2009
FNST and BPST scenarios approach ST reactor ρ*, ν* from complementary directions
Normalized larmor radius and collisionality
BPST (II)
ITER-SS
DIII-D
BPST (I)
NSTX
NSTX-U
FNST (I) / ST-PMIFFNST (II)
ARIES-ST
ITER
JET (DT) JT-60SA
EAST
ARIES-AT
FNST (III)
FNST (IV)
BPST (III)
0.000
0.005
0.010
0.015
0.020
0.001 0.010 0.100 1.000νi*(Collision frequency / bounce frequency - Sauter formula)
ρ*i(thermal)
BPST:Similar ρ*higher ν*
FNST:Higher ρ*similar ν*
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 26October 24, 2009
Confinement and the ST development path• How much would the uncertainty in confinement extrapolation to FNST
and a BPST be reduced by NSTX-U, and by an intermediate step?– We are still working on answering this one…
• How might this impact the choice of device size, auxiliary power, etc.Predicted heating power to achieve target WTOT shows wide variation for next-steps
FNST requires favorable scaling and/or high multiplier to keep Pheat < 100MW
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 27October 24, 2009
Next ST facilities operate with normalizedstability parameters comparable to NSTX/NSTX-U
• But further research needed to sustain high βT~30-40% for BPST (III), FNST (IV)Normalized Pressure vs. Normalized Current
BPST (II)
ARIES-ST
JT-60SADIII-DBPST (I)
NSTXNSTX-U
FNST (I) / ST-PMIF
FNST (II)
ITERITER-SS JET (DT)KSTAR
EAST
ARIES-AT
FNST (III)
FNST (IV)
BPST (III)
0
10
20
30
40
50
0 1 2 3 4 5 6 7
IP / a BT [MA / mT]
βT (%)
NSTX(transienthigh βT)
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 28October 24, 2009
Next STs have disruption thermal quench wallloads extending from JET/JT-60SA to ITER values
Thermal quench average wall load
BPST (II)
DIII-D
BPST (I)
NSTX-U
FNST (I) / ST-PMIF
FNST (II)
ARIES-ST
ITER
JET (DT)
JT-60SA
KSTAR
EAST
ARIES-AT
FNST (III)FNST (IV)
BPST (III)
0.01
0.10
1.00
10.00
1 10 100 1000Wtot [MJ]
Wtot /S[MJ/m2]
• High-QDT BPST (III) would have wall loading above ITER, approaching reactor– Is disruption mitigation developed for/on ITER sufficient for STs?– What is role of liquid walls for disruption survivability?
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 29October 24, 2009
Next STs operate fully non-inductively withcurrent provided by the bootstrap effect + NBI-CD• BPST would utilize scenarios with higher (80-95%) bootstrap fraction
Device bootstrap and non-inductive fractions
JT-60SA
KSTAR
DIII-DNSTXNSTX-U
FNST (I) / ST-PMIF
FNST (II)
BPST (II)ARIES-ST
ITER
ITER-SS
JET (DT)
EAST
ARIES-AT
FNST (III)FNST (IV)
BPST (III)
BPST (I)
0.2
0.4
0.6
0.8
1.0
1.2
0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1.0
Bootstrap Current Fraction
Non
-indu
ctiv
e fr
actio
n (B
S+N
BIC
D)
100% non-inductive CD
NSTX-U
(100% NICD)
Highest valuesachieved
experimentally
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 30October 24, 2009
Next STs have baseline pulse durationsbetween JT60-SA and KSTAR/EAST
• FNST would target extension to much longer pulse durations
NSTX-U
FNST (I) / ST-PMIF
FNST (II)
ITER
JT-60SA
KSTAR
DIII-DNSTX
BPST (II)BPST (I)
JET (DT)
EAST
ITER-SS
BPST (III)
1
10
100
1000
10000
1 10 100 1000 10000 100000Pulse duration [s]
Pulse duration /current redistri-bution time
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 31October 24, 2009
Magnets and the ST development path
• How much single-swing solenoid flux is available for IP ramp-up in a BPST or the break-in phase of an FNST? What are achievable plasma currents?
• Are insulated multi-turn TF/OH coils viable in BPST fusion environment?
• NSST 2-layer OH design: OFHC for outer, BeCu for inner + LN2 cooling– 9T OH field limit combined with NBI + H-mode in ramp-up for lower CEjima
– BPST: OH single-swing to ~10MA (7Wb ½ swing OH) – sufficient for QDT~2– FNST: OH single-swing to ~7MA (4Wb ½ swing OH) – sufficient for QDT~1– Allowable dpa and shielding requirements = work in progress…
• Also still need to address/develop single-turn central TF– BPST could test NI ramp-up to ~10MA – could also test single-turn TF w/o OH?
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 32October 24, 2009
Is an ST-based pilot plant possible?
• Answer: possibly, but would require aggressive approach• Example calculation:
– BPST-III at 15MA, βN = 7, QDT = 10 ~500MW fusion power– Use ARIES-ST power conversion assumptions:
• Total thermal power ~13% above Pfusion, conversion efficiency = 45%• Electricity production = 245MWe (need to recover every Watt!!!)• Estimated total TF power for 2.4T = 330MW• Minimize PF power consumption (assume SC PF coils as for ARIES-ST)• Assuming PAUX = 50MW, 35% wall-plug efficiency 140MWe• TF + auxiliary heating = 470MW QENG ~ 0.5
– BUT, with A=1.6 1.7, BT=2.4T 2.2T, H98 = 1.4 1.7• PAUX = 20MW TF + auxiliary heating ~ 250MW QENG ~ 1• Also reduces mid-plane port space required for auxiliary systems
– Improved confinement, high β critical motivates Li & stability research
• BPST-III is ½ size of ARIES-ST – would larger BPST do better?
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 33October 24, 2009
The ST provides unique contributions to all magnetic fusion research needs – for the ITER era and beyond
High heat flux at small size and cost for PMI R&D
High neutron flux at small size and cost for testing fusion nuclear components
Study multi-mode AE fast-ion transport expected in burning plasma regime
Unique physics: low A, high β,high vfast / vA at low ν*
Theme structure of OFES Research Needs Workshop
(ReNeW) – June 2009
Simplified, maintainable, affordable magnets for DEMO
Long-pulse ST applications expand knowledge-base of high-performance theme
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ST Development PathST Development Path Prospects for Future (Next-step) STs – ISTW 2009 (Menard) 34October 24, 2009
CHI has been coupled to induction and NBI-heated H-modein NSTX with substantial sustained current savings
• Extensive conditioning improved divertor conditions for successful CHI OH coupling– Upper divertor conditioned with NBI-heated USN plasmas – Lower divertor conditioned with sustained CHI plasma– Li evaporation used to reduce oxygen, increase D pumping– CHI voltage duration (absorber arcs) reduced
180kA current savings
• 300kA (or higher) current savings is goal for NSTX
• Should be possible w/ additional improvements
• 400kA needed to absorb 2nd
NBI in NSTX-U• Higher TF expected to
increase IP (CHI) in NSTX-U