Loads due to disruptions and prospects for mitigation
Transcript of Loads due to disruptions and prospects for mitigation
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
© 2019 ITER Organization
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Loads due to disruptions and
prospects for mitigation
M. Lehnen
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
© 2019 ITER Organization
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‘Damage’ limits are very low compared to what the target plasma
parameters are (already the case in ITER)
Disruption Mitigation can prevent damage during low
performance commissioning
Disruption Mitigation cannot prevent damage above certain
energies and especially not at those of the target scenario
The DEMO design has to take into account the need for
virtually 0 disruptions at target plasma
Main messages
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
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Melt limit: 𝑡𝑇𝑄~𝑅; 𝐴~𝑅𝜆; Δ𝑇 ~𝐸𝑡ℎ𝑒𝑟𝑚𝑎𝑙/𝐴 𝑡𝑇𝑄 𝐸𝑚𝑒𝑙𝑡~𝑅3/2
Beryllium
Tungsten
up to 350 MJ
Disruption Loads and Load Limits Thermal Energy
𝐸𝑡ℎ𝑒𝑟𝑚𝑎𝑙~𝑅5
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
© 2019 ITER Organization
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Disruption Loads and Load Limits Magnetic Energy
𝑃𝑟𝑎𝑑 ≪ 𝑃𝑐𝑜𝑛𝑑
Melt limit: 𝑡𝑣𝑒𝑟𝑡𝑖𝑐𝑎𝑙~𝑅2; 𝐴~𝑅𝜆; Δ𝑇 ~𝐸𝑡ℎ𝑒𝑟𝑚𝑎𝑙/𝐴 𝑡𝑇𝑄 𝐸𝑚𝑒𝑙𝑡~𝑅
2
𝐸𝑚𝑎𝑔𝑝𝑜𝑙
~𝐵𝑡2𝑅3
Assumption for ITER & DEMO: tVV > tCQ
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
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Disruption Loads and Load Limits Magnetic EnergyITER 5 MA , 1.8 T scenario*
Halo current density: 20 kA/m2
*scaled from 15 MA
t [ms] 275 325 375 425
DE [MJ] 5 14 19 18
lq [mm] 32 41 53 82
Total: 56 MJ
Coburn+ PhysScr 2019
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
© 2019 ITER Organization
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Disruption Loads and Load Limits EM loads
𝐼ℎ𝑎𝑙𝑜
FzBt
Impact of EM loads is very much
design dependent
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
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Bt
Mz
dB/dt𝐼𝑒𝑑𝑑𝑦
dB/dt dIP/dt
Disruption Loads and Load Limits EM loads
Impact of EM loads is very much
design dependent
Moment on blanket modules limits allowable current decay rates in ITER
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
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Disruption Loads and Load Limits asymmetric VDEs
Rotation frequency of
asymmetric VDEs can be in
the resonance range in ITER
Amplification factors of 10 after
2-3 rotations can be expected
Physics understanding and
model validation is still ongoing3D MHD models, sink & source model,
eddy current driven model
Myers+ NF 2018
Critical question:
How does the force amplitude scale with rotation?
Dedicated experiments with special divertor tiles in
COMPASS were performed last week for model validation
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
© 2019 ITER Organization
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Mitigation of heat loads and electro-magnetic forces ITER
Injection of high-Z impurities
Dissipate thermal and magnetic energy through photonic radiation
Shattered Pellet Injection
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
© 2019 ITER Organization
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Parameter Space for loads and mitigation ITER
ITER requires mitigation from
the first campaign onward
Limits for Eth are based on more
detailed calculations; Limits for
Emag is a first estimate
High radiation fractions for
magnetic energy on timescales
of 100 ms are possible (exp’s,
modelling)
High radiation fractions for
thermal energy are not confirmed
yet (complexity of the thermal
quench)
EM load mitigation requirement
from worst case halo current
(aVDEs not accounted for)
Lehnen+ IAEA 2014
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
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Limits on thermal load mitigation
JOREK
Ne/D2 SPI
single injection
ITER L-mode
D. Hu, ITPA MHD April 2019
Radiation flash can cause surface melting / recrystallization
Energy limits assuming a peaking of 4 (TPF = PPF = 2)
ITER: 70 MJ (SS) and 150 MJ (Be)
DEMO: 200-400 / 450-900 MJ (W recryst./melt) [R = 7.5-9.5 m]
*
* Injection plume extends toroidally over 120 deg
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
© 2019 ITER Organization
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Parameter Space for loads and mitigation DEMO
Limits are based on simple
scalings shown earlier
High radiation fractions for
magnetic energy on timescales
of 100 ms are possible (exp’s,
modelling)
High radiation fractions for
thermal energy are not confirmed
yet (complexity of the thermal
quench)
Peaking of radiation is uncertain
EM load limits depend on VV and
in-vessel component design
(aVDEs not accounted for)
Recrystallisation threshold for DT = 1400 and PF = 4
Energy at L-H transition for EU DEMO 1 (R=9.1m, IP = 19.6 MA) [Wenninger+, NF 2017] and
using L-mode scalings [Kaye+, NF 97 and Martin J.Physics 2008]
R = 7.5 – 9.5 m
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
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Disruption Loads and Load Limits Runaway electrons
RE free disruptionswith Be wall in JET
9.5 MA
Maximum initial runaway population (IRE < 0.1 MA)
105
109
Runaway seed sources
• Dreicer
• Hot tail
• T decay
• Compton scattering
Avalanche amplification
increases exponentially
with plasma current
Highly conductive VV
can mitigate to some
extent
Main source during non-active phase in ITER
Possible sources during active phase in ITER
Main sources in DEMO?
No strong contribution in ITER
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
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Disruption Loads and Load Limits Runaway electrons
MEMOS: Temperature distribution
ENDEP: Energy distribution in FW panelLpoloidal = 100 mm, Dr = 2 mm, <ERE> = 15 MeV, Etot = 1.75 MJ, Dt = 100ms (Emag conversion)
Melt threshold estimate (ITER)
~0.3 MJ / FW panel (Be)
~0.3 MJ / divertor cassette (W)
Corresponding to IP @ TQ of
~0.5 MA (deposition on single PFC)
~3-8 MA (uniformly distributed)
Variation due to different impact time
Energy distribution depends on
• Misalignment of PFCs
• Kink mode that causes RE loss
not yet quantified
Water leaks are likely for significant RE currentLehnen+ IAEA 2016
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
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Runaway electron avoidance ITER
mo
re d
eute
riu
m
Quantities from simple models
MHD and assimilation will matter
RE avoidance presently based
on massive D2 (H2) injection
JOREK D2 SPI simulation for JETHu+ NF 2018Martín-Solís+ NF2017
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Michael Lehnen – 6th IAEA DEMO Programme Workshop – 1-4 October 2019
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Runaway electron energy dissipation ITER
Presently foreseen as a second layer of defense
in ITER in case of accidental RE generation
Runaway current decays as expected with impurity
quantity for modest injections in experiments
But there are substantial issues:
• Significant current carried by RE at the final loss
[e.g. Hollmann+, NF 2019; Reux+, NF 2015]
in ITER (twall > tCQ): Z = f(IRE)
• Scraping-off effect could lead to early RE energy
deposition [Konovalov+, IAEA 2014]
• Limited fuelling efficiency
o Pellets are not better than MGI (in this
respect) [Shiraki+, NF2018]
o Slow particle transport times prevent fast
penetration [Hollmann+, NF2019]Hollmann+ NF 2019
DIII-D
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Runaway electron mitigation
Alternative schemes for mitigating RE other than material injection
Boozer NF2018
Can passive structures
in the first wall produce
long-wavelength
non-axisymmetric
perturbations?
Stochastisation
External coils?
ITER in-vessel perturbation coils
with n=3 cannot remove all REs
Papp+ IAEA2012
Passive structure?
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Runaway electron mitigation
Alternative schemes for mitigating RE other than material injection
Carnevale+ PPCF2019
Possible on present
tokamaks, example here: FTU
RE beam position control
Enables applying other techniques that require longer timescale
Position control only possible under
special conditions in ITER
(plasma to be moved to the neutral point)
Lukash+ EPS2013
0,4
0,6
0,8
1dI
p/dt,MA/s
9,5 10 10,5 11 11,5 12
Ire max
,MAcontrolled
not controlled
(a)
250
300
350
400
9,5 10 10,5 11 11,5 12
tloss min
,mscontrolled
not controlled
(b)
IRE,max [MA]
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Runaway electron mitigation
Alternative schemes for mitigating RE other than material injection
Lvovskiy+ PPCF2018
Kinetic instabilities and
RE formation in DIII-D
RE-wave interaction
Kinetic instabilities may…
…help dissipating RE energyPlasma parameters in RE plateau result in
low growth rates D2 injection may help
Aleynikov+ NF2015 / Paz-Soldan+ IAEA 2018
…prevent RE formation
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Shattered Pellet Injection
24 flight tubes in 3 equatorial ports + 3 barrels in 3 upper ports
Each pellet D = 28.5 mm and L = 57 mm
Each flight tube of D 60 mm with a shatter bend at the end
Present design of the ITER Disruption Mitigation System
SPI cryostat
(prismatic)
Cold head
Propellant
gas recovery
Optical pellet
diagnostic
Double
bellows
Pellet
shatter exit
segment
Vacuum
valve
Flyerplate
propellant
valve
x1 SPI Injector
Pellet
guide tube
Torus
vacuum
boundary
Diagnostic
first wall
(Plasma
facing
Component)
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ITER Shatter Pellet Injection Quantities
13 mm20 mm
17 mm
28 mm
Required assimilated quantities based on present knowledge
Quantity Species Purpose Minimum # of pellets
6x1024 D RE avoidance 3
~1025 Ar RE energy dissipation 11
5x1021 Ne EM loads
Mixed into D pellets5x1021 Ne CQ heat loads
4x1022 Ne TQ heat loads
Significant uncertainties on RE avoidance and energy dissipation!
Minimum required number of pellets for 100% assimilation and without redundancy
Multiple injection effective? experiments at DIII-D, KSTAR + Modelling
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ITER Shatter Pellet Injection Reaction time
13 mm20 mm
17 mm
28 mm
Overall reaction time includes:
• Delay from trigger decision to trigger arrival at the PS
• Valve opening and gas release
• Pellet acceleration + flight time
Length of flight tube in the equatorial ports: 6.3 m
He propellant
m [g] v [m/s] Dtflight [ms]
Argon 60 ~200 32
Deuterium 7 ~600 11
Hydrogen 3.5 ~800 8
Estimate of flight time
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Injection techniques
Pros
MGI Fast response if located close to
plasma
Inefficient for long delivery tubes
No direct fueling of plasma core
SPI Efficient delivery of material for
long flight tubes
Potential to fuel plasma core more
efficiently
Restricted to cryogenic pellets
Statistical fragment size distribution
could possibly not fulfil requirements
Massive multiple injection could be
ineffective
EPI* Possibility of injecting non-
cryogenic material
High velocities
Not yet explored on a tokamak
Requires sabot recovery system
Shell
Pellet
Can deliver material to plasma
core
Possibility of injecting non-
cryogenic material
Shell lifetime needs to be adjusted to
plasma parameters to guarantee core
deposition
Cons
*Electromagnetic particle injector
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Triggering the mitigation system
Trigger system to run independently of any other exception handling tools
Physics based approaches focused so far on mode lock and needs to be
further developed
AI approaches require learning and so far lack sufficient portability, but
can inform how to improve physics based schemes
Post-TQ detection has higher
success rate than pre-TQ
prediction (important for high
current operation)
DEMO: Which measurements
can contribute to the disruption
prediction scheme and what
prediction times are achievable?
Esquembri+, IEEE 2018
SPAD - Mode lock anomaly detector
Achievable success rates and
warning times in JET (ILW)
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Disruption Management
Disruption Mitigation is required from early operation onward.
The number of unmitigated disruptions is controlled by containing disruptivity (disruption avoidance) and maximising the mitigation success rate (disruption prediction and system reliability).
How many unmitigated and mitigated disruptions are acceptable at what energy and current?
The Disruption Budget Consumption is introduced as a lifetime consumption indicator.
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Disruption Budget
Based on pre-2017 ITER research plan
Lehnen+ IAEA 2016
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Based on pre-2017 ITER research plan
Disruption Budget
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Conservative assumption: unmitigated disruptions at high current always generate high halo currents
Based on pre-2017 ITER research plan
Disruption Budget
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Based on pre-2017 ITER research plan
Mitigation is load reduction, but not load avoidance!
Here: photonic radiation flash
Disruption Budget
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Based on pre-2017 ITER research plan
Disruption Budget
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Disruption rate and mitigation targets
Based on pre-2017 ITER research plan
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Based on pre-2017 ITER research plan
Disruption rate and mitigation targets
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Based on pre-2017 ITER research plan
Lifetime consumption
Disruption rate and mitigation targets
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Mitigation will be required at still low energies and currents
Mitigation at energies still far away from targets exceeds critical temperatures
RE avoidance at high current is not yet confirmed (even stronger avalanche
multiplication than in ITER)
Alternative mitigation methods for RE can still be taken into account
Prospects for Mitigating Disruptions in DEMO
Disruption Mitigation in ITER
Mitigation will be required at still low energies and currents
High confidence in mitigation of thermal and EM loads through particle injection
Mitigation at high energies is likely to exceed critical temperatures
RE avoidance at high current is not yet confirmed
Effectiveness of particle injection for RE energy dissipation questionable
Conclusions
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ITER is the Nuclear Facility INB no. 174.
The views and opinions expressed herein do not necessarily reflect those of the
ITER Organization.
This publication is provided for scientific purposes only. Its contents should not be
considered as commitments from the ITER Organization as a nuclear operator in
the frame of the licensing process.
Disclaimer