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NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A. Sabbagh 1 / S.P. Gerhardt 2 1 Department of Applied Physics, Columbia University, New York, NY, USA 2 Plasma Physics Laboratory, Princeton University, Princeton, NJ, USA For the NSTX Macroscopic Stability Topical Science Group 12th Meeting of the ITPA MHD Stability Topical Group October 20-22, 2008 CRPP, Lausanne, Switzerland Supported by Office of Science Culham Sci Ctr U St. Andrews York U Chubu U Fukui U Hiroshima U Hyogo U Kyoto U Kyushu U Kyushu Tokai U NIFS Niigata U U Tokyo JAEA Hebrew U Ioffe Inst RRC Kurchatov Inst TRINITI KBSI KAIST ENEA, Frascati CEA, Cadarache IPP, Jülich IPP, Garching ASCR, Czech Rep U Quebec College W&M Colorado Sch Mines Columbia U Comp-X General Atomics INEL Johns Hopkins U LANL LLNL Lodestar MIT Nova Photonics New York U Old Dominion U ORNL PPPL PSI Princeton U SNL Think Tank, Inc. UC Davis UC Irvine UCLA UCSD U Colorado U Maryland U Rochester U Washington U Wisconsin v1.4

NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

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Page 1: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1

Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX

S.A. Sabbagh1 / S.P. Gerhardt2

1Department of Applied Physics, Columbia University, New York, NY, USA2Plasma Physics Laboratory, Princeton University, Princeton, NJ, USA

For the

NSTX Macroscopic Stability Topical Science Group

12th Meeting of the ITPA MHD Stability Topical Group

October 20-22, 2008

CRPP, Lausanne, Switzerland

Supported byOffice ofScience

Culham Sci CtrU St. Andrews

York UChubu UFukui U

Hiroshima UHyogo UKyoto U

Kyushu UKyushu Tokai U

NIFSNiigata UU Tokyo

JAEAHebrew UIoffe Inst

RRC Kurchatov InstTRINITI

KBSIKAIST

ENEA, FrascatiCEA, Cadarache

IPP, JülichIPP, Garching

ASCR, Czech RepU Quebec

College W&MColorado Sch MinesColumbia UComp-XGeneral AtomicsINELJohns Hopkins ULANLLLNLLodestarMITNova PhotonicsNew York UOld Dominion UORNLPPPLPSIPrinceton USNLThink Tank, Inc.UC DavisUC IrvineUCLAUCSDU ColoradoU MarylandU RochesterU WashingtonU Wisconsin

v1.4

Page 2: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 2

Examining disruption eddy currents, halo currents, and Ip current quench in the spherical torus

Goals Provide electromagnetic loading data for future ST design Examine ST specific characteristics to enhance tokamak knowledge base

Considerations High elongation more subject to n = 0 instability during vertical motion (VDE)

• General issue: disruption IP quench drives eddy currents (IC) in nearby conducting structures (C); currents lead to significant JxB forces on in-vessel components

c (LC/RC time) long: total flux change matters

c short: instantaneous flux change matters

• Strong 1/R Bt variation in ST makes center column halo currents a large concern

Halo currents can flow linking the plasma and in-vessel components when plasma comes in contact with plasma facing components

• Currents are parallel to B in the plasma edge; distributed to vessel based on inductance/resistance

Disruptions are faster in the ST vs. conventional aspect ratio

• Expand studies to wider range of disruption conditions/plasma parameters

dICdt

IC c

1

LC

ddt

Page 3: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 3

Disruptions analyzed over a wide range of plasma conditions

Disruption database Greater than 900 shots, covering all operational regimes

Select shots with fast current quenches, large halo currents

Maximum halo current in all measured paths, current quench characteristics

XP833 IP & BT Range

Dedicated experiment in 2008 Triggered VDEs

IP and BT scans at fixed shape, NBI power

Detailed tracking of vertical motion More accurate characterizations than in

large database analysis

Page 4: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 4

New measurements allow study of additional halo current paths

Two Pearson current transducers on CHI Bus

Current from inner to outer vessel

Rogowskis on the Center Stack Casing (CSC)CSCL1, CSCL2, CSCU1

No Midplane Measurements

Two Arrays of 6 BT coils

Inner Ring: Just Outside the CHI GapOuter Ring: Just Outside the OBD

Difference Between These: Current into the OBD

New For 2008

Page 5: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 5

Downward Going Disruption With Large Halo Currents

Shot 129449Downward Going VDE

(PF3 Voltage Freeze + Offset)Current Flows OUT of Divertor Plate

Current flow directed to conserve

flux

Typical Pattern for Dedicated VDE Experiment

PF3 coil

PF3 coil

Page 6: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 6

More Limited Measurements for Upward Going VDE

Shot 129512Upward Going VDE

Leads to Largest Center Stack Casing Currents

Current flow directed to conserve

flux

Page 7: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 7

Halo Currents In Vessel Bottom Scale as IP/q, Consistent With Simple Models

(Quantities measured just before VDE begins) : He, High-, PNBI=0MW: He, low-, PNBI=0MW: D2, low-, PNBI=2MW: D2, low-, PNBI=0MW

Simple explanation of scaling Ip: Halo currents increase with Ip

q: halo currents flow parallel to B, poloidal component increases if q decreases

Scaling coefficient independent of working gas, PNBI, shape

(P.J. Knight, et al., Nucl. Fusion 40 (2000) 325.)

Page 8: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 8

Vessel Bottom Currents Largest in Triggered VDE Experiments

Solid Symbols: Deliberate VDEs (XP833 & XP811), Open Symbols: All Others

Vessel Bottom, IHC vs IP2/BT~IP/q

Upward Going VDEs, IHC,IR,Max~60 kA

Downward VDEs,IHC,IR,Max IP

2/BT

Lower PF1A Transition, IHC vs IP2/BT

Upward Going VDEs, IHC,CSCU1,Max~60 kA

Downward VDEs,IHC,CSCU1,Max25kA

Simplified conclusion Upward VDEs: 60 kA max center stack casing current, no observed scaling

with IP2/BT, IP/BT, or IP

Downward VDEs: IP2/BT scaling for currents into outboard divertor

Page 9: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 9

Toroidal Peaking Factor Decreases With Halo Current Fraction

TPF 10.07

HCF

TPF 0.75

HCF

Inner Ring, TPF vs. HCF

Toroidal peaking factor TPF = 6*max(Bi=1:6) / Bi Uncertainty larger at small halo current fraction (HCF)

ITER Assumption: TPFHCF < 0.75 NSTX Data Well Below This Scaling

Page 10: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 10

Fastest NSTX disruption quench times of 0.4 ms/m2, compared to ITER recommended minimum of 1.7 ms/m2

Reduced inductance at high-, low-A explains difference

Current Quench Rates Are Fast in the ST

QR(80 20) .6* IPDt20 t80

Average Quench Rate:

Maximum Quench Rates/Average Quench Rate vs. Average QR

Maximum quench rates often larger than average quench rates

Issue for components with short L/R time

Are

a N

orm

aliz

ed Q

uenc

h T

ime

(mse

c/m

2)

Pre-Disruption Current Density (MA/m2)

L / R

S

0

2ln 8

7

4

Area-normalized (left), Area and Lext-normalized (right) Ip quench time vs. toroidal Jp (ITER DB)

NSTX

Past ITPA result

Page 11: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 11

Quench rate important in determining the eddy current drive

dB/dt at Lower outboard divertor Points sorted by the axis vertical

position just before the disruption Ip-normalized dB/dt increases

with quench rate Scatter in data due to details of

plasma motion and shape

Page 12: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 12

Geometry and plasma motion affects local field variation

Mean(dB/dt)/IP vs Lower TriangularityOutboard Divertor

(Max and min)(dB/dt)/IP vs (dIP/dt)max

Outboard Divertor

At low , Shaping field coil current attracts plasma toward sensor coil during VDE

maximizes measured dB/dt

Same result for upward-going VDE and upper sensor coil

Large positive values due to large values of dIp/dt during quench

Large negative values due to rapid downward plasma motion (~constant Ip)

Current quench effect is dominant, but only factor 2 larger

Page 13: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 13

Mitigation by CT injection may have a number of advantages

The injected compact torus (CT) moves quickly Slowest step in CT mitigation is gas-puffing into the

injector (~200 s). Bias flux can be provided by permanent magnet

By coordinating MGI and CT timing, core cooling could be precisely controlled

The CT species and velocity can be varied to tailor the penetration depth

Could reduce the total amount of injected gas from the MGI system, making recovery easier

It might also allow for tailoring the shut-down to avoid the “hot-tail” runaways which are common with pellets

Further advantages if the CT system is operated in a Marshall Gun mode? A long trailing plasma containing significant neutrals and at amounts >100 times more

than the mass of a single CT can be injected These neutrals would have much higher velocity than what is possible by MGI alone

and would penetrate on a faster time scale

R. RamanU. Washington

Page 14: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 14

Halo currents, eddy currents, and current quench rates investigated in ST geometry

Large database relevant to disruption EM loading

Halo currents up 150kA measured with new diagnostics, IP/q95 scaling, in outboard divertor

Halo currents up to 60 kA, and no observed scaling, on center stack casing

Fastest IP quenches of 1GA/s, with instantaneous rates often much faster than the average

Current quench rate, plasma geometry, plasma motion important in determining the local eddy current drive

Planned for Next Run Campaign• Toroidally extended halo current measurements into four liquid lithium divertor

(LLD) sectors• Toroidally localized halo current measurements at four positions at LLD

• Fast (> 1.5 kHz) IR thermography for thermal quench studies

Page 15: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 15

Backup slides follow

Page 16: NSTX 12 th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 1 Halo Current and Current Quench Rate Characteristics During Disruptions in NSTX S.A

NSTX 12th ITPA MHD Meeting 10-2008 – S.A. Sabbagh/S.P. Gerhardt 16

NSTX Disruption Studies Contribute to ITER, Aim to Predict Disruption Characteristics & Onset For Future Large STs

Halo Current Magnitudes and Scaling

Expand Results For a Complete Characterization of Disruption Dynamics, Including Prediction Methods

IP2 BT (MA2/T)

Max

Hal

o C

urre

nt M

agni

tude

(kA

)

Lower Center StackInner to Outer Vessel

Vessel Bottom Near CHI Gap

Outboard Divertor

Are

a N

orm

aliz

ed Q

uenc

h T

ime

(mse

c/m

2)

Pre-Disruption Current Density (MA/m2)

• Fastest NSTX disruption quench times of 0.4 ms/m2, compared to ITER recommended minimum of 1.7 msec/m2

• Reduced inductance at high-, low-A explains difference

L / R

S

0

2ln 8

7

4

• New instrumentation in 2008 yields significant upward revision of halo current fractions (now up to 20%)

• reveals scaling with IP and BT

• Mitigating effect: Largest currents for deliberate VDEs• Toroidal peaking reduced at large halo current fraction

2006 Instrumentation 2008 Instrumentation

Area-normalized (left), Area and Lext-normalized (right) Ip quench time vs. toroidal Jp (ITER DB)

NSTX