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Page 1: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Kansas Annual NSF EPSCoR Statewide ConferenceWichita, KS January 12-13, 2012

Simulation of pellet ablation in DIII-D

Tianshi Lu

Patrick RinkerDepartment of Mathematics

Wichita State University

In collaboration with

Roman Samulyak, Stony Brook University

Paul Parks, General Atomics

Page 2: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Model for pellet ablation in tokamak

• MHD system at low ReM

• Explicit discretization• EOS for partially ionized gas• Free surface flow• System size ~ cm, grid size ~ 0.1 mm

Courtesy of Ravi Samtaney, PPPL

Tokamak (ITER) Fueling

• Fuel pellet ablation• Striation instabilities• Killer pellet / gas ball for

plasma disruption mitigation

Page 3: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Schematic of pellet ablation in a magnetic field

Schematic of processes in the ablation cloud

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Cloud Plasma

Sheath boundary

(z)

Sheath Fluxes

Page 4: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

MHD at low magnetic Reynolds numbers

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Equation of state for partially ionized gas

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')',(),( , ')',(),(

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Heat deposition of hot electron

Page 5: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Axisymmetric MHD with low ReM approximation

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Centripetal force

Nonlinear mixedDirichlet-Neumann boundary condition

Page 6: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Transient radial current approximation

2),(),( ,)()( ,38.1

2)

221(),(),(

)exp( ),erfc()1( ,

)1( :conditionty Ambipolari

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r,z) depends explicitly on the line-by-line cloud opacity u.

Page 7: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

1.Spherical model• Excellent agreement with NGS model

2.Axisymmetric pure hydro model• Geometric effect found to be minor (Reduction by 18% rather than 50%)

3.Plasma shielding without rotation• Subsonic ablation flow everywhere in the channel• Ablation rate depending on the ramp-up time

4.Cloud charging and rotation• Supersonic rotation causes wider channel and faster ablation• Ablation rate independent of the ramp-up time

Simulation results of pellet ablation

Spherical model Axis. hydro model Plasma shielding

Page 8: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Plasma shielding without rotation

Mach number distribution

Double transonic flow evolves to subsonic flow

st 3

st 5

st 9

cm152T20

keV2cm10

mm2

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314

0

LB

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R

w

e

e

p

Page 9: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

-.-.- tw = 5 s, ne = 1.6 1013 cm-3

___ tw = 10 s, ne = 1014 cm-3

----- tw = 10 s, ne = 1.6 1013 cm-3

Formation of the ablation channel and ablation rate strongly depends on plasma pedestal properties and pellet velocity.

Plasma shielding without rotation

Page 10: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Supersonic rotation of the ablation channel

Cloud charging and rotation

Isosurfaces of the rotational Mach number in the pellet ablation flow

Density redistribution in the ablation channel

Steady-state pressure distribution in the widened ablation channel

2TB

Page 11: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

• Gsteady of a rotating cloud is independent of tramp

• G(tramp) < Gsteady

• G(tramp) increases with tramp

• Fast pellet

• Short ramp-up distance

Fixed pellet: effect of ramp up time

Page 12: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Shrinking pellet: tumbling pellet model

“Pancake” pellet

• Due to anisotropic heating, the pellet would evolve to a pancake shape.

• In reality, the pellet is tumbling as it enters the tokamak, so its shape remains approximately spherical.

• In the simulation, the pellet shrinking velocity is averaged over the surface to maintain the spherical shape.

Tumbling spherical pellet

Page 13: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Shrinking pellet: DIII-D temperature profile

DIII-D Temperature and Density Profile G from simulation agrees with 0.8 GNGS

Page 14: Kansas Annual  NSF  EPSCoR  Statewide  Conference Wichita, KSJanuary 12-13, 2012

Conclusions and future work

Conclusions

• Supersonic rotation causes wider channel and faster ablation• Good agreement with NGS model for DIII-D profile • Smaller Ablation rate during fast ramp-up

Future work

• Inclusion of grad-B drift in the simulation• Non-transient radial current for smaller B field – finite spin up• Mechanism of striation


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