Kinetic MHD Simulation in Tokamaks H. Naitou, J.-N. Leboeuf †, H. Nagahara, T. Kobayashi, M. Yagi...
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Transcript of Kinetic MHD Simulation in Tokamaks H. Naitou, J.-N. Leboeuf †, H. Nagahara, T. Kobayashi, M. Yagi...
Kinetic MHD Simulation in Tokamaks
H. Naitou, J.-N. Leboeuf†,
H. Nagahara, T. Kobayashi, M. Yagi‡,T. Matsumoto*, S. Tokuda*
Joint Meeting of US-Japan JIFT Workshop on Theory-Based Modeling and Integrated Simulation of Burning Plasmas and 21COE Workshop on Plasma Theory ------Kyodai-Kaikan, Kyoto, 2003/12/15-17 ------
Yamaguchi University†University of California at Los Angeles
‡Kyushu University
*Japan Atomic Energy Research Institute
Key Words
• Sawtooth Crash• m=1/n=1 Internal Kink Mode • Kinetic MHD Model• Collisionless Magnetic Reconnection• Diamagnetic Effects• Sheared Poloidal Flow of m=1• Kelvin-Helmholtz (K-H) Instability• Vortex Generation
Outline
1. Motivations2. Basic Equations3. Results of Cylindrical Code
(a) Linear Calculations (b) Nonlinear Calculations
4. Toroidal Code (Kinetic-FAR)5. Summary
1. Motivation
• There is no complete theory to explain the sawteeth phenomena in tokamaks without inconsistency.
• Resistive MHD model is not appropriate.• Kinetic MHD model can elucidate (a) fast sawtooth crash. (b) nonlinear acceleration of the growth rate. (c) diamagnetic stabilization.
• Gyrokinetic particle simulation and gyro-reduced-MHD (GRM) simulation have revealed the fast full reconnection followed by the second phase of axis q-value less than unity.
• Linear and nonlinear studies by GRM code. ……… Summarized in this presentation.
• The vortex generation by K-H instability can be a critical issue for the complete understandings of the sawtooth crash.
2. Basic Equations
ezee
zes
ze
z
z
nDAbnbt
n
Anba
Adt
d
a
dbA
t
DAbbt
22*
22*2
22
*
222*22
)(
)( )(
)( )( )(
⊥⊥
⊥⊥⊥
⊥⊥⊥⊥⊥
∇+∇∇⋅−∇⋅φ∇×−=∂∂
∇∇μ−∇⋅⎟⎠
⎞⎜⎝
⎛ρ+∇⎟
⎠
⎞⎜⎝
⎛+φ∇⋅−=∂∂
φ∇∇+∇∇⋅−φ∇∇⋅φ∇×−=φ∇∂∂
∇⋅φ∇×+∂∂
=
×∇+=
) (
*
btdt
d
bAbb z
Safety factor profile :
Equilibrium density profile:
Key Parameters:
Assumption : Single Helicity
12
0 0 ) 1( 4 1 )(
−
⎥⎥⎥
⎦
⎤
⎢⎢⎢
⎣
⎡
⎟⎟⎠
⎞⎜⎜⎝
⎛−−= arqqrq
,85.00=q 125.2)( =aq
⎟⎟
⎠
⎞
⎜⎜
⎝
⎛ −ε−=n
nlrrnrn 0
0 tanh 1 )(
,0.1)5.0( =aq
de / a, ρs / a, εn
m / n = 1
r0/a = 0.5, ln/a = 0.16
(a) Linear Calculations
3. Results of Cylindrical Model
de/a = 0.0005315, ρs/a = 0.002891, 1/0 = 417μsec
Electron Diamagnetic Stabilization of Kinetic Internal Kink Mode
Mode Structure in r-
*e/0 = 1.48 (theoretically unstable)
Mode Structure in r-
*e/0 = 1.98 (theoretically close to marginal point)
Electron and Ion Diamagnetic Effects
de/a = 0.0005315, ρs/a = 0.002891, Ti/Te = 1.0, 1/0 = 340μsec
Mode Structure in r-
A B
(b) Nonlinear Calculations
de = 0.01, ρs = 0.03
0.0
0.5
1.0
0.00 0.50 1.00 1.50 2.00
É÷*e/(2É¡0)
É¡/É¡
0
Linear Growth Rate
QuickTime˛ Ç∆ êLí£ÉvÉçÉOÉâÉÄǙDZÇÃÉsÉNÉ`ÉÉÇ å©ÇÈÇΩÇflÇ…ÇÕïKóvÇ≈Ç∑ÅB
Linear Mode Pattern
Movie of Vortex Generation
Magnetic Field Structure
4. Toroidal Code (Kinetic-FAR)
• Kinetic terms are included.• Can treat realistic equilibrium with shaping, finite
beta, and curvature.• Can directly compare resistive MHD with kinetic
MHD.• Two approaches based on resistive FAR (R-FAR)
code and turbulent FAR (K-FAR) code.
Made cylindrical by keeping only m=0 and n=0 component in Grad-Shafranov toroidal equilibrium and switching off toroidal terms ( e.g. curvature ).
Comparison between GRM and K-FAR
cylindrical model de = 0.01, ρs = 0.03
0
0.002
0.004
0.006
0.008
0.01
0.012
0.014
0 0.2 0.4 0.6 0.8 1
growth rate
GRMK-FAR
εn
0
0.01
0.02
0.03
0.04
0 0.2 0.4 0.6 0.8 1
real frequency
GRMK-FAR
r
εn
Comparison Between GRM and T-FAR
GRM
r
T-FAR
r
z)
Comparison Between R-FAR and T-FAR
K-FAR
r
T-FAR
r
z)
RSTEQ Toroidal Equilibrium
0 25 50 75
75
50
25
0
R
Z
=9.8x10-3
0.8
1
1.2
1.4
1.6
1.8
2
2.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
1.1
0 0.2 0.4 0.6 0.8 1
Safety factor q(r) profile
Pressure P(r) profile
q(r) P(r)
r/a
=a/R=1/3
Comparison between Toroidal and Cylindrical Cases
de = 0.01, ρs = 0.03
0
0.002
0.004
0.006
0.008
0.01
0.012
0.014
0 0.2 0.4 0.6 0.8 1
growth rate
toroidal
cylindrical
εn
0
0.01
0.02
0.03
0.04
0 0.2 0.4 0.6 0.8 1
real frequency
toroidal
cylindrical
r
εn
Preliminary
5. Summary
• We believe that vortex generation due to K-H instability has critical effects on the nonlinear developments of kinetic internal kink modes.
• Comparison with K-H theory is underway. ------------ growth rate, threshold, etc.
• Effects of vortex generation may be important for the complete understandings of sawtooth crash phenomena.
• Kinetic modifications of FAR code are underway to tackle these issues.