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Intermittent Transport and Relaxation Oscillations of Nonlinear Reduced Models
for Fusion Plasmas
S. Hamaguchi,1 K. Takeda,2 A. Bierwage,2 S. Tsurimaki,2 H. Sato,2 T. Unemura,2 S. Benkadda, 3 and M. Wakatani2
1Osaka University, Japan 2Kyoto University, Japan
3CNRS/Université de Provence, France
Dedicated to Prof. Masahiro Wakatani
Outline
• Intermittent Thermal Transport due to ITG turbulence– a low degree-of-freedom model: how low can it
be?– full PDE
• Intermittent Particle Transport due to resistive drift turbulence
Toroidal ITG Equations
where
Toroidal ITG mode is described by the following equations, W. Horton, D-I. Choi and W. Tang, Phys. Fluids 24, 1077 (1981)
2 2 2 2 2
2
, 1 ,
, ,
1 , ln ln
i
i
i i i e i n Ti i i
pg K g
t y y
p p K pt y
K T T L L d T d n
iK
: electrostatic potential (fluctuation)
: ion temperature gradient
: viscosity
p
g
: ion pressure (fluctuation)
: effective gravity
: thermal conductivity
Low Degree-of-Freedom Model with 18 ODEs
Low-order modes in a slab geometry
If are neglected, the above model agrees with the 11 ODE model by G. Hu and W. Horton [Phys. Plasmas 4, 3262 (1997)]
, , , ,,0 03 3c s c sp
c c
s s
c
c
s
x x
x y x y
x y x y
x x
x y
x
x
x
x y
x y t t k x t k x
t k x k y t k x k y
t k x k y t k x k y
p x y t p t k x p t k x
p t k x
t k x
t k x k y
t k x k y
p t k x
0 01 2
1 2
1 2
0 01
0
2
1
3
3
3
03
, , sin sin 2
sin cos sin 2 cos
sin sin s
sin 3
sin 3 cos
sin 3 sinin 2 sin ,
, , sin sin 2 3
sin
sin
c
s ss
cx y
x
y x
y
y
x y x y
p t k x k y
p t k
k y p t k x k y
p t k x k y p t k y x k yx k
3
2 3
2
1
cos sin 2 cos
si
sin 3 cos
sin sin si n 3 sin 2 nsin .
Characteristic quantities
0 11 x Vx
i
pvdpNu pv dV
dx K
,x y y x yR y
y R
S v v dy L v v
v x St x
The mean velocity is driven by the Reynolds stress SR.
Nusselt number Nu :
Periodic Oscillation
(a)Phase space‘K0-Nu’ and
(b)Power spectrum of K1.
Time evolutions of (a)kinetic energy K and(b)Nusselt number Nufor Ki=0.4.A periodic oscillation
appears.
Chaotic Oscillations
(a)Phase space‘K0-Nu’ and
(b)Power spectrum of K1.
Time evolutions of (a)kinetic energy K and(b)Nusselt number Nufor Ki=0.6.Chaotic oscillations
appear.
Intermittent Bursts
Time evolution of kinetic energy for Ki=4.Intermittent bursts occur.
Time evolution of(a)Nusselt number Nu(b)Reynolds stress SR
Nu and SR burst when the ITG
modes grow rapidly.
Intermittent Transport: 3 Steps
1. Turbulence generates a mean flow through Reynolds stress.
2. The mean flow suppresses instability.
3. The mean flow becomes weak due to viscous damping.
Scaling Law-18 ODEs
3Nu Ki
Transition of transport scaling due to intermittency.
Dependence of the time averaged Nusselt number on the ion temperature gradient is expressed as
Intermittent oscillationsin full PDE model
Time evolutions of kinetic energy K (left) and Nusselt number Nu (right) for Ki=5. Intermittent oscillations appear.
Scaling law—full PDE simulation
Mode structures in the radial direction that are essential for the formation of intermittency
1. Low degree ODE models (18 ODE)
2. ITG (PDE): Transport scaling:
3. Resistive drift (PDE) : Transport scaling:
Summary
1/ 3Nu Ki
Velocity-Space Structures Velocity-Space Structures of Distribution Function in of Distribution Function in Toroidal Ion Temperature Toroidal Ion Temperature
Gradient TurbulenceGradient Turbulence
T.-H. Watanabe and H. SugamaT.-H. Watanabe and H. SugamaNational Institute for Fusion Science/National Institute for Fusion Science/
The Graduate University for Advanced StudiesThe Graduate University for Advanced Studies
MotivationMotivation How are the velocity-space structures How are the velocity-space structures
of of ff associated with turbulent associated with turbulent transport and zonal flows ?transport and zonal flows ? Kinetics of the zonal flow and GAMKinetics of the zonal flow and GAM Structures of Structures of ff providing the steady ITG providing the steady ITG
turbulent transportturbulent transportfocusing onfocusing on entropy balanceentropy balance and and generation of fine-scale structuresgeneration of fine-scale structures of of f f through the phase mixingthrough the phase mixing..=> Gyrokinetic-Vlasov simulation of => Gyrokinetic-Vlasov simulation of ff in in multi-dimensional phase-space with high multi-dimensional phase-space with high resolution (Flux tube configuration is resolution (Flux tube configuration is employed).employed).
Entropy Balance in the Entropy Balance in the Toroidal ITG SystemToroidal ITG System
dG
dt
d
dtS W iQi Di
S 1
2d3v ˜ f k
2FM
k
W 1
21 0
Ti
Te
k
2 Ti
Te
k
2ky ,0
k
Qi 1
2 ikyk d3vv 2J0
˜ f kk
Di d3v k ˜ f k
FM
C ˜ f k
k
(Entropy Variable)
(Potential Energy)
(Heat Transport Flux)
(Collisional Dissipation)
Steady State v.s. Steady State v.s. Quasi-steady StateQuasi-steady State
In the quasi-steady In the quasi-steady state for the state for the collisionlesscollisionless case, case,
S
time
d
dtS iQi
S
time
iQi Di
The two limiting states of turbulence have The two limiting states of turbulence have been extensively investigated by the slab ITG been extensively investigated by the slab ITG
simulations. simulations. (Watanabe & Sugama, PoP (Watanabe & Sugama, PoP 99, 2002 & PoP , 2002 & PoP 1111, ,
2004)2004) In the steady state for In the steady state for
the the weakly collisionalweakly collisional case,case,
Collisionless Damping of Collisionless Damping of Zonal Flow and GAMZonal Flow and GAM
Initial value problem for Initial value problem for n=n=0 mode with 0 mode with ff||tt=0=0=F=FMM
The residual zonal flow The residual zonal flow level agrees with level agrees with Rosenbluth & Hinton Rosenbluth & Hinton theory.theory.
What is the velocity-What is the velocity-space structure of space structure of ff ? ?
How is the entropy How is the entropy balance satisfied ?balance satisfied ?
kxt
kxt 0
1
11.6q2 1/ 2
Cyclone DIII-D base case
Conservation Law for the Conservation Law for the Zonal Flow (Zonal Flow (n=n=0) 0)
ComponentsComponents From the gyrokinetic From the gyrokinetic
equation for equation for kkyy=0,=0,
… … Subset of the Subset of the entropy balance entropy balance equationequation
dG
dt
d
dtSkx
Wkx 0
S d3v ˜ f kx
22FM
W 1
21 0(k 2) Ti
Te
kx
2 Ti
2Te
kx
2Entropy variable Entropy variable S increases S increases during the zonal during the zonal flow damping.flow damping.
Velocity-Space Velocity-Space Structures of Structures of ff in the in the Zonal Flow DampingZonal Flow Damping
Decrease of Decrease of WWkxkx with the invariant with the invariant G G means means increase of increase of SSkx kx as well as generation of as well as generation of fine-scale structures of fine-scale structures of ff due to phase due to phase mixing by passing particles mixing by passing particles <=><=> Entropy Entropy transfer in the transfer in the vv-space-space
Coherent structures for trapped particlesCoherent structures for trapped particles <=> <=> Neoclassical PolarizationNeoclassical Polarization
(2(2
vv////
passing
trapped Bounced Averaged Solution
ITG Turbulence ITG Turbulence SimulationSimulation
kkx,minx,min= 0.1715, = 0.1715, kky,miny,min= 0.175, = 0.175, = 0.001 = 0.001
(Lenard-Berstein collision model)(Lenard-Berstein collision model)
Cyclone DIII-D base case
Entropy Balance in Entropy Balance in Toroidal ITG TurbulenceToroidal ITG Turbulence
Entropy balance is satisfied (Entropy balance is satisfied (/D/Dii <~ 8%). <~ 8%).
Statistically steady state of turbulence:Statistically steady state of turbulence: ii QQii~= ~= DDii => => Entropy production balances Entropy production balances with dissipation.with dissipation.
Velocity-Space Velocity-Space Structures of Structures of ff in in
Toroidal ITG TurbulenceToroidal ITG Turbulence
Fine-scale structures generated by the phase mixing Fine-scale structures generated by the phase mixing appear in the stable mode, and are dissipated by appear in the stable mode, and are dissipated by collisions, while the transport is driven by macro-scale collisions, while the transport is driven by macro-scale vorticesvortices..
=> => Entropy variable transferred in the phase Entropy variable transferred in the phase spacespace
High-velocity space resolution is necessary.High-velocity space resolution is necessary.
Long wavelength mode Linearly stable mode
(2(2
vv////
Production, Transfer and Production, Transfer and Dissipation of Entropy Dissipation of Entropy
VariableVariable
Entropy variable produced on macro-scale is transferred Entropy variable produced on macro-scale is transferred in the phase space, and is dissipated in micro velocity in the phase space, and is dissipated in micro velocity scale.scale.
The result confirms the The result confirms the statistical theory of the entropy statistical theory of the entropy spectrumspectrum for the slab ITG turbulence (Watanabe & for the slab ITG turbulence (Watanabe & Sugama, PoP Sugama, PoP 1111, 2004)., 2004).
Production
Dissipation
Transfer
Phase Mixing
No
nlin
eari
ty
Small Velocity Scale
Small Spatial Scale
Transport
Collisionless
Slab ITG Transport (WS 2004)
SummarySummary Gyrokinetic-Vlasov simulations of ITG Gyrokinetic-Vlasov simulations of ITG
turbulence and ZF with turbulence and ZF with high velocity-space high velocity-space resolutionresolution..
Collisionless damping process of ZF & GAM is Collisionless damping process of ZF & GAM is represented by the represented by the entropy transfer from entropy transfer from macro to micro velocity scalesmacro to micro velocity scales..
Neoclassical polarization effect is identified.Neoclassical polarization effect is identified. Statistically steady stateStatistically steady state of toroidal ITG of toroidal ITG
turbulence is verified in terms of turbulence is verified in terms of the entropy the entropy balancebalance..
Production, transfer, and dissipation processes Production, transfer, and dissipation processes of the entropy variableof the entropy variable are also confirmed for are also confirmed for the toroidal ITG turbulent transport.the toroidal ITG turbulent transport.
Flux Tube CodeFlux Tube Code Toroidal Flux Tube CodeToroidal Flux Tube Code
Linear Benchmark TestA B
CD F E
0
2
B
zy
x r r0
y r0
q0
q(r) z
The gyrokinetic equation is The gyrokinetic equation is directly solved in the 5-D directly solved in the 5-D phase space.phase space.
Gyrokinetic EquationGyrokinetic Equation GK ordering + Flute ReductionGK ordering + Flute Reduction
Co-centric & Circular Flux Surface with Co-centric & Circular Flux Surface with Constant Shear and GradientsConstant Shear and Gradients
Quasi-Neutrality + Adiabatic Electron Quasi-Neutrality + Adiabatic Electron ResponseResponse
t v||
ˆ b vd ˆ b v||
f
c
B0
,f v vd v||ˆ b e
Ti
FM C f
vd v||
2 R0
cos z ˆ s zsin z y sin z
x
,
v cTi
eLnB0
1i
mv 2
2Ti
3
2
y , v
2
2
J0 kv f d3 v 1 0 k2 e
Ti
e
Te
, k2 kx ˆ s zky 2 ky
2
Selected Parameters for our simulations
・ box size : Lx=Ly=10.0 Lz=100.0
・ initial perturbations:
23
0)1,2( 2exp100.1
xLxS
24
0)2,3( 2exp100.2
xLxS
・ # of grid points in the x direction : 200
・ mode numbers: -10 m 10 , -2 n 2 ( total: 105modes )
-15 m 15 , -3 n 3 ( total: 341modes)
、
・ density profile:
nLn
n 1
0
0
( Ln : density gradient scale length)
Quasi-Linear saturation
Time evolutions of (a)kinetic energy K and(b)Nusselt number Nufor Ki=0.3.
(a)Phase space‘K0-Nu’ and
(b)Power spectrum of K1.
Periodic Oscillations
(a)Phase space‘K0-Nu’ and
(b)Power spectrum of K1.
Time evolutions of (a)kinetic energy K and(b)Nusselt number Nufor Ki=0.5.More modes are
excited.
Linear Analysis
The most unstable wave number is estimated as
In this study, the following wave number is assumed,
From the dispersion relation, the linear growth rate is as follows.
2 2 2 1 x y ik k k g K
2 2 2 4 2
22 2 2 4 2 2
1 1 2 1 ,
1 1 4 1
y i k
k y i i y
k g K k i k k k D k
D k g K k i k k k k gK k
2 1 5 , 2 1 5 x y x i y ik k k g K k g K
Normalization
0 0 0 0 0
0 0 0 0
, , ,
, ,
, .
s s n s
n e s n i i e s
n e s n e s
x x y y t t L c
eL B T p pL T p T
eL B T eL B T
The standard drift wave units are used for normalization.
Linear growth rate
1 5 , 2 1 5x i y ik g K k g K
0.21icK
Increase of Accuracy
1. 18 ODE: Two modes (m=0 and 1) in the y direction and 3 modes (l=1,2, and 3) in the x direction.
2. 1D: Two modes (m=0 and 1) in the y direction and full modes in the x direction.
3. PDE: full modes in the x and y directions.
Intermittent oscillationsin 1D model
Time evolutions of kinetic energy K (left) and Nusselt number Nu (right) for Ki =5.
Scaling LawsODE, 1D, and Full Simulations
1D model Full PDE simulation
18 ODE
Intermittent Particle Transport in Resistive Drift Turbulence
Particle Flux
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0 2000 4000 6000 8000 10000
Part
icle
Flu
x 3
Time
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0 5000 10000 15000 20000 25000 30000 35000 40000 45000 50000
Part
icle
Flu
x 3
Time
0 2000 4000 6000 8000 10000
Time
0
Lx/2
Lx
0 10000 20000 30000 40000 50000
Time
0
Lx/2
Lx(a)’ 0 < t < 10000 (b)’ 0 < t < 50000
(a) 0 < t < 10000 (b) 0 < t < 50000
Particle flux vs. Resistivity
4.0E-3
5.0E-3
6.0E-3
7.0E-3
8.0E-3
9.0E-3
1.0E-2
1.1E-2
0.1 0.2 0.3 0.5 0.8 1 2 3 5
Part
icle
Flu
x 3
Resistivity
xnv
part
icle
flu
x Γ
resistivity η