Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2...
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Transcript of Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2...
![Page 1: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/1.jpg)
Particle Distribution Modification by TAE mode and Resonant Particle Orbits
POSTECH1, NFRI1,2
M.H.Woo1, C.M.Ryu1, T.N.Rhee1,,2
![Page 2: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/2.jpg)
Outlines
-Hybrid scheme:ideal MHD background and energetic particles
-Tokamak Equilibrium and TAE
-Distribution function modification by TAE -Resonance particle interactions with the TAE wave Bouncing, circulating and potato orbits
-Conclusions
![Page 3: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/3.jpg)
Hybrid Code Structure
Equilibrium (EFIT data)
Re-normalization of Equilibrium(Chease)
TOKAMAK Experiment
Ideal MHD Solution (KINX)
Non-inductive heating & Alpha particle
TRANSP Data etc. Hot Particle Distribution
Mode Frequency & Growth rate
Test Particle code (ORBIT)
Monte-Carlo Distribution
![Page 4: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/4.jpg)
Calculation of Mode Frequency Modification
0||)(2
1 )()(3220
2 nak
ak WWxd
Dispersion Relation for TAE
]Re[2
1 )()(
00
nak
akr WW
K
Calculation of Mode Growth Rate
( )
0
1[Im ]
2na
i kWK
))((ln
4
|)~(4
2)(
||
2
*
2)(
ppk
k
jj
hak
kl l
l
kk
jj
hnak
FE
E
VBW
vk
JE
E
VBW
Mode Growth-rate
( ) ( )[1 ( ) ]
( ) (damping)i d
A t A t t t
t
All the values shown here can be estimated from Simulation
Kinetic & Fluid Contributions
![Page 5: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/5.jpg)
Why Hybrid Code ?
• Full Particle simulation is not available• Saving computation time• Individual particle trajectory• Immediate validation & examination of analytical theory• Essential issues about energetic particle• Alpha particle heating• Turbulence
Limitations
• Only perturbative treatment• Not fully self-consistent• Scale larger than Gyro-radius• Slow time scale behaviors ( Drift scale, Not gyration scale)
![Page 6: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/6.jpg)
Ideal MHD mode
![Page 7: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/7.jpg)
Relation between displacement and Magnetic perturbation
)(, Ingmq
nqmmn
Total Perturbation Dominant m=1 Perturbation
![Page 8: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/8.jpg)
Particle Distribution Modification by TAE mode
![Page 9: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/9.jpg)
• Electron distribution for ECRH• Ion distribution for NBI• Electron & Ion distribution for ICRH• Fusion Born Alpha particle distribution
b=0.1
Example: Initial Maxwellian distribution (2000 particles) in simulation
b=8
![Page 10: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/10.jpg)
•Interpolation of test particle distribution
•Smooth radial and energy profile
•These equations are used for analytical calculation of mode frequency and growth rate
2 2 2 21
1 1( , )
( ) ( )
N
pk p pk k
F Ea E E b
2 2 2 21
2( ) 1
( ) ( )
Np pk
kp p pk k
F
a E E b
2 2 2 21
2( ) 1
( ) ( )
Np pk
k p pk k
E EF
E a E E b
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Initial Distribution
First orbit loss of the particles
Final Distribution
Pitch Distribution
Energy Distribution
• Energy is conserved
• Particles with pitch around 0are dominantly lost• Large bounce orbit is the main reason for loss
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Radial Distribution
Theta Distribution
• Radially flattened due tofinite bounce orbit
• Barely trapped or circulatingparticles are mainly lost
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For the perturbation
Energy distribution
Resonance line
•More particles near the resonance line. •Some particles gain very high energy•High energetic particles (>150 keV) are lost
Radial distribution
•Particles near the edge are lost•Flattened compared to the no B perturbation case
3/ 10B B
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Particle loss due to perturbation
•Dominant particle loss begins around •First orbit loss is about 40%
210
•In average, particle gains energy•Energy gain process shows a jump
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Circulating-Passing particles: High energy
800
4transit
alpha p
t t
m m
•No perturbation•Clear precession•outward-shift of orbit
|| ||
100
/ 0.7
E keV
v v
parameters
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Non-Circulating, passing particles
Same parameters with low energy 1E keV
800
4transit
alpha p
t t
m m
||
100
0.3
E keV
•This is the orbit of the particle that interact most strongly with TAE mode
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||
3
0.3
100
0.7
/ 10
A
E keV
B B
Particle trajectory with B perturbation
Non-Resonant case, large perturbation
Orbit modification is not much.
![Page 18: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/18.jpg)
Resonant case with small perturbation
||
4
0.3
100
0.454
/ 10
A
E keV
B B
• Particle has a little bit smaller velocity• Particles are lost due to resonant interaction
0 00.3 2 0.3 2wave AV R B
Wave phase velocity is about
/ 0.455wave partV V
Here is alpha particle velocitypartV
![Page 19: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/19.jpg)
Resonant case with small perturbation -jumping orbit
•A sudden jump to other smaller orbit
||
100
4
0.43(smaller pitch)
/ 0.455
/ 10
waveV V
B B
![Page 20: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/20.jpg)
Resonant case with small perturbation- jumping orbit
||
5
0.475 ( greater pitch )
10B
B
For a very small perturbation, resonant particles change the direction of the movement,jumping to other stable orbit with pitch reversed.
![Page 21: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/21.jpg)
Detailed Motion of Resonant Particles
Phase trajectories of particles with different pitches
Bouncing
Potato
Circulating
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Conclusions
•Modification of particle distribution by the TAE mode is under investigation. •A hybrid scheme of ideal MHD and energetic particle motion is used.•Particles tend to jump from one orbit to other stable orbit•Resonant particles interacting with TAE strongly mainly come from the potato orbit.•Some particles with low pitch gain large energy and move in the reverse direction.
![Page 23: Particle Distribution Modification by TAE mode and Resonant Particle Orbits POSTECH 1, NFRI 1,2 M.H.Woo 1, C.M.Ryu 1, T.N.Rhee 1,,2.](https://reader035.fdocuments.net/reader035/viewer/2022070409/56649e9d5503460f94b9dc7a/html5/thumbnails/23.jpg)
Thank you for your attention!