Recent work on the control of MHD instabilities at ASDEX Upgrade
description
Transcript of Recent work on the control of MHD instabilities at ASDEX Upgrade
![Page 1: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/1.jpg)
Recent work on the control of MHD instabilities at ASDEX Upgrade
S. Günter, J. Hobirk, P. Lang, P. Merkel, A. Mück, G. Pereverzev, ASDEX Upgrade Team
Max-Planck-Institut für Plasmaphysik Garching, Germany
• Sawtooth control by ECCD• ELM control by plasma shaping and pellets• Current profile control by off-axis NBI?• RWM physics on ASDEX Upgrade?• NTM control, see next talk
![Page 2: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/2.jpg)
Sawtooth behaviour depends on NBI sources
one beam only
![Page 3: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/3.jpg)
Sawtooth behaviour for different NBI sources
Off-axis heating only, leads to density peaking j’ decreased (increased off-axis BS current) diagmagnetic stabilization (* increased)
one beam only
![Page 4: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/4.jpg)
Sawtooth behaviour for different NBI sources
two off-axis beams
2.0 3.0 4.0 5.0 6.0
t [s]
10000
20000
15000
12000
f [kHz]
Sawteeth/fishbones
(q=1)=0.2 (q=1)=0.2
(q=1)=0.1
two q=1 surfaces
• no sawteeth, but continous (1,1) activity
• two q=1 surfaces in the plasma (off-axis NBI-CD)
![Page 5: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/5.jpg)
Experiments with slow Bt-ramp, 0.8 MW co-ECCD and 5.1 MW NBI
Sawtooth tailoring by co- ECCD
![Page 6: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/6.jpg)
Influencing (1,1) mode activity by co-ECCD
• co-ECCD at pol = 0.4
• no sawteeth, only fishbones
• FB amplitude also decreases(SXR amplitude reduced by factor of 3)
![Page 7: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/7.jpg)
Sawtooth tailoring by ctr-ECCD
![Page 8: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/8.jpg)
Destabilisation of (1,1) activity by on-axis ctr-ECCD
• For ctr-ECCD deposition close to plasma center (here pol = 0.1) reversed q-profile destabilization of (1,1) mode
• No sawteeth or fishbones, but continous (1,1) activity
![Page 9: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/9.jpg)
NTM control by sawtooth mitigation (off-axis-ECCD)
Co –ECCD:• no sawteeth as expected• Reduced fishbone amplitude• NTM triggered after ECCD (by ST)
Counter-ECCD:• NTM triggered by FB during ECCD
![Page 10: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/10.jpg)
ELM mitigation: type II ELMs
Inner divertor
Outer divertor
power density
![Page 11: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/11.jpg)
#15865 #15863
Consider two discharges with different plasma shape
Type I Type II
![Page 12: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/12.jpg)
0.0 0.2 0.4 0.6 0.8 1.0 1.20
2
4
6
8
10
12
Ele
ctro
n de
nsity
[1019
m-3]
poloidal
15863 15865
0.0 0.2 0.4 0.6 0.8 1.0 1.20.0
0.5
1.0
1.5
2.0
2.5
Ele
ctro
n te
mpe
ratu
re [k
eV]
poloidal
15863 15865
but with similar edge temperature and density profiles
![Page 13: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/13.jpg)
Influence of closeness to Double Null
n=8 peeling mode
• Ballooning Stability unchanged• Low-n modes become more stable (broad mode structure) • Stability of medium-n modes unchanged, but eigenfunctions more localised at plasma edge
![Page 14: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/14.jpg)
Operational regime for type II ELMs
• closeness to DN/high • q95 > 3.5 • high n/nGW
![Page 15: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/15.jpg)
Why do we need high density/high q95?
JET, ELM precursorslow n modes only for high density(Perez, Koslowski et al., IAEA 2002)
Hypothesis: type II ELMs only if low-n modes are stable
![Page 16: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/16.jpg)
Influence of edge collisionality
jBS since * jBS since n
Theory: low mode number MHD activity destabilised by current gradient
![Page 17: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/17.jpg)
Is type II ELM regime accessible for ITER?
• Higher density increases edge collisionality BS current density reduced
reduced drive for low-n modes
If not n/nGW, but collisionality counts, type II ELMs would not occur in ITER Other means for ELM control?
![Page 18: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/18.jpg)
ELM mitigation: by pellets
Control of ELM frequency possible (each pellet triggers an ELM)
![Page 19: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/19.jpg)
Control of ELM frequency by pellets
• small pellets (2 … 3x1019 D atoms, not strong fuelling)• Confinement degradation ~ f-0.16
(less than for frequency change by, e.g., heating power, density puff) ~ f-0.6
![Page 20: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/20.jpg)
Mitigation of ELM size possible
• same plasma parameters• natural ELM frequency 52 Hz
![Page 21: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/21.jpg)
Mitigation of ELM size possible
![Page 22: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/22.jpg)
Energy loss per pellet triggered ELM as for type I ELMsat same frequency
![Page 23: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/23.jpg)
Current profile control by off-axis NBI?
Redirected NBI box provides off axis deposition of 93 keV ions:
• NB driven current clearly seen by reduced OH flux consumption
• current profile changes seem much smaller than expected
![Page 24: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/24.jpg)
Two off-axis beams, an example (#14513)
S3+S5 S6+S7
Plasma current
ne,0
pol dia
NBI
li
gas
Raus
![Page 25: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/25.jpg)
One off-axis beam (Te change compensated by ICRH)
S3 S6
ICRH
Plasma current
ne,0
pol dia
NBI
li
gas
Raus
#18091
![Page 26: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/26.jpg)
Strong change in li only for one-beam discharge
Change in li for one-beam casein agreement with ASTRA code
ASTRA
experiment
on- off-axis beams one-beam discharge
Very small change in li,much smaller than predicted(ASTRA li shifted up)
two-beam dischargeASTRA
experiment
![Page 27: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/27.jpg)
q-profile for two-beam discharge (q=1 surface)
ASTRA predicts observable changeof q-profile, but no change measured(MSE, q=1 radius)
But: in the plasma centre (tor < 0.15) q-profile changes as two q=1surfaces at tor < 0.10 and tor = 0.2 observed
2.0 3.0 4.0 5.0 6.0
t [s]
10000
20000
15000
12000
f [kHz]
Sawteeth/fishbones
(q=1)=0.2 (q=1)=0.2
(q=1)=0.1
two q=1 surfaces
![Page 28: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/28.jpg)
Current profile modifications due to one off-axis beam
Change in radius of q=1 surface is significant and agrees with ASTRA predictions
![Page 29: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/29.jpg)
Current profile modifications due to one off-axis beam
Current profile modifications mainly caused by off-axis beam (ASTRA)
![Page 30: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/30.jpg)
Comparison to MSE measurements
ASTRA predictions
![Page 31: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/31.jpg)
Non-stiff electron temperature profiles for one-beam discharge
one beam (without additional heating)two beams (#14513)
![Page 32: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/32.jpg)
Non-stiff ion temperature profile for one beam case
Ion temperature during off-axis NBI modeled by MMM95, agreement with measured pressures
![Page 33: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/33.jpg)
To explain unchanged current profile one needs a particle pinch!
Anomalous particle pinches are well-known in theory (density peaking)
Simple picture: strong turbulence of background plasma redistributes particles while
maintaining the two adiabatic invariants and
with the density follows from
const.
![Page 34: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/34.jpg)
Does theory predict such a particle pinch?
Need: full non-linear turbulence simulation with marker particles, in progress (B. Scott)
So far: quasi-linear GS2-calculations (G. Tardini, A. Peeters)
First results: particle pinch exists, but too smallTo be done: realistic density profile of fast particles, parameter scan
G. Tardini
![Page 35: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/35.jpg)
Simulations for realistic wall structures (as planned for AUG)
low triang.
high triang.
Plasmaseparatrix+ 3 cm in midplane
Wall structures only relevant onlow field side (ballooning mode structure)
Realistic model for AUG wall structures
![Page 36: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/36.jpg)
3D MHD code with 3d wall structures
• 3d MHD code CAS3D extended for
• 3d ideally conducting walls
• MHD eigenfunctions fully self-consistent
• Benchmark with 2d MHD code CASTOR successful
![Page 37: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/37.jpg)
Simulation results for realistic wall structures
Efficiency of realistic wallcompared to closed wall
Without wall: ßmarg = 1 %
<ß> = 4.5 %
closed wall
rw/rpl
1.2 1.4 1.6 1.8 2.0
A
0.08
0.06
0.04
0.02
0.0
![Page 38: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/38.jpg)
Wall resistivity causes mode growth on wall time (RWMs)
Further plans: - Resistive 3d walls (already started) - Feedback system (active coils to stabilise RWM)
![Page 39: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/39.jpg)
Summary
• Sawtooth mitigation by localized ECCD demonstrated• Seed island control allows to control NTM onset
• type II-ELMs achieved by plasma shaping compatible with required plasma parameters: N, q95, H, n/nGW
• open question: does collisionality count? (BS current)
• ELM mitigation by pellets demonstrated• smaller pellets at higher frequency needed
• off-axis NBI current for current profile control only for non-stiff ion temperature profiles?
• RWM physics: 3D ideal MHD code with 3D ideally conducting wall structures, finite wall resistivity being implemented
![Page 40: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/40.jpg)
Influence of edge density (BS current): ballooning modes
Experiment
Ideal ballooning limit:
ne = 9 1019 m-3
ne = 1.1 1020 m-3
Second stable regime low density
• Higher density increases edge collisionality BS current density reduced
Increased magnetic shear prevents access to second stable regime
![Page 41: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/41.jpg)
Non-stiff ion temperature profiles for one-off-axis beam
electron temperature and density constant, but diamagneticpressure decreases hint to non-stiff ion temperature profiles
one beam discharge
two beam discharge
diamagnetic pressure nearly constant,pol increases for off axis beams(fast increases, mainly ||)
![Page 42: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/42.jpg)
Non-stiff rotation profiles? (mode frequency also dependent on diamagnetic drift)
Strong reduction in (1,1) mode frequency for one-beam discharge
2.0 3.0 4.0 5.0 6.0
t [s]
10000
20000
15000
12000
f [kHz]
t [s]
2.0 3.0 4.0 5.0
1000
2000
5000
10000
20000two beams (#14513) one beam (#18091)
on-axis beams
off-axisbeams
on-axis beams
off-axisbeams
![Page 43: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/43.jpg)
Good match of electron temperature profiles ...
… by additional central ICRH for the one-beam discharge to adjust Inductive current profiles
![Page 44: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/44.jpg)
Two-beam discharges: so far non-symmetric beam deposition
0.0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.0 0.2 0.4 0.6 0.8 1.0
Q1 /+60 /z=+9.5Q2 /+70 /z=+9.5
Q3 /–70 /z=+9.5Q4 /–60 /z=+9.5
Q5, Q6, Q7, Q8
A. Stäbler
![Page 45: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/45.jpg)
Future two-beam experiments: try to match symmetricdeposition (closeness to DN)
0.0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.0 0.2 0.4 0.6 0.8 1.0
Q1 /+60 /z=+9.5Q2 /+70 /z=+9.5
Q3 /–70 /z=+9.5Q4 /–60 /z=+9.5
0.0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.0 0.2 0.4 0.6 0.8 1.0
Q1 /+69.5 /z=±0
Q2 /+79.5 /z=±0Q3 /–60.5 /z=±0
Q4 /–50.5 /z=±0
Z = 0 z = 9.5 cm
Q5, Q6, Q7, Q8 A. Stäbler
![Page 46: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/46.jpg)
CASTOR with antenna: calculate torque
Re P
jant B cos ~tor
Torque on the plasma due to external error fields:
1/
~
Maximum torque
![Page 47: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/47.jpg)
An example: Interaction of NTMs with perturbation fields
No simultaneous large NTMs of different helicities observed in experiments
![Page 48: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/48.jpg)
Analytic theory: • for NTMs stabilising effect of additional helical field can be proven for
small values of ||
• effect vanishes for ||
Is there an effect remaining for realistic values of || ?
If so: new stabilisation method for NTMs can be propsed:stabilisation by external helical perturbation fields
An example: Interaction of NTMs with perturbation fields
Many other problems, but: so far no non-linear MHD code can deal
with realistic ||
![Page 49: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/49.jpg)
Proposal for a solution in non-aligned coordinate system
( )1//11//102
0 2
1−−⊥⊥ ∇⋅+∇⋅−=∇−
∂
∂qbqbTT
t
rrχ
2//10//11//012
1 qbqbqbTTt
∇⋅−∇⋅−∇⋅−=∇−∂∂
−⊥⊥
rrrχ
3//11//12//022
2 qbqbqbTTt
∇⋅−∇⋅−∇⋅−=∇−∂∂
−⊥⊥
rrrχ
( )1111//0// 2
1−− ∇⋅+∇⋅−= TbTbq
rrχ
( )211001//1// TbTbTbq ∇⋅+∇⋅+∇⋅−= −
rrrχ
( )312011//2// TbTbTbq ∇⋅+∇⋅+∇⋅−= −
rrrχ
In the following, for simplicity (not in the code): Cartesian coordinates with one perturbation field component
Heat conduction equation for different Fourier components of temperature:
BBb ii
rrr=
… …
//2 qbTT
t∇⋅−=∇−
∂∂
⊥⊥ ( )Tbq ∇⋅−= //// χ
To close the equations one should not truncate the Fourier series in T, but in q heat flux along perturbed magnetic field line remains finite (nearly vanishing temperature gradients)
![Page 50: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/50.jpg)
Fourier decomposition for perturbation
2//10//11//012
1 qbqbqbTTt
∇⋅−∇⋅−∇⋅−=∇−∂∂
−⊥⊥
rrrχ
3//11//12//022
2 qbqbqbTTt
∇⋅−∇⋅−∇⋅−=∇−∂∂
−⊥⊥
rrrχ
( )1111//0// 2
1−− ∇⋅+∇⋅−= TbTbq
rrχ
( )211001//1// TbTbTbq ∇⋅+∇⋅+∇⋅−= −
rrrχ
( )312011//2// TbTbTbq ∇⋅+∇⋅+∇⋅−= −
rrrχ
In the following, for simplicity (not in the code): Cartesian coordinates with one perturbation field component
Heat conduction equation for different Fourier components of temperature:
BBb ii
rrr=
//2 qbTT
t∇⋅−=∇−
∂∂
⊥⊥ ( )Tbq ∇⋅−= //// χ
To lowest order (for explanation): include only terms up to first order in q
T2 adjusts itself such that q||1 becomes small
( )1//11//102
0 2
1−−⊥⊥ ∇⋅+∇⋅−=∇−
∂
∂qbqbTT
t
rrχ
![Page 51: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/51.jpg)
What about the radial derivatives?
rrebbrr
11≈ bkib ⋅=∇⋅r
perturbation field:
1102
0 qr
bTTt r ∂
∂−=∇−
∂∂
−⊥
10112
1 qbkiTTt
⋅−=∇−∂∂
⊥
rχ
( )r
qqb
ii
r Δ
−−≈
−+
−
)12/()12/(
111
iqbki1
01 ⋅−≈r
1122
2 qr
bTTt r ∂
∂−=∇−
∂∂
⊥ ( )r
qqb
ii
r Δ
−−≈
−+ )12/()12/(
111
( )2
)2/1()2/1(
0111
−+ +⋅−≈
ii qqbk
Introduces an additional error or order (r)2 , but equations for each grid point ensure vanishing temperature gradients along perturbed field lines
simplest discretisationat i’s grid point
new scheme
![Page 52: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/52.jpg)
Convergence properties: single magnetic island
||= 108
Still convergence only (r)2
But: absolute error reduced by factor of 10Improvement increases for larger ||
![Page 53: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/53.jpg)
Magnetic islands with two helicities
![Page 54: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/54.jpg)
Magnetic islands with two helicities
||= 1010
Magnetic islands seen in temperature contours, but still strong gradient in ergodic region
![Page 55: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/55.jpg)
Magnetic islands with two helicities
||= 1012
Temperature gradient vanishes in ergodic region due to increased radial transport along magnetic field lines
![Page 56: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/56.jpg)
An example: Interaction of NTMs with perturbation fields
Is there an effect remaining for realistic values of || ?
If so: new stabilisation method for NTMs can be propsed:stabilisation by external helical perturbation fields (next talk)
YES!
![Page 57: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/57.jpg)
Improved Diagnostics at the edge
Comparison with theory possible ...
![Page 58: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/58.jpg)
Plasma shape is important for ELM losses
• higher upper triangularity leads to bigger ELM losses
• can be explained by wider ELM affected region at higher triangularity
![Page 59: Recent work on the control of MHD instabilities at ASDEX Upgrade](https://reader035.fdocuments.us/reader035/viewer/2022062322/56814967550346895db6bbab/html5/thumbnails/59.jpg)
Our understanding of transition type I type II ELMs
Strong plasma shaping (high , closeness to DN)- stabilises low-n modes- reduces width of medium-n eigenfunctions
High edge density (reduced BS current density)- reduces drive for low-n modes- closes access to second stable regime for ballooning modes (limits achievable pressure gradient)
Can we expect type II ELMs in ITER ? (low collisionality!)