Studies of Improved Confinement in Heliotron J
description
Transcript of Studies of Improved Confinement in Heliotron J
Heliotron J
IAE, Kyoto University
Studies of Improved Confinement
in Heliotron J
Presented by
MIZUUCHI Tohrufor Heliotron J Team
Heliotron J IAE, Kyoto University
Studies of Improved Confinement in Heliotron J
Contents
Introduction
Transition to Improved Confinement─ Configuration Effects─ Effects of Heating Scenario
Fueling Control
Summary
Heliotron J IAE, Kyoto University
Due to the time limitation, this talk will focused on “Transition”. For other topics, please contact me or refer the proceeding
Heliotron J IAE, Kyoto University
<r> (m)
/2
4/7
4/8
8/15
8/17
8/13
12/22
Heliotron J (vacuum)
12/23
0.00 0.10 0.20
0.50
0.55
0.60
The edge magnetic surfaces are strongly modified by the resonant conditions.
STD
Ad. Ip
Sub. Ip
Vacuum Rotational Transform
i(a)/2p=0.493 i(a)/2p=0.498
i(a)/2p=0.56 i(a)/2p=0.62
The effects of rational surfaces have been studied is not only from the MHD activities but also from the appearance of transport barriers viewpoints.
HFC
Heliotron J IAE, Kyoto University
Bumpiness Control B drift can be suppressed with bumpiness control.
1
1.1
1.2
1.3
1.4
1.5
1.6
0 45 90
|B|
Toroidal angle (deg.)
Magnetic field strength at plasma axis
High eb
Medium
Low
StraightCorner Corner
High eb : Higher mirror rippleLow eb : Mirror field reversal (at axis) Constant parameters :- Rax/<ap> = 1.2 m/0.17 m, Vp ~ 0.7 m3
- Edge rotational transform- Magnetic well in entire region
-0.2
-0.1
0
High b
MediumLow
B1
4/B0
0
Helical component
-0.2
-0.1
0
B1
0/B0
0
Toroidal component
-0.1
0
0.1
0.2
B0
4/B0
0
Bumpy component
0.50
0.55
0.60
0 0.2 0.4 0.6 0.8 1
2
(=s1/2)
7/4
15/8
m/n=13/8
Rotational transform
Heliotron J IAE, Kyoto University
The Heliotron J experiments have revealed the existence of the spontaneous transition to improved confinement mode.
00.05
0.10.15
P (
A.U
.)
PECH
time (ms)200 300
00.10.2
Wb
(A.U
.)
Diamag
0.10.20.30.4
I (A
.U.)
Dalpha
#28407 H-modeDithering phase
#28407
0
0.5
1
1.5
time (ms)
I.S.
(a.
u.) Fast Langmuir Probe
200 300-1
0
1
I (a
.u.)
Magnetic Probe
ECH-only plasma
Observation with fast cameras revealed the existence of filament structure parallel to B in the peripheral plasma turbulence.
Phase image analysis suggests The CCW poloidal rotation of the filament
structure during the L-mode. During the L-H transition, this rotation
speed decreases. After the transition, it restarts the
movement but in CW direction.
Ref. Nishino, C09 (Tue)
Heliotron J IAE, Kyoto University
The transition phenomena were observed almost all (a)/2 cases for the input power range in the experiment (ECH+NBI).
Some configurations show a remarkable improvement but the others show a slight improvement.
P = PECH ( 0.29 MW) + PNBI ( 0.57 MW)
Vp (m3), R (m)
(a)vac/2
Wp (
kJ)
70GHz ECH+NBI (-Sacn) Max. Wp
before
0.0
1.0
2.0
3.0
8/17 8/15 8/13
4/8 4/7 4/6n/m
W
p/W
pb
efo
re
HJ14990-HJ15456 ECH+NBI
0.45 0.50 0.55 0.60 0.650.0
1.0
2.0
3.0
Before the transition, Wp strongly depends on i(a)/2p|vac, but it is moderated after the transition.
Heliotron J IAE, Kyoto University
One robust condition to the transition is the core density.The value of the threshold line-averaged density is not sensitive to
the heating method, Pinj level, i(a)/2p|vac.
The threshold density is a robust condition of the transition. The threshold density (lower density limit for the transition) is ~ 1-21019 m-3. Only for higher values of /2, some exceptional low threshold density cases
are observed. MHD activities?
STD configuration
Pinj (MW)
ne-b
ar
(10
19 m
-3)
ECHNBIECH+NBI
HJ09472-HJ12298 STD
0.2 0.4 0.6 0.8 1 1.20.0
1.0
2.0
3.0
ne
thr (
10
19 m
-3)
(a)/2
HJ ECH+NBI
0.45 0.5 0.55 0.6 0.650
0.5
1
1.5
2
2.5
38/17
4/8 4/7 4/6
8/15 8/13
n/m
PECH (~ 0.29 MW)+PNBI (~ 0.57 MW)
Heliotron J IAE, Kyoto University
the “quality of improvement” based on ISS04 seems to depend on the configuration.
Iota-windows for high quality H-mode close to the low-mode rationals
All configurations basically have “stellarator shear” (vacuum) hard to get edge flux surfaces on the “right-side” of the rationals.
Difference in the poloidal viscous damping among the configurations can cause the difference in the “quality”?
─ Still open question.─ Bias experiment will give us
some information.
tex
p/(
ftIS
S0
4)
F. Sano, et al., Nucl. Fusion 45 (2005) 1557.
i(a)/2p|vac
Heliotron J IAE, Kyoto University
3
Electrode of LaB6
(Hot Cathode)
Electrode Bias Exp. in Heliotron J under a Low Field ConditionS. Kitajima, et al., Tohoku Univ.
Externally controlled torque could give us a lot of (but NOT sufficient) information on the viscous damping.
Note: This experiment was performed under a special configuration for 2.45GHz ECH discharge.
Heliotron J IAE, Kyoto University
Rapid increase of IE and ne.
Vs changed from positive to negative.
Drop in the fluctuation level.
Clear hysteresis of IE.
Triangular voltage was applied in order to give rise to forward/ back transition.
Time Evolution of a Biased Discharge
Heliotron J IAE, Kyoto University
R (m)
Z (
m)
2.45GHz ECDCHeliotron J
0.8 1 1.2 1.4 1.6
-0.2
0
0.2
0.4
Bias Exp. suggests plasma rotation can modify the edge field topology.
Bias
time (s)1 2
0
2
4
0
1
2
HJ-SH365/090305
CH8
Divertor Probe Array
0
0.02
0.04
CH9
0
0.02
0.04
CH11
0
0.02
0.04
CH12
0
0.02
0.04
CH14
0
0.02
0.04
CH13
0
0.02
0.04 Time traces of ion-saturation currents at divertor probe array during biasing:Increase for some channels, but decrease for other channels. Modification of edge field topology!
Probe array
Heliotron J IAE, Kyoto University
The “quality of improvement” based on ISS04 seems to depend on the configuration.
All configurations basically have “stellarator shear” (vacuum) hard to get edge flux surfaces on the “right-side” of the rationals.
Difference in the poloidal viscous damping among the configurations?
But, is that all? How about the “plasma effects”,
especially effects of (non-induction) plasma current.
Experiments suggest the change of the iota and/or the size of the confinement region.
tex
p/(
ftIS
S0
4)
F. Sano, et al., Nucl. Fusion 45 (2005) 1557.
i(a)/2p|vac
Heliotron J IAE, Kyoto University
ad. 4kAad. 2kAad. 1kA
sub. 1kA sub. 2kA sub. 4kA
HINT2 predicts the change of the field topology caused by plasma current:
b(s) = 0.5·(1-s)2 [%], jp = jp0·(1-s)2
vacuum
0kA
“Additive” plasma current can modify not only the i/2p-profile but also the “shape” of magnetic surfaces.
Asymmetric effect of plasma current due to the “proximity” to a low-mode rational number.
<r> (m)
/2
(s)=b0(1-s)2, 0=0.5 %jp(s)=j0(1-s)2HINT2
Ip=4kA
2kA
-4kA
-2kA
1kA
-1kA0kA
4/812/23
8/15
4/7
8/13
12/22
0 0.1 0.2
0.50
0.60
Heliotron J IAE, Kyoto University
Experiments suggest the change of the edge field topology during a plasma shot.
ECH ( 0.3 MW) + NBI ( 0.7 MW, co-injection) @ STD
The observed non-inductive toroidal plasma current is gradually increases as increase of the stored energy. – In the density range shown in the figure, the observed
plasma current is considered to mainly consist of the bootstrap current and the NB induced current.
Position of Divertor Leg
R (m
)
time (ms)
Lc PeakDensity Peak
200 250
1.40
1.45
NBIECH
nel
n el (
1019
m-2
)
HJ15449
H
H
(a.u
.)
0
0.5
1
1.5
0
0.5
Wp
Wp
(kJ)
Ip
Ip (k
A)
0
1
2
0
1
2
3
n e, d
iv (1
018 m
-3)
R=1.407 m
0
2
4
(1018
m-3
) (b) t = 277 ms
R (m)1.4 1.45
0
1
2
3
(1018
m-3
) (a) t = 211 ms
HJ15449
0
1
2
The profiles of the diverted plasma density at t = 211 and 277 ms.
–At 211 ms, the density distribution is consistent with that expected from the vacuum field topology.
–At 277 ms, the density peak position shifts inward about 4 cm compared to the position at 211 ms.
The overall trend of the density-peak-position shift seems to be well synchronized with the change of Wp or Ip.
Heliotron J IAE, Kyoto University
Comparison between Co/CTR NBI-only plasmas
- No transition in CTR NBI -
In Co-NBI, the transition were observed, but no transition in CTR-NBI.
Difference in the transition condition between these NBI-only plasmas due to
Deformation of i/2p Position of rational surface, Shear, Shape of LCFS,
Direction of momentum input ?
0
2
W(k
J)
NBI
ECH
Co-NB
CTR-NB
#25892(Co-NB), #25989(CTR-NB)Config. ; (a)/2=0.54
0
2
n e(x
1019
m-3
)
-2
0
2
I p(k
A)
Co
CTR
0
2
4
6
180 200 220 240
I H(A
.U.)
time (ms)
Heliotron J IAE, Kyoto University
The transition is observed when the plasma current reaches a critical value.
The critical value of the plasma current depends on the configuration; 0.7±0.1kA in middle eb
1.3±0.2kA in high eb cases. The observed time delay would be related
to the growing-up time of the current.
− In high eb case, higher Ip was
required.
I p @
Ha
dro
p (k
A)
Dependence of IP at transition on PNB
2
1
00 200 400 600
High b
Medium b
PPortthrough
(kW)
High eb
Medium eb
Dependence of delay time on PNB
dela
y tim
e (
ms)
0
10
20
30
40
50
0 200 400 600
High b
Medium b
PPortThrough
(kW)
The effects of the plasma current on the field configuration should depend on the vacuum rotational transform. i(a)/2p|vac-scan experiment.
Heliotron J IAE, Kyoto University
2
1
00.45 0.5 0.55 0.6 0.65
(0)/2 (=1/q)
I p (
kA)
I p@
tra
nsi
tion
(kA
)
i(a)/2p|vac
4/8 4/78/17 8/15 8/1312/2212/23
(High eb)
The critical current for NBI-only plasma strongly depends on i/2pvac.
So far, the transition was observed only in Co-NBI (ad. NBCD) plasmas (Pinj < 0.6 MW).
A “critical current” for the transition exists for all config.
Does the change in the rotational transform caused by non-inductive plasma current trigger the transition? Check other heating cases.
Radial profile of iota
<r> (m)
/2
4/7
4/8
8/15
8/17
8/13
12/22
Heliotron J (vacuum)
12/23
0.00 0.10 0.20
0.50
0.55
0.60
0.25 MW < Pinj < 0.6 MW, ne ~ 1.5-21019 m-3
0.45 0.50 0.55 0.60 0.65
0.50
0.55
0.60
12/22
8/13
4/7
(a)/
2
Vacuum Iota
4/8
8/15
HJ Close to Rationals?
Heliotron J IAE, Kyoto University
Comparison of the plasma current at the transition for ECH-, NBI-, and ECH+NBI-plasmas
2
1
00.45 0.5 0.55 0.6 0.65
(0)/2 (=1/q)
I p (
kA)
I p@
tran
sitio
n (k
A)
i(a)/2p|vac
4/8 4/78/17 8/15 8/1312/2212/23
(High eb)
((a)/2)VAC
I p (
kA)
ECHdensity ramp-up
HJ15567-15587mid.-b
high-b
low-b
low-b
HJ28256-28275(ECCD, low density)
HJ18494-18860
HJ18365-18483
HJ18413-18929
0.45 0.5 0.55 0.6 0.65
0
1
2
3
NBI-only
Ip,NET itself seems not a key factor? Need profile data!
((a)/2)VAC
I p (
kA)
ECH+NBIdensity ramp-up HJ14990-15453
0.45 0.5 0.55 0.6 0.650
1
2
3ECH-only
ECH+NBI
Heliotron J IAE, Kyoto University
Even for the same net current, the deformation of i/2p and the shape of the magnetic surface strongly depend the current profile.
- MODEL CALCULATION -
<b> ~ 0.32 %, p=p0(1-s2)2
(a) j = j0(1-s)8, Inet = +2.0 kA(b) j = j0(1-s)8, Inet = -2.0 kA(c) j = j0(1-s4)2, Inet = +2.0 kA(d) j = j0(1-s4)2, Inet = -2.0 kA(e) j = j0(60(1-s2)s2-5(1-s2)),
Inet = +2.0 kA(f) j = j0(60(1-s2)s2-5(1-s2)),
Inet = -2.0 kA
r/a (=s1/2)
current profile model
curr
ent/
unit
are
a (a), (b)
(c), (d)
(e), (f)
0 0.2 0.4 0.6 0.8 1-5
0
5
10
15
20
Heliotron J IAE, Kyoto University
Comparison of the plasma current at the transition for ECH-, NBI-, and ECH+NBI-plasmas
2
1
00.45 0.5 0.55 0.6 0.65
(0)/2 (=1/q)
I p (
kA)
I p@
tran
sitio
n (k
A)
i(a)/2p|vac
4/8 4/78/17 8/15 8/1312/2212/23
(High eb)
((a)/2)VAC
I p (
kA)
ECHdensity ramp-up
HJ15567-15587mid.-b
high-b
low-b
low-b
HJ28256-28275(ECCD, low density)
HJ18494-18860
HJ18365-18483
HJ18413-18929
0.45 0.5 0.55 0.6 0.65
0
1
2
3
NBI-only
Ip,NET itself seems not a key factor? Need profile data!■ Even in low density ECH-only plasma lower than the threshold
density, the transition can be observed when the EC driven “additive” current is high enough.
■ Transition is observed in ECH+NBI plasmas even in the low eb case.
((a)/2)VAC
I p (
kA)
ECH+NBIdensity ramp-up HJ14990-15453
0.45 0.5 0.55 0.6 0.650
1
2
3ECH-only
ECH+NBI
Heliotron J IAE, Kyoto University
Transition to a better confinement mode was observed in a high ECCD current discharges.
Low-eb, i/2p(a) ~ 0.56, ECH-only with PECH > 0.3 MW
The line-averaged density is much lower than the critical low-density limit observed in the previous experiments.
No enough experiments, from this point of view, in sub. high ECCD condition.
HJ28275
ECH
Gas Puff(a.u
.)
0.0
1.0
2.0
H#11.5
(a.u
.)
0
0.01
0.02
1019
m-2
mW
b
0
0.2
0.4
0
0.1
kA
Ip
time (ms)
ad.
200 250 300-3.0
-2.0
-1.0
0.0
Heliotron J IAE, Kyoto University
Summary (1) - Transition to improved confinement -
No transition in CTR-NBI-only plasmaExistence of the “critical current” in Co-NBI-only plasma Change in the rotational transform (and/or its radial profile) caused by plasma current and/or the direction of momentum input can trigger the transition in NBI plasma.
No clear current dependence in ECH-only plasma Difference in the transition condition between NBI-only and ECH-only plasmas. ECH should have some effect on the transition condition in NBI plasma.
In low density (lower than the threshold density) ECH-only plasma, the transition can be observed when the EC driven “additive” current is high enough. Change in the rotational transform (and/or its radial profile) is effective even for ECH-only plasma.
Heliotron J IAE, Kyoto University
ECH-onlyNBI-only
(Co)NBI-only
(CTR)
NBI (Balance)ECH+NBI(Balance)
ECH+NBI (Co)
ECH+NBI(CTR)
i(a)/2p|vacX only for
0.493 OK X No Data OK No Data
eb* △
for high-eb
X for low-eb
X No Data OK No Data
Ip,th** No Yes - Yes
remarks
Transition is observed in low ne,
high Ip
Summary (2) - Transition to improved confinement -
for ne > ne,th
* Data for different i(a)/2p|vac are necessary.** Data @ Ip=0 are necessary.
Heliotron J IAE, Kyoto University
Thank you for your attention! &
Thank you All Contributors for Nice Collaborations!
F. Sano, K. Nagasaki, H. Okada, T. Minami, S. Kobayashi, S. Yamamoto, S. Ohshima, K. Hanatani, S. KonoshimaInstitute of Advanced Energy, Kyoto University
Y. Nakamura, K. Mukai, S. Kishi, H.Y. Lee, K. Minami, Y. TakabatakeGraduate School of Energy Science, Kyoto University
T. Mutoh, S. Okamura, Y. Takeiri, K. Y. Watanabe, M. Yokoyama, K. Nagaoka, Y. Yoshimura, Y. Suzuki, H. Takahashi
National Institute for Fusion Science
N. NishinoGraduate School of Engineering, Hiroshima University
S. MurakamiGraduate School of Engineering, Kyoto University
S. Kitajima, H. UtohGraduate School of Engineering, Tohoku University
Y. NakashimaPlasma Research Center, University of Tsukuba
I. PankratovNational Science Center, Kharikov Institute of Physics and Technology, Ukrina
Q. Yang, L. Yao, W. ChenSouthwestern Institute of Physics, China
Heliotron J IAE, Kyoto University
No clear threshold power for Phase-I
No clear/simple relation between nth and Pabs.
At the (a)/2 0.493, ECH-only discharges cannot make a transition. configuration effects on the power threshold.
Different power dependence for Phase-I and II?
F. Sano, et al., Nucl. Fusion 45 (2005) 1557.