1. magnetic confinement - ENEA - Fusione
1. magnetic confinement - ENEA - Fusione
1. magnetic confinement - ENEA - Fusione
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
26<br />
<strong>1.</strong> MAGNETIC CONFINEMENT<br />
<strong>1.</strong>1 Tokamak Physics<br />
t=46.5 s). No change in<br />
plasma-edge activity is<br />
observed in concomitance<br />
with the ITB collapse.<br />
1<br />
The effect of LHCD on <strong>magnetic</strong><br />
shear might have helped to<br />
sustain the ITB in shot #53429, as<br />
0<br />
suggested by the modelling<br />
analysis performed by the<br />
JETTO code [<strong>1.</strong>30] and LH ray 2-<br />
D Fokker Planck ray tracing. As -1<br />
a result [<strong>1.</strong>31], the power is fully<br />
deposited off-axis within the<br />
layer ρ≈0.4-0.7, with a maximum<br />
at ρ≈0.5 (ρ is the square root of<br />
the normalised toroidal flux).<br />
The ITB is located in this layer.<br />
The calculated fraction of LH<br />
0.3 0.4 0.5<br />
ρ<br />
0.6 0.7 0.8<br />
driven current is<br />
I LHCD /I P ≈0.25, while the<br />
noninductive current fraction is<br />
(I LHCD +I boot +I NBI )/I P ≈0.65. 0.5<br />
The q-profile of discharge<br />
t = 47s<br />
#53429 simulated by the<br />
t = 46s<br />
JETTO code shows a reversed 0<br />
shape during the main<br />
heating phase. Figure <strong>1.</strong>19<br />
reports the simulated -0.5<br />
<strong>magnetic</strong> shear profiles at<br />
0.3<br />
0.4<br />
different times during the<br />
ρ<br />
main heating phase. After the<br />
LH power is switched on, the<br />
0.5<br />
0.6<br />
s=0 layer of the <strong>magnetic</strong> shear profile moves outward and persists in the region<br />
ρ>0.3. As anomalous transport is dominant in this region, the low/negative<br />
<strong>magnetic</strong> shear could inhibit the growth of turbulent modes that cause the ITB<br />
collapse. No change in the q profile is expected at the time of the ITB collapse in the<br />
experiment. However, the collapse might be related to edge physics, as it<br />
accompanies an increase in Dα emission.<br />
Magnetic shear s<br />
Magnetic shear s<br />
For shot #53429, with LH power coupled during the main heating phase, modelling<br />
suggests that the collapse can be produced by an inward movement of the s=0 layer<br />
[(ρ