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1. magnetic confinement - ENEA - Fusione

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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

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