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1. magnetic confinement - ENEA - Fusione

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12<br />

<strong>1.</strong> MAGNETIC CONFINEMENT<br />

<strong>1.</strong>1 Tokamak Physics<br />

Energy transport and electron temperature profile stiffness with localised ECRH<br />

Off-axis ECRH clearly reveals electron temperature profile stiffness in FTU [<strong>1.</strong>3],<br />

particularly when absorption is located in the <strong>confinement</strong> region, i.e. outside the<br />

sawtooth inversion radius (r/a > 0.2) but inside the radiation-dominated periphery<br />

(r/a< 0.6). The typical marker of electron temperature profile stiffness, observed in<br />

all similar experiments on ASDEX-U, D III-D, Tore Supra and TCV, is a step in the<br />

radial dependence of the electron thermal diffusivity. The step is usually positioned<br />

at the EC-wave absorption radius, particularly when the ECRH power density<br />

greatly exceeds the Ohmic input. The step amplitude is just enough to keep the<br />

temperature profile smooth. The gradient length L T =T e /∇T e of the profile hardly<br />

changes from Ohmic heating to ECRH and is not influenced by ECRH intensity and<br />

localisation.<br />

Modulated ECH was applied to study electron temperature profile stiffness in FTU<br />

plasmas during current ramp-up. Modulated ECH experiments at current flat-top on<br />

ASDEX-UG [<strong>1.</strong>4] have shown that the heat wave propagates much faster outwards<br />

than inwards, confirming the step-wise behaviour of thermal diffusivity at the EC<br />

absorption radius. The experiments during current ramp-up were performed with<br />

ECRH at a much lower power level than Ohmic heating in order to limit as much as<br />

possible the impact of ECRH on profile shapes. In addition, target plasmas with very<br />

different shapes were obtained through control of the breakdown and density buildup<br />

phases. Figure <strong>1.</strong>3 shows two typical targets, one with peaked temperature (and<br />

current density) profiles, the other with flat-hollow profiles characterised by the<br />

occurrence of typical double tearing modes. Heat wave propagation is much more<br />

sensitive than power balance analysis to discontinuities in thermal conductivity. In<br />

addition, by looking at the amplitude and phase radial distribution of electron<br />

temperature oscillations, it can be excluded that the apparent drop in diffusivity is<br />

due mostly to a heat pinch.<br />

[<strong>1.</strong>3] S. Cirant et al., Proc.<br />

14 th AIP Conf. on Radio<br />

Frequency Power in<br />

Plasmas (Oxnard 2001),<br />

Vol. 595, p 338<br />

[<strong>1.</strong>4] F. Ryter et al., proc.<br />

28 th EPS Conf. on<br />

Controlled Fusion and<br />

Plasma Physics (Madeira<br />

2001), Vol. 25A, p. 685<br />

The experiments showed that in these conditions the low-high diffusivity transition<br />

layer is not strictly positioned at the absorption radius and that it depends to some<br />

extent on the profile shape. For a given position of the absorption layer (r/a≈0.25), in<br />

Te (keV)<br />

Te (keV)<br />

2.5<br />

2<br />

<strong>1.</strong>5<br />

1<br />

0.5<br />

0<br />

3<br />

2.5<br />

2<br />

<strong>1.</strong>5<br />

1<br />

0.05<br />

#20144<br />

#20146<br />

a)<br />

a)<br />

b)<br />

ρ ≈ 0.07<br />

r ≈ r dep ≈ 0.28<br />

P ECH<br />

0<br />

0.15 0.25 0.35 0.45<br />

Time (s)<br />

a)<br />

200<br />

100<br />

0<br />

200<br />

100<br />

PECH (kW)<br />

PECH (kW)<br />

Fig. <strong>1.</strong>3 - Evolution in time of a) electron temperature on axis and at the deposition radius; b) temperature<br />

profile for two discharges characterised by very different profile shapes. The heat wave is launched at the<br />

EC wave absorption radius, which is well inside the flat region for shot #20144 and in the steep region in for<br />

shot #20146.<br />

Te (keV)<br />

3.5<br />

3<br />

2.5<br />

2<br />

<strong>1.</strong>5<br />

1<br />

0.5<br />

t = 0.10 ÷ 0.17 s<br />

δt = 0.1 s<br />

#20144<br />

#20146<br />

0<br />

0.7 0.8 0.9 1 <strong>1.</strong>1 <strong>1.</strong>2 <strong>1.</strong>3<br />

R(m)<br />

b)

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