1. magnetic confinement - ENEA - Fusione
1. magnetic confinement - ENEA - Fusione
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)