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1 - Nuclear Sciences and Applications - IAEA

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642 ALLADIO et al.<br />

3<br />

ID<br />

10 2<br />

10'<br />

10°<br />

10 1<br />

". 0.5<br />

tu<br />

• a a o a<br />

•V.<br />

3 FAST<br />

•SLOW<br />

2 4 6 8 10 12 14 16<br />

ne/10"(cm- 3 )<br />

FIG. 4. (a) Intensity ofECE at a> = 1.6 oice, normalized to RF power as a function of density for two<br />

different spectra; (b) Ratio ofECE intensities at a — 1.4 uce <strong>and</strong> a> = 1.6 uce as a function of density.<br />

Radiation is only emitted in this range by fast electrons through the down shifted<br />

second harmonic emission. On the assumption that the perpendicular velocity is much<br />

lower than the parallel one, a precise n0 value corresponds to each detected frequency.<br />

In particular, nB = 1.4 corresponds to co = 1.4 wce <strong>and</strong> ny = 1.67 to<br />

w = 1.6 oice.<br />

ECE measurements are available for BT = 8 T <strong>and</strong> n,. < 1.4 X 10 14 cm" 3 .<br />

In this density range, the power component with nj = 1.67 can reach the plasma<br />

centre while the component with n] = 1.4 is converted to fast wave before reaching<br />

the plasma core.<br />

In Fig. 4(a), we show the ECE intensity at w = 1.6 wce normalized to RF<br />

power both for fast <strong>and</strong> slow spectra. As is expected, the fast spectrum yields a

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