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2000 PROGRESS REPORT - ENEA - Fusione

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1. Magnetic Confinement<br />

be obtained with an ECRH power as<br />

low as P ECRH ≈0.15 P OH , provided<br />

that the mode is rotating. Figure 1.32<br />

shows that stabilization with co-and<br />

counter-ECCD is identical to the one<br />

achieved with perpendicular launch,<br />

provided that the absorption radius is<br />

the same in all cases. Heating is<br />

therefore the dominant stabilizing<br />

term, CD effects being negligible in<br />

this case. TM dynamics can be<br />

modelled (fig. 1.33) by using a<br />

Rutherford-type equation [1.16], in<br />

which the change rate of the island<br />

width is dependent on the balance<br />

between de-stabilizing terms, related<br />

to the current density and pressure<br />

profiles, and stabilizing terms due to<br />

ECRH and ECCD.<br />

The beneficial effects of mode<br />

suppression on energy confinement<br />

are shown in fig. 1.34, where two<br />

discharges are compared, which are<br />

almost identical in the ohmic phase,<br />

the only difference being that ECRH<br />

absorption occurs in slightly<br />

different positions. In shot #18004,<br />

absorption is ≈3 cm internal to<br />

the island O-point, while in shot<br />

#18015 EC absorption is<br />

correctly positioned inside the<br />

island. In this case of a precise<br />

alignment, stabilization occurs<br />

on the expected resistive time<br />

scale, and a much better thermal<br />

and particle confinement is<br />

observed.<br />

Sawteeth are stabilized with<br />

P ECRH >P OH (≈2.2 times) if<br />

r dep >r inv , with a delay which is<br />

dependent on r dep -r inv and<br />

consistent with resistive diffusion<br />

times (fig. 1.30 and 1.35). A<br />

broadening of J(r), with a slow<br />

decrease in central ohmic heating<br />

Fig. 1.32 - T e at plasma centre<br />

and at r≈a/2 (left), and Mirnov<br />

oscillations (right) with co-ECCD<br />

injection (top), counter injection<br />

(bottom), and perpendicular<br />

launch (centre)<br />

keV keV keV<br />

T/s<br />

100<br />

-100<br />

50<br />

-50<br />

50<br />

-50<br />

20<br />

-20<br />

δR = -3 cm<br />

δR = 0 cm<br />

δR = 1 cm<br />

δR = 2 cm<br />

0.45 0.50 0.55 0.60 0.65 0.70<br />

Time (s)<br />

Fig. 1.31 - 4 Mirnov oscillations with different values of δR=R abs -<br />

Fig. 1.31<br />

R O–point . ECRH starts at 0.5 s. From top to bottom: δR=-3 cm, 0, +1<br />

cm and +2 cm<br />

4<br />

3<br />

2<br />

4.0<br />

3.5<br />

3.0<br />

2.5<br />

4<br />

3<br />

2<br />

0.8 0.9 1.0<br />

Time (s)<br />

10 2 T/s<br />

10 2 T/s<br />

10 2 T/s<br />

1<br />

0<br />

-1<br />

1<br />

0<br />

-1<br />

1<br />

0<br />

-1<br />

0.8 0.9 1.0<br />

Time (s)<br />

Fig. 1.32<br />

31

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