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1 - Nuclear Sciences and Applications - IAEA

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<strong>IAEA</strong>-CN-50/A-IV-l 219<br />

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FIG. 3. Profiles of electron density at 3.0 <strong>and</strong> 4.2 s <strong>and</strong> electron temperature (Thomson scattering) <strong>and</strong><br />

ion temperature (charge exchange spectroscopy) at 4.2 s for pellet (P) <strong>and</strong> no-pellet (NP) cases. Timing<br />

of fuelling <strong>and</strong> heating as in Fig. 1. Heating power (P): RF - 12.5 MW, NBI - 5 MW;<br />

(NP): RF - 11.5 MW, NBI - 5 MW (pulse numbers: 17749/17747). Solid squares: pellet case ion temperature;<br />

open squares: no-pellet case ion temperature.<br />

plasma core. Similarly the enhancement in central electron <strong>and</strong> ion heating is<br />

diminished as the neutral beam heating power is increased. At high density in JET,<br />

power deposition profiles for 40keV/nucleon beam heating are not strongly<br />

peaked within the plasma core.<br />

Fig. 3 shows density <strong>and</strong> temperature profiles after pellet injection <strong>and</strong> near the<br />

termination of the enhanced period for a pellet <strong>and</strong> no-pellet pulse. Within a<br />

central region of approximately 0.7m diameter, the profiles differ both in<br />

magnitude <strong>and</strong> scale length. In the pellet case, although the central value of the<br />

electron density decays from 1.35 to 0.6x 1 CP'ta- 3 during the first 1 s of the heating<br />

pulse, the gradient scale length of the core density perturbation has only increased<br />

from 0.5 to 0.6m. The gradient scale length of the temperature profile, both for<br />

ions <strong>and</strong> electrons, is more than 2x smaller in the pellet case than in the no-pellet<br />

case. The electron temperature profile differs markedly from a triangular shape.<br />

The concurrence of higher density <strong>and</strong> temperature within this core plasma<br />

implies enhanced central electron pressure <strong>and</strong> pressure gradients as illustrated in<br />

Fig. 4. The ideal mhd ballooning stability of the equilibria corresponding to these<br />

3.0 s<br />

4.2s<br />

4.2 s<br />

-<br />

-<br />

-

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