1. Density impact on toroidal rotation in Tore Supra: experimental observations and theoretical investigation
- Author
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Bernardo, J., Fenzi, C., Bourdelle, C., Camenen, Y., Ă Arnichand, H., Bizarro, Joao P. S., Cortes, S., Garbet, Xavier, Ă Guimaraes-Filho, Z. O., Aniel, Thierry, Artaud, J-F, Clairet, F., Ă Cottier, P., Gunn, J., Lotte, P., Team, Tore Supra, Institut de Recherche sur la Fusion par confinement Magnétique (IRFM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Physique des interactions ioniques et moléculaires (PIIM), Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS), and Département de Recherche sur la Fusion Contrôlée (DRFC)
- Subjects
[PHYS]Physics [physics] ,Physics ,Toroid ,Plasma ,Tore Supra ,Condensed Matter Physics ,Rotation ,01 natural sciences ,Instability ,010305 fluids & plasmas ,Magnetic field ,Amplitude ,Nuclear Energy and Engineering ,Physics::Plasma Physics ,0103 physical sciences ,Electric current ,Atomic physics ,010306 general physics - Abstract
International audience; The effect of plasma density on toroidal rotation was examined in ă density ramp-up experiments at a plasma current of 1 MA and a toroidal ă magnetic field of 3.6 T in Tore Supra ohmic discharges. Experimental ă measurements have shown that the toroidal rotation amplitude is reduced ă at all radii when increasing the plasma density, although it remains in ă the countercurrent direction. Neoclassical predictions including ă ripple-induced toroidal friction are in qualitative agreement with such ă observations. However, in the core (r/a < 0.5) the plasma accelerates at ă n(l) similar to 3 x 10(19) m(-2) and breaks again above n(l) similar to ă 3.5 x 10(19) m-2. This rotation bifurcation did not appear to be ă correlated to a possible influence of the sawtooth activity. ă Nonetheless, quasi-linear gyrokinetic simulations have shown that the ă transition of the nature of linear microinstabilities from ITG-TEM to ă pure ITG occurs at n(l) similar to 3 x 10(19) m-2, which could indicate ă a change on the turbulence driven contributions and explain the ă deviation from neoclassical predictions in the plasma core.
- Published
- 2015
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