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Interpretation of the I-Regime and transport associated with relevant heavy particle modes

Author(s)
Coppi, Bruno; Zhou, T.
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Abstract
The excitation of a novel kind of heavy particle [1, 2] mode at the edge of the plasma column is considered as the signature of the I-con nement Regime [3{7]. The outward transport of impurities produced by this mode is in fact consistent with the observed expulsion of them from the main body of the plasma column (a high degree of plasma purity is a necessary feature for fusion burning plasmas capable of approaching ignition). Moreover, the theoretically predicted mode phase velocity, in the direction of the electron diamagnetic velocity, has been con rmed by relevant experimental analyses [8] of the excited uctuations (around 200 kHz). The plasma \spontaneous rotation" in the direction of the ion diamagnetic velocity is also consistent, according to the Accretion Theory [9] of this phenomenon, with the direction of the mode phase velocity. Another feature of the mode that predicted by the theory is that the I-Regime exhibits a knee of the ion temperature at the edge of the plasma column but not one of the particle density as the mode excitation factor is the relative main ion temperature gradient exceeding the local relative density gradient. The net plasma current density appearing in the saturation stage of the relevant instability, where the induced particle and energy uxes are drastically reduced, is associated with the signi cant amplitudes of the poloidal magnetic eld uctuations [6, 7] observed to accompany the density uctuations. The theoretical implications of the signi cant electron temperature uctuations [10] observed are discussed.
Date issued
2012-01
URI
http://hdl.handle.net/1721.1/71984
Department
Massachusetts Institute of Technology. Department of Physics
Journal
Physics of Plasmas
Publisher
American Institute of Physics (AIP)
Citation
Coppi, B., and T. Zhou. “Interpretation of the I-Regime and transport associated with relevant heavy particle modes.” Physics of Plasmas 19.1 (2012): 012302.
Version: Author's final manuscript
ISSN
1070-664X
1089-7674

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