Neoclassical Transport in the Helical Reversed-Field Pinch

M. Gobbin, G. Spizzo, L. Marrelli, and R. B. White
Phys. Rev. Lett. 105, 195006 – Published 4 November 2010

Abstract

Test particle evaluation of the diffusion coefficient in a fusion plasma in the reversed-field pinch (RFP) configuration shows distinct similarities with stellarators when the plasma spontaneously evolves towards a helical shape. The almost total absence of superbanana particles at the levels of helical deformation seen in experiment (Bh/B=10%) causes transport to be proportional to collision frequency (at low collisions). This fact excludes the possibility that the minimum conceivable transport could be inversely proportional to collision frequency, which is typical of unoptimized stellarators. This result strengthens the perspectives of the helical RFP as a fusion configuration.

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  • Received 7 June 2010

DOI:https://doi.org/10.1103/PhysRevLett.105.195006

© 2010 The American Physical Society

Authors & Affiliations

M. Gobbin1,*, G. Spizzo1,†, L. Marrelli1, and R. B. White2

  • 1Consorzio RFX, Euratom-ENEA Association, Corso Stati Uniti, 4 35127 Padova-Italy
  • 2Plasma Physics Laboratory, Princeton University, P.O. Box 451, Princeton, New Jersey 08543 USA

  • *marco.gobbin@igi.cnr.it
  • gianluca.spizzo@igi.cnr.it

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Vol. 105, Iss. 19 — 5 November 2010

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