Rotation dynamics with \& without Internal Transport Barriers

POSTER

Abstract

We investigate the dynamics of both poloidal and toroidal flows in the presence (or absence) of a reversed safety factor profile through a scan in the incoming heat power applied to the plasma. Doing so, it incidentally also addresses the question of a power threshold for a self-consistent ITB formation in gyrokinetic modeling. As a prime candidate to drive the system away from its neoclassical prediction, we recently showed evidence of turbulence-generated poloidal rotation, consistently with earlier theories. Accurate calculation of the radial electric field is central. Accordingly, description of the mean profile dynamics, as done in {\it full--$f$} flux-driven models is shown to take on a very prominent role. The study is performed using both the \textsc{Gysela} and \textsc{Xgc--1} gyrokinetic codes with Enhanced Reverse Shear (ERS)-like parameters.

Authors

  • Guilhem Dif-Pradalier

    • Center for Astrophysics and Space Sciences, UCSD, La Jolla, CA 92093, USA
  • Patrick H. Diamond

    • Center for Astrophysics and Space Sciences, UCSD, La Jolla, CA 92093, USA
  • C.S. Chang

    • Courant Institute of Mathematical Sciences, New York University, NY 10012, USA
  • S. Ku

    • Courant Institute of Mathematical Sciences, New York University, NY 10012, USA
  • Y. Sarazin

    • Association Euratom-CEA, CEA/IRFM, F-13108 St. Paul-lez-Durance cedex, France
  • V. Grandgirard

    • Association Euratom-CEA, CEA/IRFM, F-13108 St. Paul-lez-Durance cedex, France
  • J. Abiteboul

    • Association Euratom-CEA, CEA/IRFM, F-13108 St. Paul-lez-Durance cedex, France
  • X. Garbet

    • Association Euratom-CEA, CEA/IRFM, F-13108 St. Paul-lez-Durance cedex, France
  • Ph. Ghendrih

    • Association Euratom-CEA, CEA/IRFM, F-13108 St. Paul-lez-Durance cedex, France
  • A. Strugarek

    • Association Euratom-CEA, CEA/IRFM, F-13108 St. Paul-lez-Durance cedex, France