Gyrokinetic simulation of momentum transport with residual stress from diamagnetic level velocity shears

R. E. Waltz, G. M. Staebler, W. M. Solomon

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Abstract

Residual stress refers to the remaining toroidal angular momentum (TAM) flux (divided by major radius) when the shear in the equilibrium fluid toroidal velocity (and the velocity itself) vanishes. Previously [Waltz, Phys. Plasmas 14, 122507 (2007); errata 16, 079902 (2009)], we demonstrated with GYRO [Candy and Waltz, J. Comp. Phys. 186, 545 (2003)] gyrokinetic simulations that TAM pinching from (ion pressure gradient supported or diamagnetic level) equilibrium E ×B velocity shear could provide some of the residual stress needed to support spontaneous toroidal rotation against normal diffusive loss. Here we show that diamagnetic level shear in the intrinsic drift wave velocities (or profile shear in the ion and electron density and temperature gradients) provides a comparable residual stress. The individual signed contributions of these small (rho-star level) E × B and profile velocity shear rates to the turbulence level and (rho-star squared) ion energy transport stabilization are additive if the rates are of the same sign. However because of the additive stabilization effect, the contributions to the small (rho-star cubed) residual stress is not always simply additive. If the rates differ in sign, the residual stress from one can buck out that from the other (and in some cases reduce the stabilization.) The residual stress from these diamagnetic velocity shear rates is quantified by the ratio of TAM flow to ion energy (power) flow (M/P) in a global GYRO core simulation of a null toroidal rotation DIII-D [Mahdavi and Luxon, Fusion Sci. Technol. 48, 2 (2005)] discharge by matching M/P profiles within experimental uncertainty. Comparison of global GYRO (ion and electron energy as well as particle) transport flow balance simulations of TAM transport flow in a high-rotation DIII-D L-mode quantifies and isolates the E ×B shear and parallel velocity (Coriolis force) pinching components from the larger diffusive parallel velocity shear driven component and the much smaller profile shear residual stress component.

Original languageEnglish
Article number042504
JournalPhysics of Plasmas
Volume18
Issue number4
DOIs
StatePublished - Apr 2011
Externally publishedYes

Funding

This work was supported by the U.S. Department of Energy under Grant No. DE-FG02-95ER54309. We wish to thank J. Candy and E.A. Belli for new coding consistently computing all ion toroidal and poloidal velocity profiles from experimental radial electric field profile data via the NEO (Ref. ) delta-f neoclassical code.

FundersFunder number
U.S. Department of EnergyDE-FG02-95ER54309

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