Turbulence and Zonal-Flow Impact in the Madison Symmetric Torus in Quasi-Single Helicity

Reversed-Field Pinches (RFPs) operating in the Quasi-Single-Helicity (QSH) magnetic geometry exhibit significant improvements in confinement time compared to standard discharges due to the efficient saturation of large-scale tearing modes. This modification to the magnetic geometry and profiles introduces new instabilities which drive transport. This work focuses on diagnosing the microinstabilities and microturbulence in a non-reversed Madison Symmetric Torus QSH experiment. Local gyrokinetic simulations are conducted with the GENE code to identify the dominant instabilities as ion-temperature-gradient (ITG) and density-gradient-driven trapped-electron-mode (TEM) at core and edge radial locations, respectively. It has been previously observed in the RFP (Williams PoP 2017) that residual tearing fluctuations in RFPs degrade zonal flows; the degree to which this affected turbulence and transport in that work depended on the driving instability. While initial investigations reveal strong zonal flow activity, an ad-hoc magnetic perturbation is employed to model magnetic fluctuations present in the RFP. These fluctuations degrade the zonal flow structure, resulting in a more substantial increase in electrostatic fluxes for the TEM-dominated position than for its ITG counterpart.