Experimental scaling of compressional Alfvén eigenmode stability

Abstract Both co-propagating and counter-propagating compressional Alfvén eigenmodes (CAE) are relatively ubiquitous in NSTX plasmas with toroidal field strengths of ⩽4.65 kG, but are largely absent in the NSTX-U plasmas with toroidal fields of 5.7–5.9 kG. In this paper we will study the co-propagating CAE. We show that the co-propagating CAE are seen with frequencies 0.4 ω ci ⩽ ω CAE ⩽ ω ci (with the exception of a few unique shots), that toroidal mode numbers are relatively high, ranging from 6 ⩽ n ⩽ 17, and that for plasmas with toroidal field greater than about 3.8 kG, are present for ≈2 2 which is consistent with the relative lack of CAE in the NSTX-U plasmas from the B tor ≈ 5.9 kG shots which typically have V beam / V A k | | / k < 1. While calculations of fast-ion drive are beyond the capabilities of this code, by coupling the CAEk code to a simple full-orbit code for the fast-ions we can estimate that the co-propagating CAE are primarily resonant with beam fast-ions with energies below ≈30 keV and that there are typically several strong resonances for each mode. We show that the fast-ion distribution as calculated with TRANSP has gradients at the resonant fast-ion parameters potentially capable of providing drive for the modes.