Ruffolo D.Thepthong P.Pongkitiwanichakul P.Roy S.Pecora F.Bandyopadhyay R.Chhiber R.Usmanov A.V.Stevens M.Badman S.Romeo O.Wang J.Goodwill J.Goldstein M.L.Matthaeus W.H.Mahidol University2024-12-142024-12-142024-12-10Astrophysical Journal Letters Vol.977 No.1 (2024)20418205https://repository.li.mahidol.ac.th/handle/20.500.14594/102383Using Parker Solar Probe data from orbits 8 through 17, we examine fluctuation amplitudes throughout the critical region where the solar wind flow speed approaches and then exceeds the Alfvén wave speed, taking account of various exigencies of the plasma data. In contrast to WKB theory for noninteracting Alfvén waves streaming away from the Sun, the magnetic and kinetic fluctuation energies per unit volume are not monotonically decreasing. Instead, there is clear violation of conservation of standard WKB wave action, which is consistent with previous indications of strong in situ fluctuation energy input in the solar wind near the Alfvén critical region. This points to strong violations of WKB theory due to nonlinearity (turbulence) and major energy input near the critical region, which we interpret as likely due to driving by large-scale coronal shear flows.Earth and Planetary SciencesPhysics and AstronomyArticleSCOPUS10.3847/2041-8213/ad97272-s2.0-8521121596620418213