Mapping electron temperatures within H ii regions across four of the PHANGS-MUSE galaxies (NGC 1672, NGC 1365, NGC 4254, and NGC 628). Coverage is not just limited to spiral arms, but samples the full inner star-forming disks in our sample of galaxies. NGC 1365 (Ho et al. 2017) and NGC 1672 (Kreckel et al. 2019; Ho et al. 2019) have both reported azimuthal abundance variations, with enhanced abundances along the spiral arms, which is supported by decreased T_e along the eastern arms in both galaxies. The more flocculent galaxy NGC 4254 and the bar-free grand design spiral galaxy NGC 628 both show some tentative azimuthal trends, but the connection with spiral structure is more tenuous. Small-scale (<1 kpc) homogeneity in the temperature distribution is reminiscent of the trends for more uniform metallicity on small scales reported in Kreckel et al. (2020) for these targets.