DF Tau as observed with ALMA (upper panels), as shown from left to right: 1.3 mm dust continuum emission, ¹²CO J=2-1 moment 0, and ¹²CO J=2-1 moment 1. These datasets were presented in Grant et al. (2024b). In the lower panels show the MIRI-MRS observations, from left to right: The 12.51 μm continuum emission, the moment 0 frequency of [Ne II], and the velocity at peak emission of [Ne II] relative to the rest frequency. The ellipse in the corner of each panel represents the FWHM of the PSF of each image. The box at the center of panels (d, e, f) shows the spatial extent of panels (a,b,c).