Ray-tracing images of our jets in total intensity when each jet is viewed edge-on. The images highlight similar epochs in the jet’s evolution during each 3D RMHD simulation at 86 GHz. From left to right: proportionality of the NTEs to the fluid’s density, internal energy density, and magnetic energy density. From top to bottom: purely poloidal magnetic field, helical magnetic field, and purely toroidal magnetic field. The ray-traced images are convolved with a Gaussian beam indicative of the resolution of the GMVA and with a Gaussian noise floor of 10⁻⁴ Jy beam⁻¹.