These animations display the imprint that homogeneous but anisotropic Bianchi models induce in the cosmic microwave background (CMB). scalars_movie.mp4 : Bianchi VIIh/VII0 scalar modes, imprint on the CMB for varying morphology parameters (matter and dark-energy density, rotation scale of shear principal axes) vectors_movie.mp4: Bianchi VIIh/VII0 vector modes, imprint on the CMB for varying morphology parameters (matter and dark-energy density, rotation scale of shear principal axes) tensor_movie.mp4: Bianchi VIIh/VII0 regular tensor modes, imprint on the CMB for varying morphology parameters (matter and dark-energy density, rotation scale of shear principal axes) Additional fixed parameters for the three animations above: cold-dark-matter physical density: 0.112 baryon physical density: 0.226 Pattern orientation additionally fixed to put spiral in full view _____________________________ SVTT_movie.mp4: combinations of Bianchi VIIh/VII0 scalar, vector, regular and irregular tensor modes for varying relative amplitudes of these degrees of freedom and phase angle. Additional fixed parameters: cold-dark-matter physical density: 0.112 baryon physical density 0.0226 matter density: 0.27 dark energy density: 0.7 rotation scale of shear principal axes: 0.5 Pattern orientation additionally fixed to put spiral in full view