These simulation movies were made during Federrath's undergraduate studies and show different initial conditions for the thermonuclear burning front inside the exploding star. Note that these movies are in the co-moving frame of the burning front.
c0 supernova explosion model:
c3 (three-wave perturbation) supernova explosion model:
c3 full-star (4pi) supernova explosion model:
popcorn (random perturbations) supernova explosion model:
popcorn full-star (4pi) supernova explosion model: