Fiducial galaxy orbits adopted for studying the interaction of galaxy model G1a with the three different galaxy clusters constructed for the study. a) Trajectories of the galaxy in clusters A, B, and C, scaled to the virial radius of the corresponding cluster. b) Time evolution of the distance of the galaxy to the corresponding cluster centre. c) Effective inclination angle of the galaxy (angle between the spin vector of the disk and its instantaneous velocity vector).