Redshift evolution of the magnetic anisotropy β_A and Brunt-Väisälä profiles for six example halos with pronounced dips in β_A from TNG-Cluster. There is considerable diversity in their evolution: dips can exist at z = 0, vanish and re-appear at higher redshifts, grow less weak and eventually vanish, or first grow stronger before later vanishing. There are also clusters that do not have a dip in β_A at z = 0, but had one at higher redshift, while the radial position of the dips itself can move with redshift.