There are two ways to introduce horizons in anisotropic spatially homogeneo
us universes: in the first one the anisotropy appears directly in the defin
itions, whereas in the second way a "mean horizon" is defined, with a conse
quent loss of information on the direction. In this work we give the expres
sion of horizons in all nine Bianchi types, using the Misner parametrizatio
n of metric. We examine, also, some examples regarding the Bianchi type I;
in each case the achieved expressions are compared with the correspondent m
ean horizons.