The dynamics of perfect fluid spacetime geometries which exhibit local
rotational symmetry (LRS) are reformulated in the language of a 1 + 3
'threading' decomposition of the spacetime manifold, where covariant
fluid and curvature variables are used. This approach presents a neat
alternative to the orthonormal frame formalism. The dynamical equation
s reduce to a set of differential relations between purely scalar quan
tities. The consistency conditions are worked out in a transparent way
. We discuss their various subcases in detail and focus in particular
on models with higher symmetries within the class of expanding spatial
ly inhomogeneous LRS models, via a consideration of functional depende
nces between the dynamical variables.