Theory and lattice-Boltzmann simulations are used to examine the effects of
fluid inertia, at small Reynolds numbers, on flows in simple cubic, face-c
entred cubic and random arrays of spheres. The drag force on the spheres, a
nd hence the permeability of the arrays, is determined at small but finite
Reynolds numbers, at solid volume fractions up to the close-packed limits o
f the arrays. For small solid volume fraction, the simulations are compared
to theory, showing that the first inertial contribution to the drag force,
when scaled with the Stokes drag force on a single sphere in an unbounded
fluid, is proportional to the square of the Reynolds number. The simulation
s show that this scaling persists at solid volume fractions up to the close
-packed limits of the arrays, and that the first inertial contribution to t
he drag force relative to the Stokes-flow drag force decreases with increas
ing solid volume fraction. The temporal evolution of the spatially averaged
velocity and the drag force is examined when the fluid is accelerated from
rest by a constant average pressure gradient toward a steady Stokes flow.
Theory for the short- and long-time behaviour is in good agreement with sim
ulations, showing that the unsteady force is dominated by quasi-steady drag
and added-mass forces. The short- and long-time added-mass coefficients ar
e obtained from potential-flow and quasi-steady viscous flow approximations
, respectively.