The flow structures generated and drag experienced by a rigid cylinder
moving in an arbitrary direction through a rotating electrically cond
ucting fluid in the presence of an applied magnetic field are investig
ated, with the aim of understanding better the nature of the small-sca
le flow in the core of the Earth which may be responsible for maintain
ing the geomagnetic field through dynamo action. Three cases are consi
dered in the limit of small Rossby and magnetic Reynolds numbers. In t
he case of very weak rotation, the possible flow structures consist of
a thin Hartmann layer and a long wake extending in the direction of t
he magnetic field, in which Lorentz and viscous forces balance, but on
ly the long wake plays a dynamical role. The dominant drag force is ex
perienced for motion that cuts magnetic lines of force. Motion of the
cylinder parallel to its axis induces a much weaker drag, while that i
n the direction of the magnetic field induces none to dominant order.
The cylinder also experiences weak lateral forces due to the Coriolis
effect. In the case of weak rotation, the balance in the long wake is
now magnetostrophic: between Lorentz and Coriolis forces. The drag is
qualitatively identical to that in the first case, but the drag induce
d by motion parallel to the axis of the cylinder is increased, though
still smaller than that for motions cutting magnetic lines of force. I
n the case of strong rotation, the flow structures consist of a thin E
kman layer and a foreshortened Taylor column extending in the directio
n of the rotation axis. In this column, the force balance is again mag
netostrophic. Again only the large-scale structure plays a dynamical r
ole. Motion of the cylinder perpendicular to its axis induces a larger
drag than does motion parallel to its axis. The cylinder also experie
nces large lateral Coriolis forces.