A recent study of Karate (1999) suggests that deformation induced in the in
ner core by electromagnetic (Lorentz) forces may account for the developmen
t of seismic anisotropy. The viability of this proposal depends on whether
Lorentz forces can sustain persistent flow within the inner core. We explor
e this question by establishing the conditions for static equilibrium when
Lorentz forces are present. We find that the requirements for thermodynamic
and hydrostatic equilibrium are incompatible at the surface of the inner c
ore. However, the resulting deformation redistributes mass in the interior
so as to minimize steady flow. Numerical calculations show that the flow be
comes vanishingly weak and is confined to the top of the inner core. Strain
s in the interior are small and the alignment of crystals is insufficient t
o explain the anisotropy inferred from seismological observations.