Using the induction equation, we investigate the generation of electro
magnetic fields by the motional electromagnetic induction due to ocean
currents. In this paper, solutions are presented for a linear inducti
on equation for the magnetic flux density vector which contains prescr
ibed time-independent ocean current and conductivity fields. Once the
magnetic Bur density is known, the electric held and electric current
density are easily obtained by differentiation. Solutions are given fo
r several examples of idealized flow which include: 1) Vertically and
horizontally sheared plane-parallel flow with depth-dependent conducti
vity; 2) A simple Stommel circulation gyre; and 3) Symmetric gyres. Th
e results indicate that typical ocean current features induce magnetic
fields with magnitudes reaching 100's of nT within the water and abou
t 1-10 outside of the water. For the case of a field of gyres, the oce
an-induced magnetic fields decay away from the ocean on spatial scales
set by the horizontal scale of the ocean feature. At the altitudes of
magnetic field satellite surveys, ocean-induced magnetic fields may r
etain values of a few nT, which are strong enough to be detected. Thus
it is concluded that satellite observations of the earth's main magne
tic field and, in particular, the observed temporal variations, could
be affected by the ocean circulation.