


and
,
where the
optical flow is measured to be
and
. We showed that
purely from the directions of
these flow vectors
(and without using their magnitudes), one may constrain the direction
of translation and the axis of rotation to some subset of the image
sphere. In fact, the direction of translation must lie within a lune (the name in geometry for
these wedge-shaped regions)
shown as the shaded region in the left diagram
below.
is bounded by two
great circles
and
, such that
lies in the plane of
circle
and
lies in the plane of
circle
. Likewise, the
rotation axis must lie within the lune (shaded region
) bounded by two
other great circles
and
where
is now perpendicular
to the plane of circle
, and
is also
perpendicular to the plane of the circle
.

, and either
or
will give the normal vector of a plane in
which translation
is constrained to
lie. (The intersection of that plane and the image sphere gives the
great circle C.) Furthermore,
two or more such
antipodal flow pairs will then give multiple such planes (or great
circles) and
translation may be found from taking the intersection of these planes.
Once translation has been found, rotation may be recovered also via a
second step.
