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the interior of
D
, respectively. The silhouette for an object in the image plane
provides the outline of projection. If the object has a smooth surface, then
the silhouette provides occluding boundaries, where the surface orientation is
known. Though it has a problem, even then surface orientations can be made
known depending on the nature of the reflectance map, e.g., if the reflectance
map is a strictly monotonic function of gradients along
x
and
y
axes. David
Lee, however, considered the surface orientations known on the boundary
∂D
of the image domain that contains the occluding boundary.
7.5.1 Image Irradiance Equation
For a Lambertian surface illuminated by a single distant point source, the
reflectance map is
1+
pp
s
+
qq
s
1+
p
2
+
q
2
1+
p
s
+
q
s
R
(
p, q
)=
.
(7.32)
R
(
p, q
) is the function of surface gradient (
p, q
) and the gradient (
p
s
,q
s
) speci-
fies the direction of the source. The reflectance map tells the relation of image
brightness on surface orientation. In the image plane at a particular point
(
x, y
), we record the image irradiance
I
(
x, y
). It is proportional to the image
radiance at the corresponding point on the surface.
R
(
p, q
) is known as the
image radiance. Hence, by normalizing, we get the image irradiance equation
as
R
(
p, q
)=
I
(
x, y
)
.
(7.33)
If we take
f
(
x, y
)and
g
(
x, y
) as two different functions for
p
and
q
, then the
reflectance map can also be written as
R
(
f
(
x, y
)
,g
(
x, y
)) =
I
(
x, y
)
.
(7.34)
In the present case, (
x, y
)
D
. The function
R
(
f, g
) can be determined the-
oretically or experimentally if distribution of light sources, viewing geometry,
and intrinsic reflecting properties of the materials composing the surface are
known [80]. One easily note that in stereographic projection, the Northern
Hemisphere is projected into a plane, namely the
fg
plane, tangent to the
Gaussian sphere at the North Pole with the South Pole as the center of pro-
jection. As it is a bijection of the Northern Hemisphere onto a disc
S
of radius
2inthe
fg
-plane, points in
S
provide surface orientations of visible parts of
the object's surface. Points on the circumference of
S
are, therefore, the ori-
entations of the points on the occluding boundaries. Therefore, for any point
(
x, y
) on the occluding boundary, we must have,
∈
f
2
(
x, y
)+
g
2
(
x, y
)=4
.
(7.35)
One can assume for interior points (
x, y
)
∈
D
i
,
I
(
x, y
)
>
0 and, for occluding
boundary points, (
x, y
)
∈
∂D
,
I
(
x, y
)=0.
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