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a bundle of projection lines, in particular, half straights. Second, we place the projection plane
(i) at maximum distance from
O
∗
at the North Pole to coincide with the tangential plane
T
N
S
2
R
,
(ii) at the center
2
R
as the equatorial plane, and (iii) at minimum distance from
O
∗
at the South Pole to coincide with the tangential plane
T
N
S
O
of the sphere
S
2
R
. Note that the projection lines
2
intersect the sphere
R
at
P
, while the projection plane is intersected at
p
. The perspective center
O
∗
is at distance
D
from the origin
S
2
O
∗
,
O
of the sphere
S
R
or at height
H
above S, measured by S
such that
D
=
R
+
H
holds.
Question: “How to find the polar coordinate
r
=
f
(
Δ
)in
Figs.
5.10
,
5.11
,and
5.12
,where
Δ
=
π/
2
Φ
is the spher-
ical colatitude and
Φ
is the spherical latitude of the point
P
−
2
R
?” Answer: “Consult the sub-sections that follow,
which compactly present the case studies for the individual
geometrical situations.”
∈
S
O
∗
N
/
O
∗
Q
is the fundament for the
Note that in all these cases the
perspective ratio r/QP
=
answer to the well-posed question.
Fig. 5.10.
Spherical vertical section, general normal perspective mapping of the sphere to the tangential plane
at the North Pole, projection plane at maximal distance
5-241 Case 1: Northern Tangential Plane (Tangential Plane at Maximal Distance)
This situation is shown in Fig.
5.10
. With reference to Boxes
5.7
and
5.8
,wederivethegeneral
form of the parameterized mapping
r
=
f
(
Δ
). Note that
Q
=
π
(
P
) is the point generated by an
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