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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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