Geography Reference
In-Depth Information
Fig. 13.2. Equal area pseudo-cylindrical mapping. Mollweide projection
Table 13.1 The solution of the special Kepler equation
Φ
t
Φ
t
Φ
t
Φ
t
0
30
60
90
0
0.41585
0.86698
π/ 2
10
40
70
0.13724
0.55974
1.03900
20
50
80
0.27548
0.70910
1.23877
The solution of the special Kepler equation is shown in Table 13.1 . Thus, the final mapping equa-
tions are provided by ( 13.22 ). The left principal stretches are best determined by the numerical
solution of the biquadratic characteristic equation based on the left Jacobi matrix ( 13.23 )aswell
as the left Cauchy-Green deformation matrix ( 13.24 )(G r =I 2 ).
x = 2 2
π
cos t, y = R 2sin t,
(13.22)
2 t + sin 2 t = π sin Φ,
J l =
= R 2
π
2cos t
,
πΛ tan t cos Φ
2cos t
(13.23)
π 2 cos Φ
4cos t
0
 
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