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
RΛ
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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