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Table 6.1 Direct solution of the Gauss projection: sample computation
Computational results (m)
6 zones
Ellipsoidal
parameters
3 zones
Given data
B ᄐ 40 58 0 32.33 00
L ᄐ 100 10 0
20.11 00
Krassowski Ellipsoid x ᄐ 4,538,610.951 x ᄐ 4,538,610.951
y ᄐ 98,666.625 y ᄐ 98,666.625
y false ᄐ 17, 598, 666.625 y false ᄐ 33, 598, 666.625
GRS75 Ellipsoid
x ᄐ 4,538,532.847
x ᄐ 4,538,532.847
y
98,665.022
y
98,665.022
y false
17, 598, 665.022 y false
33, 598, 665.022
GRS80 Ellipsoid
x
4,538,530.729
x
4,538,530.729
y
98,664.975
y
98,664.975
y false
17 598 664.975
y false
33, 598 664.975
35 26 0 40.38 00
B
Krassowski Ellipsoid x
3,925,560.035
x
3,924,588.054
115 08 0
51.22 00
L
y
168,198.578
y
104,193.075
y false
20, 331, 801.422 y false
38, 604, 193.075
GRS75 Ellipsoid
x
3,925,492.277
x
3,924,520.313
y
168,195.836
y
104,191.377
y false
20, 331, 804.164 y false
38, 604, 191.377
GRS80 Ellipsoid
x
3,925,490.447
x
3,924,518.483
y
168,195.757
y
104,191.328
y false
20, 331, 804.243 y false
38, 604, 191.328
Fig. 6.9 Inverse solution of
Gauss projection
footprint latitude and is denoted by B f , whose corresponding isometric latitude is q f .
The meridian arc length from the equator to B f is X f ; namely, the ordinate of point
F is x
X f , and the value of B f can be obtained reversely from X f according to the
formula for meridian arc length.
According to the symmetry property of the Gauss projection and the second
condition for the projection, the series can be directly written according to ( 6.23 ):
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