Abstract
A simple equation to determine the distance on a meridian is developed using complex numbers. Very great accuracy is obtainable. Inverse and other forms are also presented.
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Abbreviations
- a, b:
-
major, minor semiaxes of meridian ellipse
- n:
-
(a-b)/(a+b)
- A:
-
a(1+1/8n2)2/(1+n)
- B:
-
9(1−3/8n2). k=−2/13B
- B1 :
-
1−3/8n2
- C:
-
1−9/16n2
- E1, E2 :
-
errors. See (3) and (16)
- F, G, H:
-
See (5)
- M:
-
meridional distance from the equator
- θ:
-
M/A
- ϕ:
-
geodetic latitude
- u:
-
parametric latitude
- x, y:
-
Cartesian or complex number components
- r, a:
-
polar representation
- i:
-
(−1)1/2
Reference
New Geodetic Tables for Clarke's Figure of 1880 with Transformations to Madrid 1924 and Other Figures. R.G.S. Technical Series No. 4. London 1927. p.x.
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Bowring, B.R. New equations for meridional distance. Bull. Geodesique 57, 374–381 (1983). https://doi.org/10.1007/BF02520940
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DOI: https://doi.org/10.1007/BF02520940