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Revision as of 17:30, 22 December 2013 editChienlit (talk | contribs)Extended confirmed users, Rollbackers33,649 edits ==See also== {{Portal|Atlas}} * List of map projections← Previous edit Revision as of 07:01, 14 April 2014 edit undoMaurice Carbonaro (talk | contribs)Extended confirmed users11,590 editsm Hyperlinked "(...) latitude (...)" and "(...) longitude (...)" to the corresponding articlesNext edit →
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:<math>y = \pm \pi \tan {\theta / 2 }</math> :<math>y = \pm \pi \tan {\theta / 2 }</math>


In all cases, <math>\phi\,</math> is the latitude, <math>\lambda\,</math> is the longitude, and <math>\lambda_0\,</math> is the central meridian of the projection. In all cases, <math>\phi\,</math> is the ], <math>\lambda\,</math> is the ], and <math>\lambda_0\,</math> is the central meridian of the projection.


==See also== ==See also==

Revision as of 07:01, 14 April 2014

Van der Grinten projection of the world.

The van der Grinten projection is a compromise map projection that is neither equal-area nor conformal. It projects the entire Earth into a circle, though the polar regions are subject to extreme distortion. The projection was the first of four proposed by Alphons J. van der Grinten in 1904, and, unlike most projections, is an arbitrary geometric construction on the plane. It was made famous when the National Geographic Society adopted it as their reference map of the world from 1922 until 1988.

The geometric construction given by van der Grinten can be written algebraically:

x = ± π ( A ( G P 2 ) + A 2 ( G P 2 ) 2 ( P 2 + A 2 ) ( G 2 P 2 ) ) P 2 + A 2 {\displaystyle x={\frac {\pm \pi \left(A\left(G-P^{2}\right)+{\sqrt {A^{2}\left(G-P^{2}\right)^{2}-\left(P^{2}+A^{2}\right)\left(G^{2}-P^{2}\right)}}\right)}{P^{2}+A^{2}}}\,}
y = ± π ( P Q A ( A 2 + 1 ) ( P 2 + A 2 ) Q 2 ) P 2 + A 2 {\displaystyle y={\frac {\pm \pi \left(PQ-A{\sqrt {\left(A^{2}+1\right)\left(P^{2}+A^{2}\right)-Q^{2}}}\right)}{P^{2}+A^{2}}}}

where x {\displaystyle x\,} takes the sign of λ λ 0 {\displaystyle \lambda -\lambda _{0}\,} , y {\displaystyle y\,} takes the sign of ϕ {\displaystyle \phi \,} and

A = 1 2 | π λ λ 0 λ λ 0 π | {\displaystyle A={\frac {1}{2}}|{\frac {\pi }{\lambda -\lambda _{0}}}-{\frac {\lambda -\lambda _{0}}{\pi }}|}
G = cos θ sin θ + cos θ 1 {\displaystyle G={\frac {\cos \theta }{\sin \theta +\cos \theta -1}}}
P = G ( 2 sin θ 1 ) {\displaystyle P=G\left({\frac {2}{\sin \theta }}-1\right)}
θ = arcsin | 2 ϕ π | {\displaystyle \theta =\arcsin |{\frac {2\phi }{\pi }}|}
Q = A 2 + G {\displaystyle Q=A^{2}+G\,}

Should it occur that ϕ = 0 {\displaystyle \phi =0\,} , then

x = ( λ λ 0 ) {\displaystyle x=\left(\lambda -\lambda _{0}\right)\,}
y = 0 {\displaystyle y=0\,}

Similarly, if λ = λ 0 {\displaystyle \lambda =\lambda _{0}\,} or ϕ = ± π / 2 {\displaystyle \phi =\pm \pi /2\,} , then

x = 0 {\displaystyle x=0\,}
y = ± π tan θ / 2 {\displaystyle y=\pm \pi \tan {\theta /2}}

In all cases, ϕ {\displaystyle \phi \,} is the latitude, λ {\displaystyle \lambda \,} is the longitude, and λ 0 {\displaystyle \lambda _{0}\,} is the central meridian of the projection.

See also

References

  1. Flattening the Earth: Two Thousand Years of Map Projections, John P. Snyder, 1993, pp.258-262, ISBN 0-226-76747-7.
  2. Map Projections - A Working Manual, USGS Professional Paper 1395, John P. Snyder, 1987, pp.239-242

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