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Wiechel projection

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Wiechel Projection of the Earth

TheWiechel projection is anpseudoazimuthal,equal-areamap projection, and a novelty map presented by William H. Wiechel in 1879. When centered on the pole, it has semicircular meridians arranged in a pinwheel. Distortion of direction, shape, and distance is considerable in the edges.[1]

In polar aspect, the Wiechel projection can be expressed as so:[1]

x=R(sinλcosϕ(1sinϕ)cosλ),y=R(cosλcosϕ+(1sinϕ)sinλ).{\displaystyle {\begin{aligned}x&=R\left(\sin \lambda \cos \phi -\left(1-\sin \phi \right)\cos \lambda \right),\\y&=-R\left(\cos \lambda \cos \phi +\left(1-\sin \phi \right)\sin \lambda \right).\end{aligned}}}

The Wiechel can be obtained via an area-preserving polar transformation of theLambert azimuthal equal-area projection.In polar representation, the required transformation is of the form

rW=rL,θW=θL12arcsinrL,{\displaystyle {\begin{aligned}r_{W}&=r_{L},\\\theta _{W}&=\theta _{L}-{\frac {1}{2}}\arcsin r_{L},\end{aligned}}}

where(rL,θL){\displaystyle (r_{L},\theta _{L})} and(rW,θW){\displaystyle (r_{W},\theta _{W})} are the polar coordinates of the Lambert and Wiechel maps, respectively.Thedeterminant of the Jacobian of the transformation is equal to unity, ensuring that it is area-preserving.The Wiechel map thus serves as a simple example that equal-area projections of the sphere onto the disk are not unique, unlikeconformal maps which follow theRiemann mapping theorem.

See also

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References

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  1. ^abMap Projections: A Reference Manual. Lev Moiseevič Bugaevskij, John Parr Snyder. 1995. p. 132.ISBN 9780748403042. Retrieved2013-02-15.
Cylindrical
Mercator-conformal
Equal-area
Pseudocylindrical
Equal-area
Conical
Pseudoconical
Azimuthal
(planar)
General perspective
Pseudoazimuthal
Conformal
Equal-area
Bonne
Bottomley
Cylindrical
Tobler hyperelliptical
Equidistant in
some aspect
Gnomonic
Loxodromic
Retroazimuthal
(Mecca or Qibla)
Compromise
Hybrid
Perspective
Planar
Polyhedral
See also
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