Tobler hyperelliptical projection

Pseudocylindrical equal-area map projection
Tobler hyperelliptical projection of the world; α = 0, γ = 1.18314, k = 2.5
The Tobler hyperelliptical projection with Tissot's indicatrix of deformation; α = 0, k = 3

The Tobler hyperelliptical projection is a family of equal-area pseudocylindrical projections that may be used for world maps. Waldo R. Tobler introduced the construction in 1973 as the hyperelliptical projection, now usually known as the Tobler hyperelliptical projection.[1]

Overview

As with any pseudocylindrical projection, in the projection’s normal aspect,[2] the parallels of latitude are parallel, straight lines. Their spacing is calculated to provide the equal-area property. The projection blends the cylindrical equal-area projection, which has straight, vertical meridians, with meridians that follow a particular kind of curve known as superellipses[3] or Lamé curves or sometimes as hyperellipses. A hyperellipse is described by x k + y k = γ k {\displaystyle x^{k}+y^{k}=\gamma ^{k}} , where γ {\displaystyle \gamma } and k {\displaystyle k} are free parameters. Tobler's hyperelliptical projection is given as:

x = λ [ α + ( 1 α ) ( γ k y k ) 1 / k γ ] α y = sin φ + α 1 γ 0 y ( γ k z k ) 1 / k d z {\displaystyle {\begin{aligned}&x=\lambda [\alpha +(1-\alpha ){\frac {(\gamma ^{k}-y^{k})^{1/k}}{\gamma }}]\\\alpha &y=\sin \varphi +{\frac {\alpha -1}{\gamma }}\int _{0}^{y}(\gamma ^{k}-z^{k})^{1/k}dz\end{aligned}}}

where λ {\displaystyle \lambda } is the longitude, φ {\displaystyle \varphi } is the latitude, and α {\displaystyle \alpha } is the relative weight given to the cylindrical equal-area projection. For a purely cylindrical equal-area, α = 1 {\displaystyle \alpha =1} ; for a projection with pure hyperellipses for meridians, α = 0 {\displaystyle \alpha =0} ; and for weighted combinations, 0 < α < 1 {\displaystyle 0<\alpha <1} .

When α = 0 {\displaystyle \alpha =0} and k = 1 {\displaystyle k=1} the projection degenerates to the Collignon projection; when α = 0 {\displaystyle \alpha =0} , k = 2 {\displaystyle k=2} , and γ = 4 / π {\displaystyle \gamma =4/\pi } the projection becomes the Mollweide projection.[4] Tobler favored the parameterization shown with the top illustration; that is, α = 0 {\displaystyle \alpha =0} , k = 2.5 {\displaystyle k=2.5} , and γ 1.183136 {\displaystyle \gamma \approx 1.183136} .

See also

References

  1. ^ Snyder, John P. (1993). Flattening the Earth: 2000 Years of Map Projections. Chicago: University of Chicago Press. p. 220.
  2. ^ Mapthematics directory of map projections
  3. ^ "Superellipse" in MathWorld encyclopedia
  4. ^ Tobler, Waldo (1973). "The hyperelliptical and other new pseudocylindrical equal area map projections". Journal of Geophysical Research. 78 (11): 1753–1759. Bibcode:1973JGR....78.1753T. CiteSeerX 10.1.1.495.6424. doi:10.1029/JB078i011p01753.
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See also