Tobler hyperelliptical projection
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The Tobler hyperelliptical projection is a family of equal-area pseudocylindrical projections that may be used for
world map A world map is a map of most or all of the surface of Earth. World maps, because of their scale, must deal with the problem of projection. Maps rendered in two dimensions by necessity distort the display of the three-dimensional surface of th ...
s. Waldo R. Tobler introduced the construction in 1973 as the ''hyperelliptical'' projection, now usually known as the Tobler hyperelliptical projection.


Overview

As with any pseudocylindrical projection, in the projection’s normal aspect, the parallels of
latitude In geography, latitude is a coordinate that specifies the north– south position of a point on the surface of the Earth or another celestial body. Latitude is given as an angle that ranges from –90° at the south pole to 90° at the north pol ...
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'' or '' Lamé curves'' or sometimes as ''hyperellipses''. A hyperellipse is described by x^k + y^k = \gamma^k, where \gamma and k are free parameters. Tobler's hyperelliptical projection is given as: :\begin &x = \lambda alpha + (1 - \alpha) \frac\\ \alpha &y = \sin \varphi + \frac \int_0^y (\gamma^k - y^k)^ \end where \lambda is the longitude, \varphi is the latitude, and \alpha is the relative weight given to the cylindrical equal-area projection. For a purely cylindrical equal-area, \alpha = 1; for a projection with pure hyperellipses for meridians, \alpha = 0; and for weighted combinations, 0 < \alpha < 1. When \alpha = 0 and k = 1 the projection degenerates to the
Collignon projection The Collignon projection is an equal-area pseudocylindrical map projection first known to be published by Édouard Collignon in 1865 and subsequently cited by A. Tissot in 1881. For the smallest choices of the parameters chosen for this projecti ...
; when \alpha = 0, k = 2, and \gamma \approx 1.27323394 the projection becomes the
Mollweide projection 400px, Mollweide projection of the world 400px, The Mollweide projection with Tissot's indicatrix of deformation The Mollweide projection is an equal-area, pseudocylindrical map projection generally used for maps of the world or celestial sph ...
. Tobler favored the parameterization shown with the top illustration; that is, \alpha = 0, k = 2.5, and \gamma \approx 1.183136.


See also

* List of map projections


References

{{Map projections Map projections Equal-area projections