Eckert-Greifendorff projection

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Short description: Map projection by Max Eckert-Greifendorff

The Eckert-Greifendorff projection is an equal-area map projection described by Max Eckert-Greifendorff in 1935. Unlike his previous six projections, it is not pseudocylindrical.

Development

Directly inspired by the Hammer projection, Eckert-Greifendorff suggested the use of the equatorial form of the Lambert azimuthal equal-area projection instead of Aitoff's use of the azimuthal equidistant projection:

[math]\displaystyle{ \begin{align} x &= 2\operatorname{laea}_x\left(\frac{\lambda}{4}, \varphi\right) \\ y &= \tfrac12 \operatorname{laea}_y\left(\frac{\lambda}{4}, \varphi\right) \end{align} }[/math]

where laeax and laeay are the x and y components of the equatorial Lambert azimuthal equal-area projection. Written out explicitly:

[math]\displaystyle{ \begin{align} x &= \frac{4 \sqrt 2 \cos \varphi \sin \frac{\lambda}{4}}{\sqrt{1 + \cos \varphi \cos \frac{\lambda}{4}}} \\ y &= \frac{\sqrt 2\sin \varphi}{\sqrt{1 + \cos \varphi \cos \frac{\lambda}{4}}} \end{align} }[/math]

The inverse is calculated with the intermediate variable

[math]\displaystyle{ z \equiv \sqrt{1 - \left(\tfrac1{16} x\right)^2 - \left(\tfrac12 y\right)^2} }[/math]

The longitude and latitudes can then be calculated by

[math]\displaystyle{ \begin{align} \lambda &= 4 \arctan \frac{zx}{4\left(2z^2 - 1\right)} \\ \varphi &= \arcsin zy \end{align} }[/math]

where λ is the longitude from the central meridian and φ is the latitude.[1][2]

See also

References

  1. Flattening the Earth: Two Thousand Years of Map Projections, John P. Snyder, 1993, pp. 130–133, ISBN:0-226-76747-7.
  2. Weisstein, Eric W. "Hammer–Aitoff Equal-Area Projection." From MathWorld—A Wolfram Web Resource