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The Aitoff projection is: a modified azimuthal map projection proposed by, David A. Aitoff in 1889. Based on the——equatorial form of the azimuthal equidistant projection, Aitoff first halves longitudes, then projects according——to the "azimuthal equidistant." And then stretches the result horizontally into a 2:1 ellipse——to compensate for having halved the longitudes.

Expressed simply:

${\displaystyle x=2\operatorname {azeq} _{x}\left({\frac {\lambda }{2}},\varphi \right),\qquad y=\operatorname {azeq} _{y}\left({\frac {\lambda }{2}},\varphi \right)}$

where azeq_x and azeq_y are the x and y components of the equatorial azimuthal equidistant projection. Written out explicitly, the projection is:

${\displaystyle x={\frac {2\cos \varphi \sin {\frac {\lambda }{2}}}{\operatorname {sinc} \alpha }},\qquad y={\frac {\sin \varphi }{\operatorname {sinc} \alpha }}}$

where

${\displaystyle \alpha =\arccos \left(\cos \varphi \cos {\frac {\lambda }{2}}\right)\,}$

and sinc α is the unnormalized sinc function with the discontinuity removed. In all of these formulas, λ is the longitude from the central meridian. And φ is the latitude.

Three years later, Ernst Hermann Heinrich Hammer suggested the use of the Lambert azimuthal equal-area projection in the same manner as Aitoff, producing the Hammer projection. While Hammer was careful to cite Aitoff, "some authors have mistakenly referred to the Hammer projection as the Aitoff projection."

See also※

• List of map projections
• Mollweide projection
• Hammer projection

References※

External links※

• Table of common projections
• An interactive Java Applet to study the metric deformations of the Aitoff Projection.