The equirectangular projection (also called the equidistant cylindrical projection or la carte parallélogrammatique projection), and which includes the special case of the plate carrée projection (also called the geographic projection, lat/lon projection, or plane chart), is a simple map projection attributed to Marinus of Tyre, who Ptolemy claims invented the projection about AD 100.[1]
The projection maps meridians to vertical straight lines of constant spacing (for meridional intervals of constant spacing), and circles of latitude to horizontal straight lines of constant spacing (for constant intervals of parallels). The projection is neither equal area nor conformal. Because of the distortions introduced by this projection, it has little use in navigation or cadastral mapping and finds its main use in thematic mapping. In particular, the plate carrée has become a standard for global raster datasets, such as Celestia, NASA World Wind, the USGS Astrogeology Research Program, and Natural Earth, because of the particularly simple relationship between the position of an image pixel on the map and its corresponding geographic location on Earth or other spherical solar system bodies. In addition it is frequently used in panoramic photography to represent a spherical panoramic image.[2]
The forward projection transforms spherical coordinates into planar coordinates. The reverse projection transforms from the plane back onto the sphere. The formulae presume a spherical model and use these definitions:
λ
\varphi
\varphi1
\varphi0
λ0
x
y
R
\begin{align} x&=R(λ-λ0)\cos\varphi1\\ y&=R(\varphi-\varphi0) \end{align}
The French: plate carrée (French, for flat square),[3] is the special case where
\varphi1
When the
\varphi1
\varphi1=36
\varphi1=(37.5,43.5,50.5)
While a projection with equally spaced parallels is possible for an ellipsoidal model, it would no longer be equidistant because the distance between parallels on an ellipsoid is not constant. More complex formulae can be used to create an equidistant map whose parallels reflect the true spacing.
\begin{align} λ&=
x | |
R\cos\varphi1 |
+λ0\\ \varphi&=
y | |
R |
+\varphi0 \end{align}
In spherical panorama viewers, usually:
λ
\varphi
where both are defined in degrees.