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Gall stereographic projection

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Gall stereographic projection of the world. 15° graticule.
Gall stereographic projection with 1,000 km indicatrices of distortion.

TheGall stereographic projection,presented byJames Gallin 1855, is acylindrical projection.It is neitherequal-areanorconformalbut instead tries to balance the distortion inherent in any projection.

Formulae

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The projection is conventionally defined as:[1]

whereλis the longitude from the central meridian in degrees,φis the latitude, andRis the radius of the globe used as the model of the earth for projection. It is a perspective projection if the point of projection is allowed to vary with longitude: the point of projection being on the equator on the opposite side of the earth from the point being mapped and with the projective surface being a cylinder secant to the sphere at 45°N and 45°S.[2]Gall called the projection "stereographic" because the spacing of theparallelsis the same as the spacing of the parallels along the centralmeridianof the equatorialstereographic projection.

The reverse projection is defined as:

Braun stereographic projection

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This later (1867) cylindrical projection by Carl Braun is similar, differing only in the asymmetric scaling horizontally and vertically. This yields a projection tangent to the sphere.[3]Its formula is:

See also

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References

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  1. ^Snyder 1993,p. 109.
  2. ^[1]Archived2018-07-21 at theWayback Machineaccessed 20 April 2013
  3. ^[2]Archived2013-01-20 at theWayback Machinedownloaded 20 April 2013

Bibliography

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  • Snyder, John P (1993).Flattening the Earth.University of Chicago Press.ISBN978-0-226-76747-5.

Further reading

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