Mapping in Astronomy
Sky Mappings
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Hammer Projection
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Mollweide Projection
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Aitoff Projection
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Sanson Projection
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Lambert Projection
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Ortographic Projection
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Gnomonic Projection
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Stereographic Projection
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Hammer Projection
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equal-area projection
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first presented by Ernst von Hammer in 1892
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is also known as Hammer-Aitoff (the Aitoff projection looks similar, but is not equal-area)
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the border is an ellipse, equator and central meridian are straight lines
other parallels and meridians are complex curves.
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Mollweide Projection
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pseudo-cylindrical, equal-area projection
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developed by Mollweide in 1805
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Parallels are unequally spaced straight lines with the meridians being equally spaced elliptical arcs.
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The scale is only true along latitudes 40°44' north and south.
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The projection is used mainly for global maps showing data distributions.
occasionally referenced under the name homalographic projection.
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Like the Hammer projection, outlined above, we need to specify only two parameters to completely define the mapping of longitudes and latitudes into rectangular x/y coordinates:
* The central meridian
* Scale along equator in inch/degree or 1:xxxxx , or map width
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Sanson Projection
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sinusoidal, pseudo-cylindrical, equal-area projection
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Parallels are unequally spaced straight lines
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Simple mapping formulae
x= r*a*cos(d)
y= r*d
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Aitoff Projection
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equal-area projection
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The Aitoff projection is a modified azimuthal map projection.
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Proposed by David A. Aitoff in 1889,
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it is the equatorial form of the azimuthal equidistant projection,
but stretched into a 2:1 ellipse while halving the longitude from the central meridian:
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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.
Hammer did not cited Aitoff that caused confusion where Aitoff
has been attributed to Hammer's projection.
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WMAP CMB maps are presented in Aitoff projection