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==See also== {{Portal|Atlas}} * List of map projections
y is correct, and it doesn’t cause “infinite recursion”; it just doesn’t have a closed-form solution. Undid revision 1185098460 by Atavoidturk (talk)
 
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{{Short description|Pseudocylindrical equal-area map projection}}
[[File:Tobler hyperelliptical projection SW.jpg|450px|thumb|Tobler hyperelliptical projection of the world, α = 0, γ = 1.18314, k = 2.5]]
[[File:Tobler hyperelliptical projection SW.jpg|400px|thumb|Tobler hyperelliptical projection of the world; α = 0, γ = 1.18314, k = 2.5]]
The '''Tobler hyperelliptical projection''' is a family of [[Map_projection#Equal-area|equal-area]] [[Map_projection#Pseudocylindrical|pseudocylindrical]] projections used for mapping the [[earth]]. It is named for [[Waldo R. Tobler]], its inventor, who first described the family in 1973.<ref>{{cite journal|
[[File:Tobler Hyperelliptical with Tissot's Indicatrices of Distortion.svg|400px|thumb|The Tobler hyperelliptical projection with [[Tissot's indicatrix]] of deformation; α = 0, k = 3]]

The '''Tobler hyperelliptical projection''' is a family of [[Map projection#Equal-area|equal-area]] [[Map projection#Pseudocylindrical|pseudocylindrical]] projections that may be used for [[world map]]s. [[Waldo R. Tobler]] introduced the construction in 1973 as the ''hyperelliptical'' projection, now usually known as the Tobler hyperelliptical projection.<ref name="Snyder93">{{cite book
| title = Flattening the Earth: 2000 Years of Map Projections
| last = Snyder
| first = John P.
| authorlink = John P. Snyder
| year = 1993
| publisher = [[University of Chicago Press]]
| location = Chicago
| page = 220
}}</ref>

==Overview==
As with any pseudocylindrical projection, in the projection’s normal aspect,<ref>[https://mapthematics.com/ProjectionsList.php?Projection=105#hyperelliptical Mapthematics directory of map projections]</ref> the [[circle of latitude|parallels]] of [[latitude]] are parallel, [[straight lines]]. Their spacing is calculated to provide the equal-area property. The projection blends the [[cylindrical equal-area projection]], which has straight, vertical [[Meridian (geography)|meridians]], with meridians that follow a particular kind of curve known as ''[[superellipse]]s''<ref>[http://mathworld.wolfram.com/Superellipse.html "Superellipse" in MathWorld encyclopedia]</ref> or ''[[Gabriel Lamé|Lamé]] curves'' or sometimes as ''hyperellipses''. A hyperellipse is described by <math>x^k + y^k = \gamma^k</math>, where <math>\gamma</math> and <math>k</math> are free parameters. Tobler's hyperelliptical projection is given as:

:<math>\begin{align}
&x = \lambda [\alpha + (1 - \alpha) \frac{(\gamma^k - y^k)^{1/k}}{\gamma}] \\
\alpha &y = \sin \varphi + \frac{\alpha - 1}{\gamma} \int_0^y (\gamma^k - z^k)^{1/k} dz
\end{align}</math>

where <math>\lambda</math> is the longitude, <math>\varphi</math> is the latitude, and <math>\alpha</math> is the relative weight given to the cylindrical equal-area projection. For a purely cylindrical equal-area, <math>\alpha = 1</math>; for a projection with pure hyperellipses for meridians, <math>\alpha = 0</math>; and for weighted combinations, <math>0 < \alpha < 1</math>.

When <math>\alpha = 0</math> and <math>k = 1</math> the projection [[Degeneracy (mathematics)|degenerates]] to the [[Collignon projection]]; when <math>\alpha = 0</math>, <math>k = 2</math>, and <math>\gamma = 4 / \pi</math> the projection becomes the [[Mollweide projection]].<ref>{{cite journal|
last=Tobler|
last=Tobler|
first=Waldo|
first=Waldo|
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volume=78|
volume=78|
issue=11|
issue=11|
pages=pp. 1753–1759|
pages=1753–1759|
year=1973|
year=1973|
doi=10.1029/JB078i011p01753
doi=10.1029/JB078i011p01753
|bibcode=1973JGR....78.1753T
|bibcode=1973JGR....78.1753T
|
}}
citeseerx=10.1.1.495.6424}}
</ref>
</ref> Tobler favored the parameterization shown with the top illustration; that is, <math>\alpha = 0</math>, <math>k = 2.5</math>, and <math>\gamma \approx 1.183136</math>.

In the projection’s normal aspect,<ref>[http://www.csiss.org/map-projections/Pseudocylindrical/Hyperelliptical.pdf The Tobler Hyperelliptical Projection on the Center for Spatially Integrated Social Science's site]</ref> the [[circle of latitude|parallels]] of [[latitude]] are parallel [[straight line]]s whose spacing is calculated to provide the equal-area property; the [[Meridian (geography)|meridian]]s of [[longitude]] (except for the central meridian, which is a straight line perpendicular to the lines representing parallels) are curves of the form ''a''|''x''|<sup>γ</sup>&nbsp;+&nbsp;''b''|''y''|<sup>γ</sup> =&nbsp;1 (with ''a'' dependent on longitude and ''b'' constant for a given map), known as ''[[superellipse]]s''<ref>[http://mathworld.wolfram.com/Superellipse.html "Superellipse" in MathWorld encyclopedia]</ref> or [[Gabriel Lamé|Lamé]] curves. When γ=1 it becomes the [[Collignon projection]]; when γ=2 the projection becomes the [[Mollweide projection]]; the [[limiting case]] as γ→∞ is the [[Cylindrical equal-area projection]] ([[Lambert cylindrical equal-area projection|Lambert cylindrical equal-area]], [[Gall–Peters projection|Gall–Peters]], or [[Behrmann projection]]). Values of γ that are favored by Tobler and others are generally greater than&nbsp;2.


==See also==
==See also==

{{Portal|Atlas}}
* [[List of map projections]]
* [[List of map projections]]


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{{reflist}}
{{reflist}}


{{Map Projections}}
{{Map projections}}


[[Category:Cartographic projections]]
[[Category:Map projections]]
[[Category:Equal-area projections]]
[[Category:Equal-area projections]]

Latest revision as of 15:56, 14 November 2023

Tobler hyperelliptical projection of the world; α = 0, γ = 1.18314, k = 2.5
The Tobler hyperelliptical projection with Tissot's indicatrix of deformation; α = 0, k = 3

The Tobler hyperelliptical projection is a family of equal-area pseudocylindrical projections that may be used for world maps. Waldo R. Tobler introduced the construction in 1973 as the hyperelliptical projection, now usually known as the Tobler hyperelliptical projection.[1]

Overview[edit]

As with any pseudocylindrical projection, in the projection’s normal aspect,[2] the parallels of latitude are parallel, straight lines. Their spacing is calculated to provide the equal-area property. The projection blends the cylindrical equal-area projection, which has straight, vertical meridians, with meridians that follow a particular kind of curve known as superellipses[3] or Lamé curves or sometimes as hyperellipses. A hyperellipse is described by , where and are free parameters. Tobler's hyperelliptical projection is given as:

where is the longitude, is the latitude, and is the relative weight given to the cylindrical equal-area projection. For a purely cylindrical equal-area, ; for a projection with pure hyperellipses for meridians, ; and for weighted combinations, .

When and the projection degenerates to the Collignon projection; when , , and the projection becomes the Mollweide projection.[4] Tobler favored the parameterization shown with the top illustration; that is, , , and .

See also[edit]

References[edit]

  1. ^ Snyder, John P. (1993). Flattening the Earth: 2000 Years of Map Projections. Chicago: University of Chicago Press. p. 220.
  2. ^ Mapthematics directory of map projections
  3. ^ "Superellipse" in MathWorld encyclopedia
  4. ^ Tobler, Waldo (1973). "The hyperelliptical and other new pseudocylindrical equal area map projections". Journal of Geophysical Research. 78 (11): 1753–1759. Bibcode:1973JGR....78.1753T. CiteSeerX 10.1.1.495.6424. doi:10.1029/JB078i011p01753.