Robinson projection 362116 220877805 2008-06-22T01:14:12Z Sting-fr 1451862 + map [[Image:robinson-projection.jpg|thumb|512px|right|A Robinson projection of the [[Earth]].]] The '''Robinson projection''' is a [[map projection]] popularly used since the 1960s to show the entire world at once. It was specifically created in an attempt to find the good compromise to the problem of readily showing the whole globe as a flat image. ==Overview== Presented by Dr. [[Arthur H. Robinson]] in [[1963]], it is classified as a [[pseudo-cylindrical projection]] by reason of its straight parallels, along each of which the meridians are spaced evenly. The central [[meridian (geography)|meridian]] is also a straight line; other [[meridian (geography)|meridian]]s are curved. Robinson specified the projection to be constructed by referring to a table of [[cartesian coordinate]] values at specific intersections of latitude and longitude. Intermediate locations are to be found by [[interpolation]]; see below for details. This method reflects the way he developed the projection as a series of trials, iterating until he settled on the meridian shapes and parallel spacing most pleasing to him. To contrast, most other projections are formulated as mathematical equations. Several formulaic representations of Robinson's projection have appeared in the literature as alternatives to the look-up tables. ==History== [[Image:Usgs map robinson.PNG|frame|right|The Robinson projection is an example of a pseudocylindrical, or orthophanic, projection.]] Robinson was a professor in the Geography Department at the [[University of Wisconsin in Madison]] from [[1946]] until he retired in [[1980]]. He developed the projection under commission from [[Rand McNally]] who were not satisfied with the ability of existing projections to create intuitive depictions of the entire world. Rand McNally made extensive use of it in many atlases and books. It was the first major map projection to be commissioned by a large private corporation.[http://www.warnercnr.colostate.edu/class_info/nr502/lg2/projection_descriptions/robinson.html] The projection was initially named by Robinson as "orthophanic" (meaning ''correct-looking'') but the name never caught on, and it quickly became known as the Robinson projection. It has also been referred to as ''The Pseudocylindrical Projection with Pole Line'', because the [[North pole|North]] and [[South pole|South]] poles are represented as a line as opposed to points as they are on some other projections. The [[National Geographic Society]] adopted it for their world maps in [[1988]], and many educational institutions and textbook publishers followed. The National Geographic Society abandoned the Robinson projection in [[1998]] for the [[Winkel Tripel Projection|Winkel Tripel]]. ==Strengths and weaknesses== [[Image:Tissot_indicatrix_world_map_Robinson_proj.svg|thumb|right|350px|The Robinson projection with [[Tissot's Indicatrix]] of deformation]] Like many projections, the Robinson has advantages, and like all projections, it has disadvantages. The projection is neither [[equal-area]] nor [[conformal map|conformal]], abandoning both for a compromise the creator felt produces a better overall view than could be achieved by adhering to either. The meridians curve gently, avoiding extremes, but thereby stretch the poles into long lines instead of leaving them as points. Hence distortion close to the poles is severe but quickly declines to moderate levels moving away from them. The straight parallels imply severe angular distortion at the high latitudes toward the outer edges of the map, a fault inherent in any pseudocylindrical projection. However, at the time it was developed, the projection effectively met Rand McNally's goal to produce appealing depictions of the entire world. ==See also== *[[Cartography]] *[[Gall-Peters projection]] *[[Nautical chart]] *[[Mercator projection]] *[[Winkel Tripel projection]] *[[Map projection]] ==Specification== The projection is defined by the table: <table class="wikitable"> <tr><th>Latitude</th><th>PLEN</th><th>PDFE</th></tr> <tr><td>00</td><td>1.0000</td><td>0.0000</td></tr> <tr><td>05</td><td>0.9986</td><td>0.0620</td></tr> <tr><td>10</td><td>0.9954</td><td>0.1240</td></tr> <tr><td>15</td><td>0.9900</td><td>0.1860</td></tr> <tr><td>20</td><td>0.9822</td><td>0.2480</td></tr> <tr><td>25</td><td>0.9730</td><td>0.3100</td></tr> <tr><td>30</td><td>0.9600</td><td>0.3720</td></tr> <tr><td>35</td><td>0.9427</td><td>0.4340</td></tr> <tr><td>40</td><td>0.9216</td><td>0.4958</td></tr> <tr><td>45</td><td>0.8962</td><td>0.5571</td></tr> <tr><td>50</td><td>0.8679</td><td>0.6176</td></tr> <tr><td>55</td><td>0.8350</td><td>0.6769</td></tr> <tr><td>60</td><td>0.7986</td><td>0.7346</td></tr> <tr><td>65</td><td>0.7597</td><td>0.7903</td></tr> <tr><td>70</td><td>0.7186</td><td>0.8435</td></tr> <tr><td>75</td><td>0.6732</td><td>0.8936</td></tr> <tr><td>80</td><td>0.6213</td><td>0.9394</td></tr> <tr><td>85</td><td>0.5722</td><td>0.9761</td></tr> <tr><td>90</td><td>0.5322</td><td>1.0000</td></tr> </table> The table is indexed by latitude, using [[interpolation]]. The '''PLEN''' column is the length of the parallel of latitude, and the '''PDFE''' column is multiplied by 0.5072 to obtain the distance of that parallel from the equator. Meridians of longitude are equally spaced on each parallel of latitude. ==References== *Robinson, A. ''A New Map Projection: Its Development and Characteristics'', International Yearbook of Cartography '''14''', 1974, pp. 145-155. *John B. Garver Jr., "New Perspective on the World", ''National Geographic'', December 1988, pp. 911-913. *John P. Snyder, ''Flattening The Earth - 2000 Years of Map Projections'', The University of Chicago Press, 1993, pp. 214-216. ==External links== * [http://www.radicalcartography.net/?projectionref Table of examples and properties of all common projections], from radicalcartography.net * [http://www.uff.br/mapprojections/Robinson_en.html An interactive Java Applet to study the metric deformations of the Robinson Projection]. 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