Sinusoidal projection: Difference between revisions
Content deleted Content added
Update links |
No edit summary |
||
| (23 intermediate revisions by 20 users not shown) | |||
| Line 1: | Line 1: | ||
{{Short description|Pseudocylindrical equal-area map projection}} |
|||
| ⚫ | |||
| ⚫ | |||
[[File:Carte cosmographique ou Universelle description du monde, Jean Cossin, Dieppe, 1570.png|thumb|Jean Cossin, Carte cosmographique ou Universelle description du monde, Dieppe, 1570]] |
[[File:Carte cosmographique ou Universelle description du monde, Jean Cossin, Dieppe, 1570.png|thumb|Jean Cossin, Carte cosmographique ou Universelle description du monde, Dieppe, 1570]] |
||
| ⚫ | |||
| ⚫ | The '''sinusoidal projection''' is a pseudocylindrical [[equal-area projection|equal-area]] [[map projection]], sometimes called the '''Sanson–Flamsteed''' or the '''Mercator equal-area projection'''. Jean Cossin of [[Dieppe maps|Dieppe]] was one of the first mapmakers to use the sinusoidal, using it in a world map in 1570.<ref>Jean Cossin, [http://gallica.bnf.fr/ark:/12148/btv1b5901087w ''Carte cosmographique ou Universelle description du monde avec le vrai traict des vents''], 1570.</ref> |
||
| ⚫ | |||
| ⚫ | The '''sinusoidal projection''' is a pseudocylindrical [[ |
||
The projection represents the poles as points, as they are on the sphere, but the meridians and continents are distorted. The equator and the central meridian are the most accurate parts of the map, having no distortion at all, and the further away from those that one examines, the greater the distortion.<ref>{{Cite web|url=http://blogs.discovermagazine.com/d-brief/2016/11/03/most-accurate-world-map/#.XZ2CH-zP30o|title=Finally, a World Map That Doesn't Lie|date=2016-11-03|website=D-brief|archive-url=https://web.archive.org/web/20191009064547/http://blogs.discovermagazine.com/d-brief/2016/11/03/most-accurate-world-map/#.XZ2CH-zP30o |access-date=2019-07-01|archive-date=2019-10-09 }}</ref> |
|||
The projection is defined by: |
|||
:<math>\begin{align} x &= \left(\lambda - \lambda_0\right) \cos \varphi \\ y &= \varphi\,\end{align}</math> |
:<math>\begin{align} x &= \left(\lambda - \lambda_0\right) \cos \varphi \\ y &= \varphi\,\end{align}</math> |
||
where <math>\varphi</math> is the latitude, ''λ'' is the longitude, and ''λ''{{sub|0}} is the central meridian.<ref>[https://pubs.er.usgs.gov/usgspubs/pp/pp1395 ''Map Projections—A Working Manual''], [[United States Geological Survey|USGS]] Professional Paper 1395, John P. Snyder, 1987, pp. 243–248</ref> |
where <math>\varphi</math> is the latitude, ''λ'' is the longitude, and ''λ''{{sub|0}} is the longitude of the central meridian.<ref>[https://pubs.er.usgs.gov/usgspubs/pp/pp1395 ''Map Projections—A Working Manual''], [[United States Geological Survey|USGS]] Professional Paper 1395, John P. Snyder, 1987, pp. 243–248</ref> |
||
Scale is constant along the central [[meridian (geography)|meridian]], and east–west scale is constant throughout the map. Therefore, the length of each parallel on the map is proportional to the cosine of the latitude, as it is on the globe. This makes the left and right bounding meridians of the map into half of a sine wave, each mirroring the other. Each meridian is half of a sine wave with only the amplitude differing, giving the projection its name. Each is shown on the map as longer than the central meridian, whereas on the globe all are the same length. |
Scale is constant along the central [[meridian (geography)|meridian]], and east–west scale is constant throughout the map. Therefore, the length of each parallel on the map is proportional to the cosine of the latitude, as it is on the globe. This makes the left and right bounding meridians of the map into half of a sine wave, each mirroring the other. Each meridian is half of a sine wave with only the amplitude differing, giving the projection its name. Each is shown on the map as longer than the central meridian, whereas on the globe all are the same length. |
||
| Line 12: | Line 18: | ||
The true distance between two points on a meridian can be measured on the map as the vertical distance between the parallels that intersect the meridian at those points. With no distortion along the central meridian and the [[equator]], distances along those lines are correct, as are the angles of intersection of other lines with those two lines. Distortion is lowest throughout the region of the map close to those lines. |
The true distance between two points on a meridian can be measured on the map as the vertical distance between the parallels that intersect the meridian at those points. With no distortion along the central meridian and the [[equator]], distances along those lines are correct, as are the angles of intersection of other lines with those two lines. Distortion is lowest throughout the region of the map close to those lines. |
||
[[ |
[[File:Usgs map sinousidal equal area.PNG|350px|thumb|right|A sinusoidal projection shows relative sizes accurately, but distorts shapes and directions. Distortion can be reduced by "interrupting" the map.]] |
||
Similar projections which wrap the east and west parts of the sinusoidal projection around the [[ |
Similar projections which wrap the east and west parts of the sinusoidal projection around the [[North Pole]] are the [[Werner projection|Werner]] and the intermediate [[Bonne projection|Bonne]] and [[Bottomley projection|Bottomley]] projections. |
||
The MODLAND Integerized Sinusoidal Grid, based on the sinusoidal projection, |
The MODLAND Integerized Sinusoidal Grid, based on the sinusoidal projection, is a [[geodesic grid]] developed by the NASA's [[Moderate-Resolution Imaging Spectroradiometer]] ([[MODIS]]) science team.<ref>NASA: [https://web.archive.org/web/20020625130235/http://modland.nascom.nasa.gov/developers/is_tiles/is_grid.html "MODLAND Integerized Sinusoidal Grid"]</ref> |
||
is a [[geodesic grid]] |
|||
developed by the NASA's [[Moderate-Resolution Imaging Spectroradiometer]] ([[MODIS]]) science team.<ref> |
|||
NASA: [http://modland.nascom.nasa.gov/developers/is_tiles/is_grid.html "MODLAND Integerized Sinusoidal Grid"] {{https://landweb.modaps.eosdis.nasa.gov/developers/is_tiles/is_grid.html |date=2018-01-27 }} |
|||
</ref> |
|||
==See also== |
==See also== |
||
{{Portal|Atlas}} |
|||
* [[List of map projections]] |
* [[List of map projections]] |
||
* [[Gerardus Mercator]], [[Nicolas Sanson]], and [[John Flamsteed]] |
* [[Gerardus Mercator]], [[Nicolas Sanson]], and [[John Flamsteed]] – mathematicians who developed the technique. |
||
==References== |
==References== |
||
{{Reflist}} |
|||
<references/> |
|||
==External links== |
==External links== |
||
| Line 34: | Line 36: | ||
*[http://www.radicalcartography.net/?projectionref Table of examples and properties of all common projections], from radicalcartography.net |
*[http://www.radicalcartography.net/?projectionref Table of examples and properties of all common projections], from radicalcartography.net |
||
{{Map |
{{Map projections}} |
||
{{Authority control}} |
|||
[[Category:Map projections]] |
|||
[[Category:Equal-area projections]] |
[[Category:Equal-area projections]] |
||
Latest revision as of 22:24, 3 December 2024
The sinusoidal projection is a pseudocylindrical equal-area map projection, sometimes called the Sanson–Flamsteed or the Mercator equal-area projection. Jean Cossin of Dieppe was one of the first mapmakers to use the sinusoidal, using it in a world map in 1570.[1]
The projection represents the poles as points, as they are on the sphere, but the meridians and continents are distorted. The equator and the central meridian are the most accurate parts of the map, having no distortion at all, and the further away from those that one examines, the greater the distortion.[2]
The projection is defined by:
where is the latitude, λ is the longitude, and λ0 is the longitude of the central meridian.[3]
Scale is constant along the central meridian, and east–west scale is constant throughout the map. Therefore, the length of each parallel on the map is proportional to the cosine of the latitude, as it is on the globe. This makes the left and right bounding meridians of the map into half of a sine wave, each mirroring the other. Each meridian is half of a sine wave with only the amplitude differing, giving the projection its name. Each is shown on the map as longer than the central meridian, whereas on the globe all are the same length.
The true distance between two points on a meridian can be measured on the map as the vertical distance between the parallels that intersect the meridian at those points. With no distortion along the central meridian and the equator, distances along those lines are correct, as are the angles of intersection of other lines with those two lines. Distortion is lowest throughout the region of the map close to those lines.
Similar projections which wrap the east and west parts of the sinusoidal projection around the North Pole are the Werner and the intermediate Bonne and Bottomley projections.
The MODLAND Integerized Sinusoidal Grid, based on the sinusoidal projection, is a geodesic grid developed by the NASA's Moderate-Resolution Imaging Spectroradiometer (MODIS) science team.[4]
See also
[edit]- List of map projections
- Gerardus Mercator, Nicolas Sanson, and John Flamsteed – mathematicians who developed the technique.
References
[edit]- ^ Jean Cossin, Carte cosmographique ou Universelle description du monde avec le vrai traict des vents, 1570.
- ^ "Finally, a World Map That Doesn't Lie". D-brief. 2016-11-03. Archived from the original on 2019-10-09. Retrieved 2019-07-01.
- ^ Map Projections—A Working Manual, USGS Professional Paper 1395, John P. Snyder, 1987, pp. 243–248
- ^ NASA: "MODLAND Integerized Sinusoidal Grid"
External links
[edit]
Media related to Sinusoidal projection at Wikimedia Commons- Pseudocylindrical Projections
- Table of examples and properties of all common projections, from radicalcartography.net
