The Behrmann projection is a cylindrical map projection described by Walter Behrmann in 1910. It is a member of the cylindrical equal-area projection family. Members of the family differ by their standard parallels, which are parallels along which the projection has no distortion. In the case of the Behrmann projection, the standard parallels are 30°N and 30°S. The projection shares many characteristics with other members of the family such as the Lambert cylindrical equal-area projection, whose standard parallel is the equator, and the Gall–Peters projection, whose standard parallels are 45°N and 45°S. While equal-area, distortion of shape increases in the Behrmann projection according to distance from the standard parallels. The Behrmann projection has the property that half of the Earth
| Attributes | Values |
|---|
| rdf:type
| |
| rdfs:label
| - Behrmannovo zobrazení (cs)
- Behrmann projection (en)
- Проекция Бермана (ru)
|
| rdfs:comment
| - Behrmannovo zobrazení je plochojevné válcové kartografické zobrazení. Jeho autorem je německý geograf , který ho poprvé publikoval v Berlíně v roce 1910. Behrmannovo zobrazení je speciálním případem se dvěma nezkreslenými rovnoběžkami o zeměpisné šířce 30°. (cs)
- Проекция Бермана — цилиндрическая равновеликая картографическая проекция, предложенный Вальтером Берманом в 1910 году в книге «Лучшая возможная равновеликая проекция всей Земли» (нем. Die beste bekannte flächentreue Projektion der ganzen Erde). Проекция Бермана не имеет искажений на 30° параллели и обладает общими характеристиками с другими членами своей семьи — такими, как равновеликая цилиндрическая проекция Ламберта, стандартной параллелью которой является экватор, и проекция Хобо-Дайера, чей уровень параллели 37,5°. (ru)
- The Behrmann projection is a cylindrical map projection described by Walter Behrmann in 1910. It is a member of the cylindrical equal-area projection family. Members of the family differ by their standard parallels, which are parallels along which the projection has no distortion. In the case of the Behrmann projection, the standard parallels are 30°N and 30°S. The projection shares many characteristics with other members of the family such as the Lambert cylindrical equal-area projection, whose standard parallel is the equator, and the Gall–Peters projection, whose standard parallels are 45°N and 45°S. While equal-area, distortion of shape increases in the Behrmann projection according to distance from the standard parallels. The Behrmann projection has the property that half of the Earth (en)
|
| foaf:depiction
| |
| dcterms:subject
| |
| Wikipage page ID
| |
| Wikipage revision ID
| |
| Link from a Wikipage to another Wikipage
| |
| Link from a Wikipage to an external page
| |
| sameAs
| |
| dbp:wikiPageUsesTemplate
| |
| thumbnail
| |
| has abstract
| - Behrmannovo zobrazení je plochojevné válcové kartografické zobrazení. Jeho autorem je německý geograf , který ho poprvé publikoval v Berlíně v roce 1910. Behrmannovo zobrazení je speciálním případem se dvěma nezkreslenými rovnoběžkami o zeměpisné šířce 30°. (cs)
- The Behrmann projection is a cylindrical map projection described by Walter Behrmann in 1910. It is a member of the cylindrical equal-area projection family. Members of the family differ by their standard parallels, which are parallels along which the projection has no distortion. In the case of the Behrmann projection, the standard parallels are 30°N and 30°S. The projection shares many characteristics with other members of the family such as the Lambert cylindrical equal-area projection, whose standard parallel is the equator, and the Gall–Peters projection, whose standard parallels are 45°N and 45°S. While equal-area, distortion of shape increases in the Behrmann projection according to distance from the standard parallels. The Behrmann projection has the property that half of the Earth's surface is stretched horizontally and the other half is stretched vertically. This projection is not equidistant. (en)
- Проекция Бермана — цилиндрическая равновеликая картографическая проекция, предложенный Вальтером Берманом в 1910 году в книге «Лучшая возможная равновеликая проекция всей Земли» (нем. Die beste bekannte flächentreue Projektion der ganzen Erde). Проекция Бермана не имеет искажений на 30° параллели и обладает общими характеристиками с другими членами своей семьи — такими, как равновеликая цилиндрическая проекция Ламберта, стандартной параллелью которой является экватор, и проекция Хобо-Дайера, чей уровень параллели 37,5°. (ru)
|
| gold:hypernym
| |
| prov:wasDerivedFrom
| |
| page length (characters) of wiki page
| |
| foaf:isPrimaryTopicOf
| |
| is Link from a Wikipage to another Wikipage
of | |
| is Wikipage redirect
of | |
| is Wikipage disambiguates
of | |
| is foaf:primaryTopic
of | |
![[cxml]](/fct/images/cxml_doc.png)
![[csv]](/fct/images/csv_doc.png)
![[text]](/fct/images/ntriples_doc.png)
![[turtle]](/fct/images/n3turtle_doc.png)
![[ld+json]](/fct/images/jsonld_doc.png)
![[rdf+json]](/fct/images/json_doc.png)
![[rdf+xml]](/fct/images/xml_doc.png)
![[atom+xml]](/fct/images/atom_doc.png)
![[html]](/fct/images/html_doc.png)
![[RDF Data]](/fct/images/sw-rdf-blue.png)