File:2d milne dist.jpg
2d_milne_dist.jpg (288 × 288 pixels, file size: 29 KB, MIME type: image/jpeg)
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Summary[edit]
| Description |
Made myself with Mathematica 5.1, Created by finding radial coordinates of a hexagon map, then modifying the radial coordinate by treating the original coordinates as rapidity, and finding the velocity associated with it. For other images similar to this one, see Arthur Milne, http://world.std.com/~mmcirvin/milne.html http://www.mcescher.com/Gallery/recogn-bmp/LW434.jpg . The shape is sometimes called a Lobachevskian, after Nikolai Ivanovich Lobachevsky, who did research in nonEuclidian Space. To the contrary, Milne described this as a matter distribution existing in Euclidian Space, much as planets and other spheres do. Made myself with Mathematica 5.1, Created by finding radial coordinates of a hexagon map, then modifying the radial coordinate by treating the original coordinates as rapidity, and finding the velocity associated with it. For other images similar to this one, see w:Arthur Milne, http://world.std.com/~mmcirvin/milne.html http://www.mcescher.com/Gallery/recogn-bmp/LW434.jpg . The shape is sometimes called a Lobachevskian, after w:Nikolai Ivanovich Lobachevsky, who did research in nonEuclidian Space. To the contrary, Milne described this as a matter distribution existing in Euclidian Space, much as planets and other spheres do. |
| Date | |
| Source | Own work |
| Author | JDoolin (talk) (Uploads) |
Licensing[edit]
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This work has been released into the public domain by its author, JDoolin at English Wikipedia. This applies worldwide. In some countries this may not be legally possible; if so: JDoolin grants anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law. |
Original upload log[edit]
| Date/Time | Dimensions | User | Comment |
|---|---|---|---|
| 2006-08-20 15:31:10 | 288× 288× | JDoolin | Made myself with Mathematica 5.1, Created by finding radial coordinates of a hexagon map, then modifying the radial coordinate by treating the original coordinates as rapidity, and finding the velocity associated with it. For other images similar to this |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 06:13, 14 October 2016 | | 288 × 288 (29 KB) | FastilyClone (talk | contribs) | Transferred from en.wikipedia (MTC!) |
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