Image:Oblique rays.svg
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Oblique_rays.svg (SVG file, nominally 800 × 600 pixels, file size: 26 KB)
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[edit] Caption
Why the polar regions are colder: Effect of the Earth's shape and atmosphere on incoming solar radiation.
Compared to equatorial regions (b), incoming solar radiation of the polar regions (a) is less intense for two reasons:
- the solar radiation arrives at an oblique angle nearer the poles, so that the energy spreads over a larger surface area, lessening its intensity.
- The radiation travels a longer distance through the atmosphere, which absorbs, scatters and reflects the solar radiation.
Tropical areas (i.e. lower latitudes, nearer the equator) receive solar which is closer to vertical.
The angle of incidence of the rays, combined with the albedo of the surface has also a strong influence on the amount of energy being absorbed (or reflected) at the surface. In the ice-covered polar zones, almost all direct energy from the sun is reflected because it is white and the angle is small. In short, the angle of incidence affects the heating of the surface in 3 different ways: length of atmospheric track, variable flux and variable reflection
For simplicity, the diagram ignores the axial tilt of the Earth, which causes each pole to slip into darkness for around 6 months of the year, and means the equator's ground is generally not perpendicular with the sun's light.
[edit] About
- Created in Inkscape (v0.45)
Based on diagrams in:
- Ecology: Theories and Applications, 4th Edition, Peter Stiling. Figure 14.2. page 231.
- Biology, third edition. Arms & Camp. Figure 49-1. page 973.
- ...and from feedback at en:Wikipedia:Picture_peer_review/Oblique_rays
[edit] Other versions
 Original |
 With land mass |
 Northern Winter axial tilt |
 Slight Spring or Autumn tilt (my preferred version) |
[edit] See also
- Image:Flux surface.jpg, related diagram (Portuguese)
[edit] Licensing
Diagram credit: Peter Halasz. (User:Pengo)
For Creative Commons and GFDL licenses, give attribution to:
- Peter Halasz
- and/or, link to this image page:
http://commons.wikimedia.org/wiki/Image:Oblique_rays.svg
Although not a requirement of the licenses, if you use this image in print or media other than the web, I would appreciate it if you let me know. Please contact me if you require alternate licensing.
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Dimensions | User | Comment | |
|---|---|---|---|---|
| current | 02:07, 11 March 2007 | 800×600 (26 KB) | Pengo | ({{Pengo|Diagram}}) |
