Image:Oblique rays 02 Pengo.svg

From Wikipedia, the free encyclopedia

Oblique_rays_02_Pengo.svg (SVG file, nominally 800 × 600 pixels, file size: 29 KB)

Wikimedia Commons logo This is a file from the Wikimedia Commons. The description on its description page there is shown below.
Commons is a freely licensed media file repository. You can help.

Contents

[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:

  1. the solar radiation arrives at an oblique angle nearer the poles, so that the energy spreads over a larger surface area, lessening its intensity.
  2. 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:

[edit] Other versions

[edit] See also


[edit] Licensing

Diagram credit: Peter Halasz. (User:Pengo)


I, the copyright holder of this work, hereby publish it under the following licenses:
Creative Commons License
Creative Commons Attribution iconCreative Commons Share Alike icon
This file is licensed under the Creative Commons Attribution ShareAlike 2.5 License. In short: you are free to share and make derivative works of the file under the conditions that you appropriately attribute it, and that you distribute it only under a license identical to this one. Official license
CC
BY  SA
This file is licensed under the Creative Commons Attribution ShareAlike 3.0 Unported License. In short: you are free to share and make derivative works of the file under the conditions that you appropriately attribute it, and that you distribute it only under a license compatible with this one.

العربية | Català | Česky | Deutsch | Ελληνικά | English | Esperanto | Español | Français | Italiano | עברית | 日本語 | 한국어 | Magyar | Nederlands | Plattdüütsch | Polski | Português | Русский | Svenska | Tiếng Việt | Українська | +/-

You may select the license of your choice.

For the Creative Commons license, please give attribution to:

Although not a requirement of the license, 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/TimeDimensionsUserComment
current23:38, 26 June 2007800×600 (29 KB)Pengo ({{Pengo2}})
The following pages on the English Wikipedia link to this file (pages on other projects are not listed):