Diffuse sky radiation
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Diffuse sky radiation is solar radiation reaching the Earth's surface after having been scattered from the direct solar beam by molecules or suspensoids in the atmosphere. It is also called skylight, diffuse skylight, or sky radiation and is the reason for changes in the colour of the sky. Of the total light removed from the direct solar beam by scattering in the atmosphere (approximately 25% of the incident radiation when the sun is high in the sky, depending on the amount of dust and haze in the atmosphere), about two-thirds ultimately reaches the earth as diffuse sky radiation.
- See also: Wikipedia
- Related: Aerial perspective, Cyanometer, Daylight, Tyndall effect, Rayleigh scattering, Rayleigh Sky Model
| Dr. C. V. Raman lecture: Why is the sky blue? Dr. C. V. Raman lecture: Why is the sky blue? www.arvindguptatoys.com/arvindgupta/raman.htm - Web |
| Why is the sky blue? Why is the sky blue? math.ucr.edu/home/baez/physics/General/BlueSky/blue_sky.html - Web |
| Blue Sky and Rayleigh Scattering Blue Sky and Rayleigh Scattering hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html - Web |
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| Atmospheric Optics (.pdf), Dr. Craig Bohren Atmospheric Optics (.pdf), Dr. Craig Bohren homepages.wmich.edu/%7Ekorista/atmospheric_optics.pdf - Web |
