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sci.geo.meteorology (Meteorology) (sci.geo.meteorology) For the discussion of meteorology and related topics. |
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Please see:
http://www.youtube.com/watch?v=mu1PicT0TMU Below are lecture notes from a college course: The greenhouse effect of Venus From geometry, we can calculate the average solar flux over the surface of Venus. It is approximately 661 W/m2. Venus is very reflective of sunshine. In fact, it has a reflectivity (or albedo) of 0.8, so the planet absorbs approximately 661 X 0.2 = 132 W/m2. By assuming that the incoming radiation equals the outgoing radiation (energy balance), we can convert this into an effective radiating temperature by invoking the Stefan-Boltzmann law (total energy = _ T4). We find that T=220K. But Venus’ surface has a temperature of 730K!!! The explanation for this huge discrepancy is the planet’s greenhouse effect. The greenhouse effect of Earth From geometry, we can calculate the average solar flux over the surface of Earth. It is approximately 343 W/m2. The earth has a much lower albedo than Venus (0.3), so the planet absorbs approximately 343 X 0.7 = 240 W/m2. By assuming that the incoming radiation equals the outgoing radiation, we can convert this into an effective radiating temperature by invoking the Stefan-Boltzmann law (total energy = _ T4). We find that T=255K. Earth’s surface has a temperature of 288K While much smaller than Venus’ greenhouse effect, earth’s is crucial for the planet’s habitability. Without the greenhouse effect, the temperature today in Los Angeles would be about 0 degrees Fahrenheit. |
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