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![]() "Ash Wyllie" wrote in message ... Look up _radiational cooling_ . Space is in the single digits absolute, and the atmosphere is pretty much transparent to radiation. Objects will radiate energy trying to heat up interstellar space, and cool in the process. Ash, I'd like to expand a bit on your statements. In the 3-5 and 8-12 micrometer region of the electromagnetic spectrum, atmospheric transmission is, like you said, close to 100% transparent. Outer space, in those bands, is to photons like a Hoover is to dust in the carpet - it just sucks heat right out. The rate at which the transfer of photons occurs is dependent on, among other things, the emmissivity of the surface and the thermal conductivity from the mass to that surface. The perfect case is a gaussian emmissivity of one, and since perfection is difficult, the closest you can come is a bunch of nines behind the decimal point. A pure white specular surface is at the opposite end of the scale. One good example to back up your statement is in the winter time. We have all felt the phenomena when the sky is clear that the nights are much colder than when the sky is overcast. That is because interstellar space is sucking the heat off the planet's surface. The adjacent atmosphere loses a lot of its energy to the surface and its temperature decreases also. Please, don't confuse the cloud cover effect with the so-called "greenhouse" effect. I always used the term "radiative cooling" (not radiational) to keep in tune with NASA's glossary: (http://eobglossary.gsfc.nasa.gov/Lib...seg=q&segend=s) radiative cooling Cooling process of the Earth's surface and adjacent air, which occurs when infrared (heat) energy radiates from the surface of the Earth upward through the atmosphere into space. Air near the surface transfers its thermal energy to the nearby ground through conduction, so that radiative cooling lowers the temperature of both the surface and the lowest part of the atmosphere. Oh, did I mention that I spent the better part of two decades doing infrared measurements using a Michelson Interferometric Spectrometer? [Don't try saying that with more than two drinks under your belt.] A lot of that dealt with radiative transfer. |
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