How many of us actually understand how the greenhouse effect works? The simple physics explanations you find on the Internet are usually quite wrong. With this in mind, I've decided to attempt a very simple explanation of the physics behind Earth's energy balance. Bear in mind that this is a simple radiative model, there are actually many more parts to the greenhouse effect than I present here, they're just unnecessary for such a basic explanation.
I'm curious to know if any of you have any objections to this explanation, since this understanding of Earth's energy balance is fundamental to anthropogenic global warming theory.
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First, an important idea is that hot objects tend to cool off relatively quickly, while cool objects cool off more slowly, that is, the rate that energy flows from an object is dependent on the object's temperature. This means that a hot object in the presence of a constant energy source will tend to cool down until the amount of energy it emits equals the amount of energy it receives, while a cool object will warm up until the amount of outgoing energy equals the amount of incoming energy.
Get it? Got it? Good. Moving right along.
A planet is in thermal equilibrium when the amount of energy radiated from the planet to space equals the amount of radiation the planet receives from the sun. Due to its position relative to the sun, the Earth receives about 240 Watts per square meter (W/m^2) of solar energy, which means that in equilibrium, the planet must radiate 240 W/m^2 back out into space.
Some rough calculations would show that if Earth was absorbing heat from the sun and then radiating it directly out into space, the average temperature of the planet would be about 0ºF—well below freezing.
Happily for us, this isn't the case. There are certain trace gases in the atmosphere that are transparent to sunlight but opaque to radiation at wavelengths emitted from Earth's surface. These gases are called the greenhouse gases (although they have nothing to do with greenhouses). The heat radiated from the Earth's surface must pass through these greenhouse gases before it can radiate into space.
The atmosphere is free to radiate heat in all directions (but for our simple model, we can think of it as radiating either "up" or "down"). So while the atmosphere radiates 240 W/m^2 into space, it also radiates 240 W/m^2 back toward the ground. So Earth's surface receives both 240 W/m^2 from the sun and 240 W/m^2 from the atmosphere for a grand total of 480 W/m^2*.
However, unlike the atmosphere, the ground can only radiate heat in one direction: up. So the surface of the planet radiates radiates a total of 480 W/m^2 up into the atmosphere, and this heat is absorbed by the atmosphere, rather than escaping straight into space. And viola! We have a greenhouse effect that heats up the planet's surface! In fact, the greenhouse effect I just described keeps Earth's surface at a cozy average of about 15ºC (59ºF).
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All righty then, now that we understand how Earth's energy balance works, and how the greenhouse effect warms the Earth's surface (I hope you didn't have too much trouble hacking through my garbled verbiage), doesn't it make sense that changing it would have an effect on Earth's temperature? CO2 makes up 9—36% of the overall greenhouse effect, and we humans have increased its concentration in the atmosphere by about 35% over the past century. Given this understanding of the physical processes driving the Earth's climate, doesn't AGW theory seem perfectly reasonable?
I look forward to your thoughts, comments, and, most importantly, criticisms.
—EP
* If you're having trouble imagining this part, try thinking in terms of this simple progression. The planet gets 240 W/m^2 from the sun, and radiates the same back out. The heat is absorbed in the atmosphere, where 120 W/m^2 is radiated out to space, and another 120 W/m^2 is radiated back toward the ground. Now the planet has absorbed 240 W/m^2 from the sun and 120 W/m^2 from the atmosphere, which it reradiates. Now the atmosphere absorbs this 360 W/m^2 and radiates half toward the Earth, and half out to space. Now the Earth receives 240 W/m^2 from the sun, and 180 W/m^2 from the atmosphere. You can continue this progression until the atmosphere is absorbing a total of 480 W/m^2, at which point the energy flux "balances out". (Whew!)


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