Quote from Lucrum:
it's necessary for photosynthesis. You know, oxygen. 21% of the atmosphere.
Good thinking, there is lots of O2 and even more N2 by comparison with CO2, so that's good thinking. However, neither O2 nor N2 are present in fc's IR radiance chart that i tacked on below. They have the first requirement for a good GH gas, transparency to visible light, but not the second requirement, partial opaqueness to ir. They just let IR go right through them. *Well O2 has a spike absorbance in the vis-ir transition region, but it is due to something other than an ir active vibrational mode. (I think it must have a very low energy electronic transition available because it is a groundstate di-radical. We'll have to ask the photo physicists.)
Here is what the emr coming from the sun looks like. This is the official spectrum that the guys that make solar photovoltaics use.
The yellow is the spectrum coming from the sun as experience by our outermost atmosphere. It is nearly a continuum because the thermal temperature is so high. The dark line is what the theoretical continuum, Planck, Black body radiation would look like for a body at 5533 deg Kelvin. We can see immediately that the sun closely approximates a black body radiator.
The orange is what gets through to us. That little bit of uv starting to sneak in about 275 nm up to about 350 nm is what causes sunburn (Thank goodness for O3). Notice that about 3/4s of the visible gets through (about a 1/4 is taken out by rayleigh scattering, etc), and then when we get into the ir region (where most of the solar irradiance lies), we start to see chunks of the irradiance absorbed by various components of the atmosphere. We see that water vapor is the most important absorber, and then comes CO2 which takes out a little. Some of the other gases are much better ir absorbers than either water or CO2, but there just isn't enough of them to have much of an impact. Notice that Water is effective at quite short wavelength ir (it apparently has some quite energetic stretching modes available).
Now in this solar spectrum you are NOT looking at the green house effect. You are looking at one of the two necessary properties of greenhouse gases, viz. the ability to absorb emr in the ir region.
Let me make what I think is a very important point and that is that GW and AGW are two separate topics. GW is determined by direct measurement, but the AGW question is a separate and more complex issue not easily resolved. We have been asking the AGW question for more than 30 years, but only in the last decade or so have we made any real progress. We may have fallen for the post hoc fallacy, which in brief is this: If B happens after A than A must have caused B. I'm sure we will eventually know whether or not we have once again been victims of the post hoc fallacy.
Note the solar irradiance chart stops in the near ir, 2500 nm = 4000 cm<sup>-1</sup>. So unfortunately the charts don't show the same spectral regions. I'll look for a solar irradiance chart that goes further out.