For those who are interested in the scientific basis for why steveo73's last two statements are wrong, here they are for the record ... I would also like to point out that this stuff has been known very well for over 60 years and would be found in intro level textbooks on atmospheric science, astrophysics, ... and the likes.
If you want a general intro (that requires some comfort with algebra), I recommend
http://www.amazon.com/Climate-Modelling ... 47085751X/
(I guess at this point I should strongly encourage people to go read that instead of proceeding with the 500 posts of arguments-gone-nowhere in this thread.)
point 1) For those who desire to study this for more than 10 minutes (more like 10 hours), go here:
http://scienceofdoom.com/2010/01/20/co2 ... -part-two/
This is a very good site which focuses exclusively on the physics behind the arguments. Unfortunately, it's also tough to understand for people who aren't at least hard science majors although the writer does an admirable job at it.
I'd recommend reading the entire CO2 series.
Here's my quick explanation. The reason why CO2 has a direct an significant effect is that CO2 has a wide absorption band almost right in at the peak of where the infrared radiation from the surface and atmosphere is the most intense.
http://www.xylenepower.com/Mars_EarthM.gif
See the red curve (that's the emitted spectrum) and the black curve (that's what's left after absorption). This has been known since the 1950s and satellites have been continuously monitoring the spectrum of that is emitted at the "top" of the atmosphere since 1978.
Sometimes denialists will make the argument that CO2 absorption quickly saturates. That after a wavelength is absorbed there's nothing left of that wavelength and therefore adding more CO2 will have zero effect. This is true in the laboratory setting. It's called the Beer-Lambert law. It's been mentioned very early on in this thread. What this argument fails to take into account is reemission. In the atmosphere that absorbed energy gets reemitted. Unlike in the lab, the absorbed energy doesn't go away (over the distance span of a test tube) but gets reabsorbed something else in the atmosphere. This completely changes the result. Reabsorption means that the energy is not lost. That less energy escapes the atmosphere. This heats the atmosphere.
http://scienceofdoom.com/2011/01/30/und ... art-three/ (again the entire series is interesting)
Another frequent objection is that we shouldn't be concerned about CO2 when water vapor is a much stronger green house gas than CO2. While it is true that H2O is much stronger than CO2 as anyone who has walked outside in humid air will attest to ... it's the humidity you feel (the amount of water vapor), not the trace amount of CO2... here's why we should be concerned anyway.
The answer is surprising and but in retrospect (once you know it) it's so stupid-simple that it should have been obvious.
2) Here's the short answer
http://scienceofdoom.com/2011/02/24/wat ... house-gas/
And here's my quick explanation. The difference between CO2 and H20 in the atmosphere is that water responds very quickly to climate. You might have noticed this as the phenomena of rain and snow. Yes, it's as simple as that. Point being, humans have little influence on the total amount of water vapor in the atmosphere. For a given temperature, there's a given amount of vapor and there's nothing we can do about that vapor. If we try to put a lot of it into the atmosphere (by boiling lots of water), it quickly falls down as rain or snow. If we try to extract the vapor and make the atmosphere drier, more will evaporate off the oceans and quickly nullify our efforts.
Conversely, CO2 responds extremely slowly to climate (hundred to several hundred years). What we put into the atmosphere stays there for a long time. As shown in (1) above, CO2 does drive temperature. As we all know, when temperature increases, the amount of water vapor (the absolute water density) in the lower atmosphere where it is densest (highest air pressure) and warmest (temperature decreases as you go up until you reach space) goes up as the temperatures go up. You have personally experienced this as a muggy feeling after a thunderstorm. More importantly for the climate is the a CO2 driven temperature increase will increase evaporating from the oceans. Indeed, it will fall down again as rain, but this process is ongoing and so it will raise the average humidity of the atmosphere. That in turn will raise the temperature due to the greenhouse effect as described above. This in turn causes more evaporation. This is the positive feedback effect. For an increasing level of CO2, temperatures will thus continue to rise until increased precipitation balances out the evaporation.
We are already seeing increasing precipitation.
One point where science is still work in progress---because this question is very hard---is exactly what that extra water does once it gets into the air. For example, if it causes extra clouds that will actually decrease the amount of incoming radiation from the sun because it'll be reflected upwards. Note that modern climate models do contain clouds. Also, clouds (or aerosols) is the one area where humans can reduce global warming. We can pollute more with business as usual. (That's part of the consensus explanation of the hiatus). We can even do so deliberately by spraying sulfur at high altitudes and grey out the atmosphere (create a semi-permanent haze which would have to be maintained by a fleet of airliners or the ongoing launch of balloons).
Now, I'm not sure whether steveo73 will dismiss this as "my viewpoint" or reassert that "nothing has been proven" call for more data, as he usually does, but these two points have been understood for several decades already (since before the Nixon administration) and they are well documented in far more detail than I did here in the scientific literature. They would also be explained in practically all text books on atmospheric science. As well, some of the physics (the thermodynamics) dates back to the early 1800s, underlies much of our civilization (power plants, engines, materials), and is taught to freshman scientists and engineers. The radiation physics is also solid and about as old as quantum mechanics (almost 100 years) and is the basis for ability to build radio antenna, lasers, and understand materials science. Finally, the effects on the system have been in continuous observation by orbiting satellites since 1978 verifying the predictions made by the models.
In short, these are not controversial points.