k scott denison
As a chemical engineer, I have also asked myself the same question you ask yourself.
It seems pretty basic to me.
We have a IR absorption mechanism, which has been demonstrated empirically in the laboratory for CO2 H2O and other GH gases, but we have not carried this one step further, as you suggest, in order to establish empirically what the CO2 temperature impact really is.
Ironically, an alternate hypothesis ( the galactic cosmic ray cloud nucleation hypothesis of Svensmark et al, which has gotten much less ballyhoo and hype) has also just completed the first step at CERN in Geneva. The GCR cloud nucleation mechanism, itself, in the presence of naturally occurring aerosols, has been validated empirically, but the researchers caution that more work is needed to test empirically whether or not and to what extent this mechanism works in our atmosphere.
But, unlike the AGW hypothesis, it is planned to go the next step for this hypothesis, by either corroborating and quantifying or falsifying it at CERN in a controlled experiment simulating our atmosphere.
Like you, I cannot understand why something similar is not planned for the AGW hypothesis.
I have seen rationalizations or excuses saying this would be “impossible”.
Why should it be possible for one hypothesis and not for another?
And don’t tell me it is “impossible” when we are able to send a robot to Mars.
If only half of the money being spent on “climate related” research were channeled into empirically corroborating and quantifying (or falsifying) the AGW hypothesis, I’m sure we could have some real answers.
Is the “consensus” community afraid of what these experiments would show?
Would it rather continue doing all its projections based on model simulations, which are easier to control (but which provide no real empirical evidence)?
I’m skeptical.
Max