Andre said:
Now let's concentrate on that. How about running a null hypothesis on Earth instead of using a -perhaps too simple- model that leads to the 33 degrees?
Assume that the atmosphere of our model is completely inert, no radiative properties and that the Model- Earth acts as a radiative transmitter, but not completely like a black body, since it does not meet its qualifications (like an ideal conductor, while the Earth is a near ideal insulator).
There's a very simple mathematical theorem here that applies in this case, for all possible permutations of your proposed model.
The total energy received from the Earth is the solar constant of ~1365 W/m
2, and 30% of that is reflected, using your numbers, with which I concur. The cross section of the Earth is one quarter of the surface area, which is why we divide by four when taking average energy inputs per unit area. But in any case, the total energy is
\pi R^2 \times 1365 \times 0.3 \approx 5.3\times10^{16} \; \text{Watts}
Now, by the first law of thermodynamics, all that has to be radiated back to space. Because Earth distributes heat around the globe fairly well -- much better than the Moon, for example -- it is usual to give an "effective" temperature for the planet, which is the temperature that would radiate that amount of energy if uniform over the whole sphere.
You are proposing we take into account the obvious fact that temperature is NOT uniformly distributed. Here's the thing, however. The power radiated goes as the fourth power of temperature. So if you increase the temperature in some places and reduce it in others, the increase has a proportionally larger impact on the energy output. That is, you have to make the colder regions take a LARGER fall than the increase in the warmer regions. This applies for any redistribution of temperature, by any means.
This is a necessary consequence of
Hölder's inequality, which means:
\frac{1}{S} \int_S T dS \leq \left( \frac{1}{S} \int_S T^4 dS \right)^{0.25}
Added in edit. The above formula was originally incorrect; I had omitted the normalization with area S. See [post=2296963]msg #99[/post] by vanesch for the original incorrect version, and why it needed fixing. I've updated this post with the corrected formula he provided.
The above represents a surface integral. One is the integral of temperature; the other is an integral of power emission. The power integral is constrained to balance the solar input by the first law.
What that means is that the value 255K (-18C) as an effective surface temperature is a strong upper bound on the average temperature, given any redistribution of temperature around the globe at all which maintains the energy output.
The only way you can actually get higher temperatures than a 255K average; the ONLY way, is if the energy radiated from the surface can't actually get directly out into space. In other words, the 33 degrees is a strong [strike]UPPER[/strike]
LOWER BOUND on the consequence of absorption of radiant energy in our atmosphere.
That's a theorem; as strong as any result you can get in physics. Given your stated assumptions, of a radiatively inert atmosphere, and the unstated assumption of a surface emissivity of close to unity (which it certainly is, at the relevant wavelengths; I include this for completeness) the 33 degrees falls out from the laws of thermodynamics. It's that fundamental.
Andre said:
Note that this heat energy is assumed to be in radiation equilibrium, as dissipation via radiation into space is already accounted for. Other ways of energy dissipation are both conduction to deeper layers under the surface and conduction to the boundary layer of the atmosphere. Conduction is a very ineffective way of losing heat. However, while heating, the atmosphere boundary layer decreases in density and gets buoyant. Via convection the heat is dissipated higher into the atmosphere. So, even without radiation absorption, there is a way to bring surface heat into the atmosphere during daytime, convection.
But not out into space. Convection can heat up the atmosphere, but if the atmosphere cannot absorb infrared radiation then it cannot emit it either. There's nowhere for the heat to go. By the first law of thermodynamics, such a planet has an atmosphere which reaches a pure convective equilibrium. The atmosphere may heat up and cool down with the diurnal day night cycle or seasons, in various complex ways, but only through an exchange of energy to the surface. There's no way the atmosphere can actually be a net sink for heat from the surface; so ALL the radiation from the surface goes to space; and that means the surface is at a temperature to balance solar input. By Holder's inequality, this is necessarily an average temperature of -18 degrees, or less.
That is, the greenhouse effect -- absorption of IR radiation -- accounts for AT LEAST 33 degrees of extra surface warmth.
This is not advanced physics. This is very elementary thermodynamics.
I sympathize with people who get confused on these points, because there is a lot of outright pseudoscience expressed on this topic, which can easily lead the unwary astray. It's not always easy to pick the pseudoscience at first sight, for a non-professional. There are even a couple of cases where scientists have managed to express such ideas in the actual scientific literature. This is really unusual, and represents a startling failure of the journal to manage basic quality control; but it happens, in this and other fields. The cases I know of are in low impact journals, with authors who are not active in the relevant fields of physics. Even that is not enough to explain how this happens... I am honestly at a loss to account for how anyone could possibly write papers like Gerlich and Tscheusner, or Chilingar et al.
But second guessing how that happens is beside the point. The actual argument expressed is on a par with young Earth creationism -- another field of pseudoscience with its own credential scientists also writing rock bottom crank science.
Andre said:
So, if we make the inert atmosphere in our null hypothesis radiative again with the addition of radiative gasses (mistakenly known as greenhouse gasses) more processes can take place. Now the heating of the lower atmosphere during daytime is also enhanced by the absorption of the surface out-radiation, which stimulates more convection. But also the atmosphere can radiate energy to outer space, and help cooling the atmosphere that way. Now obviously these processes act in opposite directions And then we did not add the water cycle with latent heat and clouds, adding to the complexity.
The "complexity" here is smoke and mirrors. There is certainly plenty of complexity and a whole pile of open research questions here that can be legitimately a focus for more rational skepticism of various conclusions.
But not the question of "cooling". That is not an open question at all. As you give the atmosphere a capacity to interact with thermal radiation, you inevitably find that the atmosphere heats up; it gets more energy from the surface than when radiatively inert. What complexity means is that you can't easily derive how much it will heat up, nor whether you'll get local reductions offset by larger increases elsewhere, in complex ways. But the net effect of additional heating is a necessary consequence of basic thermodynamics, entirely independent of any concerns about the acknowledged complexity.
In a convective equilibrium, you will find temperatures fall with altitude. That is because pressure falls with altitude; as packets of air move up or down, they expand or contract, giving lower temperatures at altitude. There's a well developed theory for the "dry adiabat" that derives this relation, using basic thermodynamics. Note that this result is independent of the thermal emissivity. It depends simply on the "potential temperature", which is the temperature that air at a certain pressure would have if compressed in a return to surface levels. Allowing the atmosphere to absorb and emit radiation will drive stronger convection, certainly; but the adiabat is unaffected because the potential temperature is unaffected.
Now... since the main part of the atmosphere is necessarily cooler than the surface, the effect of adding a capacity to absorb and emit radiation will result in a net flow of energy from the surface into the cooler atmosphere. That follows from the second law. The additional energy going into the atmosphere will help drive additional convection, which also increases the net flow of energy into the atmosphere. This is now balanced by the loss of radiant energy out from the top of the atmosphere. What we have now is called "radiative-convective equilibrium". And that involves a higher temperature than the pure convective equilibrium.
I repeat, this is basic first year level physics. It's not in any doubt whatsoever. It is also completely irrelevant to most expressions of skepticism about conventional climatology; it's part of the rock bottom lunatic fringe of denial, in conflict with fundamentals of physics that are a basis for even to starting to look at the real complexities and uncertainties that exist in the field.
Conclusion: the 33-degrees black body radiation model is meaningless considering the more complex processes on Earth.
This is on a par with claiming that the conservation of momentum model is meaningless given the complexities of interactions of orbits in a multi-body gravitationally bound system.
On an exam, your comment could only be marked wrong. The 33 degrees is a necessary lower bound on the impact of the atmosphere's capacity to absorb infrared radiation, that holds by basic physics no matter how complex the processes you invoke. Complexity can't overrule the basic laws like conservation of energy; and that's the level of fundamentals from which the 33 degree bound follows.
This is basically the idea of the much quoted Chilingar et al 2008 and I would appreciate it to see what exactly is wrong with the physics of that.
The idea that adding a capacity to interact with thermal radiation has a net cooling effect.
(And by the way: you say "much quoted"... but by whom? You know the citation count on that paper? Zero. There's a handful of citations in an earlier error ridden paper he wrote in 2006; most importantly a devastating rebuttal response. In my opinion, finding the people who quote Chilingar is a good way to identify people whose skepticism is grounded in a profound lack of comprehension of the relevant physics... mainly amongst bloggers or the like. But scientists? Not so much...)
Chilingar ignores the standard and completely uncontroversial thermodynamics of lapse rate, and comes up with his own definitions, without any experimental or observation support, without any refutations of the conventional thermodynamics of potential temperature and lapse rate, and in complete conflict with what should be learned in first year uni by anyone studying atmospheric physics.
I don't expect you to believe me on my own authority here. I'm making strong criticisms of Chilingar's competence in basic physics, despite the acknowledged fact he is a prominent and successful scientist in his own field. That may give you pause before accepting my analysis above. Good! That's skepticism, and skepticism is good. The thing is, you should on the same basis be skeptical of Chilingar's claims.
It is possible to be a "climate skeptic", but many people who identify themselves that way are better described as credulous naifs. My suggestion is... don't take my word for anything, and don't presume Chilingar's word either. After all, if Chilingar's lapse rate ideas have any merit then we'll have to rewrite all the physics of the dry adiabat! That's possible in principle, but a genuine skeptic should be cautious of jumping on that bandwagon too quickly!
Instead, take a bit of time to check the background. I cited for you an online text above. Try reading through chapter 2, of
Principles of Planetary Climate, by Professor Ray Pierrehumbert. This chapter is "Thermodynamics in a Nutshell", and it includes derivations of the dry and the moist adiabat. Pretty much any other text on atmospheric physics should deal with this topic as well. I appreciate that this will take time; and I am not demanding you simply accept my claims at once. I anticipate we'll eventually wind up this discussion without reaching a mutual recognition the implications of thermodynamics for the hard bounds on properties of a complex climate system, and that's fine with me. But I hope I might have shaken your confidence enough to look into the physics more thoroughly over coming months, offline.
Cheers -- sylas