Guest Post by Willis Eschenbach [note new Update at the end, and new Figs. 4-6]
In climate science, linearity is the order of the day. The global climate models are all based around the idea that in the long run, when we calculate the global temperature everything else averages out, and we’re left with the claim that the change in temperature is equal to the climate sensitivity times the change in forcing. Mathematically, this is:
∆T = lambda ∆F
where T is global average surface temperature, F is the net top-of-atmosphere (TOA) forcing (radiation imbalance), and lambda is called the “climate sensitivity”.
In other words, the idea is that the change in temperature is a linear function of the change in TOA forcing. I doubt it greatly myself, I don’t think the world is that simple, but assuming linearity makes the calculations so simple that people can’t seem to break away from it.
Now, of course people know it’s not really linear … but when I point that out, often the claim is made that it’s close enough to linear over the range of interest that we can assume linearity with little error.
So to see if the relationships really are linear, I thought I’d use the CERES satellite data to compare the surface temperature T and the TOA forcing F. Figure 1 shows that graph:
Figure 1. Land only, forcing F (TOA radiation imbalance) versus Temperature T, on a 1° x 1° grid. Colors indicate latitude. Note that there is little land from 50S to 65S. Net TOA radiation is calculated as downwelling solar less reflected solar less upwelling longwave radiation. Click graphics to enlarge.
As you can see, far from being linear, the relationship between TOA forcing and surface temperature is all over the place. At the lowest temperatures, they are inversely correlated. In the middle there’s a clear trend … but then at the highest temperatures, they decouple from each other, and there is little correlation of any kind.
The situation is somewhat simpler over the ocean, although even there we find large variations:
Figure 2. Ocean only, net forcing F (TOA radiation imbalance) versus Temperature T, on a 1° x 1° grid. Colors indicate latitude.
While the changes are not as extreme as those on land, the relationship is still far from linear. In particular, note how the top part of the data slopes further and further to the right with increasing forcing. This is a clear indication that as the temperature rises, the climate sensitivity decreases. It takes more and more energy to gain another degree of temperature, and so at the upper right the curve levels off.
At the warmest end, there is a pretty hard limit to the surface temperature of the ocean at just over 30°C. (In passing, I note that there also appears to be a pretty hard limit on the land surface air temperature, at about the same level, around 30°C. Curiously, this land temperature is achieved at annual average TOA radiation imbalances ranging from -50 W/m2 up to 50 W/m2.)
Now, what I’ve shown above are the annual average values. In addition to those, however, we are interested in lambda, the climate sensitivity which those figures don’t show. According to the IPCC, the equilibrium climate sensitivity (ECS) is somewhere in the range of 1.5 to 4.5 °C for each doubling of CO2. Now, there are a several kinds of sensitivities, among them monthly, decadal, and equilibrium climate sensitivities.
Monthly sensitivity
Monthly climate sensitivity is what happens when the TOA forcing imbalance in a given 1°x1° gridcell goes from say plus fifty W/m2 one month (adding energy), to minus fifty W/m2 the next month (losing energy). Of course this causes a corresponding difference in the temperature of the two months. The monthly climate sensitivity is how much the temperature changes for a given change in the TOA forcing.
But the land and the oceans can’t change temperature immediately. There is a lag in the process. So monthly climate sensitivity is the smallest of the three, because the temperatures haven’t had time to change. Figure 3 shows the monthly climate sensitivities based on the CERES monthly data.
Figure 3. The monthly climate sensitivity.
As you might expect, the ocean temperatures change less from a given change in forcing than do the land temperatures. This is because of the ocean’s greater thermal mass which is in play at all timescales, along with the higher specific heat of water versus soil, as well as the greater evaporation over the ocean.
Decadal Sensitivity
Decadal sensitivity, also called transient climate response (TCR), is the response we see on the scale of decades. Of course, it is larger than the monthly sensitivity. If the system could respond instantaneously to forcing changes, the decadal sensitivity would be the same as the monthly sensitivity. But because of the lag, the monthly sensitivity is smaller. Since the larger the lag, the smaller the temperature change, we can use the amount of the lag to calculate the TCR from the monthly climate response. The lag over the land averages 0.85 months, and over the ocean it is longer at 2.0 months. For the land, the TCR averages about 1.6 times the monthly climate sensitivity. The ocean adjustment for TCR is larger, of course, since the lag is longer. Ocean TCR is averages about 2.8 times the monthly ocean climate sensitivity. See the Notes below for the calculation method.
Figure 4 shows what happens when we put the lag information together with the monthly climate sensitivity. It shows, for each gridcell, the decadal climate sensitivity, or transient climate response (TCR). It is expressed in degrees C per doubling of CO2 (which is the same as degrees per a forcing increase of 3.7 W/m2). The TCR shown in Figure 4 includes the adjustment for the lag, on a gridcell-by-gridcell basis.
Figure 4. Transient climate response (TCR). This is calculated by taking the monthly climate sensitivity for each gridcell, and multiplying it by the lag factor calculated for that gridcell. [NOTE: This Figure, and the values derived from it, are now updated from the original post. The effect of the change is to reduce the estimated transient and equilibrium sensitivity. See the Update at the end of the post for details.]
Now, there are a variety of interesting things about Figure 3. One is that once the lag is taken into account, some of the difference between the climate sensitivity of the ocean and the land disappears, and some is changed. This is particularly evident in the southern hemisphere, compare Southern Africa or Australia in Figures 3 and 4.
Also, you can see, water once again rules. Once we remove the effect of the lags, the drier areas are clearly defined, and they are the places with the greatest sensitivity to changes in TOA radiative forcing. This makes sense because there is little water to evaporate, so most of the energy goes into heating the system. Wetter tropical areas, on the other hand, respond much more like the ocean, with less sensitivity to a given change in TOA forcing.
Equilibrium Sensitivity
Equilibrium sensitivity (ECS), the longest-term kind of sensitivity, is what would theoretically happen once all of the various heat reservoirs reach their equilibrium temperature. According to the study by Otto using actual observations, for the past 50 years the ECR has stayed steady at about 130% of the TCR. The study by Forster, on the other hand, showed that the 19 climate models studied gave an ECR which ranged from 110% to 240% of the TCR, with an average of 180% … go figure.
This lets us calculate global average sensitivity. If we use the model percentages to estimate the equilibrium climate sensitivity (ECS) from the TCR, that gives an ECS of from 0.14 * 1.1 to 0.14 *2.4. This implies an equilibrium climate sensitivity in the range of 0.2°C to 0.3°C per doubling of CO2, with a most likely value (per the models) of 0.25°C per doubling. If we use the 130% estimate from the Otto study, we get a very similar result, .14 * 1.3 = 0.2°C per doubling. (NOTE: these values are reduced from the original calculations. See the Update at the end of the post for details.]
This is small enough to be lost in the noise of our particularly noisy climate system.
A final comment on linearity. Remember that we started out with the following claim, that the change in temperature is equal to the change in forcing times a constant called the “climate sensitivity”. Mathematically that is
∆T = lambda ∆F
I have long held that this is a totally inadequate representation, in part because I say that lambda itself, the climate sensitivity, is not a constant. Instead, it is a function of T. However, as usual … we cannot assume linearity in any form. Figure 5 shows a scatterplot of the TCR (the decadal climate sensitivity) versus surface temperature.
Figure 5. Transient climate response versus the average annual temperature, land only. Note that the TCR only rarely goes below zero. The greatest response is in Antarctica (dark red).
Here, we see the decoupling of the temperature and the TCR at the highest temperatures. Note also how few gridcells are warmer than 30°C. As you can see, while there is clearly a drop in the TCR (sensitivity) with increasing temperature, the relationship is far from linear. And looking at the ocean data is even more curious. Figure 6 shows the same relationship as Figure 5. Note the different scales in both the X and Y directions.
Figure 6. As in Figure 5, except for the ocean instead of the land. Note the scales differ from those of Figure 5.
Gotta love the climate system, endlessly complex. The ocean shows a totally different pattern than that of the land. First, by and large the transient climate response of the global ocean is less than a tenth of a degree C per doubling of CO2 (global mean = 0.08°C/2xCO2). And contrary to my expectations, below about 20°C, there is very little sign of any drop in the TCR with temperature as we see in the land in Figure 5. And above about 25°C there is a clear and fast dropoff, with a number of areas (including the “Pacific Warm Pool”) showing negative climate responses.
I also see in passing that the 30°C limit on the temperatures observed in the open ocean occurs at the point where the TCR=0 …
What do I conclude from all of this? Well, I’m not sure what it all means. A few things are clear. My first conclusion is that the idea that the temperature is a linear function of the forcing is not supported by the observations. The relationship is far from linear, and cannot be simply approximated.
Next, the estimates of the ECS arising from this observational study range from 0.2°C to 0.5°C per doubling of CO2. This is well below the estimate of the Intergovernmental Panel on Climate Change … but then what do you expect from government work?
Finally, the decoupling of the variables at the warm end of the spectrum of gridcells is a clear sign of the active temperature regulation system at work.
Bottom line? The climate isn’t linear, never was … and succumbing to the fatal lure of assumed linearity has set the field of climate science back by decades.
Anyhow, I’ve been looking at this stuff for too long. I’m gonna post it, my eyeballs are glazing over. My best regards to everyone,
w.
NOTES
LAG CALCULATIONS
I used the Lissajous figures of the interaction between the monthly averages of the TOA forcing and the surface temperature response to determine the lag.
Figure N1. Formula for calculating the phase angle from the Lissajous figure.
This lets me calculate the phase angle between forcing and temperature. I always work in degrees, old habit. I then calculate the multiplier, which is:
Multiplier = 1/exp(phase_angle°/360°/-.159)
The derivation of this formula is given in my post here. [NOTE: per the update at the end, I’m no longer using this formula.]
To investigate the shape of the response of the surface temperature to the TOA forcing imbalance, I use what I call “scribble plots”. I use random colors, and I draw the Lissajous figures for each gridcell along a given line of latitude. For example, here are the scribble plots for the land for every ten degrees from eighty north down to the equator.
Figure N2. Scribble plots for the northern hemisphere, TOA forcing vs surface temperature.
And here are the scribble plots from 20°N to 20°S:
Figure N3. Scribble plots for the tropics, TOA forcing vs surface temperature.
As you can see, the areas near the equator have a much smaller response to a given change in forcing than do the extratropical and polar areas.
DATA AND CODE
Land temperatures from here.
CERES datafile requisition site
CERES datafile (zip, 58 MByte)
sea temperatures from here.
R code is here … you may need eyebeach, it’s not pretty.
All data in one 156 Mb file here, in R format (saved using the R instruction “save()”)
[UPDATE] Part of the beauty of writing for the web is that my errors don’t last long. From the comments, Joe Born identifies a problem:
Joe Born says:
December 19, 2013 at 5:37 am
My last question may have been a little obscure. I guess what I’m really asking is what model you’re using to obtain your multiplier.
Joe, you always ask the best questions. Upon investigation, I see that my previous analysis of the effect of the lags was incorrect.
What I did to check my previous results was what I should have done, to drive a standard lagging incremental formula with a sinusoidal forcing:
R[t] = R[t-1] + (F[t] – F[t-1]) * (1 – timefactor) + (R[t-1] – R[t-2]) * timefactor
where t is time, F is some sinusoidal forcing, R is response, timefactor = e ^ (-1/tau), and tau is the time constant.
Then I measured the actual drop in amplitude and plotted it against the phase angle of the lag. By examination, this was found to be an extremely good fit to
Amplitude as % of original = 1 – e ^ (-.189/phi)
where phi is the phase angle of the lag, from 0 to 1. (The phase angle is the lag divided by the cycle length.)
The spreadsheet showing my calculations is here.
My thanks to Joe for the identification of the error. I’ve replaced the erroneous figures, Figure 4-6. For Figs. 5 and 6 the changes were not very visible. They were a bit more visible in Figure 4, so I’ve retained the original version of Figure 4 below.
NOTE: THE FIGURE BELOW CONTAINS AN ERROR AND IS RETAINED FOR COMPARISON VALUE ONLY!! 
NOTE: THE FIGURE ABOVE CONTAINS AN ERROR AND IS RETAINED FOR COMPARISON VALUE ONLY!!
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Greg: “The spreadsheet you put on dropbox does not display because it seems to contain lots of refs to a local file.”
Just replace his …dsin(x) with sin(x/180*pi())
Frank says:
December 19, 2013 at 11:05 pm
… Fewer than 10% of the photons emitted by the surface escape directly to space, …
———————————-
I don’t think I’ve heard that before. Not exactly the “atmospheric window” and “GHG interception wavelengths” explanation. The window is supposed to be huge, not 10%.
Which makes the argument “How does energy move in and out of the Earth system”. Take it down to the photon level, collisional energy exchange level and include time. Because that is the level it operates at. Climate theory operates many levels above that and probably misses all the important processes.
Willis-
Your Figure 5 is extremely interesting. In my opinion, it demonstrates that water vapor feedback overall is strongly negative. Over land at very low temperatures, the climate sensitivity approaches 1 C per CO2 doubling, which is the no-feedback value. There is very little water vapor at these temperatures. As temperature increases, the atmospheric water vapor absolute concentrations generally increase, and climate sensitivity drops asymptotically towards the values over the oceans shown in Figure 6.
“I don’t think I’ve heard that before. ”
The whole argument is mistaken. It is true that straight CO2 lines are totally saturated. The supposed logarithmic dependency now is due to spectral line broadening, specifically collision broadening.
His calculation is probably correct as far as it goes but misses the reason for the broadening.
Thanks Joe, that fixed it. Now we just need to know what col Q is !
I have not checked this through the maths but that curve in the spread sheet looks a lot like my graph’s A = S/(1+(ωτ)^2) , where S is tau/(heat capacity of mixed layer)
http://climategrog.wordpress.com/?attachment_id=399
Col Q must come from the data but not sure exactly what it is.
This may be getting somewhere but I still say it needs to combine delta_T and d/dt(delta_T) to get the correct response to the linear relaxation model.
The full response is:
A * forcing – Aτ * d/dt(forcing) + Aωτ * transient
(The transitory term can be ignored in the real data, it is model spin-up.)
It seems like Willis is currently looking at the first term since he’s only examining the in-phase response. My tau will be similar in magnitude to the lag, so there is a strong chance monthly changes will be neither clearly in-phase of clearly orthogonal, We need to take account of both or justify that one is negligible since we are not in the cross-over regime.
This has the potential to provide a method to evaluate independent sensitivity for different latitude bands, That would be informative.
Question is, if Rad goes up by say 0.5W/m2 and stays there how long will it take the mixed layer to stabilise? My gut feel is 3 or 4 months at least, that gives tau of the order of a month. If the major variation here is the annual cycle (probably with strong 6 months in tropics) , omega = 0.5 or 1 per month.
Thus omega.tau is of similar size and we are bang in the zone of the cross-over where T and dT/dt are about equal. That means Willis’ current estimations could be off by a factor of 2 or 3 but I have not worked out in which direction yet.
It may account for his figures being so far off every other estimation. 0.3 * 3 would be getting near the low end of the range that other are ready to conceive of (assuming the correction goes that way ).
oops, just remembered , omega in those equations in not in radians, it’s straight frequency but it needs to be established if this reaction is in cross-over for the annual cycle. Since that seems to be what the derived lag is related to.
Willis,
Take a function and perturb it by a small enough amount and it will appear to respond in a linear fashion. Only as the perturbation becomes llarger does one start to see the nonlinearity.
cba says:
December 21, 2013 at 7:15 am
Thanks, cba. I’m well aware of that, but it doesn’t apply here. If things were only perturbed a small amount, you would be right. But look at Figure 1. The size of the “perturbation” in the natural system goes from -60°C to plus 30°C, and it’s more than that if we look on a daily basis. As a result, any assumption of normality is suspect, the perturbation in natural systems is often far from small.
Regards,
w.
Curt says:
December 19, 2013 at 5:40 pm
george e. smith says:
December 19, 2013 at 3:00 pm
“The solar physicists keep telling us there has been NO statistically significant change in TSI in recorded history, so how can top of atmosphere flux change ?”
George: While the variation in radiative flux density from the sun is very small, on the order of +/-0.1% IIRC, the change in the percentage of this shortwave radiation reflected, mostly due to changes in cloud cover, and snow/ice surface cover, can be a lot larger. Similarly, the changes in longwave radiation from the earth at TOA can vary quite significantly due to temperature changes, humidity changes, and cloud cover changes. These variations are what the CERES satellites are monitoring.
Willis Eschenbach says:
December 19, 2013 at 5:53 pm
george e. smith says:
December 19, 2013 at 3:00 pm
“The solar physicists keep telling us there has been NO statistically significant change in TSI in recorded history, so how can top of atmosphere flux change ?”
George, there are a few things at work. First, we’re talking about the solar flux that is available gridcell by gridcell … consider the gridcells right by one of the poles as example of the extreme variations in solar flux.
Next, the earth is not always the same distance from the sun, which makes an annual difference of (from memory) about 28 W/m2.
Next, the TOA flux is not just the solar radiation. It is the solar minus the upwelling longwave and the reflected shortwave. Both of these later variables change constantly.
As a result, the Net TOA imbalance varies both in space for a given time, and in time for a given location.
w………..””””””””
Well I didn’t come down with the last shower. I do know that the earth sun distance changes throughout the year, and I do know that the sun’s radiance changes about 0.1% p-p over the solar cycle. All of those factors are averaged out in the published value for TSI, which was about 1362 Watts per square meter, the last time, I recall NASA/NOAA stating a recommended value. It is that averaged best value that they tell us hasn’t changed perceptibly. Well when I went to school the value was 1353 W/m^2, but that was based on balloon and rocket borne measures, in the upper atmosphere. But TSI is not affected by clouds. Absorption by the oceans is, and loss of outgoing IR is; and we have no ground level global monitoring of surface tsi, so there is no reliable surface energy absorption. Satellite cloud measurements, don’t tell you what radiation reaches the ground, and the satellites don’t give you full 4pi global 24hour continuous cloud measurement. Clouds come and go while a satellite crosses the sky, but the lost surface radiant energy happens in real time, and isn’t properly Nyquist sampled by any means. I have about zero confidence, that anybody knows what cloud influence on earth’s radiant energy balance is.