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All IPCC definitions taken from Climate Change 2007: The Physical Science Basis. Working Group I Contribution to the Fourth Assessment Report of the Intergovernmental Panel on Climate Change, Annex I, Glossary, pp. 941-954. Cambridge University Press.

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The human fingerprint in global warming

What the science says...

Select a level... Basic Intermediate Advanced

Multiple sets of independent observations find a human fingerprint on climate change.

Climate Myth...

It's not us

'What do the skeptics believe? First, they concur with the believers that the Earth has been warming since the end of a Little Ice Age around 1850. The cause of this warming is the question. Believers think the warming is man-made, while the skeptics believe the warming is natural and contributions from man are minimal and certainly not potentially catastrophic à la Al Gore.' (Neil Frank)

At-a-glance

Since the pre-industrial era, we have burned ever-increasing amounts of fossil fuels. This we can see for ourselves, often just by looking out of the window or hear, by listening to the flow of traffic. The sights and sounds of fossil fuel burning, constant, perpetual.

We cannot see or taste carbon dioxide, one of the two main products of that combustion, the other being water vapour. But it's constantly heading up into our atmosphere – in 2021 alone the figure for such emissions, according to the International Energy Agency, was 36,300,000,000 tonnes of the stuff. Just imagine for a moment that amount of sand piled up in a heap!

Once up there, one key difference between carbon dioxide and water vapour becomes critically important. Water vapour condenses to form clouds and freezes to form ice crystals. Rain, hail, sleet and snow all fall from clouds – it's a constant, ongoing cyclic process, even though different places see much more – or much less precipitation.

Carbon dioxide has no liquid state at the pressures encountered in Earth's atmosphere. Instead, at normal atmospheric pressures, it sublimes from solid to gas at −78 °C. Solid carbon dioxide is also known as dry ice, but cannot form in the range of temperatures found within Earth's atmosphere, although it is produced industrially for various purposes. So as opposed to water vapour, carbon dioxide is an example of a non-condensing gas: once up there it stays up there for a long time. That's why our vast CO2 emissions are causing levels of the gas to build and build.

If you needed a smoking gun in order to accept the above, there is one: carbon dioxide derived from fossil fuel burning has a very distinct chemical fingerprint that is readily measurable in air samples. To find out how we do that, read the further details below. Such measurements, with a trend precisely following the pathway we would expect due to our increasing emissions, show that far from being someone else's problem, one way or another we are all bang to rights in this case.

Please use this form to provide feedback about this new "At a glance" section. Read a more technical version below or dig deeper via the tabs above!


Further details

If you wanted to find a smoking gun with respect to human carbon emissions and their role in global warming, where would you look? There are several and the Intermediate version of the rebuttal lists and describes many of them, but we’ll start here with the most important one.

Fossil fuel production and usage is all well-documented. For that reason, CO2 emissions are also well-documented. In 2019, some 44.25 billion tons (or gigatons) were emitted to the atmosphere (IPCC AR6, WG III Technical Summary 2022). That figure was the highest recorded in a steady year-on year upward annual trend.

So we know all too well that every year of late we have added tens of billions of tonnes of CO2 to the atmosphere. How do we detect that fossil fuel signature in the air? 

Human fingerprints

Fig. 1: human fingerprints on the crime-scene of climate change. Note several lines of evidence refer to 'fossil fuel carbon'. Now read on….

The answer lies in carbon isotopes.

Most chemical elements exist in nature as more than one version. These different versions are an element's isotopes. Carbon is no exception to the rule. Its most important natural isotopes are carbon 12, carbon 13 and carbon 14, written 12C, 13C and 14C. All three contain six protons in their atomic nuclei – that's carbon's atomic number and it's fixed. But carbon 12 atomic nuclei contain six neutrons whereas 13C has seven and 14C has eight.

Carbon 14 only occurs in tiny traces – about one atom per gram of carbon is a ballpark figure. It forms in nature through neutron bombardment of nitrogen atoms from cosmic rays near the top of our atmosphere. Man has had a hand here too: nuclear explosions also produce high-energy neutrons and the weapons-testing mania last century increased the amount of 14C by two orders of magnitude. The isotope is useful since it is radioactive and can be used to radiometrically date geologically young materials. Because its decay-rate is rapid (half-life of 5,700 years), anything more than about 50,000 years old is too 14C-depleted for radiocarbon dating. The fossil fuels, millions to hundreds of millions of years old, are devoid of 14C.

Carbon 12 is stable and very common, constituting 98.93% of all carbon on Earth, with carbon 13 making up the remainder, apart from the tiny amount of carbon 14. In that vital process of photosynthesis, carbon dioxide and water are absorbed by plants. These raw ingredients are converted into nutrients (sugar) and as a by-product, two thirds of their contained oxygen are released to the atmosphere, making it breathable by us and our fellow life-forms. The important bit is that during photosynthesis, carbon isotopes fractionate, meaning that the proportions of 12C and 13C are changed by the chemical reactions involved, with a preferential uptake of 12C in that sugar. So photosynthesis produces a shift in favour of 12C.

Any carbon-bearing sample – a bottle of oil, lump of coal, a piece of calcium carbonate such as limestone or a sea-shell, a flask of air - there are numerous examples – can be analysed and its carbon isotopic composition determined. Therefore, its ratio of 13C to 12C (known as delta or d13C) can be calculated and compared to an internationally-agreed standard composition. The equation is as follows:

delta 13C = ((13C/12C sample)/(13C/12C standard) -1) x 1000%

Now, because of that preferential take-up of 12C in plants, the d13C value, expressed in ‰, of anything derived from their decomposition, combustion, preservation or consumption will be similar. As such the smaller (or more negative) d13C value spreads up the food chain, gets preserved in coal, oil or gas deposits, in carbonate rocks like limestones and in shelly fossils.

It should come as no surprise, then, that if you dig up and set fire to fossil fuels, the CO2 emitted in that process will give the atmosphere a more negative d13C – and that's exactly what we find. If all the CO2 in the atmosphere was that outgassed by volcanoes, we would see d13C closer to zero; instead the ongoing trend is more and more negative; a cumulative plot from the Mauna Loa and South Pole air sampling stations (fig. 1) shows values of -7.5‰ in 1980, heading steadily downwards to -8.5‰ in 2020. The estimated pre-industrial value is around -6.6‰ (Graven et al. 2020). This is one smoking gun of man-made carbon dioxide emissions. Another is that because the fossil fuels are devoid of 14C, it follows that fossil fuel CO2 emissions are, too - thereby further diluting the already tiny amount of 14C in the atmosphere.

The carbon isotope record

 

Fig. 1: the carbon isotope record, 1975-2022. Black Dots: Monthly average carbon isotope ratio (d13C) of atmospheric carbon dioxide at Mauna Loa Observatory, Hawai. As with the Keeling Curve of CO2 levels, the graph shows the seasonal wobble caused by photosynthetic plants as leaves grow and then die.Red Dots: Monthly average d13C of atmospheric carbon dioxide at the South Pole, Antarctica.

Carbon isotope ratios are also very useful in geology. Sudden changes in their values, known as positive or negative “excursions”, tell us something monumental has occurred. For example, one of the biggest negative d13C excursions in the geological record marks the end-Permian mass extinction, 250 million years ago (Saitoh & Isozaki 2021).

That one of the most prolonged and voluminous episodes of volcanism in the past 500 million years occurred at the same time as the end Permian mass extinction suggests a lot of CO2 was released back at the time. But volcanogenic CO2, originating in Earth's Mantle, has a “heavier” or more positive d13C of around -6‰. It cannot have caused the negative excursion, but one thing could. In the sedimentary basin through which the magma rose from deep in the Earth there were vast oil and coal deposits and they got comprehensively roasted in the process. It is estimated that as a consequence, the Siberian Traps eruptions released between ten trillion and one hundred trillion tons of carbon dioxide over just a few tens of thousands of years, some of volcanic origin but a heck of a lot from those cooked fossil fuel deposits. What happened in Siberia 250 million years ago thereby presents Mankind with its starkest possible warning about messing with Earth's carbon cycle.

Last updated on 2 July 2023 by John Mason. View Archives

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Argument Feedback

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Further reading

Professor Scott Mandia has a detailed explanation of why more CO2 causes stratospheric cooling that is well worth a read.

Denial101x video

Here is a related lecture-video from Denial101x - Making Sense of Climate Science Denial

Comments

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Comments 101 to 113 out of 113:

  1. David Kirtley and MA Rodger

    Thank you both for the responses.  David, the Bloomberg link did not get me to the article, and neither did their search option.  Do you happen to have a copy?

  2. Hmmm...that's odd. The link works for me. Maybe try google?

  3. The Bloomsberg link is not to an "article" as such but to a set of graphs beneath which is set out the methodology behind the graphs. And within that methodology is a link to what could be construed as the underlying "article" - Miller et al (2014) 'CMIP5 historical simulations (1850–2012) with GISS ModelE2' although it has broader coverage.

  4. For a purely empirical fit of ENSO, Volcano, solar to temps since 1950, try here. Unlike other curve-fitting exercises which try to show warming is due orbit of jupiter, rise of irrigation etc, this uses half the data as training set and then uses the result to model the other half.

    Benestad & Schmidt 2009 challenged Scafetta nonsense with naive empirical analysis of effects of forcing which I think may be closer to what you want.

  5. richieb1234 - As MA Roger pointed out, volcanic activity adds complexity to any kind of curve-fitting. Climate response to volcanic aerosols is quite fast compared to other forcings. 

    Tamino did an excellent article on using a combination of a simple 2-box model (one fast response, one slow) along with ENSO, and and showed an excellent fit to the observed climate response, see Once is not enough. Two time constants (2 and 26 years) and one large oscillation appear to be sufficient parameters to map the climate response to forcings. 

  6. David Kirtley:  I did get into the Bloomberg link using Google.  Very intereting.  But I was surprised that it shows a negative trend on temperature effect of aerosols all the way to 2005.  The information I have shows worldwide aerosol concentrations dropping by about 30% between 1980 and 2010.  Shouldn't that have caused somewhat of a reversal in the temperature contribution?

  7. :As I mentioned earlier, I am a trainer.  As I read and reread the original post, I think a good analogy to use is the way in which police organizations identify the source of an illicit drug.  A drug that's intercepted on the street could come from anywhere: Colombia, Bangladesh, a rooftop in New York.  "You just can't tell for sure."  But international law enforcement agencies have developed the forensic methods to identify the source by examining its physical and chemical signatures.  It works for natural and synthetic drugs.  One can even identify where drugs have been "cut" by the signatures of the chemicals used.  The same approach is used to distinguish natural causes of warming from man-made causes.  I think this is a good analogy that most adults can identify with.  Once they understand the approach, their minds will be much more open to hearing about the 10 signatures of anthropogenic warming.

  8. richieb124 - the IPCC reports each have a chapter on attribution which is what the literature calls it. I agree that your analogy is a good one but doing real-world attribution is a very complex task. The "fingerprints" in this post I think is about as good as it gets without using a physics-based model. Each individual one is ambiguous, but the sum is telling.

  9. richieb1234 @106,

    It is correct that there has been a substantial reduction on SO2 emissions over recent decades. The graphic on this webpage suggests 30% reduction 1980-2010 and other data suggests reductions do continue but less strongly. Yet when the aerosol forcing is shown (eg IPCC AR5 AII Table 1.2), we see a peak in 2000 and a very minor decline.

    One reason that this may be so is that aerosols are very short lived and thus their effects dependent on the region of their emissions. NASA data (since 2005) allows the latitude of emissions to be easily quantified. Since 2005 thre have been small reductions in higher northern latitudes (eg USA & Europe), quite large reductions in lower northern latitudes (eg China) while emissions in the tropics and the southern latitudes have remained roughly constant. I would suggest that there is little relationship between global totals for SO2 emissions and the global size of the resulting climate forcing. The location of the emissions has a big effect on the overall forcing levels.

  10. MA Rodger

    Thanks for the response.  I will look into the IPCC and NASA references.

    "The graphic on this webpage suggests 30% reduction 1980-2010 and other data suggests reductions do continue but less strongly."

    Yes.  If anything, particulate concentrations may rise for the rest of the century.  The graphic shows a very small contribution from Africa.  U.N. Population projections for Africa show 4 billion people by the end of this century, comparable to Asia.  That could ramp up worldwide average particulate concentrations and spread them more equally across the globe.  Qualitatively, the competition between GHG warming and particulate cooling could be the biggest uncertainty in the future.

    "One reason that this may be so is that aerosols are very short lived and thus their effects dependent on the region of their emissions"

    I see your point, but wouldn't the total amount of solar reflection be the most important variable, no matter where it occurs?  Wouldn't the resulting cooling eventually even out across the globe?  I will take your suggestion and look at the IPCC reference.     --Richieb

  11. richieb1234 @110,

    The reflectiveness of cloud is the method by which SO2 provides climate forcing, this by providing aerosols to make the forming clouds shinier. But there is much complication. SO2 is not the only aerosol agent and such mechanisms are short-lived and local. Thus, say, SO2 emissions causing shiny clouds at high latitudes, especially during winter with long nights, will not have as much sunlight to reflect. And the longevity/altitude of the aerosol will differ by location.

    The resulting cooling will be less localised.

    And globally there is an unresolved issue here. The reductions in SO2 emissions which will follow from eliminating FF use and the resulting loss of its negative climate forcing has got some to worry that there will be a boost to AGW as we de-carbon our economies. Some work is saying this is not really much of a concern (eg Shindell & Smith 2019 [Abstract]) while on the other side of the debate we find Cowern (2018) who argues that such a boost is already happening and the strong warming in recent years is due to the reducing SO2 emissions.

  12. One fingerprint seems wrong to me
    Fingerprint 'Less heat escaping to space'

    Assuming that the starting point of the energy balance is that the incoming radiation (IN) is equal to the outgoing radiation (OUT) (without taking into account the small part that is recorded as biomass in the lithosphere per year).

    If this is not the case and more energy is left behind on Earth every second, the temperature on Earth will continue to rise. This is not the case. More CO2 iterates to a new equilibrium at higher temperature.

    When more CO2 enters the atmosphere, an iteration takes place to a new equilibrium of IN = OUT, as follows: more radiation back means a higher surface temperature and therefore more blackbody long IR of the earth's surface, that means in a next step a little more LW IR back to Earth until it iterates to a new balance. The temperature of the earth's surface has then risen to such an extent that it compensates for the delay of the extra CO2.

    But seen from space, in the new equilibrium, the amount of radiation coming from the Earth per unit time is again equal to that from the sun, because the increase in the temperature of the Earth's surface has compensated for the delay by more CO2.

    If this reasoning is correct, then one of the fingerprints is not correct. If the reasoning is wrong, where is it wrong? You can easily calculate the iteration to a new equilibrium yourself with a simple formula or in an Excel spreadsheet.

  13. Marcel:

    The sequence of initial equilibrium --> CO2 added, equilibrium upset --> system changes to adapt and new equilibrium is reached more or less the way you describe it.

    In the Hansen et al 1981 paper examined here, figure 4 shows the modelled response to an instantaneous increase in CO2. The left side shows the immediate response, with the increased downwelling IR and a reduction in the loss to space. That continues in panel b), which is the state after the atmosphere has responded but before land an ocean can increase in temperature. The right panel shows the final new equilibrium after everything has warmed up.

    Hansen et al 1981 figure 4

    (Clicking on the image source should give you a larger version. I've scaled the display to fit the page.)

    We're a long way from reaching that final equilibrium, though, so we're still in panel b, more or less. We won't reach equilibrium until we stop adding CO2 and things can stabilize. If we only had to heat the ocean mixed layer (60-100m deep), then we'd still see heating for a few decades after CO2 stops rising. With deep oceans involved,  we're looking at centuries.

    The "fingerprint" relates to the current warming, not future equilibrium state.

  14. Please note: the basic version of this rebuttal has been updated on July 2, 2023 and now includes an "at a glance“ section at the top. To learn more about these updates and how you can help with evaluating their effectiveness, please check out the accompanying blog post @ https://sks.to/at-a-glance

    Thanks - the Skeptical Science Team.

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