CL
Climate: Past, Present & Future

Climate: Past, Present & Future

The Climate Tango of ENSO and CO2

In 1904, the Swedish chemist Svante Arrhenius suggested that the burning of fossil fuels to satiate our hunger for energy would increase the percentage of carbon dioxide (CO2) in the atmosphere, which would change the Earth’s temperature. Regular measurements of atmospheric CO2, started in the late 1950’s at remote locations such as Mauna Loa in Hawaii and the South Pole, confirmed his hypothesis about increasing CO2, with one important caveat. The rate at which CO2 was accumulating in the atmosphere did not match the rate at which it was being produced by fossil fuel burning. In fact, the atmosphere was apparently retaining only half of what was pouring in. Figure 1 shows the observed atmospheric mole fraction of CO2 – moles of CO2 per mole of dry air, usually expressed in “parts per million” – changing with time, along with the change we would have expected if all our fossil fuel emissions would have stayed in the atmosphere.

Figure 1: Measured (CO2) mole fraction (moles of (CO2) per mole of dry air) at Mauna Loa, Hawaii in blue, which is a good approximation to the global average atmospheric (CO2). In red is what the global average mole fraction would have been if all the fossil fuel and land use change (mostly biomass burning) emissions since preindustrial times had accumulated in the atmosphere. The green shaded area, therefore, is (CO2) that was emitted due to human activity but did not stay in the atmosphere. Compared to the preindustrial baseline of 280 parts per million (ppm), the (CO2) accumulated in the atmosphere is roughly half of what was emitted. Monthly mean Mauna Loa (CO2) measurements from the Scripps Institute of Oceanography (SIO, http://scrippsco2.ucsd.edu/) and National Oceanic and Atmospheric Administration (NOAA, https://www.esrl.noaa.gov/gmd/ccgg/trends/), fossil fuel emissions from the Carbon Dioxide Information Analysis Center (CDIAC, http://cdiac.ornl.gov/), and land use change emissions from the Global Carbon Project.

Today, we know that the other half – the fossil fuel CO2 emission “missing” from the atmosphere – is taken up by the land biosphere and oceans. The land biosphere accumulates carbon from the atmosphere by increasing plant mass, while the oceans dissolve atmospheric CO2 as the accumulating fossil fuel CO2 in the atmosphere drives the ocean-atmosphere carbon equilibrium out of balance. Beyond this large-scale picture, however, much still remains uncertain. Which part of the land biosphere – the tropics, the temperate latitudes, or the boreal forests and grasslands – takes up the most carbon? How does that uptake change from, say, a drought year to a rainy year? Do old growth forests and young forests take up carbon differently? To what extent do the land and ocean uptakes respond to natural climate cycles such as El Niño or the Pacific Decadal Oscillation?

Answering these questions accurately will not only tell us how the carbon cycle works today, but also how it might respond to a changing climate in the future. Almost all climate models used today to predict future climate contain a model to simulate the response of the carbon cycle (such as the land uptake of CO2) to future climate forcings such as droughts, floods, and elevated temperatures. The prediction skill of a climate model depends crucially on the fidelity of these carbon cycle responses built into the model. However, for the future land carbon uptake these models do not even agree on the sign of the response. Natural climate variations such as the El Niño Southern Oscillations (ENSO) provide us with experiments to evaluate and improve our understanding of these carbon cycle responses.

ENSO is a climate pattern that involves periodic oscillation in winds and sea surface temperatures over the tropical eastern Pacific Ocean. It represents a major control on the year-to-year variation in temperature and precipitation in the Tropics, going through its El Niño and La Niña phases in an irregular fashion that is still difficult to predict but repeating in roughly four-year cycles on average. Less known is the control of ENSO on the atmospheric chemical composition. The global abundance of several gases including greenhouse gases of the natural atmosphere, such as CO2 and CH4, show a clear relation with ENSO. In the case of CO2, both the land and the ocean contribute to this variation in ways that are not well quantified yet, making ENSO an excellent test for models. Closest to the imagination are probably pictures with vague contours of Indonesian farmland covered in thick smoke during El Nino. Indeed, fire is an important mechanism connecting precipitation variability to CO2 variability.

Figure 2 shows the carbon cycle response to the ENSO cycle, as manifest in the atmospheric mole fraction of CO2. Atmospheric CO2 (as well as other greenhouse gases such as CH4) is measured cooperatively by multiple laboratories at a global network of sampling sites, an effort that began more than fifty years ago with Mauna Loa and South Pole. Our knowledge of the carbon cycle response to ENSO – such as the amount of additional carbon in the atmosphere during a strong El Niño, or the partitioning of that signal into contributing factors such as fires in Tropical Asia versus drought in Amazonia – derives to a large degree from these measurements.

Figure 2: The (CO2) growth rate as measured by the increment of one month over the same month in the previous year. The inter-annual variations in the (CO2) growth rate show a clear imprint of ENSO. Large El Niño events such as the 1997-98 and 2015-16 ones show up as anomalously large spikes in the growth rate. Most of the additional (CO2) in the atmosphere during and after an El Niño comes from the Tropics, and therefore the response measured at Mauna Loa (red) is usually larger than the global average response across a network of background sites (blue). (CO2) data taken from the NOAA (CO2) trends page at https://www.esrl.noaa.gov/gmd/ccgg/trends/.

The atmospheric growth rate of the CO2 mole fraction spikes right after a big El Niño event, such as after 1997-98 and 2015-2016 in Figure 2. Since we know the total mass of air in the atmosphere, we can translate between CO2 mole fraction spikes of Figure 2 and mass of carbon added to the atmosphere. The 1997-98 El Niño added ~2 Petagrams carbon (PgC) to the atmosphere, while preliminary estimates suggest that the more recent 2015-16 event injected ~3 PgC (for comparison, our current global fossil fuel emission is ~10 PgC/year). Having a global network of sites – instead of just background sites such as Mauna Loa – allows us to drill down into the mechanisms behind each of these CO2 increments. For example, we know now that most of the additional 2 PgC carbon from the 1997-98 El Niño was injected from extended fires in the Tropics. Due to the sheer magnitude of the carbon cycle response to El Nino, with the year 2015 setting the record in global CO2 growth to just above 3 ppm/yr, ENSO events present natural experiments against which we can verify our understanding of the interaction between climate and the carbon cycle.

Even for the large changes in CO2 as observed during strong El Nino’s the attribution to specific processes remains a challenge, because of the various coupled responses in the Earth system. For example, the ocean-atmosphere exchange of CO2 is also influenced by ENSO, as shifting patterns in tropical sea surface temperature change the mixing rate of deep and surface waters, influencing gas exchange. Therefore, to get the process-attribution correct, scientist try to disentangle the various influences on atmospheric CO2, which requires a lot of measurements.

Over the past couple of decades, it has become clear that our cooperative network of atmospheric measurements has large gaps over areas that play very important roles in determining the climate impact on the carbon cycle. The gaps are usually due to logistical reasons, such as the difficulty of maintaining measurement sites in Tropical forests, or the expense of making regular shipboard measurements to cover the oceans. To fill this data gap, space based measurements have emerged as a promising yet challenging alternative.

Carbon cycle gases such as CO2 and CH4 (and to a lesser extent CO), by virtue of being greenhouse gases, absorb and emit electromagnetic radiation at certain specific frequencies, usually in the infrared (IR). In theory, a downward-looking IR sensor at the top of the atmosphere should be able to estimate the amount of these gases by measuring the strength of IR radiation at those frequencies. Figure 3 shows the average CO2 mole fraction between the surface and the top of the atmosphere (“column average CO2”) retrieved from the Orbiting Carbon Observatory 2 (OCO2) satellite over Equatorial Africa, showing elevated values due to biomass burning.

Figure 3: Column average CO2 over Central Africa in 2015 from the Orbiting Carbon Observatory 2 (OCO2) satellite. The bright red band over Equatorial Africa due to biomass burning is visible in contrast to lower (CO2) elsewhere. Column average CO2 from the ACOS algorithm available at https://co2.jpl.nasa.gov/#mission=OCO-2

In practice, IR measured from space is sensitive to many interfering species other than CO2 or CH4, such as the amount of water vapor and dust particles, complicating the estimation of CO2 and CH4 from space. If these complications can be resolved in the near future, space-based measurements could potentially fill the data gap between surface measurement sites (such as Equatorial Africa, which has almost no surface measurements) and enrich our knowledge of the carbon cycle. With such improvements to our measurement capabilities, we hope to better understand today’s carbon cycle and its response to climate. The clearer we see this carbon-climate tango, the better we will be able to predict its imprint on tomorrow’s climate. The most recent climax was one of the most well observed in history. Data are pouring in from multiple sources, and the coming few years promises a lot of interesting analysis as we try to decipher the steps of this complicated dance. Keep your eyes peeled for updates on this blog!

This post has been written by:

Dr Sourish Basu,  NOAA Earth System Research Laboratory, USA
Dr Sander Houweling, SRON Netherlands Institute for Space Research, NL

and edited by the new editor of this blog Célia Julia Sapart, Université Libre de Bruxelles, B.

EGU, Vienna 2015: the round-up

EGU by numbers

In April, the EGU returned to Vienna for their annual Congress meeting. Over 11,837 scientists from 108 countries descended in the Vienna International Centre for the six-day conference. Delegates enjoyed over 4,870 oral presentations, 8,489 posters, and 705 PICO presentations. That’s a lot of science!

The Vienna International Centre – where the magic happens

 

Science and ice cream for everyone!

As always, the EGU were excellent hosts and organised over 300 side events that included a range of activities, workshops, and networking events for all delegates. Among this year’s favourites were the Geo Cinema, Science Communication workshops, and Ask the Expert panel sessions. Another added bonus this year was the ice cream stall in the foyer – my personal favourite was the pumpkin seed flavour (tastier than it sounds, I promise).

 

With 23% of delegates being students, and a strong Early Career Scientist contingent, the Young Scientists’ lounge proved very popular, and provided a great social space to grab a coffee, talk to friends, finalise PowerPoint slides, and peruse the latest job adverts.

 

The exhibition hall where delegates can peruse the latest journals, textbooks, and equipment. And buy their ice creams!

The exhibition hall where delegates can peruse the latest journals, textbooks, and equipment. And buy their ice creams!

 

The best bits of Climate: Past, Present and Future

The Climate division hosted over 75 scientific sessions, covering climate science research from the poles to the tropics. We also enjoyed some excellent workshops including an ‘Introduction to climate modelling’ session and a ‘Meet the Editors’ panel discussion with Professor Carlo Barbante (Editor of Climate of the Past) and Professor Axel Kleidon (Editor of Earth System Dynamics).

 

Thanks EGU and see you next year!

Amid the scientific sessions and workshops, the EGU is always a great place to catch up with old friends and colleagues, and make new collaborations. There is also time to sample the delights of Vienna, while discussing research projects over a Wiener Melange. After another impressively productive and enjoyable conference, we are all looking forward to EGU Vienna 2016!

A Climate Modeling Workshop in the South of France!

Climate and its effects on the past, present and future of the human race is a heated, topic of debate these days. There are many competing interests at stake from governments and politicians to the big oil and energy companies of the world to the scientists trying to work on climate change problems to the people of the world most acutely affected by these changes on the Earth we live. Thus, I think it is extremely important that everyone works together in this day and age to bring together what each individual party excels at to the table and to combine these things into a powerful plan to help mitigate the effects of climate change for future generations that will call Earth home. This is why a group of young and senior scientists gathered in Aix-en-Provence, France the last week of January: to pave the way forward for future generations to investigate, reflect upon and solve climatic problems that plague our civilization.

It was quite a diverse group with PhD students, Post-Docs and professors from all over the world including France, Germany, the U.K., Spain, The Netherlands, the U.S., Canada, Italy and many others. It was not only diverse culturally, but also in the geologic disciplines we come from with all of the big fields in representation such as isotope geochemistry, climate modelers, organic geochemists, geochronologists and thermochronologists, sedimentologists, structural geologists and of course many others.

The climate workshop was sponsored by the Marie Curie Initial Training Network (ITN) called iTECC, which stands for Integrating Tectonic Erosion Climate Couplings (www.itecc-eu.eu). We are a group of 15 PhD students, 4 Post-Docs, all of our respective advisors and a number of other organizations and institutions involved in various ways with the project. Of course, each student and post-doctorate has his or her respective project within the frame work of the iTECC ITN, but as a whole group we are generally concerned about Himalayan geology in all forms. But more specifically we have these goals and aims:

  • Training of scientists with the ability to contribute to multi-disciplinary research ranging from solid Earth processes to climate dynamics, and application of these skills in academia and industry;
  • Integration of research on present-day deformation with information from the geological record to understand how the lithosphere deforms;
  • Significant improvement in the recovery and exploitation of tectonic, erosive, weathering and climatic records from sedimentary sequences;
  • Evaluation of the impact of elevation and exhumation of the Himalayas on climate;
  • Evaluation of the impact of climate, through erosion, on the tectonic evolution of the Himalayan orogeny;
  • Validation of climate models and applying them to verify the interconnections between tectonics and climate;
  • Building a bridge between science and the local community through outreach.

It is quite an extensive and connected project and I feel very grateful for the opportunity to be involved in something so expansive and important. Anyway, part of our training is to attend these “mini-workshops” as a group every few months. iTECC has organized an Earth Observation Workshop, an Isotope Geochemistry workshop, a so-called “Research in Progress” workshop as well as a Thermochronology workshop, among others. These workshops serve as opportunities to expand our knowledge base and make connections between our specific projects/fields and new geo-disciplines that maybe we would have not made otherwise.

The climate workshop that we are now talking about in Aix brought together, of course iTECC, but a number of professors, scientists and PhD and Post-Docs outside of iTECC. For example, the University of Chicago, University of Bristol, University of Paris Saclay, the University of Bergen, GFZ Potsdam and others.

Here is a list of the speakers that presented at this conference and their topics:

  • Didier Paillard (U Paris-Saclay): On the diversity of “climate” models
  • Matt Huber: Eocene Warm climates and the transition into our icehouse world
  • Dan Lunt (U. Bristol): The role of palaeogeography in controlling Cretacous and Paleogene climate and climate variability
  • Jérémy Jacob (ISTO): Should representativness of sedimentary lipid and their dD values be discussed with palaeoclimatologists?
  • Ray Pierrehumbert (U. Chicago): Approaches to idealized modeling of the climate system
  • Zhongshi Zhang (U. Bergen): Tethys shrinkage and monsoon evolution in Asia and Africa
  • Francis Codron (U. Paris 6): Middle latitudes atmospheric circulation
  • Dorian Abbott (U. Chicago): Dealing with cloud uncertainty when modeling paleoclimate
  • Dirk Sachse (GFZ Potsdam): Compound-specific C and H isotopes from lipid biomarkers as molecular rain gauges
  • Bodo Bookhagen (U. Bergen): Extreme Events and Intensified Monsoon Periods in the Himalayan Field
The goal is to model these complex systems at the present time but also into the recent and geologic past and into the future. This gets complicated quickly with all of the factors involved.

The goal is to model these complex systems at the present time but also into the recent and geologic past and into the future. This gets complicated quickly with all of the factors involved.

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Of course, all of the students and post-doc’s were able to take away some amazing new information about unfamiliar analytical techniques or maybe remote sensing or even new knowledge about these popular(?) and infamous(?) Global Climate Models (GCMs). But I think what I took away from this workshop the most was first pointed out by Didier Paillard in the first lecture and then confirmed by many of the other modelers present, especially since I come from a modeling background. Didier really wanted us to understand that it is ok for our models to be wrong, or that is, not represent the data or findings that we want to compare the model too. And, in fact, he expressed to us that we should want our models to be wrong!

One type of GCM displaying the sea surface temperature and the sea ice concentration.

One type of GCM displaying the sea surface temperature and the sea ice concentration.

Now you are saying, “Hold on there for just one minute! Don’t we need models to be right to be able to understand what happened in the past and also what might happen in the future?” Well, yes this is obviously true. But, to be wrong means that we know how to analyze the output of a model and then adjust the input so that model is more accurate for the next time. Also, being wrong can lead to an amazing new discovery that would have never happened if the model(s) were always right. Some of the most famous discoveries in science (and other fields) happened not because the scientists did the right things, but because they made a mistake and were subsequently smart about it! As Didier called them, “smart mistakes.” What, smart mistakes? Yes, well obviously you can make mistakes while doing anything, but the point is that you can learn from that mistake and not make it again or can continually make the same mistake. Hence, the former is considered a “smart mistake.”

And I think these lessons that we learned in this climate workshop and in general in our studies our especially important as young scientists in crucial fields such as climate change, where I tend to think that some (but not all) of the older generation, especially those outside the technical fields, have not learned these lessons and experienced them at work. Thus, we are trying so very hard to find the perfect solution to the world’s climate problems in one try, that, unfortunately, we do not learn from our mistakes and many times perpetuate them over and over again. But maybe there is hope with our generation that can take these lessons and knowledge about climate change and how it works and use it find sustainable solutions for the future. Who knows! But I do know I am very much looking forward to the next iTECC workshop! Stay up to date with iTECC and what we are doing via our website’s blog and social media pages!

Welcome to the world of climate: past, present and future!

Just like the Earth’s ocean-climate system itself, the climate of climate science is ever evolving and changing, both politically and scientifically. On the 21st of December 1872, HMS Challenger set sail from Portsmouth on a three year long voyage of discovery. The pioneering work that happened during those intrepid months aboard, laid the foundations for the climate science that happens today. I recently embarked upon a research cruise (or as we call them, a scientific campaign), and each time we sent the coring barrel 2 km – 3 km down into the abyss below and an hour or so later hauled our finds onboard, it was like unwrapping a Christmas present when we split open each core, due to the potential of new discoveries to come. So, I can only imagine the excitement each time the scientists aboard HMS Challenger cast their nets, or measured their next sample. It was during that very first oceanographic voyage that we learnt that basically, the chemistry of the world’s oceans was roughly (give or take) the same, we learnt how salty the oceans were and in the years that followed that cruise, the diversity of life in the oceans started to reveal itself. Even now, we discover new species as we sample further into the abyssal depths (http://www.coml.org/), highlighting how much we don’t know about a resource that is so precious to us.

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But I digress… climate science has progressed in leaps and bounds over the past few decades and likely much further beyond the wildest dreams of those who participated in the HMS Challenger expedition, which was embarked upon over a century ago. Facilitated by step changes in the underpinning technologies and funding initiatives, we now have long-term monitoring programmes that aim to measure the current state of our oceans, we can combine remote satellite and radar data with ground-truthing measurements in the cryospheric (glacial) parts of our globe, we can assess future impacts by using highly sophisticated computer simulations, and we can test these by looking at past climate changes. These past climatic changes can be assessed by measuring proxies. We can use ice cores to tell us about past temperatures and atmospheric gas concentrations, we can use microfossils in the marine sediments to indicate past oceanic temperatures and salinity, and we can use tracers and sediment properties to better understand how oceanic circulation patterns differed from the present-day. We can use tree rings, lake proxies and cave records to reconstruct precipitation patterns, and we can also turn to geomorphology, sedimentology and geophysics to inform us of past ice limits. For the climate of the last millennium, further evidence can be found in archaeological remains, as well as in historic records, and for the past few decades, we can generate temperature series from instrumental measurements. By knitting together the information within these different disciplines, there is a thriving community focussed towards driving our understanding of all aspects of the Earth’s climate, and the Intergovernmental Panel on Climate Change (IPCC) and the EGU Climate Division: Past, Present and Future are key instruments to do exactly that.

Historic and instrumental records of climatic change demonstrate that global average temperatures have risen by 0.72 ºC since the 1950’s (IPCC, 2013) and that as a response to this, mountain glaciers, as well as the Greenland and Antarctic ice sheets are diminishing at an astonishing rate. According to the IPCC (2013), projected rates of increased atmospheric CO2 concentration suggests that by 2100 we might experience 0.5 – 4 ºC of further enhanced warming and 0.5 – 0.9 m of sea-level change. By 2050, we might expect an almost ice-free world. The EGU-CLIMATE blog aims to take you through a journey of discovery as to how we put all the pieces of the climate jig-saw puzzle together.

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