Hydrofluorocarbons (HFCs) are replacements for chlorofluorocarbons (CFCs), whose use is being phased out because they are primarily responsible for depleting the ozone layer. While HFCs don’t destroy ozone, they are often very powerful greenhouse gases, so it is important that we monitor their concentration and emissions. One difficulty in doing this is that there are many HFCs emitted into the atmosphere, and new ones are appearing all the time.
To keep track of these gases, my colleagues in the AGAGE network have developed a system that can measure gas concentrations using mass spectrometry. The system is able to detect gases at very low concentrations, by removing most of the nitrogen and oxygen from the measured samples, increasing the concentration of the pollutants they want to measure. This means that we can now detect ‘new’ gases very soon after they appear in the atmosphere.
In this paper, Martin Vollmer from Empa in Switzerland describes the measurement of four HFCs that have appeared in the atmosphere over he last decade or so (HFC-227ea, HFC-236fa, HFC-245fa, HFC-365mfc). Using a combination of in situ measurements, and new measurements of archived air samples, we can determine the entire air history of the four gases, from the year they first appeared in detectable amounts.
Using these observations, and a two-dimensional model of the atmosphere, we calculated the annual global emission rates. As is often the case, the emissions we found differed from inventory estimates by substantial amounts, highlighting the value of these sort of ‘top-down’ verification techniques.
Over the last couple of years, a few of us at MIT and Scripps have been thinking about how we could estimate trace gas emissions over several decades using archived air samples. For example, the Cape Grim Air Archive, from Tasmania, is a really nice collection of air samples that have been taken under carefully controlled conditions over many decades. The archive was set up so that as measurement techniques improved, we could monitor the history of important atmospheric gases that were difficult to measure in the past. We’ve used these observations to determine global emissions of species like the perfluorocarbons (see Jens Muhle’s paper), and some newly-observed HFCs (in Martin Vollmer’s recent paper), all of which are very potent greenhouse gases.
However, one problem that we kept encountering was that, using our usual methods for determining emissions, we would get large ‘jumps’ in our derived emission, which we knew were unlikely to have occurred in the real world. These fluctuations were probably caused by slight biases in the observations, or inaccuracies in the independent emissions inventories that we have to use as a first guess. To get around this problem, we tried to think about how we could derive emissions using information on how we would expect emissions to change from one year to the next. For example, if a gas is emitted by Aluminium smelters, then emissions are not very likely to change by more than a few percent per year, because the number of smelters, or the emissions processes, are unlikely to change very fast.
We found some techniques that addressed similar problems in other fields (notably Oceanography), and modified them so that they could easily be applied to atmospheric trace gas emissions estimation. The result is a method that firstly allows you to estimate the emissions growth rate, based on some prior information, and the uncertainty that you expect this estimate to have. Then a chemical transport model is used to produce an emissions estimate that best matches both the measurements, and our emissions growth constraint. The paper, written with Anita Ganesan and Ron Prinn, can be found here.
Sulfur hexafluoride (SF6) is a particularly potent greenhouse gas. It is used in large electrical equipment, and leaks into the atmosphere during maintenance. Once it is in the atmosphere, it is only destroyed if it reaches very high altitudes, making it last for hundreds to thousands of years. It is also a very strong absorber of infra-red radiation. These factors result in it being one of the most potent greenhouses yet discovered. One tonne of emissions is thought to be equivalent to releasing over 22,000 tonnes of CO2.
In collaboration with many of my AGAGE and NOAA colleagues, we examined how concentrations of this gas have increased in the atmosphere since the 1970s, and determined global and regional emissions (see Atmospheric Chemistry and Physics paper). We find that concentrations of SF6 have increased by more than a factor of 10 since our first measurement in 1973. We also find that global emissions are now higher than ever, and have increased by almost 50% in the last 5-10 years.
We wanted to find out where this increase in emissions was originating from. To do this, we used measurements made by the AGAGE and NOAA monitoring networks and a three-dimensional chemical transport model. The model (called MOZART, developed by the National Center for Atmospheric Research), uses wind speeds and other meteorological information that have been calculated using weather forecasting models, to simulate how pollutants are transported around the world. By testing how this model responds to changes in emissions from different regions, we can use the measurements to find out where SF6 originated from.
There were two major findings from our work. Firstly, we find that it is very likely that all of the recent emissions increase is being driven by an increase in emissions from Asian countries that do not report detailed emissions to the United Nations Framework Convention on Climate Change (UNFCCC), such as China, India and South Korea. Secondly, we find that developed countries that do report emissions to the UNFCCC (e.g. USA, UK, Germany), are likely to be underestimating their emissions.
EDGAR emissions interpolated to 5×5 degrees and scaled in each hemisphere using AGAGE measurements between 1970 – 2008 can be found here in NetCDF format.
Regionally optimized EDGAR emissions at 1.8×1.8 degrees for 2004-2005 and 2006-2008 can be found here in NetCDF format.
Optimized 3D mole fraction fields at 5×5 degrees, and 28 vertical (sigma) levels are here in NetCDF format (10MB).
Methane is a strong greenhouse gas, and plays an important role in the chemistry of the atmosphere. Global concentrations are currently more than double their pre-industrial values (as shown by ice core data). However, in recent years this dramatic growth has slowed, and was close to zero between 1999 and 2006 (see graph below).
In this paper, published in Geophysical Research Letters, we presented AGAGE and CSIRO data showing renewed global growth of methane concentrations starting in 2007. We speculated that some natural process was most likely responsible for such a rapid change in concentration, since anthropogenic emissions tend to change more slowly (a few percent per year). For example, wetlands, the single largest source of methane, could have increased their emission rates in response to changes in temperature and precipitation (2007 was an extremely warm year over Siberian wetlands). Alternatively, we note that a modest decrease in the concentration of the chemical that destroys methane, the hydroxyl radical (OH), could produce a sudden growth.
There was an additional puzzle to this methane increase, which was that growth occurred across the globe at almost the same rate. Most of the methane sources are in the Northern hemisphere, so we would usually expect to see growth beginning in the North, and then propagating to the South later on. This near-simultaneous rise in concentration in both hemispheres suggested that tropical emissions could have played an important role.
In the two years since the publication of this paper, lots of groups have examined these strange fluctuations in methane levels. In particular, Ed Dlugokencky at NOAA and Philippe Bousquet at LSCE in France have written some very nice papers on the subject (Dlugokencky et al, 2009 in Geophysical Research letters and Bousquet et al, 2010 in Atmospheric Chemistry and Physics Discussions). They find that the most likely explanation for the rise since 2007 has been an increase in emissions from northern wetlands in 2007 and then an increase in tropical wetland emissions in 2007-2008. They find little evidence for a large change in OH concentration or large increases in biomass burning.
In addition to these articles, the paper also caught the attention of some people who drew slightly unusual conclusions from the work. Some thought we had “inadvertently disproved global warming” (“MIT Scientists Baffled by Global Warming Theory, Contradicts Scientific Data”, TG Daily). The article also triggered an interesting discussion on the popular “climate sceptic” website Watts Up With That?. I hope it goes without saying to most readers that the rise in methane concentrations since 2007 does not “disprove global warming”. Whilst the recent fluctuations do seem to be driven by changes in natural emissions, it is worth bearing in mind that man-made emissions account for around 60% of the total emission rate (and hence the more than doubling of concentration since pre-industrial times). The continuing rise in concentration of all greenhouse gases is of a great deal of concern (see the latest Intergovernmental Panel on Climate Change report for a comprehensive review of the latest climate science).
As we become more concerned about rising CO2 levels in the atmosphere, people are beginning to think about ways of monitoring emission rates. In this pilot study, we investigated the potential for monitoring London’s CO2 using mixing ratio measurements in the city centre.
In order to obtain measurements of CO2 that are representative of a wide area, you need to measure at the top of a tower. At the centre of the Imperial College campus, the 80m Queen’s Tower was an excellent location for CO2 monitoring (and, since there isn’t a lift, provided some much-needed exercise for an out-of-shape atmospheric scientist).
We made one year of CO2 measurements during 2007 and 2008, and compared them to observations taken outside of London, made by Rebecca Fisher, Dave Lowry and Euan Nisbet at Royal Holloway University of London.
There were several surprising aspects to this work. We found that, generally speaking, the CO2 levels at 80m in London were not much higher than those outside, and were often significantly lower. This is partly due to the differences in sampling heights. The site outside London samples just above roof level, and is therefore likely to be more strongly influenced by emissions from the local biosphere than the site in the city. This potential influence of natural emissions close to the ‘background’ site makes it difficult to determine London’s CO2 emissions by comparing the two measurements. However, we found that it may be possible to determine emissions during the winter, when natural emissions are very small.
Atmospheric Scientist at the University of Bristol