EGU Blogs

Black Carbon

AGU 2013 day 1: Short-lived climate forcers

My first day at AGU 2013 revolved around sessions on short-live climate forcers, which are components in the atmosphere that have short lifetimes (compared to carbon dioxide for example) and generally warm the atmosphere. Reduction of these compounds, such as methane and black carbon, has been mooted as a way to reduce global mean temperatures in coming decades.

This is summarised in the figure below, where the modelled impact of reducing black carbon and methane alongside reductions in carbon dioxide emissions are shown. The majority of the benefit in reducing methane and black carbon is felt by 2040 – if you look at longer time scales, then the effect diminishes relative to carbon dioxide.

image

Modelled impact of various reductions in carbon dioxide, methane and black carbon (BC) on global mean temperature. Figure courtesy of UNEP Integrated Assessment of Black Carbon and Tropospheric Ozone.

The problem with this idea is that there is much uncertainty related to these short-lived components, so it isn’t clear how much global temperatures would respond to a reduction in their atmospheric concentrations. This is represented in the above figure by the vertical bars to the left of the graph – there is much overlap here, which reflects this uncertainty. The health benefits of reducing black carbon in particular are quite clear though. Most of the talks focussed on black carbon and that is what I am also going to focus on below.

Fuzzy metrics

Tami Bond made some excellent and thought-provoking points on how short-lived climate forcers are framed relative to carbon dioxide. The key property for black carbon in the framework of near-term reductions in global temperature is its short lifetime in the atmosphere (days-to-weeks). This means that it is not evenly distributed across the globe, unlike greenhouse gases such as carbon dioxide and methane. This results in its radiative forcing being spatially distinct – the perturbation it has on our planets energy balance occurs close to its source of emission. The impact of such changes is usually felt more at the regional level, rather than the global scale associated with carbon dioxide. Her main point was that this is then an apples-to-oranges comparison, so for example, reducing black carbon emissions in Asia might not have a great impact of global mean surface temperatures but it may well reduce temperatures in the region and slow the effects of carbon dioxide driven warming.

She also reiterated the difficulties associated with the pollutants that are co-emitted with black carbon, which complicate the picture and are one of the major reasons that there is substantial uncertainty surrounding reducing black carbon. In the real world, you can’t really just reduce black carbon – any technological  solution will likely perturb the other pollutants, which tend to cool our climate. Attempts to reduce black carbon might actually result in temperatures rising – I’ve written more on studies that have considered this here.

Other highlights

Yi Deng presented a fascinating study of how aerosol particles can influence the atmosphere far away from their actual location by modelling the impact of biomass burning in Southern Africa on the Asian Summer Monsoon. He showed that the substantial burning that occurs actually strengthens the monsoon by inducing circulation changes up-wind of the Indian sub-continent and south-east Asia. We tend to think of aerosol impacts being confined to their atmospheric location but this illustrated how joined-up our atmosphere is.

One of the issues with black carbon is that some sources have received little attention previously. Ed Fortner from Aerodyne Research Inc. presented measurements of emissions from brick kilns in Mexico, which produce a lot of black carbon. There are around 300,000 kilns worldwide producing 1.5 billion bricks per year! Over half of these are in China (54%), with India (11%), Pakistan (8%) and Mexico (7%)  being the other major kiln hotspots. Characterising the emissions from these and other sources is likely going to be in important for efforts to constrain the impact of black carbon on both our climate and health.

Chris Cappa presented follow-up work to his 2012 paper in Science that investigated how much warming by black carbon is enhanced by other aerosol species that coat it. Black carbon warms the atmosphere by absorbing sunlight and both laboratory and theoretical evidence suggests that this is increased by coatings on the black carbon particles. This coating focusses sunlight onto the black carbon core, like a magnifying glass held to the sun does and this increases the absorption by the black carbon, a phenomenon known as “lensing”. Chris has been busy testing how much enhancement we see in the real world using measurements and typically to enhancement ranges from 10-30%, which is lower than is often suggested by aerosol models. There are significant caveats here as the measurements are challenging and require the aerosols to be “dry” – this is important as water often condenses onto aerosol particles and increases their reflective and lensing ability. This could be a vital ingredient in this process and it is a significant challenge to overcome.

My final highlight was presenting my poster! The AGU poster hall is absolutely massive and must span several football pitches. Despite this, the sessions are hugely rewarding and are a great opportunity to discuss science with a variety of people. The posters are a major part of the AGU fall meeting, which is not always true of other conferences. I’m looking forward to roaming the hall now that my own poster is done.

Me presenting my poster on day 1 of AGU 2013. Image courtesy of Sam Illingworth.

Me presenting my poster on day 1 of AGU 2013. Image courtesy of Sam Illingworth.

Communicating uncertainty

With all this complexity revolving around black carbon and the interest it has received from policy makers, Tami Bond was asked how to communicate this to non-scientists. Her response was:

Keep it simple but don’t ignore physical reality.

That seems like a pretty good mantra to me.

A continent on fire

While preparing my poster for the upcoming AGU Fall Meeting, I downloaded some data on fire activity in South America for background on why we are interested in biomass burning in the region. I wanted to quickly check I had the data in the correct format, so I just plotted the coordinates of the fire counts without an outline of South America.

I was surprised to see that the fire locations for August-October 2012 did a great job of outlining South America on their own!

Fire map.

Map of fire locations during August-October 2012 in South America from MODIS data from the Terra and Aqua satellites provided by NASA’s Earth Observing System Data and Information System (EOSDIS).

The data is from the MODIS instrument on NASA’s Terra and Aqua satellites. The data reports fire locations based on measuring  the emission of infrared radiation by the land surface from space (like the infrared cameras on your favourite police chase tv show).  Any 1km pixel with a fire detected within it is then included in the data – there could be more than one fire within the pixel but the instrument can’t distinguish these. You can find out more information about the technique here.

The widespread nature of the burning across South America is striking. Huge areas of the continent have fires detected within them. This is an annual endeavour with many of the fires started by people for land use change and agriculture. The main “season” runs from August to October, with the peak usually in September. These fires have been occurring for several decades now and they have transformed vast swathes of South America.

The burning produces large amounts of smoke, which can build up and pollute our atmosphere. This has important consequences for regional and global climate, air quality and also ecosystem development. I’m part of a project called SAMBBA, which as well as being a great acronym, is attempting to address some of the aspects of biomass burning that we don’t understand (which is a long list). I’ve written about the project and my part in it here and here previously.

As the map above illustrates, it is quite a big deal in the region. Stay tuned for future updates on the project.

The role of aerosol uncertainty in climate change

For those who follow [pun intended] the world of climate science on Twitter, you’ll very likely have noticed a string of tweets from a meeting at the Royal Society on the “Next steps in climate science“. The programme (PDF here) has included a wide range of topics relating to climate science and has included a number of scientists who heavily contributed to the recent IPCC Working Group One assessment report.

I put together a Storify of the discussion relating to a talk by Dr Oliver Boucher from the Met Office Hadley Centre on the role of aerosols in the session on “How large are uncertainties in forcings and feedbacks and how can they be reduced?” – the discussion can be accessed below or by clicking here.

Image of the global aerosol distribution produced by NASA. The image was produced using high-resolution modelling by William Putman from NASA/Goddard. The colours show the swirls of aerosol particles formed from the numerous sources across the globe. The colours show aerosol particles as dust (gold/brown), sea-spray (blue), biomass burning/wildfires (green) and industrial/urban (white).

Image of the global aerosol distribution produced by NASA. The image was produced using high-resolution modelling by William Putman from NASA/Goddard. The colours show the swirls of aerosol particles formed from the numerous sources across the globe. The colours show aerosol particles as dust (gold/brown), sea-spray (blue), biomass burning/wildfires (green) and industrial/urban (white). Trying to untangle all of this is extremely challenging!

The event itself has been an excellent distraction example of scientists communicating with a wide audience and is yet another example of social media adding something extra to scientific meetings. I wasn’t able to attend but I found the discussions on Twitter interesting, engaging and thought provoking. Many thanks to the speakers, tweeters and the Royal Society.

http://storify.com/willtmorgan/how-large-are-uncertainties-in-forcings-and-feedba?

Biomass burning birthday

Last September I spent a month in Brazil for a research project aiming to study the pollution produced by deforestation fires in the Amazon Basin. The fires are mainly started by people for agricultural needs or land clearing for buildings and infrastructure. These fires produce huge amounts of smoke that blanket vast regions of South America during the “dry” season, which can lead to significant affects on weather, climate and people’s health. The name of the project was SAMBBA (South American Biomass Burning Analysis) and I’ve written a little about it previously here. There are several aspects to the project but my major role was on board the Facility for Airborne Atmospheric Measurement’s BAe-146 research aircraft. I was a mission scientist, which basically means I get to tell the pilots where to fly (subject to standard aircraft operating procedures like avoiding mountains, severe storms and not running out of fuel).

The Amazon usually conjures up images of pristine rainforest and giant meandering rivers but in the quest for air pollution, we were based in Porto Velho, which is the capital of Rondonia – a global poster-child for deforestation. Recently, a project involving Google, the U.S. Geological Survey (USGS), NASA and Time published an extraordinary series of satellite images from the Landsat program showing how the surface of the Earth has changed since the program began in 1984. One of the areas highlighted was Rondonia and the images showed how dramatically the landscape has changed over several decades. While deforestation began there in the 1970’s, the changes detailed in the images from Landsat are clear to see and are shown below. In 1984, the typical ‘fish-bone’ pattern of deforestation is already evident as pathways into the Amazon rainforest are cleared and tributaries of fire branch out from these. By 2012, the deforestation has spread out to envelop large swathes of areas that were previously rainforest.

Comparison of deforestation of part of the Amazon rainforest in Rondonia state, Brazil from 1984 and 2012. The area pictured is to the south and south-east of Ji Parana and covers an area of approximately 60 x 120 miles. Images are from Google. An interactive version where you can expand the view and also visit other areas of the globe is available here, which is worth doing as it gives a feel for the scale over which the deforestation occurs.

This tweet by the EGU twitter account reminded me that it is a whole year since one of our most successful flights of the campaign, which took place in Rondonia. The image below shows the view of the fire we flew through from a satellite, with the smoke plume extending over 80km downwind and also a side-on view of the fire that I took from the aircraft. The fire was to the south-west of Porto Velho in a protected area, where you wouldn’t usually expect to see fires. After travelling to the home of deforestation in Brazil, the largest fire we found was actually a wildfire!

Satellite (top) and side-on view taken from Bae-146 research aircraft (bottom) of a large fire plume that was sampled in Rondonia on 20th September 2012 during SAMBBA. The red line overlayed on the satellite image is 80km long, with the fire plume visible to the left of the line. The satellite image is from NASA’s Terra mission.

The key thing we were trying to investigate during the flight was how the properties of the smoke plume changed as it blew downwind. This is the crucial intermediate step between the actual initial conditions on the ground where the fire starts and the regional build up of smoke haze that affects weather and climate. To do this, we performed a series of flight patterns including:

  1. Flying across the plume at regular intervals along the length of the plume e.g. above the fire, 20km from the fire, 40km from the fire etc.
  2. Flying directly up the length of plume, which is a particular challenge for the pilots as the plume doesn’t generally follow a straight line and you can’t actually see anything.

With these measurements, we can can compare how the properties of the smoke change with distance from the fire. We can combine this information with measurements just a few hundred metres above the fire, as well as flights in older regional pollution to understand the entire life cycle of fires in this region and compare it with other types of fire in various areas of the globe.

We’ve been working hard over the past year analysing the data from this flight and all of the other SAMBBA flights and hopefully there will be much more of the actual science story to tell on this over the next 12 months and more. Stay tuned.