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GCOS Atmospheric Composition ECV*
Precursors supporting the Aerosol and Ozone ECVs

*over land, sea and ice

Introduction: Observations of precursors of ozone and aerosols are studied to improve the ability to detect and attribute changes in ozone and earosol in both the troposphere and the lower stratosphere. Moreover, some precursors are important variables for air quality and this climate-change impacts in their own right.

N20 is a greenhouse gas which mainly originates from agriculture, but is also producted by natural sources, i.e soils and ocean. There sources are diffusive and therefore it is not easy to obtain from inverse modelling. There is also a large variablitity in the stratosphere.

Holcarbons are currently a minor contribution to GHGs but they are potent GHGS and represent a potential long-term threat. Some of them (cholorfluorocarbons (CFCs) and Hydrofluorocarbons (HFCs) are regulated by the Montreal Protocol, since they are also ozone depleting gases, but they might not be phased out before 2040 and may show increasing concentration before 2040. Others do not deplete ozone and are therefore not governed by the Montreal Protocol. Concentrations of some of them are increasing rapidly.
 
N20, CFCs, HCFCs, hydrofluorocarbons (HFCs), SF6 and perfluorocarbons (PFCs), are generally well-mixed in the troposphere, and it is sufficient for monitoring purposes to measure them with a limited number of stations world-wide. Observations of N20 by in situ flask networks are in place. Stratospheric trend monitoring of N20 is done by FTIR measurements. The Microwave Limb Sounder (MLS) performs measurements of N20 in the stratosphere. It is very difficult to measure N20 in the troposphere from satellites. The Advanced Global Atmospheric Gases Experiment (AGAGE) network comprises five stations and collaborating networks contribute with another six stations. This gives global coverage from Spitsbergen in the north to Tasmania in the south. Halocarbons must be monitored closely, albeit from a relatively small number of stations, because once they enter the atmosphere, some of them will remain for hundreds, even thousands of years.  

International Data Centers and Archives for Atmospheric Composition:

  • World Data Centre for Greenhouse Gases (WDCGG)
  • NOAA Earth System Research Laboratory (ESRL)
  • Carbon Dioxide Information Analysis Center (CDIAC)

Coordinating Body: WMO Commission for Atmospheric Science (CAS)

Contributing Networks:

  • WMO GAW observing network for CO (continous and flasks measurements)
    • status: operational; partial network; operation data management
  • WMO GAW network for reactive nitrogen
    • Currently in the stage of establishment, several stations world-wide
  • EMEP (GAW contributing network)
    • operational European network for monitoring of primary pollutants
  • Research programmes using MAXDOAS, SAOZ, FTIR and other techniquest (for NO2)
    • sparse, research-oriented
  • In situ network from environmental agencies
    • operational at national level
  • Aircraft (IAGOS, CO)
    • limited operational aircraft vertical profiling initiated
  • NDACC
    • operational, partial network; operational data management

Contributing Satellite Data:

  • UV/VIS/NIR/SWIR sounders
    • precursors are measured by research satellites and operational satellites in future
  • Nadir IR sounders
    • Information on high spatial and temporal resolution is limited

(Source: WMO/IOC Implementation Plan for the Global Observing System for Climate in Support of the UNFCCC (2010 Update) GCOS-138/GOOS-184/GTOS-76/WMO-TD/No. 1523)

Satellite Observations: Trace gases other than ozone may be divided into three categories: — greenhouse gases affecting climate change; — chemically aggressive gases affecting the environment (including the biosphere); — gases and radicals impacting on the ozone cycle, thereby affecting both climate and environment. The presence of trace gases in the atmosphere can have a significant effect on global change as well as potentially harmful local effects through increased levels of pollution. The chemical composition of the troposphere, in particular, is changing at an unprecedented rate. Meanwhile, the rate at which pollutants from human activities are being emitted into the troposphere is now thought to exceed that from natural sources (such as volcanic eruptions). As explained in Part I of this document, the IPCC noted in 2007 that: — changes in atmospheric concentrations of greenhouse gases and aerosols, land cover and solar radiation alter the energy balance of the climate system; — global greenhouse gas emissions due to human activities have grown since pre-industrial times, with an increase of 70% between 1970 and 2004; — carbon dioxide (CO2) is the most important anthropogenic greenhouse gas. Its annual emissions grew by about 80% between 1970 and 2004. The IPCC concluded that “most of the observed increase in globally averaged temperatures since the mid-20th century is very likely (over 90% probability) due to the observed increase in anthropogenic (man-made) greenhouse gas concentrations”. They consider that reductions in greenhouse gas emissions and the gases that control their concentration would be necessary to stabilise radiative forcing.

Measurements from satellite sensors have already made an important contribution to the recognition that human activities are modifying the chemical composition of both the stratosphere and the troposphere, even in remote regions. A variety of instruments provide measurements on the concentration of trace gases. In general, high spectral resolution is required to detect absorption, emission and scattering from individual species. Some instruments offer measurements of column totals, i.e. integrated column measurements, whilst others provide profiles of gas concentration through the atmosphere (usually limited to the upper troposphere and stratosphere, using limb measurements). To date, the instruments on UARS (operated 1991–2005) have provided the most significant source of data on trace gases and have been vital for studies of stratospheric chlorine chemistry, stratospheric tracer-tracer correlation, tropospheric water vapour, the chemistry of the Arctic lower stratosphere in winter, and tropospheric aircraft exhaust studies The last few years have seen the arrival of new and significant capabilities, with advanced instruments on Terra (MOPITT, providing global measurements of carbon monoxide and methane in the troposphere), and Envisat (GOMOS, MIPAS and SCIAMACHY, providing profiles of trace gases through the stratosphere and troposphere). AIRS (on Aqua) and IASI (on MetOp) also contribute to such information and their sounder products can help quantify atmospheric mixing and help determine sources and sinks. On NASA’s Aura mission, HiRDLS, an infrared limb-scanning radiometer, carries out soundings of the upper troposphere, stratosphere and mesosphere to determine concentrations of trace gases, with horizontal and vertical resolutions superior to those previously obtained. On the same mission, MLS measures concentrations of trace gases for their effects on ozone depletion, TES provides a primary input to a database of 3D distribution on global, regional and local scales of gases important to tropospheric chemistry, and OMI continues the TOMS record for atmospheric parameters related to ozone chemistry and climate. JAXA’s GOSAT mission (from 2008) and NASA’s OCO mission (also from 2008) are expected to make significant contributions to observations of trace gases, particularly carbon dioxide and methane. The IGOS IGACO Theme for observations of atmospheric chemistry has considered all relevant chemical species to interpret properly the observations and intends to monitor the research required to improve understanding of Earth processes so that air quality evolution can be predicted. ESA is considering atmospheric composition missions (such as TRAQ, PREMIER and A-SCOPE) to meet these needs. The CEOS Response to the GCOS IP cautions that demonstrations of potential future operational measurements are neither complemented by plans for operational implementation nor any R&D follow-on. CEOS agencies will participate in planning, by 2011, the current chemistry missions and those planned for the next 5 to 7 years. (Satellite Missions) (Source: CEOS)

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