ozone monitoring mission

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Professor Pieternel Levelt works on the satellite-mounted Ozone Monitoring Instrument and the Dutch- European Space Agency Tropospheric Monitoring Instrument. Here, she explains their importance in monitoring emissions for air quality and climate, and discusses her hopes for miniaturised satellite instrumentation Could you provide an outline of your objectives for the Ozone Monitoring Instrument (OMI) project? In 1998, NASA asked The Netherlands to deliver OMI for the Low Earth Orbit (LEO) EOS-Aura satellite. The instrument was developed for measurements of the ozone layer, air quality and climate change. The scientific objectives of OMI are to answer four questions: • Is the ozone layer recovering as expected? • What are the sources of aerosols and trace gases that affect global air quality and how are they transported? • What are the roles of tropospheric ozone and aerosols in climate change? • What are the causes of surface UV-B change? The Royal Netherlands Meteorological Institute (KNMI) is Principal Investigator of OMI, and the Finnish Meteorological Institute (FMI) is the co- Principal Investigator. From what context did the investigation emerge and to what extent is your approach different from prior studies? The GOME and SCIAMACHY instruments were previously developed to fly on European Space Agency satellites ERS-2 and ENVISAT. From this, KNMI, in cooperation with industry and the Dutch Space Agency NSO, began to think about a new instrument that could measure several trace gases at the same time, like GOME and SCIAMACHY, and also measure the atmosphere with daily global coverage and high spatial resolution like the Total Ozone Mapping Spectrometer (TOMS). This led to the design of OMI, in which, for the first time for ultraviolet–visible (UVVIS) satellite instruments, a two-dimensional detector is used. Due to its high spatial resolution, OMI is able to look ‘in between’ the clouds (that hamper our view of the troposphere), making the instrument suitable for measuring tropospheric trace gas columns for air quality. In what ways does the Dutch-European Space Agency Tropospheric Monitoring Instrument (TROPOMI), planned for launch in 2015, differ from the OMI launched in 2004? For TROPOMI, we decided to develop even higher spatial resolution (7 x 7 km 2 ) and a higher sensitivity for low concentrations. We will also measure additional information on clouds and new trace gases (CO and CH 4 ), which are important for air quality and climate change. Why does the University of Technology, Delft, together with KNMI, want to develop smaller satellite instrumentation? Smaller satellite instrumentation would minimise cost which is an important consideration in these time frames. Smaller instrumentation is also significant for operational monitoring in order to reduce cost and increase launching possibilities. This is of importance for the continuation of the Copernicus programme, and for the monitoring capabilities of countries themselves. Furthermore, for large science missions, smaller instrumentation can increase the number of trace gases and parameters measured by the same platform. This creates the opportunity to add more channels and more instruments with different capabilities. Smaller instrumentation would therefore help us answer complex science questions and improve our understanding of atmospheric chemistry. What role can the satellite measurements of pollutants play in emission monitoring for air quality and climate? Measurements of the troposphere have only been made in the last two decades, during which period they have vastly improved. We are now able to calculate emissions from satellite- based concentration maps and can quantify the emission source size and its change. For example, we can measure the change in emission sources over Europe, the US and China. There is often no other means to obtain this information over areas like China and Africa due to lack of ground- based measurements. KNMI was able to develop an inverse method that is extremely fast and able to detect new emission sources. The current practice of obtaining the information to build these emission maps is based on evidence gathered by the government from industry and agriculture etc., and/or using ground-based measurements (the bottom-up method). Updates to these maps often take at least a year. With our new satellite based (top-down) method, this can be achieved in a few weeks. We are currently working on miniaturised satellite instrumentation that will reveal pixel sizes of 2 x 2 km 2 (TROPOLITE). This will greatly enhance our capability to measure individual emission sources. As we obtain longer data records, I expect that satellite data will become an important source of information to check the effectiveness of emission regulation measures. Because it is possible to measure the whole atmosphere with only one instrument, there are no issues with biases in emission maps between countries. Moreover, the satellite data is not only capable of measuring over land, but also over oceans where ground-based measurements are lacking, and can therefore also provide quantified information of ship emissions. Ozone monitoring mission ARNOT POWER STATION, SOUTH AFRICA © GERHARD ROUX WWW.RESEARCHMEDIA.EU 39 PROFESSOR PIETERNEL LEVELT

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Professor Pieternel Levelt works on the satellite-mounted Ozone Monitoring Instrument and the Dutch-European Space Agency Tropospheric Monitoring Instrument. Here, she explains their importance in monitoring emissions for air quality and climate, and discusses her hopes for miniaturised satellite instrumentation

Could you provide an outline of your objectives for the Ozone Monitoring Instrument (OMI) project?

In 1998, NASA asked The Netherlands to deliver OMI for the

Low Earth Orbit (LEO) EOS-Aura satellite. The instrument was developed for measurements of the ozone layer, air quality and climate change. The scientific objectives of OMI are to answer four questions:

• Is the ozone layer recovering as expected?

• What are the sources of aerosols and trace gases that affect global air quality and how are they transported?

• What are the roles of tropospheric ozone and aerosols in climate change?

• What are the causes of surface UV-B change?

The Royal Netherlands Meteorological Institute (KNMI) is Principal Investigator of OMI, and the Finnish Meteorological Institute (FMI) is the co-Principal Investigator.

From what context did the investigation emerge and to what extent is your approach different from prior studies?

The GOME and SCIAMACHY instruments were previously developed to fly on European Space Agency satellites ERS-2 and ENVISAT. From this, KNMI, in cooperation with industry and the Dutch Space Agency NSO, began to think about a new instrument that could measure several trace gases at the same time, like GOME and SCIAMACHY, and also measure the atmosphere with daily

global coverage and high spatial resolution like the Total Ozone Mapping Spectrometer (TOMS). This led to the design of OMI, in which, for the first time for ultraviolet–visible (UVVIS) satellite instruments, a two-dimensional detector is used. Due to its high spatial resolution, OMI is able to look ‘in between’ the clouds (that hamper our view of the troposphere), making the instrument suitable for measuring tropospheric trace gas columns for air quality.

In what ways does the Dutch-European Space Agency Tropospheric Monitoring Instrument (TROPOMI), planned for launch in 2015, differ from the OMI launched in 2004?

For TROPOMI, we decided to develop even higher spatial resolution (7 x 7 km2) and a higher sensitivity for low concentrations. We will also measure additional information on clouds and new trace gases (CO and CH4), which are important for air quality and climate change.

Why does the University of Technology, Delft, together with KNMI, want to develop smaller satellite instrumentation?

Smaller satellite instrumentation would minimise cost which is an important consideration in these time frames. Smaller instrumentation is also significant for operational monitoring in order to reduce cost and increase launching possibilities. This is of importance for the continuation of the Copernicus programme, and for the monitoring capabilities of countries themselves. Furthermore, for large science missions, smaller instrumentation can increase the number of trace gases and parameters measured by the same platform. This creates the opportunity to add more channels and more instruments with different capabilities. Smaller instrumentation would therefore help us answer complex science questions and improve our understanding of atmospheric chemistry.

What role can the satellite measurements of pollutants play in emission monitoring for air quality and climate?

Measurements of the troposphere have only been made in the last two decades, during which period they have vastly improved. We are now able to calculate emissions from satellite-based concentration maps and can quantify the emission source size and its change. For example, we can measure the change in emission sources over Europe, the US and China. There is often no other means to obtain this information over areas like China and Africa due to lack of ground-based measurements.

KNMI was able to develop an inverse method that is extremely fast and able to detect new emission sources. The current practice of obtaining the information to build these emission maps is based on evidence gathered by the government from industry and agriculture etc., and/or using ground-based measurements (the bottom-up method). Updates to these maps often take at least a year. With our new satellite based (top-down) method, this can be achieved in a few weeks. We are currently working on miniaturised satellite instrumentation that will reveal pixel sizes of 2 x 2 km2 (TROPOLITE). This will greatly enhance our capability to measure individual emission sources.

As we obtain longer data records, I expect that satellite data will become an important source of information to check the effectiveness of emission regulation measures. Because it is possible to measure the whole atmosphere with only one instrument, there are no issues with biases in emission maps between countries. Moreover, the satellite data is not only capable of measuring over land, but also over oceans where ground-based measurements are lacking, and can therefore also provide quantified information of ship emissions.

Ozone monitoring mission

ARNOT POWER STATION, SOUTH AFRICA © GERHARD ROUX

WWW.RESEARCHMEDIA.EU 39

PROFESSO

R PIETERNEL LEV

ELT

Monitoring the atmosphereHumankind is under great pressure to better understand and predict global atmospheric changes. The Royal Netherlands Meteorological Institute is coordinating two satellite instruments that will help to face this challenge

Global distribution of tropospheric NO2 as observed from 2005 to 2008 by the Ozone Monitoring Instrument (OMI). Various sources of air pollution can clearly be distin-guished: traffic, heavy industry, fossil fuel power plants, biomass burning, oil refineries and shipping routes. OMI was built by The Netherlands and is on board NASA’s Aura satellite. More data and information can be found at www.temis.nl.

PROFESSOR PIETERNEL LEVELT

40 INTERNATIONAL INNOVATION

EARTH’S ATMOSPHERE HAS changed dramatically since the Industrial Revolution. Human activities have greatly increased emissions and the resultant changes to the composition of the atmosphere are manifest as climate change, air pollution and ozone depletion. There have been several international agreements in response to these changes, including the Montreal Protocol, a treaty designed to protect the ozone layer.

Many components of the atmosphere need to be monitored for protection of the environment, first of which is the ozone layer. This layer of the atmosphere limits the amount of harmful UV radiation that reaches the surface of the Earth, and its breakdown has been primarily attributed to chlorofluorocarbons (CFCs).

Beyond ozone destruction, atmospheric gases, including CO2, CH4 and O3, heat the atmosphere and the Earth’s surface by trapping infrared radiation. Alongside this, NO2 and SO2 result in acid rain and photochemical smog. The Environmental Protection Agency (EPA) has designated certain pollutants, including tropospheric ozone, NO2 and aerosols, as serious threats to agricultural productivity and human health. The recent Intergovernmental Panel on Climate Change Fifth Assessment Report (AR5) has also focused attention on short-lived climate pollutants (SLCPs) like black carbon, tropospheric ozone and CH4. The Climate and Clean Air Coalition (CCAC), initiated by Hillary Clinton in 2012, is meant to take win-win measures for air quality and climate change via these short-lived climate pollutants.

It is important to monitor the concentrations of atmospheric trace gases to understand Earth system processes, to appreciate just how the environment is being affected by global warming, and predict what may happen in the future. Earth observation satellites are a

major source of information to enable this. The NASA Total Ozone Mapping Spectrometer (TOMS) instrument provided a unique insight into the evolution of the ozone layer, but did not measure the troposphere. The GOME and SCIAMACHY instruments on European Space Agency (ESA) satellites introduced the concept of measuring the complete spectrum in the UV/visible (Vis) wavelength range with a high spectral resolution enabling the measurement of trace gases in the troposphere.

A team at the Royal Netherlands Meteorological Institute (KNMI) is currently leading two satellite instruments: the Ozone Monitoring Instrument (OMI) and the Tropospheric Monitoring Instrument (TROPOMI). The satellites will allow research on climate change, but because the data collected by the two instruments are available in near real-time, they can be also be used for UV and air quality forecasts, as well as aviation rerouting in case of volcanic eruptions. OMI was launched on the NASA EOS-Aura satellite in 2004 and remains in operation; TROPOMI will be launched on the ESA Sentinel-5 Precursor satellite in 2015. The instrument will be followed by ESA’s Sentinel-4 and -5 missions. These three sentinel missions form the EU Copernicus Programme for operational monitoring of the atmospheric composition. Professor Pieternel Levelt leads the climate observations department at KNMI, is Principal Investigator of the OMI instrument and scientific initiator of TROPOMI: “In order to make the next step in understanding the complex relationship between air quality and climate, we need accurate measurements from space,” she explains.

OMI

OMI represents a major contribution to our understanding of stratospheric and tropospheric chemistry and is a nadir-viewing imaging

spectrometer that gives daily global coverage. It uses a wide-field telescope feeding two image-grating spectrometers to observe Earth’s backscattered radiation. The light entering the telescope is depolarised using a scrambler and split into two channels: UV and Vis.

OMI measures key air quality components such as NO2 and SO2. Able to differentiate between aerosol types and measures cloud pressure and coverage, it can provide the necessary data to derive information on tropospheric ozone. The instrument maps pollution products from an urban to super-regional scale and provides measurements which are highly synergistic with the other instruments on the Aura platform. It also extends the 30 year total ozone record measured by the TOMS instruments.

One axis of the detector is used for the spectral information, and the other for spatial information, enabling daily global coverage with high unprecedented spatial resolution. While OMI is based on TOMS and GOME, it is able to measure many more atmospheric constituents than the former and provides much greater resolution than the latter. It can detect volcanic ash and SO2 produced by volcanic eruptions with sensitivity at least 100 times greater than TOMS, which is hugely important for aircraft safety. The spatial resolution of OMI is 13 km x 24 km2 in nadir. Such small pixel size enables OMI to measure ‘in between the clouds’, vastly improving its capacity to sense the troposphere.

TROPOMI

TROPOMI is also a space-borne nadir-viewing spectrometer, with bands in the UV, Vis, near infrared and shortwave infrared. Its data products will be developed to include state-of-the-art methods that will utilise the new instrument

Nitrogen oxide emissions for the South African Highveld region. The grey outline indicates the densely populated Gauteng province, containing the cities of Johannesburg and Pretoria. Blue circles indicate the location of coal-fired power stations, important hot spots of nitrogen oxide emissions. The left panel shows the emission strength of the model-based emission inventory, based on 2008 inventory data. The right panel shows the emission estimates from the spaceborne OMI instrument for 2009–10. The use of satellite data improves the identification of the emission hot spots ©Van der A and Mijling, KNMI, 2013.

capabilities, at the same time as extending current data records from OMI and SCIAMACHY.

The instrument’s scientific objectives expand on those of OMI and include better estimation of long-term trends in the troposphere related to air quality and climate, and developing and improving air quality forecast models and emission estimates.

TROPOMI will make daily global observations of O3, NO2, SO2, CO and CH4 (the second most important anthropogenic greenhouse gas) as well as aerosol properties. It uses a two-dimensional detector, as introduced by OMI, enabling retrieval of an unprecedented small pixel size of 7 x 7 km2 maintaining daily global coverage and, while it builds on the solid foundation of its heritage instruments, it also represents a pioneering advance. The combination of a high spatial resolution, high signal-to-noise ratio and improved cloud detection will provide stimulating new high accuracy information on the composition of the troposphere.

EMISSION CALCULATIONS AND TREND MONITORING

In addition to generating satellite data, KNMI constructs long-term trends in emissions, based upon the data of several successive instruments. A study based on data from OMI provided, for the first time, a space-based NOx emission inventory for shipping, offering a framework for future studies to constrain ship emissions using satellite NO2 emissions. During 2011, in research published in Nature, OMI measured exceptionally low ozone on the North Pole and it was found, using additional satellite instrumentation on the same Aura satellite (MLS), that chemical ozone destruction over the Arctic in early 2011 was comparable to the Antarctic ozone hole. The finding was surprising, because temperatures are much milder in the Arctic and ozone loss in the region had previously had been far more limited than in the Antarctic.

Inventories of air pollutants provide crucial information for policy makers and are important for air quality models. Using satellite observations for emission estimates has many advantages over bottom-up inventories: they have global coverage

and allow updates soon after the satellite data becomes available, whereas bottom-up inventories are infrequently updated and dependent on local information of differing quality, limiting their value. The satellite data ultimately serve as an independent tool for validating and updating bottom-up emission maps.

LOOKING TO THE FUTURE

The data provided by OMI and TROPOMI are invaluable. These satellite instruments enable monitoring and prediction of atmospheric changes, both globally and regionally. This will lead to an ability to anticipate and manage environmental change, which is strongly needed in this time of radical transformation.

KNMI is also in the process of developing a device to test NO2 concentration – known as a sonde – for satellite validation. In satellite retrievals, some assumptions must be made, one of which is the profile of the trace gas under study. If the assumption is incorrect, it will affect the quality of the retrieval. The cheap and easy-to-use NO2 sonde will solve many of these problems, as Levelt elaborates: “It will improve our assumptions of NO2, by validating our models and/or by generating an NO2 climatology profile”. The sonde can measure very low concentrations of NO2, be used under several weather conditions and has garnered a lot of interest from the scientific community. Moreover, Levelt is working on miniaturised satellite instrumentation, together with industry, to further advance understanding of atmospheric chemistry. Overall, her efforts, and those of her colleagues, are providing a significant step forward in atmospheric observations.

OZONE MONITORING INSTRUMENT

© DUTCH SPACE/KNMI/TNO

INTELLIGENCE

WWW.RESEARCHMEDIA.EU 41

OZONE MONITORING INSTRUMENT (OMI) AND TROPOSPHERIC MONITORING INSTRUMENT (TROPOMI)

OBJECTIVES

OMI and TROPOMI main objectives:

• Daily global air quality and climate-related measurements with unprecedented spatial resolution from space

• Measurements of the ozone layer for the Montreal Protocol

PARTNERS

OMI: Dutch-Finnish instrument • KNMI (Principal Investigator – PI) • FMI (co-PI) • Industry main partners: Dutch Space and TNO • Agencies: Netherlands Space Agency (NSO) and NASA

TROPOMI: Dutch-ESA instrument • KNMI (PI) • SRON (co-PI) • Industry main partners: Dutch Space and TNO • Agencies: Netherlands Space Office (NSO) and ESA

FUNDING

OMI: The Netherlands: ministries for Infrastructure and Environment, Education, Culture and Science and Economical Affairs • Finland: TEKES • USA: NASA

TROPOMI: The Netherlands: ministries for Infrastructure and Environment, Education, Culture and Science and Economical Affairs • ESA • EU Copernicus Program

CONTACT

Professor Pieternel Levelt Principal Investigator, OMI Scientific Initiator, TROPOMI Head Climate Observation Department, KNMI Professor at the University of Technology, Delft

Royal Netherlands Meteorological Institute Wilhelminalaan 10 3732 GK De Bilt The Netherlands

T +31 302 206 667 E [email protected]

PIETERNEL LEVELT obtained her Master’s degree in Chemistry in 1987 and her PhD in Physics in 1992, both at the Free University of Amsterdam. In 1998 she became Principal Investigator of OMI (Launched on NASA’s EOS-Aura satellite in 2004) and she is still managing the international OMI Science Team. She is scientific initiator of the new Dutch/ESA TROPOMI instrument, to be launched on ESA’s Sentinel 5 precursor in 2015. She also chairs ESA’s Mission Advisory Group (MAG) for the sentinel 5 precursor and is member of the sentinel 4 and 5 MAG. She is Head of the Climate Observations Department at KNMI, interim Head of Chemistry and Climate at KNMI, and Professor in Remote Sensing of the Atmospheric Composition at the University of Technology, Delft.