Tropospheric emissions: Monitoring of pollution (TEMPO)
TEMPO was selected in 2012 by NASA as the first Earth Venture Instrument, for launch between 2018 and 2021. It will measure atmospheric pollution for greater North America from space using ultraviolet and visible spectroscopy. TEMPO observes from Mexico City, Cuba, and the Bahamas to the Canadian oi...
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| Published in: | Journal of quantitative spectroscopy & radiative transfer Vol. 186; pp. 17 - 39 |
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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format: | Journal Article |
| Language: | English |
| Published: |
Goddard Space Flight Center
Elsevier Ltd
01-01-2017
Journal of Quantitative Spectroscopy and Radiative Transfer |
| Subjects: | |
| Online Access: | Get full text |
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| Abstract | TEMPO was selected in 2012 by NASA as the first Earth Venture Instrument, for launch between 2018 and 2021. It will measure atmospheric pollution for greater North America from space using ultraviolet and visible spectroscopy. TEMPO observes from Mexico City, Cuba, and the Bahamas to the Canadian oil sands, and from the Atlantic to the Pacific, hourly and at high spatial resolution (~2.1km N/S×4.4km E/W at 36.5°N, 100°W). TEMPO provides a tropospheric measurement suite that includes the key elements of tropospheric air pollution chemistry, as well as contributing to carbon cycle knowledge. Measurements are made hourly from geostationary (GEO) orbit, to capture the high variability present in the diurnal cycle of emissions and chemistry that are unobservable from current low-Earth orbit (LEO) satellites that measure once per day. The small product spatial footprint resolves pollution sources at sub-urban scale. Together, this temporal and spatial resolution improves emission inventories, monitors population exposure, and enables effective emission-control strategies.
TEMPO takes advantage of a commercial GEO host spacecraft to provide a modest cost mission that measures the spectra required to retrieve ozone (O3), nitrogen dioxide (NO2), sulfur dioxide (SO2), formaldehyde (H2CO), glyoxal (C2H2O2), bromine monoxide (BrO), IO (iodine monoxide), water vapor, aerosols, cloud parameters, ultraviolet radiation, and foliage properties. TEMPO thus measures the major elements, directly or by proxy, in the tropospheric O3 chemistry cycle. Multi-spectral observations provide sensitivity to O3 in the lowermost troposphere, substantially reducing uncertainty in air quality predictions. TEMPO quantifies and tracks the evolution of aerosol loading. It provides these near-real-time air quality products that will be made publicly available. TEMPO will launch at a prime time to be the North American component of the global geostationary constellation of pollution monitoring together with the European Sentinel-4 (S4) and Korean Geostationary Environment Monitoring Spectrometer (GEMS) instruments.
•TEMPO is under development to collect geostationary air quality measurements.•TEMPO will measure every hour during daylight over greater North America.•TEMPO will have the spatial resolution to measure sub-urban variability.•The mission’s primary data products include tropospheric ozone and related species.•TEMPO’s time-resolved observations form a revolutionary data set for air quality. |
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| AbstractList | TEMPO was selected in 2012 by NASA as the first Earth Venture Instrument, for launch between 2018 and 2021. It will measure atmospheric pollution for greater North America from space using ultraviolet and visible spectroscopy. TEMPO observes from Mexico City, Cuba, and the Bahamas to the Canadian oil sands, and from the Atlantic to the Pacific, hourly and at high spatial resolution (~2.1 km N/S×4.4 km E/W at 36.5°N, 100°W). TEMPO provides a tropospheric measurement suite that includes the key elements of tropospheric air pollution chemistry, as well as contributing to carbon cycle knowledge. Measurements are made hourly from geostationary (GEO) orbit, to capture the high variability present in the diurnal cycle of emissions and chemistry that are unobservable from current low-Earth orbit (LEO) satellites that measure once per day. The small product spatial footprint resolves pollution sources at sub-urban scale. Together, this temporal and spatial resolution improves emission inventories, monitors population exposure, and enables effective emission-control strategies.
TEMPO takes advantage of a commercial GEO host spacecraft to provide a modest cost mission that measures the spectra required to retrieve ozone (O
3
), nitrogen dioxide (NO
2
), sulfur dioxide (SO
2
), formaldehyde (H
2
CO), glyoxal (C
2
H
2
O
2
), bromine monoxide (BrO), IO (iodine monoxide),water vapor, aerosols, cloud parameters, ultraviolet radiation, and foliage properties. TEMPO thus measures the major elements, directly or by proxy, in the tropospheric O
3
chemistry cycle. Multi-spectral observations provide sensitivity to O
3
in the lowermost troposphere, substantially reducing uncertainty in air quality predictions. TEMPO quantifies and tracks the evolution of aerosol loading. It provides these near-real-time air quality products that will be made publicly available. TEMPO will launch at a prime time to be the North American component of the global geostationary constellation of pollution monitoring together with the European Sentinel-4 (S4) and Korean Geostationary Environment Monitoring Spectrometer (GEMS) instruments. TEMPO was selected in 2012 by NASA as the first Earth Venture Instrument, for launch between 2018 and 2021. It will measure atmospheric pollution for greater North America from space using ultraviolet and visible spectroscopy. TEMPO observes from Mexico City, Cuba, and the Bahamas to the Canadian oil sands, and from the Atlantic to the Pacific, hourly and at high spatial resolution (~2.1 km N/S×4.4 km E/W at 36.5°N, 100°W). TEMPO provides a tropospheric measurement suite that includes the key elements of tropospheric air pollution chemistry, as well as contributing to carbon cycle knowledge. Measurements are made hourly from geostationary (GEO) orbit, to capture the high variability present in the diurnal cycle of emissions and chemistry that are unobservable from current low-Earth orbit (LEO) satellites that measure once per day. The small product spatial footprint resolves pollution sources at sub-urban scale. Together, this temporal and spatial resolution improves emission inventories, monitors population exposure, and enables effective emission-control strategies. TEMPO takes advantage of a commercial GEO host spacecraft to provide a modest cost mission that measures the spectra required to retrieve ozone (O ), nitrogen dioxide (NO ), sulfur dioxide (SO ), formaldehyde (H CO), glyoxal (C H O ), bromine monoxide (BrO), IO (iodine monoxide),water vapor, aerosols, cloud parameters, ultraviolet radiation, and foliage properties. TEMPO thus measures the major elements, directly or by proxy, in the tropospheric O chemistry cycle. Multi-spectral observations provide sensitivity to O in the lowermost troposphere, substantially reducing uncertainty in air quality predictions. TEMPO quantifies and tracks the evolution of aerosol loading. It provides these near-real-time air quality products that will be made publicly available. TEMPO will launch at a prime time to be the North American component of the global geostationary constellation of pollution monitoring together with the European Sentinel-4 (S4) and Korean Geostationary Environment Monitoring Spectrometer (GEMS) instruments. TEMPO was selected in 2012 by NASA as the first Earth Venture Instrument, for launch between 2018 and 2021. It will measure atmospheric pollution for greater North America from space using ultraviolet and visible spectroscopy. TEMPO observes from Mexico City, Cuba, and the Bahamas to the Canadian oil sands, and from the Atlantic to the Pacific, hourly and at high spatial resolution (~2.1km N/S×4.4km E/W at 36.5°N, 100°W). TEMPO provides a tropospheric measurement suite that includes the key elements of tropospheric air pollution chemistry, as well as contributing to carbon cycle knowledge. Measurements are made hourly from geostationary (GEO) orbit, to capture the high variability present in the diurnal cycle of emissions and chemistry that are unobservable from current low-Earth orbit (LEO) satellites that measure once per day. The small product spatial footprint resolves pollution sources at sub-urban scale. Together, this temporal and spatial resolution improves emission inventories, monitors population exposure, and enables effective emission-control strategies. TEMPO takes advantage of a commercial GEO host spacecraft to provide a modest cost mission that measures the spectra required to retrieve ozone (O3), nitrogen dioxide (NO2), sulfur dioxide (SO2), formaldehyde (H2CO), glyoxal (C2H2O2), bromine monoxide (BrO), IO (iodine monoxide), water vapor, aerosols, cloud parameters, ultraviolet radiation, and foliage properties. TEMPO thus measures the major elements, directly or by proxy, in the tropospheric O3 chemistry cycle. Multi-spectral observations provide sensitivity to O3 in the lowermost troposphere, substantially reducing uncertainty in air quality predictions. TEMPO quantifies and tracks the evolution of aerosol loading. It provides these near-real-time air quality products that will be made publicly available. TEMPO will launch at a prime time to be the North American component of the global geostationary constellation of pollution monitoring together with the European Sentinel-4 (S4) and Korean Geostationary Environment Monitoring Spectrometer (GEMS) instruments. •TEMPO is under development to collect geostationary air quality measurements.•TEMPO will measure every hour during daylight over greater North America.•TEMPO will have the spatial resolution to measure sub-urban variability.•The mission’s primary data products include tropospheric ozone and related species.•TEMPO’s time-resolved observations form a revolutionary data set for air quality. TEMPO (Tropospheric Emissions: Monitoring of Pollution) was selected in 2012 by NASA as the first Earth Venture Instrument, for launch between 2018 and 2021. It will measure atmospheric pollution for greater North America from space using ultraviolet and visible spectroscopy. TEMPO observes from Mexico City, Cuba, and the Bahamas to the Canadian oil sands, and from the Atlantic to the Pacific, hourly and at high spatial resolution (approximately 2.1 kilometers N/S by 4.4 kilometers E/W at 36.5 degrees N, 100 degrees W). TEMPO provides a tropospheric measurement suite that includes the key elements of tropospheric air pollution chemistry, as well as contributing to carbon cycle knowledge. Measurements are made hourly from geostationary (GEO) orbit, to capture the high variability present in the diurnal cycle of emissions and chemistry that are unobservable from current low-Earth orbit (LEO) satellites that measure once per day. The small product spatial footprint resolves pollution sources at sub-urban scale. Together, this temporal and spatial resolution improves emission inventories, monitors population exposure, and enables effective emission-control strategies. TEMPO takes advantage of a commercial GEO host spacecraft to provide a modest cost mission that measures the spectra required to retrieve ozone (O3), nitrogen dioxide (NO2), sulfur dioxide (SO2), formaldehyde (H2CO), glyoxal (C2H2O2), bromine monoxide (BrO), IO (iodine monoxide),water vapor, aerosols, cloud parameters, ultraviolet radiation, and foliage properties. TEMPO thus measures the major elements, directly or by proxy, in the tropospheric O3 chemistry cycle. Multi-spectral observations provide sensitivity to O3 in the lowermost troposphere, substantially reducing uncertainty in air quality predictions. TEMPO quantifies and tracks the evolution of aerosol loading. It provides these near-real-time air quality products that will be made publicly available. TEMPO will launch at a prime time to be the North American component of the global geostationary constellation of pollution monitoring together with the European Sentinel-4 (S4) and Korean Geostationary Environment Monitoring Spectrometer (GEMS) instruments. |
| Audience | PUBLIC |
| Author | Chan Miller, C. Neil, D.O. Arola, A. Al-Saadi, J.A. Spurr, R.J.D. Veihelmann, B. Wang, J. Lindfors, A. Pierce, R.B. Grutter, M. Janz, S.J. Szykman, J.J. Martin, R.V. Pennington, W.F. McLinden, C. Hilton, B.B. Andraschko, M.R. Jacob, D.J. Davis, J.E. González Abad, G. Lamsal, L. Pippin, M.R. Kerridge, B.J. Suleiman, R.M. Zoogman, P. Houck, J. Palmer, P.I. Dussault, M.E. Nicks, D.K. Newchurch, M.J. Krotkov, N.A. Liu, X. Wang, H. Natraj, V. Li, C. Chance, K. Carr, J.L. Ghulam, A. Saiz-Lopez, A. Baker, B.D. Cohen, R.C. Torres, O. Fishman, J. Joiner, J. Veefkind, J.P. Flittner, D.E. Kim, J. Canova, B.P. O׳Sullivan, E.J. McElroy, C.T. Herman, J.R. Nowlan, C.R. Edwards, D.P. |
| AuthorAffiliation | a Harvard-Smithsonian Center for Astrophysics q Dalhousie University n Rutherford Appleton Laboratory d University of Alabama at Huntsville v National Oceanic and Atmospheric Administration w Instituto de Química Física Rocasolano, CSIC, Spain o Yonsei University u University of Edinburgh bb University of Nebraska h Harvard University y Environmental Protection Agency b NASA Langley Research Center t NASA Jet Propulsion Laboratory g Finnish Meteorological Institute x RT Solutions, Inc f NASA Goddard Space Flight Center m University of Maryland, Baltimore County z Koninklijk Nederlands Meteorologisch Instituut aa European Space Agency j National Center for Atmospheric Research k Saint Louis University c Ball Aerospace & Technologies Corp i University of California at Berkeley s Environment and Climate Change Canada e Carr Astronautics p GESTAR, University Space Research Association l Universidad Nacional Autónoma de México r York University, Canada |
| AuthorAffiliation_xml | – name: m University of Maryland, Baltimore County – name: u University of Edinburgh – name: bb University of Nebraska – name: i University of California at Berkeley – name: k Saint Louis University – name: g Finnish Meteorological Institute – name: o Yonsei University – name: d University of Alabama at Huntsville – name: l Universidad Nacional Autónoma de México – name: s Environment and Climate Change Canada – name: c Ball Aerospace & Technologies Corp – name: e Carr Astronautics – name: z Koninklijk Nederlands Meteorologisch Instituut – name: h Harvard University – name: f NASA Goddard Space Flight Center – name: aa European Space Agency – name: y Environmental Protection Agency – name: j National Center for Atmospheric Research – name: q Dalhousie University – name: a Harvard-Smithsonian Center for Astrophysics – name: w Instituto de Química Física Rocasolano, CSIC, Spain – name: p GESTAR, University Space Research Association – name: b NASA Langley Research Center – name: x RT Solutions, Inc – name: n Rutherford Appleton Laboratory – name: r York University, Canada – name: v National Oceanic and Atmospheric Administration – name: t NASA Jet Propulsion Laboratory |
| Author_xml | – sequence: 1 givenname: P. surname: Zoogman fullname: Zoogman, P. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 2 givenname: X. surname: Liu fullname: Liu, X. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 3 givenname: R.M. surname: Suleiman fullname: Suleiman, R.M. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 4 givenname: W.F. surname: Pennington fullname: Pennington, W.F. organization: NASA Langley Research Center, USA – sequence: 5 givenname: D.E. surname: Flittner fullname: Flittner, D.E. organization: NASA Langley Research Center, USA – sequence: 6 givenname: J.A. surname: Al-Saadi fullname: Al-Saadi, J.A. organization: NASA Langley Research Center, USA – sequence: 7 givenname: B.B. surname: Hilton fullname: Hilton, B.B. organization: NASA Langley Research Center, USA – sequence: 8 givenname: D.K. surname: Nicks fullname: Nicks, D.K. organization: Ball Aerospace & Technologies Corp, USA – sequence: 9 givenname: M.J. surname: Newchurch fullname: Newchurch, M.J. organization: University of Alabama at Huntsville, USA – sequence: 10 givenname: J.L. surname: Carr fullname: Carr, J.L. organization: Carr Astronautics, USA – sequence: 11 givenname: S.J. surname: Janz fullname: Janz, S.J. organization: NASA Goddard Space Flight Center, USA – sequence: 12 givenname: M.R. surname: Andraschko fullname: Andraschko, M.R. organization: NASA Langley Research Center, USA – sequence: 13 givenname: A. surname: Arola fullname: Arola, A. organization: Finnish Meteorological Institute, Finland – sequence: 14 givenname: B.D. surname: Baker fullname: Baker, B.D. organization: Ball Aerospace & Technologies Corp, USA – sequence: 15 givenname: B.P. surname: Canova fullname: Canova, B.P. organization: Ball Aerospace & Technologies Corp, USA – sequence: 16 givenname: C. surname: Chan Miller fullname: Chan Miller, C. organization: Harvard University, USA – sequence: 17 givenname: R.C. surname: Cohen fullname: Cohen, R.C. organization: University of California at Berkeley, USA – sequence: 18 givenname: J.E. surname: Davis fullname: Davis, J.E. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 19 givenname: M.E. surname: Dussault fullname: Dussault, M.E. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 20 givenname: D.P. surname: Edwards fullname: Edwards, D.P. organization: National Center for Atmospheric Research, USA – sequence: 21 givenname: J. surname: Fishman fullname: Fishman, J. organization: Saint Louis University, USA – sequence: 22 givenname: A. surname: Ghulam fullname: Ghulam, A. organization: Saint Louis University, USA – sequence: 23 givenname: G. surname: González Abad fullname: González Abad, G. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 24 givenname: M. surname: Grutter fullname: Grutter, M. organization: Universidad Nacional Autónoma de México, Mexico – sequence: 25 givenname: J.R. surname: Herman fullname: Herman, J.R. organization: University of Maryland, Baltimore County, USA – sequence: 26 givenname: J. surname: Houck fullname: Houck, J. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 27 givenname: D.J. surname: Jacob fullname: Jacob, D.J. organization: Harvard University, USA – sequence: 28 givenname: J. surname: Joiner fullname: Joiner, J. organization: NASA Goddard Space Flight Center, USA – sequence: 29 givenname: B.J. surname: Kerridge fullname: Kerridge, B.J. organization: Rutherford Appleton Laboratory, UK – sequence: 30 givenname: J. surname: Kim fullname: Kim, J. organization: Yonsei University, South Korea – sequence: 31 givenname: N.A. surname: Krotkov fullname: Krotkov, N.A. organization: NASA Goddard Space Flight Center, USA – sequence: 32 givenname: L. surname: Lamsal fullname: Lamsal, L. organization: NASA Goddard Space Flight Center, USA – sequence: 33 givenname: C. surname: Li fullname: Li, C. organization: NASA Goddard Space Flight Center, USA – sequence: 34 givenname: A. surname: Lindfors fullname: Lindfors, A. organization: Finnish Meteorological Institute, Finland – sequence: 35 givenname: R.V. surname: Martin fullname: Martin, R.V. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 36 givenname: C.T. surname: McElroy fullname: McElroy, C.T. organization: York University, Canada – sequence: 37 givenname: C. surname: McLinden fullname: McLinden, C. organization: Environment and Climate Change Canada – sequence: 38 givenname: V. surname: Natraj fullname: Natraj, V. organization: NASA Jet Propulsion Laboratory, USA – sequence: 39 givenname: D.O. surname: Neil fullname: Neil, D.O. organization: NASA Langley Research Center, USA – sequence: 40 givenname: C.R. surname: Nowlan fullname: Nowlan, C.R. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 41 givenname: E.J. surname: O׳Sullivan fullname: O׳Sullivan, E.J. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 42 givenname: P.I. surname: Palmer fullname: Palmer, P.I. organization: University of Edinburgh, UK – sequence: 43 givenname: R.B. surname: Pierce fullname: Pierce, R.B. organization: National Oceanic and Atmospheric Administration, USA – sequence: 44 givenname: M.R. surname: Pippin fullname: Pippin, M.R. organization: NASA Langley Research Center, USA – sequence: 45 givenname: A. surname: Saiz-Lopez fullname: Saiz-Lopez, A. organization: Instituto de Química Física Rocasolano, CSIC, Spain – sequence: 46 givenname: R.J.D. surname: Spurr fullname: Spurr, R.J.D. organization: RT Solutions, Inc., USA – sequence: 47 givenname: J.J. surname: Szykman fullname: Szykman, J.J. organization: Environmental Protection Agency, USA – sequence: 48 givenname: O. surname: Torres fullname: Torres, O. organization: NASA Goddard Space Flight Center, USA – sequence: 49 givenname: J.P. surname: Veefkind fullname: Veefkind, J.P. organization: Koninklijk Nederlands Meteorologisch Instituut, Netherlands – sequence: 50 givenname: B. surname: Veihelmann fullname: Veihelmann, B. organization: European Space Agency, France – sequence: 51 givenname: H. surname: Wang fullname: Wang, H. organization: Harvard-Smithsonian Center for Astrophysics, USA – sequence: 52 givenname: J. surname: Wang fullname: Wang, J. organization: University of Nebraska, USA – sequence: 53 givenname: K. surname: Chance fullname: Chance, K. organization: Harvard-Smithsonian Center for Astrophysics, USA |
| BackLink | https://www.ncbi.nlm.nih.gov/pubmed/32817995$$D View this record in MEDLINE/PubMed |
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| Snippet | TEMPO was selected in 2012 by NASA as the first Earth Venture Instrument, for launch between 2018 and 2021. It will measure atmospheric pollution for greater... TEMPO (Tropospheric Emissions: Monitoring of Pollution) was selected in 2012 by NASA as the first Earth Venture Instrument, for launch between 2018 and 2021.... |
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| SubjectTerms | Environment Pollution |
| Title | Tropospheric emissions: Monitoring of pollution (TEMPO) |
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