Tropospheric ozone increases over the southern Africa region: bellwether for rapid growth in Southern Hemisphere pollution?
| dc.contributor.author | Thompson, Anne M. | |
| dc.contributor.author | Balashov, N. V. | |
| dc.contributor.author | Witte, J. C. | |
| dc.contributor.author | Coetzee, J. G. R. | |
| dc.contributor.author | Thouret, V. | |
| dc.contributor.author | Posny, F. | |
| dc.date.accessioned | 2024-06-20T17:31:31Z | |
| dc.date.available | 2024-06-20T17:31:31Z | |
| dc.date.issued | 2014-09-17 | |
| dc.description.abstract | Increases in free-tropospheric (FT) ozone based on ozonesonde records from the early 1990s through 2008 over two subtropical stations, Irene (near Pretoria, South Africa) and Réunion (21° S, 55° E; ~2800 km NE of Irene in the Indian Ocean), have been reported. Over Irene a large increase in the urban-influenced boundary layer (BL, 1.5–4 km) was also observed during the 18-year period, equivalent to 30% decade⁻¹. Here we show that the Irene BL trend is at least partly due to a gradual change in the sonde launch times from early morning to the midday period. The FT ozone profiles over Irene in 1990–2007 are re-examined, filling in a 1995–1999 gap with ozone profiles taken during the Measurements of Ozone by Airbus In-service Aircraft (MOZAIC) project over nearby Johannesburg. A multivariate regression model that accounts for the annual ozone cycle, El Niño–Southern Oscillation (ENSO) and possible tropopause changes was applied to monthly averaged Irene data from 4 to 11 km and to 1992–2011 Réunion sonde data from 4 to 15 km. Statistically significant trends appear predominantly in the middle and upper troposphere (UT; 4–11 km over Irene, 4–15 km over Réunion) in winter (June–August), with increases ~1 ppbv yr⁻¹ over Irene and ~2 ppbv yr⁻¹ over Réunion. These changes are equivalent to ~25 and 35–45% decade⁻¹, respectively. Both stations also display smaller positive trends in summer, with a 45% decade⁻¹ ozone increase near the tropopause over Réunion in December. To explain the ozone increases, we investigated a time series of dynamical markers, e.g., potential vorticity (PV) at 330–350 K. PV affects UT ozone over Irene in November–December but displays little relationship with ozone over Réunion. A more likely reason for wintertime FT ozone increases over Irene and Réunion appears to be long-range transport of growing pollution in the Southern Hemisphere. The ozone increases are consistent with trajectory origins of air parcels sampled by the sondes and with recent NOx emissions trends estimated for Africa, South America and Madagascar. For Réunion trajectories also point to sources from the eastern Indian Ocean and Asia. | |
| dc.description.sponsorship | This study was begun during a Fulbright Scholar grant that allowed A. M. Thompson to spend 8 months in South Africa during 2010–2011, with extraordinary support and hospitality from North-West University Potchefstroom (D. J. J. Pienaar and his group), the CSIR Pretoria (V. Sivakumar), the University of the Witwatersrand Climatology Research Group (S. J. Piketh) and co-author G. J. R. Coetzee (South African Weather Service). Helpful comments on the manuscript were received from D. Waugh (Johns Hopkins Univ.), J.-L. Baray (LaMP/OPGC, France) and from L. D. Oman and S. Strode at NASA/GSFC. Irene sondes are made possible by the South African Weather Service. The sonde program at Réunion is supported by CNRS and SHADOZ with technical assistance from NOAA/Global Monitoring Division (GMD; S. J. Oltmans and B. J. Johnson). SHADOZ has been funded since 1998 by the Upper Atmosphere Research Program of NASA (thanks to M. J. Kurylo and K. W. Jucks) with contributions from NOAA/GMD and NASA’s Aura Validation. Support for this analysis came from grants to the Pennsylvania State University: NNG05GP22G, NNG05GO62G and NNX09AJ23G. The authors acknowledge the strong support of the European Commission, Airbus, and the airlines (Lufthansa, Air France, Austrian, Air Namibia, Cathay Pacific and China Airlines so far) who carry the MOZAIC or IAGOS equipment and have performed maintenance on it since 1994. MOZAIC is presently funded by INSU-CNRS (France), Météo-France, CNES, Université Paul Sabatier (Toulouse, France) and Forschungszentrum Jülich (FZJ; Jülich, Germany). IAGOS has been additionally funded by the EU projects IAGOS-DS and IAGOS-ERI. The MOZAICIAGOS data are available via the CNES/CNRS-INSU Ether web site: http://www.pole-ether.fr. | |
| dc.description.uri | https://acp.copernicus.org/articles/14/9855/2014/ | |
| dc.format.extent | 15 pages | |
| dc.genre | journal articles | |
| dc.identifier | doi:10.13016/m2f8vg-ejnh | |
| dc.identifier.citation | Thompson, A. M., N. V. Balashov, J. C. Witte, J. G. R. Coetzee, V. Thouret, and F. Posny. “Tropospheric Ozone Increases over the Southern Africa Region: Bellwether for Rapid Growth in Southern Hemisphere Pollution?” Atmospheric Chemistry and Physics 14, no. 18 (September 17, 2014): 9855–69. https://doi.org/10.5194/acp-14-9855-2014. | |
| dc.identifier.uri | https://doi.org/10.5194/acp-14-9855-2014 | |
| dc.identifier.uri | http://hdl.handle.net/11603/34664 | |
| dc.language.iso | en | |
| dc.publisher | EGU | |
| dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
| dc.relation.ispartof | UMBC GESTAR II | |
| dc.rights | CC BY 3.0 DEED Attribution 3.0 Unported | |
| dc.rights.uri | https://creativecommons.org/licenses/by/3.0/ | |
| dc.title | Tropospheric ozone increases over the southern Africa region: bellwether for rapid growth in Southern Hemisphere pollution? | |
| dc.type | Text | |
| dcterms.creator | https://orcid.org/0000-0002-7829-0920 |
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