Measuring the Antarctic ozone hole with the new Ozone Mapping and Profiler Suite (OMPS)

• Published in: Atmospheric Chemistry and Physics
• Main Authors: Kramarova, N. A., Nash, E. R., Newman, P. A., Bhartia, P. K., McPeters, R. D., Rault, D. F., Seftor, C. J., Xu, P. Q., Labow, G. J.
• Format: Article in Journal/Newspaper
• Language: English
• Published: Copernicus Publications 2014
• Subjects: article; Verlagsveröffentlichung; Antarctic; The Antarctic; Antarc*; Antarctica
• Online Access: https://doi.org/10.5194/acp-14-2353-2014; https://noa.gwlb.de/receive/cop_mods_00045125; https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00044745/acp-14-2353-2014.pdf; https://acp.copernicus.org/articles/14/2353/2014/acp-14-2353-2014.pdf

The new Ozone Mapping and Profiler Suite (OMPS), which launched on the Suomi National Polar-orbiting Partnership satellite in October 2011, gives a detailed view of the development of the Antarctic ozone hole and extends the long series of satellite ozone measurements that go back to the early 1970s. OMPS includes two modules – nadir and limb – to measure profile and total ozone concentrations. The new limb module is designed to measure the vertical profile of ozone between the lowermost stratosphere and the mesosphere. The OMPS observations over Antarctica show excellent agreement with the measurements obtained from independent satellite and ground-based instruments. This validation demonstrates that OMPS data can ably extend the ozone time series over Antarctica in the future. The OMPS observations are used to monitor and characterize the evolution of the 2012 Antarctic ozone hole. While large ozone losses were observed in September 2012, a strong ozone rebound occurred in October and November 2012. This ozone rebound is characterized by rapid increases of ozone at mid-stratospheric levels and a splitting of the ozone hole in early November. The 2012 Antarctic ozone hole was the second smallest on record since 1988.