1. Ozone and temperature trends in the upper stratosphere at five stations of the Network for the Detection of Atmospheric Composition Change
- Author
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Alan Parrish, Greg Bodeker, F. Schönenborn, Alain Hauchecorne, Klemens Hocke, Stacey M. Frith, John P. Burrows, Niklaus Kämpfer, D. P. J. Swart, Philippe Keckhut, Richard S. Stolarski, I. S. Boyd, Thierry Leblanc, A. Rozanov, Hans Claude, C. von Savigny, Sophie Godin-Beekmann, Larry W. Thomason, Ellis E. Remsberg, J. A. E. van Gijsel, I. S. McDermid, Wolfgang Steinbrecht, Meteorologisches Observatorium Hohenpeißenberg (MOHp), Deutscher Wetterdienst [Offenbach] (DWD), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), STRATO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), National Institute for Public Health and the Environment [Bilthoven] (RIVM), National Institute of Water and Atmospheric Research [Lauder] (NIWA), Department of Astronomy [Amherst], University of Massachusetts [Amherst] (UMass Amherst), University of Massachusetts System (UMASS)-University of Massachusetts System (UMASS), Institut für angewandte Physik [Bern] (IAP), Universität Bern [Bern], NASA Goddard Space Flight Center (GSFC), NASA Langley Research Center [Hampton] (LaRC), Institut für Umweltphysik [Bremen] (IUP), Universität Bremen, and Universität Bern [Bern] (UNIBE)
- Subjects
[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph] ,Ozone ,Stratospheric Aerosol and Gas Experiment ,010504 meteorology & atmospheric sciences ,Microwave radiometer ,Global Ozone Monitoring by Occultation of Stars ,010502 geochemistry & geophysics ,Atmospheric sciences ,01 natural sciences ,SCIAMACHY ,chemistry.chemical_compound ,chemistry ,13. Climate action ,Ozone layer ,Montreal Protocol ,General Earth and Planetary Sciences ,Environmental science ,Stratosphere ,0105 earth and related environmental sciences - Abstract
International audience; Upper stratospheric ozone anomalies from the satellite-borne Solar Backscatter Ultra-Violet (SBUV), Stratospheric Aerosol and Gas Experiment II (SAGE II), Halogen Occultation Experiment (HALOE), Global Ozone Monitoring by Occultation of Stars (GOMOS), and Scanning Imaging Absorption Spectrometer for Atmospheric Chartography (SCIAMACHY) instruments agree within 5% or better with ground-based data from lidars and microwave radiometers at five stations of the Network for the Detection of Atmospheric Composition Change (NDACC), from 45°S to 48°N. From 1979 until the late 1990s, all available data show a clear decline of ozone near 40 km, by 10%–15%. This decline has not continued in the last 10 years. At some sites, ozone at 40 km appears to have increased since 2000, consistent with the beginning decline of stratospheric chlorine. The phaseout of chlorofluorocarbons after the International Montreal Protocol in 1987 has been successful, and is now showing positive effects on ozone in the upper stratosphere. Temperature anomalies near 40 km altitude from European Centre for Medium Range Weather Forecast reanalyses (ERA-40), from National Centers for Environmental Prediction (NCEP) operational analyses, and from HALOE and lidar measurements show good consistency at the five stations, within about 3 K. Since about 1985, upper stratospheric temperatures have been fluctuating around a constant level at all five NDACC stations. This non-decline of upper stratospheric temperatures is a significant change from the more or less linear cooling of the upper stratosphere up until the mid-1990s, reported in previous trend assessments. It is also at odds with the almost linear 1 K per decade cooling simulated over the entire 1979–2010 period by chemistry–climate models (CCMs). The same CCM simulations, however, track the historical ozone anomalies quite well, including the change of ozone tendency in the late 1990s.
- Published
- 2009