Hamish Struthers
Stockholm University
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Publication
Featured researches published by Hamish Struthers.
Journal of Geophysical Research | 2010
John Austin; Hamish Struthers; J. F. Scinocca; David A. Plummer; Hideharu Akiyoshi; A. J. G. Baumgaertner; Slimane Bekki; G. E. Bodeker; Peter Braesicke; C. Brühl; Neal Butchart; M. P. Chipperfield; David Cugnet; Martin Dameris; S. Dhomse; S. M. Frith; Hella Garny; Andrew Gettelman; Steven C. Hardiman; Patrick Jöckel; Douglas E. Kinnison; Anne Kubin; Jean-Francois Lamarque; Ulrike Langematz; E. Mancini; Marion Marchand; M. Michou; Olaf Morgenstern; Tetsu Nakamura; J. E. Nielsen
Coupled chemistry-climate model simulations covering the recent past and continuing throughout the 21st century have been completed with a range of different models. Common forcings are used for the halogen amounts and greenhouse gas concentrations, as expected under the Montreal Protocol (with amendments) and Intergovernmental Panel on Climate Change A1b Scenario. The simulations of the Antarctic ozone hole are compared using commonly used diagnostics: the minimum ozone, the maximum area of ozone below 220 DU, and the ozone mass deficit below 220 DU. Despite the fact that the processes responsible for ozone depletion are reasonably well understood, a wide range of results is obtained. Comparisons with observations indicate that one of the reasons for the model underprediction in ozone hole area is the tendency for models to underpredict, by up to 35%, the area of low temperatures responsible for polar stratospheric cloud formation. Models also typically have species gradients that are too weak at the edge of the polar vortex, suggesting that there is too much mixing of air across the vortex edge. Other models show a high bias in total column ozone which restricts the size of the ozone hole (defined by a 220 DU threshold). The results of those models which agree best with observations are examined in more detail. For several models the ozone hole does not disappear this century but a small ozone hole of up to three million square kilometers continues to occur in most springs even after 2070.
Geophysical Research Letters | 2012
Laura E. Revell; Greg Bodeker; Dan Smale; Ralph Lehmann; Petra E. Huck; Bryce E. Williamson; E. Rozanov; Hamish Struthers
Recently, it was shown that of the ozone-depleting substances currently emitted, N2O emissions (the primary source of stratospheric NOx) dominate, and are likely to do so throughout the 21st century. To investigate the links between N2O and NOx concentrations, and the effects of NOx on ozone in a changing climate, the evolution of stratospheric ozone from 1960 to 2100 was simulated using the NIWA-SOCOL chemistry-climate model. The yield of NOx from N2O is reduced due to stratospheric cooling and a strengthening of the Brewer-Dobson circulation. After accounting for the reduced NOx yield, additional weakening of the primary NOx cycle is attributed to reduced availability of atomic oxygen, due to a) stratospheric cooling decreasing the atomic oxygen/ozone ratio, and b) enhanced rates of chlorine-catalyzed ozone loss cycles around 2000 and enhanced rates of HOx-induced ozone depletion. Our results suggest that the effects of N2O on ozone depend on both the radiative and chemical environment of the upper stratosphere, specifically CO2-induced cooling of the stratosphere and elevated CH4 emissions which enhance HOx-induced ozone loss and remove the availability of atomic oxygen to participate in NOx ozone loss cycles.
Geoscientific Model Development | 2012
A. Kirkevåg; Trond Iversen; Øyvind Seland; C. Hoose; Jón Egill Kristjánsson; Hamish Struthers; Annica M. L. Ekman; Steven J. Ghan; Jan Griesfeller; E. D. Nilsson; Michael Schulz
Atmospheric Chemistry and Physics | 2008
Andrew Gettelman; Thomas Birner; Veronika Eyring; Hideharu Akiyoshi; Slimane Bekki; C. Brühl; Martin Dameris; Douglas E. Kinnison; Frank Lefèvre; François Lott; E. Mancini; Giovanni Pitari; David A. Plummer; E. Rozanov; Kiyotaka Shibata; Andrea Stenke; Hamish Struthers; W. Tian
Atmospheric Chemistry and Physics | 2010
Hamish Struthers; Annica M. L. Ekman; Paul Glantz; Trond Iversen; A. Kirkevåg; E. M. Mårtensson; Øyvind Seland; E. D. Nilsson
Atmospheric Chemistry and Physics | 2009
Chiara Cagnazzo; Elisa Manzini; Natalia Calvo; Anne R. Douglass; Hideharu Akiyoshi; Slimane Bekki; M. P. Chipperfield; Martin Dameris; Makoto Deushi; Andreas M. Fischer; Hella Garny; Andrew Gettelman; Marco A. Giorgetta; David A. Plummer; E. Rozanov; Theodore G. Shepherd; Kiyotaka Shibata; Andrea Stenke; Hamish Struthers; W. Tian
Atmospheric Chemistry and Physics | 2009
Hamish Struthers; Greg Bodeker; John Austin; Slimane Bekki; Irene Cionni; Martin Dameris; Marco A. Giorgetta; Volker Grewe; Frank Lefèvre; François Lott; Elisa Manzini; Thomas Peter; E. Rozanov; M. Schraner
Atmospheric Chemistry and Physics | 2011
Daniel G. Partridge; Jasper A. Vrugt; Peter Tunved; Annica M. L. Ekman; Hamish Struthers; Armin Sorooshian
Atmospheric Chemistry and Physics | 2010
Patrick Eriksson; Bengt Rydberg; Marston Sheldon Johnston; Donal P. Murtagh; Hamish Struthers; Sylvaine Ferrachat; Ulrike Lohmann
Journal of Geophysical Research | 2010
W. Allan; Hamish Struthers; D. C. Lowe; S. E. Mikaloff Fletcher