1Laboratoire de Glaciologie et Géophysique de l'Environnement(UMR CNRS/INSU 5183), CNRS-UJF, BP 96, 38 402 Saint Martin d'Hères, France
2School of Environmental Sciences, University of East Anglia, UK
3Rosenstiel School of Marine and Atmospheric Science, University of Miami, USA
4Department of Meteorology, University of Reading, UK
5National Center for Atmospheric Research, Boulder, Colorado, USA
*now at: Department of Environmental Sciences, Policy and Management, University of California, Berkeley, USA
**now at: Met. Office, Hadley Centre Reading Unit, Meteorology building, University of Reading, RGB BB, UK
Abstract. The budgets of seven halogenated gases (CFC-11, CFC-12, CFC-113, CFC-114, CFC-115, CCl4 and SF6) are studied by comparing measurements in polar firn air from two Arctic and three Antarctic sites, and simulation results of two numerical models: a 2-D atmospheric chemistry model and a 1-D firn diffusion model. The first one is used to calculate atmospheric concentrations from emission trends based on industrial inventories; the calculated concentration trends are used by the second one to produce depth concentration profiles in the firn. The 2-D atmospheric model is validated in the boundary layer by comparison with atmospheric station measurements, and vertically for CFC-12 by comparison with balloon and FTIR measurements. Firn air measurements provide constraints on historical atmospheric concentrations over the last century. Age distributions in the firn are discussed using a Green function approach. Finally, our results are used as input to a radiative model in order to evaluate the radiative forcing of our target gases. Multi-species and multi-site firn air studies allow to better constrain atmospheric trends. The low concentrations of all studied gases at the bottom of the firn, and their consistency with our model results confirm that their natural sources are insignificant. Our results indicate that the emissions, sinks and trends of CFC-11, CFC-12, CFC-113, CFC-115 and SF6 are well constrained, whereas it is not the case for CFC-114 and CCl4. Significant emission-dependent changes in the lifetimes of halocarbons destroyed in the stratosphere were obtained. Those result from the time needed for their transport from the surface where they are emitted to the stratosphere where they are destroyed. Efforts should be made to update and reduce the large uncertainties on CFC lifetimes.