Modelling stable water isotopes during “high-precipitation” events at Dome C, Antarctica

• Main Authors: E. Schlosser, V. Masson Delmotte, C. Risi, M. Valt, J. G. Powers, K. W. Manning, M. G. Duda, A. Cagnati, STENNI, BARBARA
• Other Authors: European Geosciences Union, E., Schlosser, V., Masson Delmotte, C., Risi, Stenni, Barbara, M., Valt, J. G., Power, K. W., Manning, M. G., Duda, A., Cagnati
• Format: Conference Object
• Language: English
• Published: Copernicus Publications 2014
• Subjects: Antarctica; Dome C; precipitation; water stable isotope; mesoscale atmospheric model; Antarctic; The Antarctic; East Antarctica; Antarc*; ice core
• Online Access: http://hdl.handle.net/11368/2798725

For a correct paleoclimatologic interpretation of stable water isotopes from ice cores both pre- and postdepositional processes and their role for isotope fractionation have to be better understood. Our study focuses on “pre-depositional processes”, namely the atmospheric processes that determine moisture transport and precipitation formation. At the deep ice core drilling site "Dome C", East Antarctica, fresh snow samples have been taken since 2006. These samples have been analysed crystallographically, which enables us to clearly distinguish between blowing snow, diamond dust, and "synoptic precipitation". Also the stable oxygen/hydrogen isotope ratios of the snow samples were measured, including measurements of 17-O. This is the first and only multi-year fresh-snow data series from an Antarctic deep drilling site. The Antarctic Mesoscale Prediction System (AMPS) employs Polar WRF for aviation weather forecasts in Antarctica. The data are archived and can be used for scientific purposes. The mesoscale atmospheric model was adapted especially for polar regions. The horizontal resolution for the domain that covers the Antarctic continent is 10 km. It was shown that precipitation at Dome C is temporally dominated by diamond dust. However, comparatively large amounts of precipitation are observed during several “high-precipitation” events per year, caused by synoptic activity in the circumpolar trough and related advection of relatively warm and moist air from lower latitudes to the interior of Antarctica. AMPS archive data are used to investigate the synoptic situations that lead to “high-precipitation” events at Dome C; in particular, possible moisture sources are determined using back-trajectories. With this meteorological information, the isotope ratios are calculated using two different isotope models, the Mixed Cloud Isotope Model, a simple Rayleigh-type model, and the LMDZ-iso (Laboratoire de Météorologie Dynamic Zoom), a General Circulation Model (GCM) with implementation of stable isotopes. The results ...