C21D-02
Dust, Elemental Carbon and Other Impurities on Central Asian Glaciers: Origin and Radiative Forcing

Tuesday, 15 December 2015: 08:15
3002 (Moscone West)
Julia Schmale1,2, Mark Flanner3, Shichang Kang4, Michael Sprenger5, Qianggong Zhang6,7, Yang Li6,7, J. Guo6,7 and Margit Schwikowski8, (1)Paul Scherrer Institute, Villingen, Switzerland, (2)Institute for Advanced Sustainability Studies, Potsdam, Germany, (3)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (4)ITP Institute of Tibetan Plateau Research, Chinese Academy of Sciences, Beijing, China, (5)ETH Zurich, Institute for Atmospheric and Climate Science, Zurich, Switzerland, (6)State Key Laboratory of Cryospheric Sciences, Cold and Arid Regions Environmental and Engineering Research Institute (CAREERI), Chinese Academy of Sciences (CAS), Lanzhou, China, (7)Key Laboratory of Tibetan Environment Changes and Land Surface Processes, Institute of Tibetan Plateau Research, Chinese Academy of Sciences (CAS), Lanzhou, China, (8)Paul Scherrer Institute, Laboratory of Radiochemistry and Environmental Chemistry, Villingen, Switzerland
Abstract:
In Central Asia, more than 60 % of the population depends on water stored in glaciers and mountain snow. While temperature, precipitation and dynamic processes are key drivers of glacial change, deposition of light absorbing impurities such as mineral dust and black carbon can lead to accelerated melting through surface albedo reduction. Here, we discuss the origin of deposited mineral dust and black carbon and their impacts on albedo change and radiative forcing (RF).

218 snow samples were taken from 13 snow pits on 4 glaciers, Abramov (Pamir), Suek, Glacier No. 354 and Golubin (Tien Shan), representing deposition between summer 2012 and 2014. They were analyzed for elemental and organic carbon by a thermo-optical method, mineral dust by gravimetry, and iron by ICP-MS. Back trajectory ensembles were released every 6 hours with the Lagranto model for the covered period at all sites. Boundary layer “footprints” were calculated to estimate general source regions and combined with MODIS fire counts for potential fire contributions. Albedo reduction due to black carbon and mineral dust was calculated with the Snow-Ice-Aerosol-Radiative model (SNICAR), and surface spectral irradiances were derived from atmospheric radiative transfer calculations to determine the RF under clear-sky and all sky conditions using local radiation measurements.

Dust contributions came from Central Asia, the Arabian Peninsula, the Sahara and partly the Taklimakan. Fire contributions were higher in 2014 and generally came from the West and North. We find that EC exerts roughly 3 times more RF than mineral dust in fresh and relatively fresh snow (~5 W/m2) and up to 6 times more in snow that experienced melting (> 10 W/m2) even though EC concentrations (average per snow pit from 90 to 700 ng/g) were up to two orders of magnitude lower than mineral dust (10 to 140 µg/g).