[AAS06-P26] Do hypohalous acids play important roles on sulfate formation in the Antarctic atmosphere?
Keywords:Antarctica, Sulfate aerosols, Reactive bromine, 17O excess
Bry (= HBr + HOBr + Br2 + BrO + BrNO2 + BrNO3 + Br) is thought to play important roles in atmospheric chemistry in the Antarctic boundary layer through e.g., ozone destruction by Br atoms and oxidation of dimethyl sulfide by BrO [1,2]. A series of studies has indicated that a major source of Bry in coastal Antarctica is blowing-snow which takes a part of brine on the sea ice surface to the atmosphere [3,4]. Therefore, it has been suggested that the importance of Bry is limited at Dumont d’Urville (DDU; 66°40'S, 140°01'E), one of coastal Antarctic stations where the sea ice extent is relatively low compared to other coastal stations and highly exposed to the continental winds from the East Antarctic plateau [5]. Nevertheless, 17O-excess (Δ17O ≒ δ17O – 0.52 x δ18O) of atmospheric sulfate (SO42-) at DDU showed relatively low values in spring compared to autumn, which indicates the possibility of a significant contribution of hypohalous acids (HOBr, HOCl) to aqueous S(IV) oxidation in the spring time [6].
To test this hypothesis, we simulate 17O excess of SO42- using 3D chemical transport model (GEOS-Chem) in which reactions of S(IV) and hypohalous acids were recently implemented. We discuss the results by comparison of the observations at DDU with those from Concordia (75°06'S, 123°33'E), the inland Antarctic station which is located more than 1,000 km away from the sea ice.
References:
[1] Saiz-Lopez et al. (2008), ACP, Vol.8, p.887-900, doi: 10.5194/acp-8-887-2008
[2] Read et al. (2008), ACP, Vol.8, p.2985-2997, doi: 10.5194/acp-8-2985-2008
[3] Yang et al. (2008), GRL, Vol.35, L16815, doi: 10.1029/2008GL034536
[4] Lieb-Lappen and Obbard (2015), ACP, Vol.15, p7537-7545, doi: 10.5194/acp-15-7537-2015
[5] Legrand et al. (2009), JGRA, Vo.114, D20, doi: 10.1029/2008JD011667
[6] Ishino et al. (2017), ACP, Vol.17, p.3713-3727, doi:10.5194/acp-17-3713-2017
To test this hypothesis, we simulate 17O excess of SO42- using 3D chemical transport model (GEOS-Chem) in which reactions of S(IV) and hypohalous acids were recently implemented. We discuss the results by comparison of the observations at DDU with those from Concordia (75°06'S, 123°33'E), the inland Antarctic station which is located more than 1,000 km away from the sea ice.
References:
[1] Saiz-Lopez et al. (2008), ACP, Vol.8, p.887-900, doi: 10.5194/acp-8-887-2008
[2] Read et al. (2008), ACP, Vol.8, p.2985-2997, doi: 10.5194/acp-8-2985-2008
[3] Yang et al. (2008), GRL, Vol.35, L16815, doi: 10.1029/2008GL034536
[4] Lieb-Lappen and Obbard (2015), ACP, Vol.15, p7537-7545, doi: 10.5194/acp-15-7537-2015
[5] Legrand et al. (2009), JGRA, Vo.114, D20, doi: 10.1029/2008JD011667
[6] Ishino et al. (2017), ACP, Vol.17, p.3713-3727, doi:10.5194/acp-17-3713-2017