Venkataraman, Chandra ; Mehra, Anurag ; Mhaskar, Prashant (2001) Mechanisms of sulphate aerosol production in clouds: effect of cloud characteristics and season in the Indian region Tellus B: Chemical and Physical Meteorology, 53 (3). pp. 260-272. ISSN 0280-6509
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Official URL: https://www.tandfonline.com/doi/abs/10.3402/tellus...
Related URL: http://dx.doi.org/10.3402/tellusb.v53i3.16595
Abstract
Measurements made during the Indian Ocean Experiment (INDOEX) in 1998, indicate likely regional atmospheric effects of sulphate aerosol over India including the potential for cloud processing of SO2 to sulphate. Sulphate aerosol production in clouds was examined for cloud characteristics and pollutant concentrations typical of the Indian region, to assess the contribution of different mechanisms to sulphate formation. A simple model was formulated incorporating gas-liquid equilibria, gas-phase mass transfer, SO2 oxidation in the gas phase by OH• radicals and in the aqueous phase by H2O2, O3 and O2 catalysed by Fe3+ and Mn2+ in a cloud with uniformly sized drops. Sulphate formation was simulated in St/Sc, Cu and Cb clouds using an initial pH of 6.5, likely to occur in this region, for cloud drop diameters of 10, 50 and 100 μm. The clouds were assumed to have nucleated on ammonium sulphate aerosols and contained reported background concentrations of these ions in clean rainwater over the Indian ocean. The simulations produced final cloud pHs of 4.5–5 and final sulphate concentrations of 25–90 μM, in agreement with the range of reported preliminary measurements. An examination of mass transfer effects showed that the characteristic diffusion times of H2O2 and SO2 were lower by a factor of 10 or more than the respective reaction times, indicating that mass transfer effects would not limit the rate of SVI formation under likely atmospheric conditions. Sulphate formation in St/Sc clouds was shown to likely be SO2 limited in July and H2O2 limited in January. In all cases, the gas phase reaction and the O2 reaction catalysed by Mn2+ and Fe3+ contributed less than 1% to the SVI produced. In St/Sc and Cu clouds, 85–96% of the SVI was from the H2O2 reaction. In Cb clouds about 60–75% of the SVI was from the H2O2 reaction and 25–41% from the O3 reaction. In Cb clouds, the short residence and the persistence of alkaline conditions in the earlier part of the cloud cycle, enhance the contribution of the O3 reaction to the greatest extent. If alkaline conditions were to persist throughout the cloud cycle (from cation chemistry not simulated in this model), the contribution of the O3 reaction to SVI could be further enhanced.
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Deposited On: | 28 May 2018 11:02 |
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