Source terms and source strengths of the carbonaceous aerosol in the tropics Tập 3 - Trang 469-489 - 1985
Hélène Cachier, Patrick Buat-Menard, Michel Fontugne, Jacques Rancher
Atmospheric aerosol samples were collected in the Ivory Coast, primarily at Lamto (6°N, 5°W) between 1979 and 1981. The samples were analysed for total particulate carbon concentration and isotopic composition (13C/12C) by mass spectrometry. Observed concentrations were found high compared to values reported for temperate regions. Fine particulate carbon in the submicrometersize range accounted for 50 to 80% of the reported concentrations. At Lamto, both particulate carbon concentrations and isotopic ratios exhibit a large temporal variability which is shown to reflect the diversity of sources and their seasonal evolution. Natural emissions from the equatorial forest during the wet season, and biomass burning during the dry season, appear to be the major sources. The latter, though active during only a third of the year, is, on an annual basis, the most important source. Based on the data obtained at Lamto, an attempt has been made to estimate the flux of fine particulate carbon emitted from the tropical regions into the global troposphere. This flux, which is of the order of 20×1012 g C/yr, appears to be equivalent to the flux of fine particulate carbon emitted from industrial sources. These results suggest that the tropospheric burden of fine particulate carbon in lowlatitude regions is dominated by the long-range transport of carbonaceous aerosols originating from the Tropics.
Nitrogen and sulfur species in Antarctic aerosols at Mawson, Palmer Station, and Marsh (King George Island) Tập 17 Số 2 - Trang 95-122 - 1993
Dennis L. Savoie, Joseph M. Prospero, Randy J. Larsen, Fen Huang, Miguel Izaguirre, Ting Chang Huang, T. H. Snowdon, Lillian Custals, C.G. Sanderson
Diffuse radiation, twilight, and photochemistry — II Tập 13 - Trang 393-406 - 1991
D. J. Lary, J. A. Pyle
A photochemical scheme including a detailed description of multiple seattering up to solar zenith angles of 960 has been used to study a number of different datasets. The good agreement of the model with these datasets and the improvement over previous intercomparisons emphasise the importance of both the diffuse radiation field at wavelengths below 310 nm and multiple scattering at solar zenith angles greater than 90o. These features are ignored in some photochemical models but prove to be very important in modelling photochemistry at dawn and dusk.