干旱区生态环境知识资源中心

Aerosol optical depth and Angstroom exponent were obtained from multi filter rotating shadowband radiometer (MFRSR) observations carried out at the island of Lampedusa, in the Central Mediterranean, in the period July 2001-September 2003. The average aerosol optical depth at 495.7 nm, tau, is 0.24 +/- 0.14; the average Angstrom exponent, alpha, is 0.86 +/- 0.63. The observed values of tau range from 0.03 to 1.13, and the values of alpha vary from -0.32 to 2.05, indicating a large variability in aerosol content and size. In cloud-free conditions, 36% of the airmasses come from Africa, 25% from Central-Eastern Europe, and 19% from Western France, Spain and the North Atlantic. In summer, 42% of the airmasses is of African origin. In almost all cases African aerosols display high values of tau and low values of alpha, typical of Saharan dust (average values of tau and alpha are 0.36 and 0.42, respectively). Particles originating from Central-Eastern Europe show relatively large average values of tau and alpha (0.23 and 1.5, respectively), while particles from Western France, Spain and the North Atlantic show the lowest average values of tau (0.15), and relatively small values of alpha (0.92). Intermediate values of alpha are often connected with relatively fast changes of the airmass originating sector, suggesting the contemporary presence of different types of particles in the air column. Clean marine conditions are rare at Lampedusa, and are generally associated with subsidence of the airmasses reaching the island. Average values of tau and alpha for clean marine conditions are 0.11 and 0.86, respectively. The largest values of alpha (about 2) were observed in August 2003, when large scale forest fires in Southern Europe produced consistent amounts of fine combustion particles, that were transported to the Central Mediterranean by a persistent high pressure system over Central Europe. Smoke particles in some cases mix with desert dust, producing intermediate values of alpha. The seasonal distribution of the meteorological patterns over the Mediterranean, the efficiency of the aerosol production mechanisms, and the variability of the particles’ residence time produce a distinct seasonal cycle of aerosol optical depths and Angstrom exponent values. Particles originating from all sectors show a summer maximum in aerosol optical depth. The summer increase in optical depth for European aerosols is linked with an increment in the values of alpha, that indicates an enhancement in the number of fine particles. The summer maximum of tau for African particles is associated with a weak reduction in the Angstrom exponent, suggesting an increase in the total number of particles and a relatively more intense transport of large particles. The observations were classified according to the aerosol optical properties, and two main classes have been identified: desert dust and biomass burning/urban-industrial aerosols. Values of tau and alpha averaged over the whole observing period are 0.37 and 0.15 for desert dust, and 0.27 and 1.77 for urbanindustrial/biomass burning aerosols.