1Department of Chemistry, University of Florence, Sesto Fiorentino, 50019 Florence, Italy
2ENEA, Laboratory for Observations and Analyses of Earth and Climate, 90141 Palermo, Italy
3Department of Physics & INFN, University of Genoa, 16146 Genoa, Italy
4ARPAL-Unità Operativa CFMI-PC, 16129 Genova, Italy
5Department of Physics, University of Florence & INFN-Firenze, Sesto Fiorentino, 50019 Florence, Italy
6ENEA, Laboratory for Observations and Analyses of Earth and Climate, 00123 Rome, Italy
7Department of Earth Physics and Thermodynamics, University of Valencia, Valencia, Spain
8ENEA, Laboratory for Observations and Analyses of Earth and Climate, 92010 Lampedusa, Italy
9ISAC CNR, Via Gobetti 101, 40129, Bologna, Italy
Received: 08 Jun 2016 – Discussion started: 01 Jul 2016
Abstract. Particulate matter with aerodynamic diameters lower than 10 µm, (PM10) aerosol samples were collected during summer 2013 within the framework of the Chemistry and Aerosol Mediterranean Experiment (ChArMEx) at two sites located north (Capo Granitola) and south (Lampedusa Island), respectively, of the main Mediterranean shipping route in the Straight of Sicily.
Revised: 23 Nov 2016 – Accepted: 19 Jan 2017 – Published: 10 Feb 2017
The PM10 samples were collected with 12 h time resolutions at both sites. Selected metals, main anions, cations and elemental and organic carbon were determined.
The evolution of soluble V and Ni concentrations (typical markers of heavy fuel oil combustion) was related to meteorology and ship traffic intensity in the Straight of Sicily, using a high-resolution regional model for calculation of back trajectories. Elevated concentration of V and Ni at Capo Granitola and Lampedusa are found to correspond with air masses from the Straight of Sicily and coincidences between trajectories and positions of large ships; the vertical structure of the planetary boundary layer also appears to play a role, with high V values associated with strong inversions and a stable boundary layer. The V concentration was generally lower at Lampedusa than at Capo Granitola V, where it reached a peak value of 40 ng m−3.
Concentrations of rare earth elements (REEs), La and Ce in particular, were used to identify possible contributions from refineries, whose emissions are also characterized by elevated V and Ni amounts; refinery emissions are expected to display high La ∕ Ce and La ∕ V ratios due to the use of La in the fluid catalytic converter systems. In general, low La ∕ Ce and La ∕ V ratios were observed in the PM samples. The combination of the analyses based on chemical markers, air mass trajectories and ship routes allows us to unambiguously identify the large role of the ship source in the Straight of Sicily.
Based on the sampled aerosols, ratios of the main aerosol species arising from ship emission with respect to V were estimated with the aim of deriving a lower limit for the total ship contribution to PM10. The estimated minimum ship emission contributions to PM10 were 2.0 µg m−3 at Lampedusa and 3.0 µg m−3 at Capo Granitola, corresponding with 11 and 8.6 % of PM10, respectively.
Becagli, S., Anello, F., Bommarito, C., Cassola, F., Calzolai, G., Di Iorio, T., di Sarra, A., Gómez-Amo, J.-L., Lucarelli, F., Marconi, M., Meloni, D., Monteleone, F., Nava, S., Pace, G., Severi, M., Sferlazzo, D. M., Traversi, R., and Udisti, R.: Constraining the ship contribution to the aerosol of the central Mediterranean, Atmos. Chem. Phys., 17, 2067-2084, doi:10.5194/acp-17-2067-2017, 2017.