Chemical and morphological characterization of PM2.5 collected during MILAGRO campaign using scanning electron microscopy Article uri icon

abstract

  • PM2.5 were collected in March 2006 during the MILAGRO campaign (Megacities Initiative: Local and Global Research Observations) carried out in the northern region of the Mexico City Metropolitan Area (MCMA), in order to realize an individual characterization of particulate matter through scanning electron microscopy coupled with an energy-dispersive X-Ray analyzer (SEM-EDX), acquiring information from around 6 000 particles about their morphology, size and superficial chemical composition. Measurements of the aerosol were obtained at a site located in the northern part of Mexico City (T0) and also at a site located 30 km northeast (T1) in four time intervals 6:00 - 9:00; 11:00 - 14:00; 16:00 - 19:00 and 21:00 - 0:00 hrs. Employing backscattered electron detector (BSD) anthropogenic phases were analyzed with the EDX and elemental composition of individual particles showed mainly elemental composition of Fe-O (24%25 relative abundance) with spherical morphology congruent to emissions from metal-mechanic industrial process and soil re-suspension. Twenty percent of the aerosol was Pb-rich particles identified as agglomerations of nanometric spheres of individual size distributions among 1.0 - 600 nm and they are related to high temperature industrial emissions. The Ba- rich particles (16%25) presented chemical associations of Ba-S-O and irregular morphologies and they were related to emissions from the mineral phase of barite that constitutes the asbestos of the automobile pieces. C-rich group was the fourth most abundant (12%25) one with predominant morphology corresponds to nanometric spheres (between 600 and 800 nm) of compact and continuous surface, this kind of particles are mainly related to vehicle exhaust emissions and their temporal distribution presented a clear decrease during weekends when vehicle traffic is reduced on the MCMA. Elements like Ca, Zn, Cu, Sr, Sn, Al, Sb, Na and W were also detected in less relative abundance (28%25 of the total), and their individual morphology and possible source emissions are described. © Author(s) 2012.

publication date

  • 2012-01-01