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Speciated PM10 Emission Inventory for Delhi, India

Emission inventories can serve as a basis for air quality management programs. The focus has been mainly on building inventories for criteria pollutants including particulate matter (PM). Control efforts in developing countries are mostly limited to total suspended particles (TSP) and/or PM 10 . Sin...

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Bibliographic Details
Published in:Aerosol and air quality research 2014, Vol.14 (5), p.1515-1526
Main Authors: Gargava, Prashant, Chow, Judith C., Watson, John G., Lowenthal, Douglas H.
Format: Article
Language:English
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Summary:Emission inventories can serve as a basis for air quality management programs. The focus has been mainly on building inventories for criteria pollutants including particulate matter (PM). Control efforts in developing countries are mostly limited to total suspended particles (TSP) and/or PM 10 . Since the adverse effects of PM 10 depend on its chemical composition, it is important to control emissions of toxic species. The first step is to identify key pollution sources and estimate quantities of various chemical species in emissions. This paper presents a speciated PM 10 emission inventory for Delhi, the capital and one of the most polluted cities in India. An established PM 10 inventory for Delhi in conjunction with source profiles was used to estimate emissions of major PM 10 components including organic and elemental carbon (OC and EC, respectively), sulphates (SO 4 2– ), and nitrates (NO 3 – ), as well as selected toxic trace metals (i.e., Pb, Ni, V, As, and Hg), some of which are subject to India’s National Ambient Air Quality Standards (NAAQS). For the base year of 2007, emission estimates for PM 10 mass, OC, EC, SO 4 2– , and NO 3 – are 140, 22, 6.4, 2.8, and 2.1 tonnes/day (TPD; 1 tonne = 1000 kg), respectively. Emissions of Pb, Ni, V, As, and Hg are estimated to be 203, 43, 37, 26, and 9.4 kg/day, respectively. This inventory underestimated Pb and Hg emissions because sources of PM 10 from unorganized secondary lead smelters are not specifically identified and gas-to-particle conversion of Hg is not accounted for.
ISSN:1680-8584
2071-1409
DOI:10.4209/aaqr.2013.02.0047