Mixing State of Carbonaceous Aerosols of Primary Emissions from “Improved” African Cookstoves
Author(s) -
Yu-Chieh Ting,
Edward John Mitchell,
J. D. Allan,
Dantong Liu,
Dominick V. Spracklen,
A. Williams,
J.M. Jones,
Amanda LeaLangton,
G. McFiggans,
Hugh Coe
Publication year - 2018
Publication title -
environmental science and technology
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.851
H-Index - 397
eISSN - 1520-5851
pISSN - 0013-936X
DOI - 10.1021/acs.est.8b00456
Subject(s) - stove , aerosol , particulates , combustion , soot , environmental science , environmental chemistry , solid fuel , coal , tonne , coal combustion products , chemistry , fraction (chemistry) , carbon fibers , mass concentration (chemistry) , waste management , materials science , organic chemistry , composite number , engineering , composite material
Designs of "improved" stoves are introduced recently to benefit the solid fuel consumption of cooking activities in developing countries, but the uncertainties concerning the combustion processes and particulate emissions remain poorly characterized. To help understand this, combustion in three examples of "improved" African cookstoves was investigated in the laboratory. A typical European heating stove was included for comparison purpose. Detailed aerosol emissions were studied in real-time with an Aerosol Mass Spectrometer and Single Particle Soot Photometer, to explore interactions between black carbon (BC) and organic carbon aerosols, which were parametrized according to modified combustion efficiency (MCE), a common metric used within the atmospheric emission community. Greater than 50% of the total organic matter (OM) was found in BC-containing particles when MCE was >0.95 for dry oak and coal fuels, whereas at lower MCE, over 80% of the total OM for most of the fuels existed in particles without detectable BC. When the OM mass fraction of total particulate matter (PM 1 ) > 0.9, the mass ratio of OM to refractory BC in BC-containing particles was about 2-3, but only ∼0.8 when OM mass fraction <0.9. These findings are not currently included in models and such information should be considered in the future emission scenarios.
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