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Title: Constraining the emission of particulate matter from Indonesian peatland burning using continuous observation data
Authors: Kuwata, Mikinori
Neelam-Naganathan, Gautham-Giri
Miyakawa, Takuma
Kozan, Osamu
Kawasaki, Masahiro
Mohd Talib Latif
Syahrial Sumin
Md Firoz Khan
Keywords: DRNTU::Science::Chemistry
Carbon Monoxide
Issue Date: 2018
Source: Kuwata, M., Neelam-Naganathan, G.-G., Miyakawa, T., Md Firoz Khan., Kozan, O., Kawasaki, M., . . . Mohd Talib Latif. Constraining the emission of particulate matter from Indonesian peatland burning using continuous observation data. Journal of Geophysical Research: Atmospheres, 123(17), 9828-9842. doi:10.1029/2018JD028564
Series/Report no.: Journal of Geophysical Research: Atmospheres
Abstract: Tropical peatland, which dominantly distributes in Indonesia and Malaysia, has experienced recurring fires in the last few decades. Constraining the enhancement ratios and emission factors of gas and particulate matter emitted by the wildfires is necessary to evaluate their environmental and climatic impacts. We analyzed continuous observation data at Pekanbaru in Indonesia and Muar in Malaysia to investigate the emissions of gas and particulate matter. The enhancement ratios of particulate matter to carbon monoxide (PM10/CO) of wildfires in Riau province in June 2013 and February–March 2014 were analyzed. The PM10/CO ratios of peatland burning plumes ranged from 77 to 97 μg mg−1 for the event in June 2013, whereas the corresponding value was 127 μg mg−1 in February–March 2014. These enhancement ratios were translated to the emission factors of particulate matter using previous data on the emission factors of CO, assuming that secondary formation was ignorable. The estimated emission factors for PM10 were 13 ± 2 g kg−1 (2013) and 19 ± 2 g kg−1 (2014). These values are comparable to those reported by recent field observations in Indonesia and Malaysia (17.3 ± 6.0 to 34.4 ± 18.8 g kg−1). The estimated emission factors from both the present study and recent field work are consistently higher than that used in the current emission inventory, which suggests that it should be updated. A caveat for this analysis is possible influence of secondary formation, which will still be needed to be investigated in future studies.
ISSN: 2169-897X
DOI: 10.1029/2018JD028564
Rights: © 2018 American Geophysical Union. This paper was published in Journal of Geophysical Research: Atmospheres and is made available as an electronic reprint (preprint) with permission of American Geophysical Union. The published version is available at []. One print or electronic copy may be made for personal use only. Systematic or multiple reproduction, distribution to multiple locations via electronic or other means, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper is prohibited and is subject to penalties under law.
Fulltext Permission: open
Fulltext Availability: With Fulltext
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