Difference in production routes of water-soluble organic carbon in PM sub(2.5) observed during non-biomass and biomass burning periods in Gwangju, Korea

4 h integrated PM sub(2.5) samples were collected from an urban site of Gwangju, Korea, for five days and analyzed for organic carbon and elemental carbon (OC and EC), total water-soluble OC (WSOC), hydrophilic and hydrophobic WSOC fractions (WSOC sub(HPI) and WSOC sub(HPO)), oxalate, and inorganic...

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Veröffentlicht in:Environmental science--processes & impacts 2014-06, Vol.16 (7), p.1726-1736
Hauptverfasser: Yu, Geun-Hye, Cho, Sung-Yong, Bae, Min-Suk, Park, Seung-Shik
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description 4 h integrated PM sub(2.5) samples were collected from an urban site of Gwangju, Korea, for five days and analyzed for organic carbon and elemental carbon (OC and EC), total water-soluble OC (WSOC), hydrophilic and hydrophobic WSOC fractions (WSOC sub(HPI) and WSOC sub(HPO)), oxalate, and inorganic ionic species (sodium (Na super(+)), ammonium (NH sub(4) super(+)), potassium (K super(+)), calcium (Ca super(2+)), magnesium (Mg super(2+)), chloride (Cl super(-)), nitrate (NO sub(3) super(-)), and sulfate (SO sub(4) super(2-))) to investigate the possible sources of water-soluble organic aerosols. Two types of sampling periods were classified according to the regression relationship between black carbon (BC) concentrations measured at wavelengths of 370 nm (BC sub(370nm)) and 880 nm (BC sub(880nm)) using an aethalometer; the first period was traffic emission influence ("non-biomass burning (BB) period") and the second was biomass burning influence ("BB period"). The slope of the regression equation (BC sub(370nm)/BC sub(880nm)) was 0.95 for the non-BB period and 1.29 for the BB period. However, no noticeable difference in the WSOC/OC ratio, which can be used to infer the extent of secondary organic aerosol (SOA) formation, was found between the non-BB (0.61, range = 0.43-0.75) and BB (0.61, range = 0.52-0.68) periods, due to significant contribution of primary BB emissions to the WSOC. The concentrations of OC, WSOC and K super(+), which were used as the BB emission markers, were 15.7 mu g C m super(-3) (11.5-24.3), 9.4 mu g C m super(-3) (7.0-12.7), and 1.2 mu g m super(-3) (0.6-2.7), respectively, during the BB period, and these results were approximately 1.7, 1.7, and 3.9 times higher than those during the non-BB period. During the non-BB period, good correlations among WSOC, SO sub(4) super(2-) and oxalate, and poor correlations among WSOC, EC, and K super(+) suggest that SOA is probably an important source of WSOC (and WSOC sub(HPI)) concentration. For the WSOC fractions, better correlations among WSOC sub(HPI), oxalate (R super(2) = 0.52), and SO sub(4) super(2-) (R super(2) = 0.57) were found than among WSOC sub(HPO), oxalate (R super(2) = 0.23), and SO sub(4) super(2-) (R super(2) = 0.20), suggesting that a significant proportion of the WSOC sub(HPI) fraction of OC could be produced through processes (gas-phase and heterogeneous oxidations) such as SOA formation. However, during the BB period, the BB emission source accounted for the high correlations
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Two types of sampling periods were classified according to the regression relationship between black carbon (BC) concentrations measured at wavelengths of 370 nm (BC sub(370nm)) and 880 nm (BC sub(880nm)) using an aethalometer; the first period was traffic emission influence ("non-biomass burning (BB) period") and the second was biomass burning influence ("BB period"). The slope of the regression equation (BC sub(370nm)/BC sub(880nm)) was 0.95 for the non-BB period and 1.29 for the BB period. However, no noticeable difference in the WSOC/OC ratio, which can be used to infer the extent of secondary organic aerosol (SOA) formation, was found between the non-BB (0.61, range = 0.43-0.75) and BB (0.61, range = 0.52-0.68) periods, due to significant contribution of primary BB emissions to the WSOC. The concentrations of OC, WSOC and K super(+), which were used as the BB emission markers, were 15.7 mu g C m super(-3) (11.5-24.3), 9.4 mu g C m super(-3) (7.0-12.7), and 1.2 mu g m super(-3) (0.6-2.7), respectively, during the BB period, and these results were approximately 1.7, 1.7, and 3.9 times higher than those during the non-BB period. During the non-BB period, good correlations among WSOC, SO sub(4) super(2-) and oxalate, and poor correlations among WSOC, EC, and K super(+) suggest that SOA is probably an important source of WSOC (and WSOC sub(HPI)) concentration. For the WSOC fractions, better correlations among WSOC sub(HPI), oxalate (R super(2) = 0.52), and SO sub(4) super(2-) (R super(2) = 0.57) were found than among WSOC sub(HPO), oxalate (R super(2) = 0.23), and SO sub(4) super(2-) (R super(2) = 0.20), suggesting that a significant proportion of the WSOC sub(HPI) fraction of OC could be produced through processes (gas-phase and heterogeneous oxidations) such as SOA formation. However, during the BB period, the BB emission source accounted for the high correlations between total WSOC (and WSOC fractions) and other relevant atmospheric parameters (EC, Na super(+), Cl super(-), K super(+), and oxalate), with higher correlations in WSOC sub(HPI) than in WSOC sub(HPO). 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Two types of sampling periods were classified according to the regression relationship between black carbon (BC) concentrations measured at wavelengths of 370 nm (BC sub(370nm)) and 880 nm (BC sub(880nm)) using an aethalometer; the first period was traffic emission influence ("non-biomass burning (BB) period") and the second was biomass burning influence ("BB period"). The slope of the regression equation (BC sub(370nm)/BC sub(880nm)) was 0.95 for the non-BB period and 1.29 for the BB period. However, no noticeable difference in the WSOC/OC ratio, which can be used to infer the extent of secondary organic aerosol (SOA) formation, was found between the non-BB (0.61, range = 0.43-0.75) and BB (0.61, range = 0.52-0.68) periods, due to significant contribution of primary BB emissions to the WSOC. The concentrations of OC, WSOC and K super(+), which were used as the BB emission markers, were 15.7 mu g C m super(-3) (11.5-24.3), 9.4 mu g C m super(-3) (7.0-12.7), and 1.2 mu g m super(-3) (0.6-2.7), respectively, during the BB period, and these results were approximately 1.7, 1.7, and 3.9 times higher than those during the non-BB period. During the non-BB period, good correlations among WSOC, SO sub(4) super(2-) and oxalate, and poor correlations among WSOC, EC, and K super(+) suggest that SOA is probably an important source of WSOC (and WSOC sub(HPI)) concentration. For the WSOC fractions, better correlations among WSOC sub(HPI), oxalate (R super(2) = 0.52), and SO sub(4) super(2-) (R super(2) = 0.57) were found than among WSOC sub(HPO), oxalate (R super(2) = 0.23), and SO sub(4) super(2-) (R super(2) = 0.20), suggesting that a significant proportion of the WSOC sub(HPI) fraction of OC could be produced through processes (gas-phase and heterogeneous oxidations) such as SOA formation. However, during the BB period, the BB emission source accounted for the high correlations between total WSOC (and WSOC fractions) and other relevant atmospheric parameters (EC, Na super(+), Cl super(-), K super(+), and oxalate), with higher correlations in WSOC sub(HPI) than in WSOC sub(HPO). 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Two types of sampling periods were classified according to the regression relationship between black carbon (BC) concentrations measured at wavelengths of 370 nm (BC sub(370nm)) and 880 nm (BC sub(880nm)) using an aethalometer; the first period was traffic emission influence ("non-biomass burning (BB) period") and the second was biomass burning influence ("BB period"). The slope of the regression equation (BC sub(370nm)/BC sub(880nm)) was 0.95 for the non-BB period and 1.29 for the BB period. However, no noticeable difference in the WSOC/OC ratio, which can be used to infer the extent of secondary organic aerosol (SOA) formation, was found between the non-BB (0.61, range = 0.43-0.75) and BB (0.61, range = 0.52-0.68) periods, due to significant contribution of primary BB emissions to the WSOC. The concentrations of OC, WSOC and K super(+), which were used as the BB emission markers, were 15.7 mu g C m super(-3) (11.5-24.3), 9.4 mu g C m super(-3) (7.0-12.7), and 1.2 mu g m super(-3) (0.6-2.7), respectively, during the BB period, and these results were approximately 1.7, 1.7, and 3.9 times higher than those during the non-BB period. During the non-BB period, good correlations among WSOC, SO sub(4) super(2-) and oxalate, and poor correlations among WSOC, EC, and K super(+) suggest that SOA is probably an important source of WSOC (and WSOC sub(HPI)) concentration. For the WSOC fractions, better correlations among WSOC sub(HPI), oxalate (R super(2) = 0.52), and SO sub(4) super(2-) (R super(2) = 0.57) were found than among WSOC sub(HPO), oxalate (R super(2) = 0.23), and SO sub(4) super(2-) (R super(2) = 0.20), suggesting that a significant proportion of the WSOC sub(HPI) fraction of OC could be produced through processes (gas-phase and heterogeneous oxidations) such as SOA formation. However, during the BB period, the BB emission source accounted for the high correlations between total WSOC (and WSOC fractions) and other relevant atmospheric parameters (EC, Na super(+), Cl super(-), K super(+), and oxalate), with higher correlations in WSOC sub(HPI) than in WSOC sub(HPO). These results suggest a significant contribution of BB emissions to WSOC.</abstract><doi>10.1039/c4em00126e</doi></addata></record>
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title Difference in production routes of water-soluble organic carbon in PM sub(2.5) observed during non-biomass and biomass burning periods in Gwangju, Korea
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