2021
DOI: 10.1016/j.carbon.2020.10.032
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The impact of organic carbon on soot light absorption

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Cited by 44 publications
(24 citation statements)
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“…LII measures the thermal emission emitted from soot particles heated by the Nd:YAG pulsed laser (usually 1064 nm) to temperatures in the range from 2500 K to 4500 K. The laser fluence is set to a value, which heats the soot particles below their sublimation threshold values (4000 K for BC) [44][45][46]. The LII is by default insensitive to liquid particles and metal salts, which vaporise during the heating, although some impact of OC coating of soot in LII response has been reported [47,48]. The size of the soot agglomerates may have an impact on the LII response, which needs to be taken into account in calibration of the LII signal to the BC concentration [49].…”
Section: Introductionmentioning
confidence: 99%
“…LII measures the thermal emission emitted from soot particles heated by the Nd:YAG pulsed laser (usually 1064 nm) to temperatures in the range from 2500 K to 4500 K. The laser fluence is set to a value, which heats the soot particles below their sublimation threshold values (4000 K for BC) [44][45][46]. The LII is by default insensitive to liquid particles and metal salts, which vaporise during the heating, although some impact of OC coating of soot in LII response has been reported [47,48]. The size of the soot agglomerates may have an impact on the LII response, which needs to be taken into account in calibration of the LII signal to the BC concentration [49].…”
Section: Introductionmentioning
confidence: 99%
“…This is due to the enhanced light scattering by the BC coating. 41 The SSA of BC agglomerates (solid line, light green-shaded area) is smaller than that of equivalent spheres (broken line, purple-shaded area) at m c /m = 1−10. This is attributed to the internal light scattering between the constituent primary particles of agglomerates that increases their light absorption (Figure S1) but reduces their external light scattering.…”
Section: Resultsmentioning
confidence: 99%
“…The MAC of bare BC spheres and agglomerates derived here at λ = 532 nm are interfaced with an absorption Angstrom exponent of 1.1 to estimate their MAC at λ = 550 nm accounting for the wavelength dependence of C-rich BC . Furthermore, the MAC c of coated BC is estimated directly from the MAC of emitted BC by a scaling law from DDA simulations: where m and m c are the mass of BC before and after coating with non-absorbing compounds, respectively.…”
Section: Methodsmentioning
confidence: 99%
“…The three sets of curves represent different assumptions about particle density in Equation 8. In particular, the curves assume the density of mature soot, nascent (young) soot, or a maturity-dependent density based on the carbon/hydrogen-ratio (C/H) and parameterized by [74]. Although the parameterization of [74] assumed 𝐸 𝑔 = 0.25 eV for mature soot, we have extrapolated down to 0 eV for illustration.…”
Section: S17mentioning
confidence: 99%
“…In particular, the curves assume the density of mature soot, nascent (young) soot, or a maturity-dependent density based on the carbon/hydrogen-ratio (C/H) and parameterized by [74]. Although the parameterization of [74] assumed 𝐸 𝑔 = 0.25 eV for mature soot, we have extrapolated down to 0 eV for illustration. This parameterization may not be applicable for all flames discussed in the main text, and it does not predict the upper range of MACs reported in the main text.…”
Section: S17mentioning
confidence: 99%