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Measurement and modeling of the multiwavelength optical properties of uncoated flame-generated soot

机译:未涂覆火焰产生烟灰多波长光学性质的测量和建模

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Optical properties of flame-generated black carbon (BC) containing soot particles were quantified at multiple wavelengths for particles produced using two different flames: a methane diffusion flame and an ethylene premixed flame. Measurements were made for (i) nascent soot particles, (ii) thermally denuded nascent particles, and (iii) particles that were coated and then thermally denuded, leading to the collapse of the initially lacy, fractal-like morphology. The measured mass absorption coefficients (MACs) depended on soot maturity and generation but were similar between flames for similar conditions. For mature soot, here corresponding to particles with volume-equivalent diameters similar to 160 nm, the MAC and absorption Angstrom exponent (AAE) values were independent of particle collapse while the single-scatter albedo increased. The MAC values for these larger particles were also size-independent. The mean MAC value at 532 nm for larger particles was 9.1 +/- 1.1m(2) g(-1), about 17% higher than that recommended by Bond and Bergstrom (2006), and the AAE was close to unity. Effective, theory-specific complex refractive index (RI) values are derived from the observations with two widely used methods: Lorenz-Mie theory and the Rayleigh-Debye-Gans (RDG) approximation. Mie theory systematically underpredicts the observed absorption cross sections at all wavelengths for larger particles (with x 0.9) independent of the complex RI used, while RDG provides good agreement. (The dimensionless size parameter x = pi d(p)/lambda, where d(p) is particle diameter and lambda is wavelength.) Importantly, this implies that the use of Mie theory within air quality and climate models, as is common, likely leads to underpredictions in the absorption by BC, with the extent of underprediction depending on the assumed BC size distribution and complex RI used. We suggest that it is more appropriate to assume a constant, size-independent (but wavelength-specific) MAC to represen
机译:含有烟灰颗粒的火焰产生的黑碳(BC)的光学性质在使用两种不同火焰中产生的颗粒的多个波长下量化:甲烷扩散火焰和乙烯预混火焰。对(i)爆炸的烟灰颗粒进行测量,(ii)热剥离的新生颗粒,(III)涂覆,然后热剥离,导致最初花边,分形形态的塌陷。测量的质量吸收系数(MAC)依赖于烟灰成熟度和生成,但在类似条件的火焰之间类似。对于成熟的烟灰,这里对应于体积当量直径和gt的颗粒。类似于160nm,MAC和吸收抗疟埃指数(AAE)值与颗粒塌陷无关,同时单散散玻璃增加。这些较大粒子的MAC值也是依赖性的。较大颗粒532nm的平均MAC值为9.1 +/- 1.1M(2 )g(2 )g(-1),比键和伯氏泡沫(2006)推荐的约17%,并且AAE接近统一。有效的,理论特异性复合折射率(RI)值源自具有两个广泛使用的方法的观察结果:Lorenz-Mie理论和瑞利 - 德by(RDG)近似。 MIE理论系统地低估了所有波长的观察到的吸收横截面,用于较大的颗粒(具有x> 0.9),与所使用的复合RI无关,而RDG则提供良好的一致性。 (无量纲尺寸参数X = PI D(P)/ Lambda,其中D(P)是粒径,Lambda是波长。)重要的是,在空气质量和气候模型中使用MIE理论,常见,可能导致BC吸收的欠低,这取决于假定的BC尺寸分布和所用复杂的RI。我们建议使用常量,大小独立(但是波长特定)MAC来代表更合适

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