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Perturbations of the optical properties of mineral dust particles by mixing with black carbon: a numerical simulation study

机译:用黑碳混合使用矿物粉尘颗粒的光学性质的扰动:数值模拟研究

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Field observations show that individual aerosol particles are a complex mixture of a wide variety of species, reflecting different sources and physico-chemical transformations. The impacts of individual aerosol morphology and mixing characteristics on the Earth system are not yet fully understood. Here we present a sensitivity study on climate-relevant aerosols optical properties to various approximations. Based on aerosol samples collected in various geographical locations, we have observationally constrained size, morphology and mixing, and accordingly simulated, using the discrete dipole approximation model (DDSCAT), optical properties of three aerosols types: (1) bare black carbon (BC) aggregates, (2) bare mineral dust, and (3) an internal mixture of a BC aggregate laying on top of a mineral dust particle, also referred to as polluted dust. DDSCAT predicts optical properties and their spectral dependence consistently with observations for all the studied cases. Predicted values of mass absorption, scattering and extinction coefficients (MAC, MSC, MEC) for bare BC show a weak dependence on the BC aggregate size, while the asymmetry parameter (g) shows the opposite behavior. The simulated optical properties of bare mineral dust present a large variability depending on the modeled dust shape, confirming the limited range of applicability of spheroids over different types and size of mineral dust aerosols, in agreement with previous modeling studies. The polluted dust cases show a strong decrease in MAC values with the increase in dust particle size (for the same BC size) and an increase of the single scattering albedo (SSA). Furthermore, particles with a radius between 180 and 300 nm are characterized by a decrease in SSA values compared to bare dust, in agreement with field observations. This paper demonstrates that observationally constrained DDSCAT simulations allow one to better understand the variability of the measured aerosol optical properties in ambient air and to define benchmark biases due to different approximations in aerosol parametrization.
机译:现场观察表明,各种气溶胶颗粒是各种物种的复杂混合物,反映不同来源和物理化学转化。单个气溶胶形态和混合特性对地球系统的影响尚未完全理解。在这里,我们对各种近似的气候相关气溶胶光学性质提出了一种敏感性研究。基于各种地理位置收集的气溶胶样品,我们具有观察到的大小,形态和混合,并因此使用离散偶极逼近模型(DDSCAT),三种气溶胶类型的光学性质,如下:(1)裸黑碳(BC)聚集体,(2)裸矿物粉尘,(3)铺设在矿物粉尘颗粒的顶部的BC骨料的内部混合物,也称为污染的粉尘。 DDSCAT通过对所有研究案例的观察结果预测光学性质及其光谱依赖性。裸BC的质量吸收,散射和消光系数(MAC,MSC,MEC)的预测值显示对BC骨料大小的弱依赖性,而不对称参数(G)表示相反的行为。裸矿物粉尘的模拟光学性质取决于模拟的灰尘形状,呈现出大的灰尘形状,确认球体在不同类型和矿物粉尘气溶胶的不同类型和大小的结构上的适用性,同意以前的建模研究。污染的粉尘案件显示MAC值的强烈降低随着灰尘粒度的增加(相同的BC尺寸)和单次散射Albedo(SSA)的增加。此外,在与裸露灰尘相比,具有180和300nm之间的半径之间的颗粒的特征在于与裸露的灰尘相比,与现场观测相比。本文表明,观测到受约束的DDSCAT模拟允许更好地理解环境空气中测量的气溶胶光学性质的可变性,并由于气溶胶参数化的不同近似而定义基准偏差。

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