Uncertainties in laboratory-measured shortwave refractive indices of mineral dust aerosols and derived optical properties: a theoretical assessment

IF 5.2 1区 地球科学 Q1 ENVIRONMENTAL SCIENCES Atmospheric Chemistry and Physics Pub Date : 2024-06-14 DOI:10.5194/acp-24-6911-2024
Senyi Kong, Zheng Wang, Lei Bi
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Abstract

Abstract. Mineral dust particles are nonspherical and inhomogeneous; however, they are often simplified as homogeneous spherical particles for retrieving the refractive indices from laboratory measurements of scattering and absorption coefficients. The retrieved refractive indices are then employed for computing the optical properties of spherical or nonspherical dust model particles with downstream applications. This study aims to theoretically investigate uncertainties involved in the aforementioned rationale based on numerical simulations and focuses on a wavelength range of 355–1064 nm. Initially, the optical properties of nonspherical and inhomogeneous dust aerosols are computed as baseline cases. Subsequently, the scattering and absorption coefficients of homogeneous spheres and super-spheroids are computed at various refractive indices and compared with those of inhomogeneous dust aerosols to determine the dust refractive index. To mimic the real laboratory measurement, the size distribution of the baseline case is assumed to be unknown and determined through a process akin to using optical particle counters for sizing. The resulting size distribution differs from the original one of the baseline cases. The impact of discrepancies in size distributions on retrieving the dust refractive index is also investigated. Our findings reveal that these discrepancies affect scattering and absorption coefficients, presenting challenges in accurately determining the refractive index, particularly for the real parts. Additionally, the retrieved refractive indices are noted to vary with particle size primarily due to differences in size distribution, with imaginary parts decreasing as the particle size increases. A comparison between sphere models and super-spheroid models shows that the former tend to underestimate the imaginary parts, leading to an overestimation of single-scattering albedo. This study underscores the importance of employing consistent nonspherical models for both refractive index retrieval and subsequent optical simulation in downstream applications. Nevertheless, the impact of refractive index uncertainties on the asymmetry factor and phase matrix is found to be minimal, with particle shape playing a more significant role than differences in the imaginary parts of the dust refractive index.
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实验室测量的矿物尘埃气溶胶短波折射率和衍生光学特性的不确定性:理论评估
摘要。矿物粉尘颗粒是非球形和非均质的,但通常被简化为均质球形颗粒,以便从实验室测量的散射和吸收系数中获取折射率。然后,利用检索到的折射率计算球形或非球形尘埃模型颗粒的光学特性,并将其应用于下游领域。本研究旨在基于数值模拟从理论上研究上述原理所涉及的不确定性,重点研究波长范围为 355-1064 nm。首先,计算非球形和非均质尘埃气溶胶的光学特性作为基线情况。随后,计算均质球体和超球体在不同折射率下的散射和吸收系数,并与非均质尘埃气溶胶的散射和吸收系数进行比较,以确定尘埃折射率。为了模拟真实的实验室测量,基线情况的粒度分布被假定为未知,并通过类似于使用光学粒子计数器进行粒度测量的过程来确定。由此得出的粒度分布与基线案例的原始粒度分布不同。我们还研究了粒度分布差异对灰尘折射率检索的影响。我们的研究结果表明,这些差异会影响散射和吸收系数,给准确确定折射率,尤其是实际部分的折射率带来挑战。此外,我们还注意到,主要由于粒度分布的差异,检索到的折射率随粒度的变化而变化,虚部随着粒度的增大而减小。球体模型和超球体模型的比较表明,前者往往低估虚部,导致高估单散射反照率。这项研究强调了在下游应用中采用一致的非球面模型进行折射率检索和后续光学模拟的重要性。尽管如此,研究发现折射率的不确定性对不对称系数和相位矩阵的影响微乎其微,颗粒形状比尘埃折射率虚部的差异起着更重要的作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Atmospheric Chemistry and Physics
Atmospheric Chemistry and Physics 地学-气象与大气科学
CiteScore
10.70
自引率
20.60%
发文量
702
审稿时长
6 months
期刊介绍: Atmospheric Chemistry and Physics (ACP) is a not-for-profit international scientific journal dedicated to the publication and public discussion of high-quality studies investigating the Earth''s atmosphere and the underlying chemical and physical processes. It covers the altitude range from the land and ocean surface up to the turbopause, including the troposphere, stratosphere, and mesosphere. The main subject areas comprise atmospheric modelling, field measurements, remote sensing, and laboratory studies of gases, aerosols, clouds and precipitation, isotopes, radiation, dynamics, biosphere interactions, and hydrosphere interactions. The journal scope is focused on studies with general implications for atmospheric science rather than investigations that are primarily of local or technical interest.
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