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https://doi.org/10.5194/egusphere-2023-1849
https://doi.org/10.5194/egusphere-2023-1849
21 Sep 2023
 | 21 Sep 2023

The uncertainties in the laboratory-measured short-wave refractive indices of mineral dust aerosols and the derived optical properties: A theoretical assessment

Senyi Kong, Zheng Wang, and Lei Bi

Abstract. Mineral dust particles are typically 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. This study theoretically investigated uncertainties in refractive indices and corresponding optical properties resulting from this simplification at various sizes within the wavelength range of 355 to 1064 nm. Different numerical experiments were conducted under both ideal and realistic scenarios, taking into account instrumental bias in the realistic scenarios. In the numerical experiments, the inhomogeneous super-spheroid models were considered as the dust samples, while the homogeneous super-spheroid models and sphere models were used to retrieve the refractive indices. Under the ideal scenario, the look-up tables for the homogeneous super-spheroid models satisfactorily covered the measurements at any size and wavelength, while those for the sphere models failed when considering large sizes. Under the realistic scenario, both the homogeneous super-spheroid models and sphere models were ineffective for large sizes due to discrepancies in size distribution resulting from the measurements using an optical particle counter. Nevertheless, it was possible to retrieve the imaginary parts of the refractive indices based solely on the absorption coefficients. The imaginary parts obtained from the sphere models were generally consistent with those from the super-spheroid models under ideal conditions, while the former was significantly smaller than the latter under the realistic conditions. In addition, the retrieved imaginary parts were found to be size-dependent, which could be attributed to the inherent limitations of homogeneous models in characterizing inhomogeneous particles. Results showed that the uncertainties in the imaginary part and single scattering albedo should be smaller than 0.002 (0.0007) and 0.03 (0.01), respectively, under conditions of high (low) absorption. The sphere models tended to overestimate the asymmetry factor. The uncertainty in the asymmetry factor exhibited a significant variation, reaching up to 0.04 or even larger. Nonetheless, the uncertainties in the phase matrices resulting from the uncertainties in refractive indices were generally acceptable within a specific model.

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Senyi Kong, Zheng Wang, and Lei Bi

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2023-1849', Anonymous Referee #1, 25 Nov 2023
    • AC1: 'Reply on RC1', Lei Bi, 16 Mar 2024
  • RC2: 'Comment on egusphere-2023-1849', Anonymous Referee #2, 18 Dec 2023
    • AC2: 'Reply on RC2', Lei Bi, 16 Mar 2024

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2023-1849', Anonymous Referee #1, 25 Nov 2023
    • AC1: 'Reply on RC1', Lei Bi, 16 Mar 2024
  • RC2: 'Comment on egusphere-2023-1849', Anonymous Referee #2, 18 Dec 2023
    • AC2: 'Reply on RC2', Lei Bi, 16 Mar 2024
Senyi Kong, Zheng Wang, and Lei Bi
Senyi Kong, Zheng Wang, and Lei Bi

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Short summary
The retrieval of refractive indices of dust aerosols from laboratory optical measurements is commonly done assuming spherical particles. This paper aims to investigate the uncertainties in the shortwave refractive indices and corresponding optical properties by considering inhomogeneous models for dust samples. The study emphasizes the significance of using non-spherical models for simulating dust aerosols.