Parameterization of The Single-Scattering Properties of Dust Aerosols in Radiative Flux Calculations

Abstract

In this study, we present parameterization schemes of dust single-scattering properties (SSPs) in order to establish a fast and accurate way to obtain the SSPs for dust shortwave radiative flux calculation. Based on the assumption that dust particles are spheroids, we represent a single nonspherical particle with a collection of monodisperse spheres that contain the same total surface area and volume as the original particle to convert the spheroid to a sphere. The SSPs of dust particles were parameterized in terms of the effective radius (R e ) and imaginary part of the refractive index (M i ). The averaged relative errors of the parameterized to the "exact" single-scattering properties, which refer to the results from the Mie theory program, are below 1.5%. To further quantify the impact of parametrization on the radiative flux simulation, we computed the radiative fluxes at both the top of the atmosphere (TOA) and the surface by using SSPs from the parameterization and the "exact", respectively. The maximum relative errors were below 1% at both the TOA and the surface, proving that the SSPs of dust calculated by our parameterization schemes are well suited for radiative flux calculations. This parameterization differs from previous works by being formulated not only with R e but also with M i . We also investigated the sensitivity of dust-aerosol forcing to R e , M i , optical depth (τ), and solar zenith angle (SZA). The results show that the value of shortwave (SW) radiative forcing (RF) at the TOA changes from negative to positive as the M i is increasing, which means that, as the absorption of dust particles becomes stronger, more energy is kept in the atmosphere to heat the earth-atmosphere system. The SW RF gradually becomes less negative at the TOA and more negative at the surface with increasing R e , due to the decreases of reflection and transmission along with the single-scattering albedo decreasing. As the optical depth increases, the values of the SW RF decrease because of the strong attenuation for heavy loading. When SZA increases, the SW RF becomes more negative at both the TOA and the surface due to the long optical path at a large SZA. The errors induced from the parameterized SSPs of dust in the SW RF calculation are very small, which are less than 2.1%, demonstrating the accuracy of the parameterization and its reliability for climate model applications.

Climatology of Dust‐Forced Radiative Heating Over the Tibetan Plateau and Its Surroundings

“…The enhanced detection technology of CALIPSO can not only provide more accurate profile information but also reduce the uncertainties in the DRH. While the assumption of the transported SSA and LR may introduce inevitable uncertainties in the DRH (Huang et al, 2009), the SSA may contribute more considerably to the uncertainties in the SW DRH (Dubovik et al, 2002; Wang et al, 2019). This study also evaluated the uncertainties in the estimated DRHs by introducing the ranges of SSA (±6%) and LR (±9) into the SBDART model.…”

Understanding Haze: Modeling Size-Resolved Mineral Aerosol from Satellite Remote Sensing

“…The AOD spectrum (Equation ( 4) is thus decoupled into these defined 91 spectral models (of different mineral types and particle sizes) from our mineral suite in Equation ( 6). The wavelength-dependent optical properties such as the extinction efficiency (Q ext ), single-scattering albedo, and asymmetry factor of the particle of each mineral type (from 91 models) are pre-computed and tabulated in LUT (Equation ( 4) by supplying the size parameter (2πr/λ) and complex refractive index as the input parameters through the Lorenz-Mie theory for homogeneous spheres [38][39][40]. The real and imaginary components of the complex refractive index for common dust minerals in the window (0-2200 nm) are exhibited in Appendix A.…”