The hemispherical harmonic method for radiative transfer in plane-parallel atmospheres. (August 2021)

• Record Type: Journal Article
• Authors: Wang, Biao
• Is Part Of: Journal of quantitative spectroscopy & radiative transfer. Volume 270(2021)
• Publication Date: 2021-08
• Subjects: Radiative transfer -- Hemispherical harmonic method -- Radiative model; Spectrum analysis -- Periodicals; Radiation -- Periodicals; Analyse spectrale -- Périodiques; Rayonnement -- Périodiques; Radiation; Spectrum analysis; Periodicals; 543.0858
• DOI: 10.1016/j.jqsrt.2021.107702
• Languages: English
• ISSNs: 0022-4073

Abstract

Highlights: A new method for radiative transfer in plane-parallel atmospheres is introduced and a prototype model is developed. The numerical results of radiance and irradiance are obtained by the model and compared with benchmark results. The method has good accuracy, efficiency, and flexibility to be a useful tool in the modeling studies on the earth system. Abstract: A new approach - Hemispherical Harmonic Method (HSHM) is proposed for radiative transfer in plane-parallel atmospheres and a prototype model is developed. The algorithm is derived from the unified formulation with the shifted Legendre polynomials prescribed as the basis functions decomposing the Fourier components of radiance and the radiative transfer equation. The solutions to the decomposed equations for homogenous layers and the inhomogeneous atmosphere-surface system are derived and numerically implemented. The primary numerical experiments show the prototype model gives accurate results when the order is sufficiently high, and has reasonable accuracy and efficiency relative to its discrete ordinate method (DOM) counterpart does with the same orders, including the numbers of the basis functions, the Fourier components, and the expansion terms of the scattering phase function. The HSHM model allows more flexible settings to further improve the accuracy and/or the efficiency. The method is inherently immune to the singularity problems suffered by the DOM for the special solar zenith angles. While further refinement is to be done, the HSHM provides another option for the modeling and remote sensing studies involving radiance and irradiance in planetary atmospheres with radiative absorption, scattering, and emission.