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A hybrid mode of diffuse and specular reflector for computation of the emergent radiation by the adding method

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Abstract

A method of computing the diffuse reflection and transmission radiation from an inhomogenous, plane-parallel planetary atmosphere bounded by the hybrid surface of a diffuse and specular reflector is discussed by using the ‘addition’ method. If the atmosphere is simulated by a number of homogeneous sublayers, the radiation diffusely reflected and transmitted by the atmosphere can be expressed in terms of the diffuse reflection and transmission matrices of radiation of sublayers (Laciset al., 1974; Takashima, 1973, 1975). With this method (Takashima, 1975), the troublesome treatment due to the effect of polarity of radiation is overcome. Moreover, if the surface reflects radiation in accordance with the Lambert law as well as a quite arbitrary phase matrix (Takashima, 1974), the addition method can be easily extended. It is shown in this paper that the addition method is suitable for numerical computation even if the surface reflects light according to the hybrid mode of the diffuse and specular law (Uenoet al., 1974; Mukai, 1976).

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On leave from the Meterological Research Institute, Tokyo, Japan.

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Takashima, T., Taggart, C.I. & Morrissey, E.G. A hybrid mode of diffuse and specular reflector for computation of the emergent radiation by the adding method. Astrophys Space Sci 40, 157–165 (1976). https://doi.org/10.1007/BF00651196

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