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Scattering parameterization for interpreting asteroid polarimetric and photometric phase effects

机译:散射参数化,用于解释小行星偏振和光度学的相位效应

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We derive an analytical parameterization of the amplitude and Mueller scattering matrices of a system composed of a small number of electric dipoles. The appeal of this derivation is that it provides a wide range of light-scattering polarization states with a minimal number of parameters. Such a tool can be used to interpret observations in terms of physical parameters. We aim to utilize these results in multiple-scattering studies, such as the interpretation of polarimetric and photometric phase effects of asteroids and other atmosphereless solar-system objects.
机译:我们推导了由少量电偶极子组成的系统的振幅和穆勒散射矩阵的解析参数化。该推导的吸引力在于,它以最少的参数提供了广泛的光散射偏振态。这样的工具可用于根据物理参数解释观测结果。我们旨在在多散射研究中利用这些结果,例如小行星和其他无大气层太阳系物体的偏振和光度相位效应的解释。

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