Abstract
In this chapter, we provide an introduction to spectro-polarimetric imaging. We show that the radiance transmitted through a linear polariser varies as a sinusoidal function of the polariser angle, i.e. the transmitted radiance sinusoid curves. We review different techniques to decompose polarisation images into their reflection compoents including the unpolarised intensity, the phase and the degree of linear polarisation. We then analyse the underlying physical process of polarisation upon the penetration, scattering, refraction and reflection of light from materials. Furthermore, we relate the polarisation components to the Fresnel reflection ratio resulting from specular reflection and the Fresnel transmission ratio resulting from diffuse reflection. Finally, we present a polarimetric reflection model for rough surfaces under spatially varying illumination. This model extends the specular component of the Torrance–Sparrow model to account for light polarisation upon off-specular reflection from rough surfaces. As a result, the specular polarimetric components can be expressed as functions of the perpendicular and parallel Fresnel reflection coefficients and the illuminant spectrum.
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Robles-Kelly, A., Huynh, C.P. (2013). Polarisation of Light. In: Imaging Spectroscopy for Scene Analysis. Advances in Computer Vision and Pattern Recognition. Springer, London. https://doi.org/10.1007/978-1-4471-4652-0_10
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DOI: https://doi.org/10.1007/978-1-4471-4652-0_10
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