Reflection of visible light from a dense vegetation canopy—a physical model

Abstract Monitoring vegetation condition by remote sensing is made difficult by the variation of canopy brightness (radiance) with view direction and sun position. In this paper, we develop a physical model of canopy radiance that models this variation as a product of three functions, each being expressed as a simple analytical formula. The first function, the S function, represents the proportion of canopy seen as sunlit, excluding the hotspot. The second function, the hotspot function, corrects the S function for the higher probability of seeing sunlit leaves near the anti-solar point. The third function represents the average radiance of sunlit leaves. The model was fitted to densely-sampled, multi-view radiance measurements of pine forest ( Pinus radiata ) and pasture ( Lolium spp.), taken at a large (⋍ 60°) sun zenith angle. Radiance predictions for multiple views were then made for a small sun zenith angle (⋍ 20°). Comparison of predicted with measured radiances showed that the model out-performed the linear Roujean et al. model ( J. Geo. Res. , 97: 20,455–20,468) and the non-linear Verstraete et al. model ( J. Geo. Res. , 95: 11,755–11,765). The improvement is due to two factors: The hotspot function has a sun zenith angle dependence; and the S function allows the average projected leaf area to vary with off-nadir view angle.

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