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Variation of Clumping Index With Zenith Angle for Forest Canopies | IEEE Journals & Magazine | IEEE Xplore

Variation of Clumping Index With Zenith Angle for Forest Canopies


Abstract:

Canopy clumping index (CI) characterizes the extent of the nonrandom spatial distribution of foliage elements within a canopy and is critical for determining the radiativ...Show More

Abstract:

Canopy clumping index (CI) characterizes the extent of the nonrandom spatial distribution of foliage elements within a canopy and is critical for determining the radiative transfer, photosynthesis, and transpiration processes in the canopy. It is widely perceived that the CI increases with zenith angle ( \theta ), because between-crown gaps decrease in size and number with increasing \theta . In this study, we demonstrate that this is not always true. Analytical equations between CI and \theta are first developed based on widely used forest canopy gap fraction (GF) theories. The results show that the zenith angular variation of CI is closely related to crown-projected area or crown shapes [i.e., the ratio of the crown height to its diameter (RHD)]: CI increases with \theta for canopies with “tower” crowns (RHD > 1), but decreases with \theta for “umbrella” crowns (RHD < 1) and does not vary much with \theta for “sphere” crowns (RHD = 1). These results are validated in a large-scale remote sensing data and image simulation framework (LESS) platform and published datasets, including the measurements in field and radiative transfer model intercomparison (RAMI) forest stands. The findings are essential for the derivation of angular-integrated (hemispherical) CI from in situ measurements and multiangular remote sensing.
Article Sequence Number: 4416311
Date of Publication: 02 December 2022

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I. Introduction

Forests generally have a high degree of natural variability and typically exhibit complex levels of organization, such as crowns, that cause their foliage to be grouped or clumped [1]. Clumping index (CI) is defined as the ratio of the effective leaf area index (LAI) to the true LAI and quantifies the degree of deviation of the leaf spatial distribution from the random case (i.e., the Poisson model) [2], [3]. CI is of great significance in terrestrial carbon and water cycle studies, as it determines radiation absorption and distribution within plant canopies. CI is closely linked to canopy gap fraction (GF) from which the ratio of sunlit LAI to shaded LAI can be calculated [2]. For a canopy with a random distribution of leaves, the relationship between canopy GF and LAI can be described with the well-known Beer–Lambert theory [4] \begin{equation*} P_{\text {Poisson}} \left ({\theta }\right)=e^{-LG\left ({\theta }\right)/\cos \theta }\tag{1}\end{equation*} where is the probability of the transmission of a beam of light at the zenith angle through the canopy, i.e., the canopy GF; is the extinction coefficient, which is 0.5 for canopies with a spherical distribution of leaf angles; and is the LAI, which is most commonly defined as one half the total (all sided) leaf area per unit ground surface area [5], [6]. As leaves often have nonrandom distributions in reality, i.e., they often aggregate in crowns in forests, CI was first introduced in the modified Beer–Lambert theory for calculating canopy GF by Nilson [4] \begin{equation*} P\left ({\theta }\right)=e^{-L\Omega G\left ({\theta }\right)/\cos \theta }\tag{2}\end{equation*} where is canopy GF. expresses the zenith angle dependence of the CI [1]. Combining (1) and (2), we can obtain [7] \begin{equation*} \Omega \left ({\theta }\right)=\frac {\log \left [{P\left ({\theta }\right)}\right]}{\log \left [{P_{\text {Poisson}} \left ({\theta }\right)}\right]}.\tag{3}\end{equation*}

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