Spectral heterogeneity from the spaceborne imaging spectrometer EnMAP reveals biodiversity patterns in forest ecosystems
作者:Michele Torresani, Christian Rossi, Marco Mina, Irene Menegaldo, Matteo Cappuccio, Michela Perrone, Christopher R. Hakkenberg, Duccio Rocchini, Nicola Puletti, Laura Stendardi, Leonardo Montagnani, Roberto Tognetti · 发表于:International Journal of Applied Earth Observation and Geoinformation · 年份:2025 · DOI:10.1016/j.jag.2025.104902 · 被引用次数:3 · 研究领域:Remote Sensing in Agriculture、Remote-Sensing Image Classification、Remote Sensing and LiDAR Applications
The Spectral Variation Hypothesis (SVH) proposes that spectral heterogeneity (SH), derived from optical data, can serve as a proxy for estimating biodiversity. In this study, we tested the SVH across 42 forest plots in the Italian Alps using imaging spectroscopy data from the EnMAP satellite. We investigated the relationship between SH—quantified using two different metrics, Rao’s Q and the coefficient of variation (CV)—and tree species diversity (using Shannon’s H index and species richness). We applied three levels of spectral analysis: (1) SH calculated for each individual EnMAP band; (2) SH aggregated across broader spectral ranges (Visible -VIS-, Near Infrared -NIR-, and Shortwave Infrared -SWIR-) and (3) SH derived from vegetation indices (VIs). These analyses were performed under three spatial approaches: (A) a normal approach assigning equal weight to all four EnMAP pixels intersecting a plot; (B) a weighted approach based on the proportional overlap of each pixel with the plot area; and (C) a weighted canopy cover (CC) > 70% approach, which included only plots with CC greater than 70% as derived from airborne laser scanning (ALS) LiDAR data. Weak to moderate correlations were observed when SH was derived from single bands, with the strongest relationships in the NIR (R 2 approaching 0.4), followed by the VIS and SWIR regions. A similar trend emerged when SH was aggregated across broader spectral ranges, with the highest correlations again found in the NIR (R 2 up to ...