Automated Spectral Feature Detection for Mapping Ash Contamination on Western Himalayan Snow
摘要
Dark particulate matter, biomass-burning residues, and emissions from vehicular and industrial sources, such as ash, get deposited on Himalayan snow, reducing its albedo and accelerating melt, which disrupts seasonal water availability for irrigation, hydropower production, and drinking water for downstream communities. This study introduces an automated hyperspectral workflow for detecting and quantifying ash contamination on snow surfaces. Field measurements of pure and ash-contaminated snow (2.5–10 g) weights were collected using an SVC 1024i spectroradiometer across 350–2500 nm. A seven-step absorption-feature-detection algorithm identified the NIR (1034 nm), SWIR1 (1505 nm), and SWIR2 (1982 nm) water-ice absorption centres, achieving 100% validation for pure snow and mean spectral shifts of − 9.0 ± 3.1 nm (NIR, p < 0.01) and − 13.5 ± 6.2 nm (SWIR1, p < 0.05) with increasing contamination. SWIR2 responses were inconsistent (mean + 6.2 ± 25.4 nm, p > 0.05), indicating complex nonlinear effects. A data-driven band-selection routine computed wavelength-wise standard deviations, applied a 90th percentile threshold, and grouped contiguous sensitive wavelengths into three operational bands (blue-green: 350–522 nm; red-1: 657–659 nm; red-2: 664–693 nm), demonstrating superior discrimination (separability scores ≥ 3.8). The NIR band proved to be most reliable for early contamination detection. We outline future work to refine SWIR2 analysis, incorporate machine learning for adaptive banding, and apply the algorithm to PRISMA and EMIT satellite imagery over critical Western Himalayan sites (Sissu, Manali, and Koti passes). This automated, reproducible workflow is compatible with current hyperspectral missions. It provides a foundation for operational mapping of ash-induced albedo reduction, informing water resource management and hazard mitigation under climate change.