1. Introduction
Plant secondary metabolites are not directly involved in primary growth or production but are essential to long-term fitness [
1,
2,
3]. Phenolic compounds are one important subcategory of secondary metabolites, including flavonoids, tannins, and lignin precursors [
4,
5]. They are fundamental to plant survival and ecological interactions, serving as chemical defense against herbivores and pathogens, mediating responses to environmental stress, affecting litter decomposition and nutrient cycling, and shaping soil microbial communities and plant–soil feedback [
6,
7,
8,
9,
10]. The concentration of foliar phenolics is affected by genetic factors, plant growth stages, and environmental conditions [
11,
12,
13]; therefore, accurately monitoring spatial and temporal variation in foliar phenolic concentrations is crucial for understanding their roles in plant physiology and ecosystem processes.
Spectroscopy provides continuous and narrowband spectral information and offers an efficient non-destructive approach for estimating foliar chemicals by detecting their absorption features [
14,
15,
16]. This approach overcomes the spatial and temporal limitations of conventional field surveys and chemical analysis [
16,
17,
18]. The ability of spectroscopy to predict leaf phenolics arises from characteristic absorption features associated with phenolic chemical bonds, particularly in the shortwave infrared region [
14,
19,
20,
21,
22]. Previous studies have identified informative wavelength regions near 1120, 1450, 1650–1670, 1720, 1870, 1930, 2140, 2170, and 2260 nm, including a prominent absorption feature around 1660 nm attributed to the first overtone of C–H stretching in aromatic rings [
23,
24]. Compared to primary chemicals such as leaf chlorophyll, protein, and cellulose, relatively few studies have focused on predicting foliar phenolics at leaf [
23,
24,
25,
26,
27] and canopy levels [
16,
17,
18,
28,
29,
30].
Airborne imaging spectroscopy, characterized by high spectral resolution and strong signal-to-noise ratios, can resolve subtle absorption features of phenolic compounds and generate accurate, high-resolution maps of foliar phenolics at local to landscape scales [
16,
17,
28]. However, airborne acquisitions are associated with high operational costs and limited spatial coverage compared with satellite missions such as the Italian Precursore Iperspettrale della Missione Applicativa (PRISMA) and Environmental Mapping and Analysis Program (EnMAP) [
31,
32]. Moreover, conducting field sampling that matches the coarse spatial resolution of satellite pixels (often ~30 m) remains challenging in forests with diverse species composition [
17,
33,
34]. Therefore, approaches that preserve biochemical information from airborne imaging spectroscopy while extending predictions to broader spatial scales are increasingly important. High-resolution phenolic maps (often at ~1 m) derived from airborne imaging spectroscopy can provide an effective bridge between field observations and satellite imagery and serve as training data for large-scale applications. Previous studies have demonstrated the feasibility of combining airborne and spaceborne spectroscopy to estimate canopy phenolics [
29].
Current hyperspectral satellite missions remain constrained by relatively narrow swath widths and long revisit times, limiting their ability to achieve global monitoring. Sentinel-2 multispectral imagery provides systematic, frequent, and freely available observations across terrestrial ecosystems and has demonstrated strong capability for vegetation monitoring, including plant diversity and trait estimation over large scales [
33,
34,
35]. A promising strategy for large-scale foliar phenolic mapping is therefore to combine the spectral fidelity of airborne imaging spectroscopy with the extensive spatial and temporal coverage of Sentinel-2 observations. Airborne imaging spectroscopy can provide high-quality training information for phenolic retrieval, while Sentinel-2 enables broader spatial extrapolation. In parallel, empirical machine learning-based modeling approaches have become the dominant framework for estimating foliar chemicals because weak phenolic absorption features are not explicitly represented in radiative transfer models such as PROSPECT [
36,
37]. Partial least squares regression (PLSR) [
24,
38,
39], random forest regression (RFR) [
40,
41], and Gaussian process regression (GPR) [
24,
40,
42,
43] have each shown strong performance for vegetation trait retrieval and provide complementary advantages in handling spectral information and prediction uncertainty.
Despite these advances, several challenges remain for transferring foliar phenolic estimation from airborne imaging spectroscopy to operational satellite monitoring. Existing studies have primarily relied on hyperspectral observations with limited spatial coverage or have focused on relatively homogeneous forest systems, leaving the generalizability of phenolic retrieval approaches across diverse vegetation types insufficiently evaluated. In addition, differences in spectral resolution and spatial support between airborne imaging spectroscopy and Sentinel-2 observations may introduce uncertainty during model transfer and spatial aggregation. The relative effectiveness of different machine learning-based modeling approaches for addressing these challenges also remains unclear. Consequently, it is uncertain whether airborne imaging spectroscopy can serve as a robust intermediate scale for transferring foliar phenolic information to Sentinel-2 and enabling broad-scale monitoring.
Therefore, this study aims to evaluate the feasibility of scaling foliar phenolic estimation from airborne imaging spectroscopy to Sentinel-2 observations across diverse vegetation types. Specifically, the objectives are: (1) to evaluate whether Sentinel-2 multispectral imagery can accurately predict foliar phenolics; (2) to determine the optimal spatial aggregation window for matching airborne imaging spectroscopy and Sentinel-2 observations; and (3) to compare partial least squares regression, random forest regression, and Gaussian process regression for foliar phenolic prediction using Sentinel-2 data.
2. Materials and Methods
2.1. Study Area and Field Sampling
Field sampling was conducted during the 2016–2017 growing seasons following National Ecological Observatory Network (NEON) vegetation sampling protocols. The field campaigns at each site were conducted within two weeks of the corresponding NEON-AOP overflights, ensuring temporal consistency between field measurements and airborne observations (
Figure 1A) [
16]. These sites span a broad climatic gradient across the eastern United States, encompassing humid continental, humid subtropical, and temperate grassland environments. Mean annual temperature across the sampled sites ranges from 4.3 to 17.2 °C, while mean annual precipitation ranges from 457 to 1383 mm, reflecting substantial variability in climatic conditions among the study locations.
In total, 634 sampling plots (~5 × 5 m
2) were established to collect foliar samples from seven NEON ecological domains (D02, D03, D05, D06, D07, D08, and D09). The geographic coordinates of each sampling plot were precisely recorded using a differential global positioning system (GPS) (Trimble Geo 7X; Trimble Inc., Sunnyvale, CA, USA) to ensure accurate spatial alignment between field measurements and NEON imaging spectroscopy observations. The sampling plots represented six plant functional types (PFTs), including broadleaf trees (
n = 432), conifers (
n = 74), shrubs (
n = 33), grasses (
n = 61), forbs (
n = 25), and crops (
n = 9). The sampling sites encompassed a wide range of ecosystems, including eastern deciduous forests (SERC), northern mixed hardwood–conifer forests (CHEQ, STEI, and UNDE), tallgrass prairie and old-field grasslands (KONZ and UKFS), southeastern mixed pine–hardwood forests (TALL), and northern mixed-grass prairie with wetlands and agricultural vegetation (NOGP). This diversity of vegetation communities provided a broad range of canopy structures and foliar phenolic characteristics for model development. A complete list of the plant species sampled at each NEON site is provided in
Supplementary Table S1.
Leaf sampling was conducted following NEON vegetation sampling protocols to obtain representative foliar trait measurements [
16]. For each plot, sunlit and healthy leaves were collected from representative vegetation individuals, with multiple samples collected when necessary to account for within-plot variability. Sampling strategies were adjusted according to vegetation structure and growth form, including species-level sampling for woody vegetation and representative community sampling for herbaceous and mixed-species plots. Then, leaves were oven-dried at 65 °C for at least 48 h and subsequently analyzed for total phenolics concentration following the established protocol [
44]. Finally, community-weighted mean (CWM) phenolic concentrations were calculated by aggregating species-level phenolic values according to species composition and relative abundance within each plot [
16]. Since broadleaf tree plots were mainly occupied by one species, the CWM was typically represented by the dominant canopy species. In conifer plots, species-level phenolic concentrations were weighted according to the relative proportions of different needle age classes visually identified for each sampling branch. For shrub, grass, and forb communities, species-level phenolic concentrations were combined using species fractional cover within each plot. The resulting plot-level CWM phenolic concentrations were then paired with canopy reflectance extracted from the corresponding NEON-AOP imagery for model development.
2.2. NEON Airborne Observation Platform Imaging Spectroscopy Data
Airborne imaging spectroscopy data were obtained from the NEON Airborne Observation Platform (AOP) for the corresponding sampling plots. The AOP imaging spectrometer collects hyperspectral radiance data across 426 spectral bands spanning 380–2520 nm, with approximately 5 nm spectral resolution and 1 m spatial resolution. The data were radiometrically calibrated, atmospherically corrected, and ortho-rectified to generate surface reflectance products [
45]. Wavelength regions strongly affected by atmospheric absorption and low signal-to-noise ratios (381–412, 1338–1454, 1784–1980, and 2400–2511 nm) were excluded. A Savitzky–Golay filter with a window size of 7 bands was applied to smooth spectral data within the VNIR (415–1335 nm) and SWIR (1460–1780 nm and 1990–2350 nm) wavelength regions separately. To minimize the differences in brightness, NEON spectra were vector-normalized to unit vectors [
46]. The surface reflectance imagery covering the field sampling plots was extracted for foliar phenolics estimation using GPS data. Vegetation pixels within each plot were averaged to obtain representative spectral signatures, which were subsequently used for foliar phenolics modeling (
Section 2.4). All spatial datasets, including NEON AOP imagery, Sentinel-2 imagery, and field plot locations, were processed in the Universal Transverse Mercator (UTM) coordinate reference system using the corresponding UTM zone for each study site to ensure consistent spatial alignment during data processing and analysis.
To facilitate upscaling of fine-resolution foliar phenolics estimates to Sentinel-2 observations, additional NEON AOP flightlines during 2017 were selected based on their spatial overlap with Sentinel-2 tiles and the availability of temporally matched Sentinel-2 acquisitions (
Figure 1B;
Table S2). In total, seven Sentinel-2 tiles covering corresponding NEON sites across five ecological domains (D02, D05, D06, D08, and D09) were included. These tiles corresponded to NEON sites including KONZ (Site full name: Konza Prairie Biological Station; NEON domain ID: D06; Sentinel tile ID: T14SQJ), NOGP (Northern Great Plains Research Station; D09; T14TLS), UKFS (University of Kansas Field Station; D06; T15SUD), CHEQ (Chequamegon Ecosystem-Atmosphere Study Site) and STEI (Steigerwaldt-Chequamegon Experimental Forest; D05; T15TYL), UNDE (University of Notre Dame Environmental Research Center; D05; T15TYM), TALL (Talladega National Forest; D08; T16SDB), and SERC (Smithsonian Environmental Research Center; D02; T18SUJ). The selected Sentinel-2 tiles contained 17–37 available AOP flightlines, which provided multiple airborne observations for generating fine-resolution foliar phenolics estimates. These 1 m resolution phenolics maps were subsequently used to extract ROI (Regions-Of-Interest)-level mean phenolic concentrations across multiple window sizes for evaluating cross-scale transferability (
Section 2.5). Instead of mosaicking overlapping flightlines, each flightline was processed independently to extract ROI-level mean phenolics.
2.3. Sentinel-2 Multispectral Data
Sentinel-2 multispectral imagery was acquired from the Copernicus Sentinel-2 mission to support the upscaling of fine-resolution foliar phenolics estimates from NEON AOP observations to satellite spatial resolution (
Figure 1B). Level-2A surface reflectance products were obtained for seven Sentinel-2 tiles (T14SQJ, T14TLS, T15SUD, T15TYL, T15TYM, T16SDB, and T18SUJ) corresponding to the NEON sites used in this study. The selected Sentinel-2 observations were acquired between May and September 2017 and were selected to closely match the available NEON-AOP acquisitions. The temporal differences between paired NEON-AOP and Sentinel-2 observations ranged from −6 to +10 days (
Table S2), reducing potential discrepancies associated with short-term phenological changes.
The Level-2A products provide atmospherically corrected surface reflectance measurements across the visible, red-edge, near-infrared (NIR), and shortwave infrared (SWIR) regions. Nine Sentinel-2 spectral bands were used in this study, including the visible bands (B02, B03, and B04), red-edge bands (B05, B06, and B07), NIR band (B8A), and SWIR bands (B11 and B12), covering wavelengths from 490 to 2190 nm. The original 20 m resolution bands (B05, B06, B07, B8A, B11, and B12) were resampled to 10 m to match the spatial resolution of the native 10 m bands (B02–B04). Cloud-contaminated pixels were removed using the Sentinel-2 cloud probability (CLD) product to ensure that only clear-sky observations were retained for subsequent analysis.
2.4. Foliar Phenolics Modeling Using NEON Imaging Spectroscopy
Foliar phenolics were modeled by linking NEON imaging spectroscopy data (
Section 2.2) with laboratory-measured foliar phenolic concentrations (
Section 2.1). The dataset was divided into calibration (75%) and validation (25%) subsets using stratified sampling based on PFTs to ensure that all vegetation functional groups were represented in both datasets. Two complementary regression approaches were evaluated to characterize potential linear and nonlinear relationships between canopy reflectance and foliar phenolics, including partial least squares regression (PLSR) and Gaussian process regression (GPR).
PLSR was implemented as a linear modeling approach that reduces spectral dimensionality by transforming correlated reflectance variables into a set of latent components. The optimal number of latent components was determined using repeated cross-validation (4 folds; 25 repeats) on the calibration dataset. GPR was implemented as a nonlinear regression approach, with model calibration performed using the same repeated cross-validation strategy and a radial basis function kernel to capture nonlinear relationships between spectral reflectance and foliar phenolic concentrations. To account for variability associated with model calibration, 100 models were generated from the repeated cross-validation procedure. Predictions were obtained as the ensemble mean of the 100 models, and the standard deviation among model predictions was used to quantify prediction uncertainty. Both PLSR and GPR models were independently evaluated using the same validation dataset, and model performance was assessed using the coefficient of determination (R2), root mean square error (RMSE, in mg·g−1), and normalized root mean square error (NRMSE = RMSE/(Max − Min) × 100%, in %).
To identify spectral regions associated with foliar phenolics, wavelength importance was evaluated for both PLSR and GPR models. For PLSR, standardized regression coefficients from the repeated cross-validation models were extracted, and the mean coefficient value across all models was calculated for each wavelength. The magnitude and sign of the coefficients were used to characterize the contribution and direction of spectral bands to phenolics prediction. For GPR, wavelength importance was quantified based on the automatic relevance determination (ARD) length scales derived from the radial basis function kernel. The inverse length scale was calculated, with larger values indicating greater sensitivity of the model to specific wavelengths. Known vegetation biochemical absorption regions were additionally indicated to facilitate interpretation of model-identified spectral features in relation to reported foliar chemical absorption characteristics [
24].
2.5. Foliar Phenolics Modeling Using Sentinel-2 Multispectral Data
2.5.1. Generation of AOP-Derived Phenolics Reference Data
The optimized NEON hyperspectral phenolics models (
Section 2.4) were first applied to available NEON Airborne Observation Platform (AOP) flightlines (
Section 2.2 and
Figure 1B) to generate spatially continuous foliar phenolics estimates at 1 m spatial resolution. These AOP-derived phenolics maps provided fine-resolution trait information within Sentinel-2 coverage areas and served as reference data for satellite-scale upscaling.
To address potential spatial misalignment between NEON AOP-derived phenolics estimates and Sentinel-2 observations, multiple spatial aggregation windows were evaluated. Although AOP imagery provides fine-resolution (1 m) phenolics estimates, direct pixel-to-pixel matching with Sentinel-2 imagery is challenging because of differences in spatial resolution, geolocation accuracy, and sensor acquisition geometry. Therefore, square regions of interest (ROIs) with four window sizes (10, 20, 60, and 100 NEON AOP pixels) were generated around the same center locations for each NEON AOP flightline. These window sizes were selected to evaluate the effects of increasing aggregation scale on cross-sensor phenolics estimation. The 10 m and 20 m windows represented aggregation levels close to the native spatial resolutions of Sentinel-2 observations, while the 60 m and 100 m windows evaluated broader aggregation scales where canopy heterogeneity, geolocation mismatch, and differences between airborne and satellite observations were expected to be reduced. The 100 m window further represented a landscape-level aggregation scale commonly used in ecosystem remote sensing and trait mapping studies.
To ensure reliable aggregation of AOP-derived phenolics estimates, each ROI was required to contain more than 80% valid vegetation pixels, where valid pixels were defined as pixels with NDVI > 0.6 and valid phenolics predictions. In addition, ROIs were spatially separated to minimize the influence of spatial autocorrelation among samples. Specifically, the centers of the 100 × 100-pixel windows were required to be separated by more than 1.5 km. These criteria ensured that extracted ROI samples represented independent spatial observations while maintaining sufficient vegetation coverage. For each ROI, the mean AOP-derived phenolics concentration was calculated and used as the reference value for corresponding Sentinel-2 observations.
2.5.2. Sentinel-2 Spectral Feature Construction
Sentinel-2 spectral features were constructed from atmospherically corrected surface reflectance data to capture spectral information related to foliar phenolics. Three categories of predictors were generated, including: (1) raw spectral reflectance; (2) published vegetation indices; and (3) normalized difference spectral indices (NDSIs) (
Table 1).
Raw spectral reflectance features consisted of nine Sentinel-2 bands, including visible bands (B02, B03, and B04), red-edge bands (B05, B06, and B07), near-infrared band (B8A), and shortwave infrared bands (B11 and B12). These bands were retained because visible, red-edge, and near-infrared regions are sensitive to vegetation pigment and canopy structural properties, whereas shortwave infrared regions provide information related to vegetation water content and dry matter constituents [
14].
Published vegetation indices were calculated to enhance vegetation-related signals and summarize specific canopy properties. A total of 13 vegetation indices were generated, including indices related to vegetation greenness (e.g., NDVI and EVI), chlorophyll status (e.g., CI
green, CIred-edge, and MTCI), pigment variation (e.g., ARI and SIPI), and water status (e.g., NDMI). The formulas and corresponding Sentinel-2 bands used for each index are provided in
Table 1.
In addition, normalized difference spectral indices (NDSIs) were generated to capture pairwise spectral relationships among Sentinel-2 bands. For each possible band pair, NDSI values were calculated as:
where
and
represent Sentinel-2 surface reflectance values at spectral bands i and j, respectively. These band combinations provide additional information on spectral contrasts that may be associated with foliar biochemical variation. Six NDSI combinations corresponding to commonly used normalized difference vegetation indices (NDVI, NDRE, NDRE1, NDRE2, MTCI, and NDMI in
Table 1) were excluded to avoid exact duplication with published vegetation indices. Therefore, 30 independent NDSI features were retained. The final Sentinel-2 predictor dataset consisted of nine reflectance bands, 13 vegetation indices, and 30 NDSI features.
2.5.3. Sentinel-2 Phenolics Modeling and Validation
The ROI datasets were randomly divided into calibration (75%) and validation (25%) subsets. Model development was conducted independently for each ROI size (10, 20, 60, and 100 pixels) to evaluate the influence of spatial aggregation on Sentinel-2-based phenolics estimation.
Three modeling approaches were evaluated, including partial least squares regression (PLSR), Gaussian process regression (GPR), and random forest (RF) regression. PLSR was used to characterize linear relationships between Sentinel-2 spectral features and foliar phenolics concentrations, whereas GPR and RF were used to capture potential nonlinear relationships. For PLSR and GPR, model calibration was performed using repeated cross-validation (4 folds; 25 repeats). In PLSR, the optimal number of latent components was selected based on cross-validation performance, while GPR employed a radial basis function kernel to model nonlinear spectral–trait relationships. RF models were implemented as ensemble regression trees using bootstrap aggregation.
Model performance was evaluated on the independent validation dataset using R2, RMSE (mg·g−1), and NRMSE (%). Model performance was compared across ROI sizes and modeling approaches to identify the optimal configuration for Sentinel-2-based phenolics estimation.
Following model evaluation, the best-performing model developed from the 100-pixel ROI dataset was selected for regional phenolics mapping. The selected model was applied to Sentinel-2 Level-2A imagery using the same set of spectral features used during model training, generating spatially continuous estimates of foliar phenolics across the study regions.
All data processing, statistical analyses, and model development were implemented in Python 3.12.2. Numerical computations and data management were performed using NumPy (v1.26.4), pandas (v2.2.2), and SciPy (v1.17.1). Geospatial processing was conducted using rasterio (v1.4.3), GDAL (v3.6.2), GeoPandas (v1.0.1), Shapely (v2.1.2), and pyproj (v3.6.1). Partial least squares regression (PLSR) and random forest regression (RFR) were implemented using scikit-learn (v1.5.1), while Gaussian process regression (GPR) was implemented using GPy (v1.13.2). Figures were generated using Matplotlib (v3.8.4).
4. Discussion
This study evaluated the feasibility of scaling foliar phenolics from airborne imaging spectroscopy to Sentinel-2 multispectral imagery across diverse vegetation types. Using the full spectral information from the airborne platform, both Partial Least Squares Regression (PLSR) and Gaussian Processes Regression (GPR) accurately predicted foliar phenolics and successfully distinguished the characteristic absorption features of these compounds. The resulting fine-resolution airborne phenolic maps served as a high-quality training dataset for upscaling to broader spatial extents with Sentinel-2. An optimal window size of 100 m was identified for matching the airborne-derived phenolic maps to Sentinel-2 pixels, effectively reducing geolocation mismatches between the two sensors. The foliar phenolic maps generated from the hyperspectral airborne data and the upscaled Sentinel-2 multispectral imagery showed strong spatial consistency across heterogeneous landscapes.
4.1. Accurate Prediction of Foliar Phenolics Across Vegetation Types Using Airborne Imaging Spectroscopy
Imaging spectroscopy demonstrated the ability to capture the variation in foliar phenolics from leaf to canopy levels [
17,
23,
24,
28,
47]. Our findings further confirmed the feasibility of airborne imaging spectroscopy for accurately predicting foliar phenolics across a wide range of vegetation types including trees, shrubs and graminoids. The estimation accuracies achieved in this study were comparable to or higher than those reported in previous studies [
16,
17,
18,
29]. We found that the widely used PLSR, which captured linear relationships between foliar phenolics and canopy spectra, achieved similarly good performance with GPR, which could model the non-linear relationships. This finding is consistent with a previous study on predicting multiple foliar traits in grasslands [
42], as well as a study on predicting foliar phenolics using leaf spectroscopy [
24]. However, it contrasted with another study on canopy-level phenolic prediction using airborne and spaceborne imaging spectroscopy, in which GPR outperformed PLSR [
29]. Careful hyperparameter optimization is critical for machine learning algorithms like GPR to achieve satisfactory estimation accuracy [
43]. In our study, the prediction uncertainties associated with GPR were generally higher than those of PLSR. However, GPR offers the intrinsic advantage of providing per-pixel uncertainty estimates directly alongside predicted values, whereas PLSR must rely on a permutational approach to approximate prediction uncertainties [
18,
42]. Both uncertainty quantification methods are important for trait mapping, as they supply the confidence information necessary to inform and constrain subsequent trait-based analyses [
16].
The underlying mechanism of predicting foliar phenolics from spectra lies in their distinct absorption features, located at approximately 1200, 1450, 1460, 1641, 1650, 1658, 1660, 1670, 1720, 2140, 2170, and 2260 nm [
14,
19,
20,
21,
22]. Among these, the absorption feature centered near 1660 nm is particularly diagnostic, as it corresponds to the first overtone of aromatic C–H bond stretching—a fundamental structural signature of phenolic compounds [
23]. Our results revealed that this prominent absorption feature was adequately captured by both models, as evidenced by the band importance metrics derived from each. In addition to the 1660 nm feature, PLSR also captured absorption features at 1200, 1450, 1460, 1720, and 2260 nm, whereas GPR captured a more limited set of additional features, notably those at 2140 and 2260 nm. Xie et al. [
24] reported that the center wavelength of the key phenolic absorption feature may shift between 1653 and 1667 nm depending on factors such as plant species and environmental conditions. Consistent with this finding, our models identified the entire spectral region between 1650 and 1670 nm as important for predicting foliar phenolics, encompassing the range of variation expected across the diverse vegetation types, plant species, and broad geographic conditions represented in our study.
4.2. Airborne Imaging Spectroscopy as a Bridge for Scaling Foliar Phenolics to Sentinel-2
The highly accurate estimation of foliar phenolics from airborne imaging spectroscopy provided a robust foundation for scaling predictions to Sentinel-2 imagery. However, bridging the gap between field measurements and satellite observations remains challenging due to the coarse spatial resolution of satellite pixels and the inherent spatial mismatch with ground-based surveys. Previous studies have highlighted the difficulties in directly linking field measurements to airborne or satellite data [
17,
33]. Moreover, the requirement for both leaf traits and species abundance to compute community-weighted means adds another layer of complexity to the spectral matching process, especially in species-rich plots where taxonomic and functional diversity are high. In this study, we employed a 5 × 5 m field plot design specifically aligned with the 1 m spatial resolution of the airborne imagery, resulting in a fine-resolution phenolic map that served as a high-quality training dataset for upscaling to Sentinel-2. Among the three empirical approaches evaluated, RFR achieved the highest prediction accuracy for foliar phenolics, followed by GPR, while PLSR yielded comparatively lower accuracies. This outcome likely reflects the ability of RFR and GPR to capture the non-linear relationships between foliar phenolics and canopy spectra, which PLSR, as a linear method, may not fully represent [
29,
43].
Furthermore, the spatial mismatch inherent between the two data types significantly influenced model performance, as evidenced by the effect of varying the aggregation window size. A window size of 10 m—corresponding to the finest spatial resolution of Sentinel-2 imagery—yielded only moderately accurate predictions, underscoring the geolocation discrepancies between the airborne-derived phenolic maps and Sentinel-2 pixels. As the window size increased, these spatial mismatches were progressively alleviated, leading to corresponding improvements in estimation accuracy. The optimal aggregation window was found to be 100 m, a scale that effectively minimized spatial misalignment between the two datasets while preserving the spectral absorption features of foliar phenolics necessary for accurate retrieval.
The estimation accuracies of foliar phenolics derived from Sentinel-2 were comparable to those reported in previous studies and notably higher than those from a prior effort that utilized time series Sentinel-2 data for upscaling [
48]. This improvement is largely attributable to the near-simultaneous acquisition of airborne and satellite imagery, which minimized temporal mismatch. By reducing the reliance on multi-temporal data, our approach is more readily transferable to other regions. We note, however, that inter- and intra-annual variation in foliar phenolics and canopy spectra can affect model performance, and the use of single-date imagery may not fully capture such dynamics [
18]. The most informative spectral features were the Normalized Difference Spectral Indices (NDSI) based on the green and red-edge bands, together with the SWIR2 band. The SWIR2 band likely captures part of the phenolic absorption near 2260 nm, while the contributions from green and red-edge bands point to indirect correlations between foliar phenolics and co-varying traits such as chlorophyll and nitrogen.
Landscape-scale application of the models revealed broadly consistent spatial patterns in foliar phenolics between the airborne and Sentinel-2 maps across diverse sites. However, the fine spatial detail visible in the high-resolution airborne maps was inevitably obscured in the coarser Sentinel-2 maps, especially in areas with extreme high or low values. This is an inherent trade-off in spaceborne remote sensing between spatial and spectral resolution. The new generation of satellite imaging spectrometers—such as EnMAP, PRISMA, Gaofen-5, DESIS, and the forthcoming SBG mission—typically operate at 30 m or 60 m spatial resolutions. We expect that their enhanced spectral resolution will help offset the coarser spatial detail by better resolving the characteristic phenolic absorption features. Nevertheless, none of the current operational hyperspectral missions are designed for full global coverage. In this context, Sentinel-2 retains a distinct advantage for mapping foliar phenolics across large areas, offering both systematic global coverage and short revisit times.
Beyond demonstrating the feasibility of cross-scale phenolic mapping, the proposed framework has several potential practical applications. Spatially explicit estimates of foliar phenolic concentrations can facilitate monitoring of plant defense strategies, vegetation responses to environmental stress, and ecosystem functioning across large spatial extents [
1,
2,
3,
4]. Because foliar phenolics are closely associated with herbivory resistance, nutrient cycling, and carbon dynamics, regional phenolic maps may also support biodiversity assessments, ecological monitoring, and conservation planning. Furthermore, the integration of airborne imaging spectroscopy with freely available Sentinel-2 observations provides a scalable framework that can be readily updated as new airborne and satellite observations become available.
4.3. Limitations and Future Perspectives
Overall, our results demonstrate that the spatial variation in foliar phenolics can be accurately predicted by integrating airborne imaging spectroscopy with Sentinel-2 multispectral imagery, offering a viable pathway for scaling phenolic mapping to continental and even global extents. Nevertheless, several limitations should be acknowledged. First, although our study encompassed a relatively large number of plant species from diverse vegetation types compared to prior work, the spatial coverage remains largely confined to temperate and subtropical regions. Whether this approach can be successfully extended to tundra and tropical ecosystems, which harbor greater species diversity and more heterogeneous environmental conditions, warrants further investigation. Furthermore, although the sampled NEON sites represent a broad range of vegetation communities and climatic conditions across the eastern United States, the influence of environmental variability on phenolic retrieval performance was not explicitly quantified. Differences in climate, species composition, canopy structure, and stand characteristics may affect canopy reflectance–trait relationships and introduce additional uncertainty when transferring models across ecosystems. Although community-weighted mean phenolic concentrations were used to incorporate within-plot species composition, future studies should integrate broader environmental gradients, structural measurements, and long-term ecological observations to better evaluate model transferability.
Second, our study focused exclusively on the peak growing season; foliar phenolics, however, is known to vary across phenological stages [
18]. Future research should therefore target multiple growth stages, contingent on the availability of concurrent airborne and Sentinel-2 acquisitions.
Third, the airborne imaging spectroscopy data and field measurements used in this study were collected in 2017, predating the launch of recent spaceborne imaging spectrometers and thereby precluding direct upscaling to these newer satellite platforms. However, the National Ecological Observatory Network (NEON) is designed as a long-term observation program spanning 30 years, which will enable concurrent measurements with current hyperspectral missions such as PRISMA and EnMAP, ultimately supporting repeated, synoptic monitoring of foliar traits at broader scales [
29,
49].
Another consideration is that the optimal aggregation window identified in this study should be interpreted within the context of the evaluated ecosystems, sensors, and spatial configurations. The improved performance observed at the 100 × 100 m window likely reflects a balance between reducing spatial mismatch between NEON AOP and Sentinel-2 observations and preserving meaningful variation in canopy phenolic signals. Increasing the aggregation window can reduce the effects of geolocation uncertainty, differences in spatial support between airborne and satellite observations, and fine-scale canopy heterogeneity, thereby improving agreement between the two datasets. However, excessive aggregation may also smooth local variations in vegetation composition and canopy chemistry, potentially reducing sensitivity to fine-scale ecological patterns. Therefore, the 100 m aggregation window identified here should not be considered a universal optimal scale, but rather an empirically determined scale for the NEON sites and Sentinel-2 observations evaluated in this study. Future applications across different ecosystems, spatial resolutions, and sensor configurations should evaluate multiple aggregation scales to identify the most appropriate spatial scale for trait retrieval.
Finally, Sentinel-2 phenolic predictions were evaluated against airborne-derived phenolic estimates, which themselves contain uncertainties associated with airborne retrieval models and spatial aggregation. Although increasing aggregation windows improved agreement between airborne and satellite observations, future studies should incorporate uncertainty-aware validation strategies and independent field observations to further quantify the reliability of satellite-based phenolic products. While the present study focused specifically on foliar phenolics, the methodological framework we developed is readily extendable to other foliar chemical traits, paving the way for comprehensive analyses of the links between foliar chemistry, ecosystem function, and functional diversity.