1. Introduction
The Landsat Next satellite, scheduled for launch at the end of this decade, is expected to provide multispectral imagery at spatial resolutions of 10 m to 20 m [
1,
2]. Increases in the number of bands and finer spatial resolutions compared to previous Landsat missions (multispectral imagery at 30 m) will advance remote sensing-based studies in many fields including agriculture, ecology, forestry, hydrology, and minerology. In this research effort, we focus on Landsat Next capabilities in characterizing non-photosynthetic vegetation (NPV) which has critical applications in agricultural and ecological studies. An important type of NPV is crop residue, namely the NPV that remains on agricultural fields post-harvest. Agricultural fields that are managed with higher levels of fractional crop residue cover (
fR) are less prone to erosion, have greater soil organic carbon, and more stable soil moisture [
3,
4,
5,
6]. The amount of
fR on fields also serves as an important indicator of tillage intensity, particularly when measured in late spring immediately after the planting of summer crops [
7,
8].
In past Landsat missions, a shortwave infrared (SWIR) spectral region spanning 2000–2500 nm (sometimes referred to as “SWIR2”) has been measured by a single band [
9]. The SWIR2 band spanned approximately 2080 to 2350 nm for Landsat 4 and 5 Thematic Mapper (TM) and Landsat 7 Enhanced Thematic Mapper+ (ETM+) [
10]. A single SWIR2 band is still used for Landsat 8 and 9 Operational Land Imagers (OLI and OLI2, respectively) but has a narrowed spectral response (approximately 2110 to 2290 nm). Similarly, the Sentinel-2 MultiSpectral Instruments (MSI) use a single SWIR2 band, approximately 2100 to 2280 nm. Use of a single SWIR2 band in global Earth resource monitoring missions limits the spectral separation of NPV from soils, green vegetation, and other land cover types, even when using approaches comparing SWIR2 reflectance to SWIR1 reflectance [
1,
11]. SWIR1, spanning 1400–1850 nm, is also covered by a single band centered at approximately 1610 nm [
12].
Over the past 30 years, the lignin and cellulose (lignocellulose) absorption features centered near 2100 nm and 2300 nm have been exploited by applying imaging spectrometer data to NPV detection and characterization [
13,
14,
15,
16,
17]. Some of these imaging spectrometers/missions include the Airborne Visible/Infrared Imaging Spectrometer (AVIRIS), Earth Observing One (EO-1) Hyperion, and
PRecursore IperSpettrale della Missione Applicativa (PRISMA). To date, both airborne and spaceborne imaging spectrometers have been limited in coverage, e.g., swath footprint and revisit intervals. Narrow band multispectral imagers with multiple SWIR bands, like those on the WorldView-3 (WV3), also offer capabilities in resolving lignocellulose absorption features, but, like spaceborne and airborne imaging spectrometers, are limited in coverage. In comparison, current imaging systems with global coverage and regular revisit intervals, such as sensors on Landsat and Sentinel-2, have limited capabilities in resolving lignocellulose absorption features due to poor SWIR sampling by broad band sensors, e.g., SWIR2. To better resolve the lignocellulose absorption features present in NPV, Landsat Next’s imaging system is expected to feature regular global coverage and three relatively narrow bands covering the heritage SWIR2 spectral region.
Figure 1 provides a depiction of potential Landsat Next SWIR band placements compared to ETM+, OLI, MSI, WV3, and spectrometer data with similar spectral sampling as hyperspectral AVIRIS and PRISMA bands.
Despite band width limitations,
fR estimates have, at times, been provided by Landsat/Sentinel-2 satellites with global coverage [
18,
19,
20,
21,
22]. In some of the most successful regional-scale crop residue studies incorporating Landsat/Sentinel-2 SWIR imagery, the accuracy assessing broad categories of
fR and associated tillage intensity generally ranges between 55 and 79% and requires the use of regionally-specific approaches [
22,
23,
24]. Well-calibrated, site-specific studies utilizing Landsat/Sentinel-2 SWIR bands may offer higher accuracies in
fR estimation (>80%). In general, both regional-scale and site-specific crop residue studies using Landsat/Sentinel-2 imagery make use of spectral indices computed from SWIR2 and SWIR1 bands like the Normalized Difference Tillage Index (NDTI) [
18,
20]. While site-specific studies using NDTI to estimate
fR can achieve fairly high accuracies, high levels of inter-site variability in NDTI values for fixed
fR values make such indices ill-suited for global mapping efforts [
19,
20,
21]. Site-specific studies incorporating spectral angle mapping (SAM) from Landsat/Sentinel-2 bands have demonstrated some of the highest levels of performance in
fR estimation (>90%) [
25,
26]. Additionally, South et al. (2004) [
27] demonstrated that SAM consistently outperformed statistical classification approaches when using Landsat imagery to classify tillage intensity categories (>92% vs. <72%). However, it remains unclear how effectively such approaches can be scaled regionally or globally, as no such large-scale studies have been carried out to our knowledge, and current SAM approaches are ultimately reliant on spectrally broad reflectance contrasts that may lack sufficient biophysical specificity, e.g., near infrared—SWIR1—SWIR2 comparisons.
For
fR estimation, finer spectral resolution data sources offer improved accuracies over coarser resolution data sources since the later cannot accurately detect lignocellulose absorption features at 2100 and 2300 nm [
11,
20,
28] (
Figure 1). Finer spectral resolution data sources are particularly suited for application of spectral unmixing for
fR estimation when there is a preponderance of mixed pixels containing
fR, fractional soil (
fS), and fractional green vegetation (
fGV) that result from different field management practices like tillage and planting. Bannari et al. (2006) [
28] provide an illustrative comparison of spectral unmixing approaches applied to hyperspectral and broad band multispectral data sources, with the former yielding higher accuracies in
fR estimation. Daughtry et al. (2006) [
11] provide a similar hyperspectral vs. broad band multispectral comparison using spectral index approaches, demonstrating higher
fR estimation performance for hyperspectral indices with
R2 ranging from 0.774 to 0.850 while broad band indices
R2 ranged from 0.108 to 0.498. Yue et al. (2019) [
29] provide a comparison of both hyperspectral indices and SAM approaches compared to broad band multispectral indices, demonstrating that both hyperspectral approaches outperform broad band multispectral indices in laboratory-based
fR estimation. Multispectral imagery with narrow-to-moderate band widths (<60 nm) offers similar improvements in
fR estimation accuracy compared to broad band multispectral data sources. Hively et al. (2018) [
20] demonstrated performance differences between narrow band multispectral SWIR indices derived from WV3 imagery compared to Landsat-simulated SWIR indices derived from convolved WV3 bands, with the former exhibiting
fR estimation performance improvements of 10% or greater under conditions of minimal
fGV and minimal surface moisture variability. In
fR estimation studies where significant
fGV is present or surface moisture is highly variable, finer spectral resolution imagery vastly outperforms heritage Landsat SWIR bands [
30,
31,
32].
The prior paragraphs convey a critical limitation for accurate spaceborne monitoring of crop residue and associated agricultural tillage: few current satellites possess the optimal characteristics for retrieving
fR including regular revisit cadence, global coverage, fine spatial resolution, and fine spectral resolution in the SWIR2 region. These current limitations and future satellite needs extend beyond conventional agricultural applications as accurate characterization of fractional NPV cover (
fNPV) is critical in the assessment of wild vegetation health, drought condition, and rangeland forage quality [
33,
34,
35,
36]. Although our study focused on
fR assessment for agricultural applications, many of our findings could be broadly applicable to non-agricultural
fNPV assessment as well.
An initial evaluation of prospective Landsat Next SWIR bands for
fR and
fNPV characterization was carried out by Hively et al. (2021) [
37] using established spectral band locations from satellite missions including Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), Hyperion, and WV3, in addition to heritage Landsat bands. These bands are shown in
Figure 1. This previous study found that narrow bands positioned near lignocellulose absorption features were substantially more accurate in
fR estimation than heritage Landsat bands (
R2 of 0.81 and 0.77, respectively, for two-band and three-band indices, compared to
R2 of 0.44 for Landsat heritage indices). In the current research effort, we sought to improve upon the evaluation of previous band locations by implementing an iterative wavelength shift approach that assesses
fR estimation capabilities across all band combinations in the portions of the SWIR most relevant to crop residue characterization (2000–2350 nm) [
38]. We evaluated
fR estimation error using spectral indices based on two- and three-band combinations covering the SWIR2 region. After identifying the top-performing spectral bands using the iterative wavelength shift approach, we assessed how well these wavelengths performed in
fR estimation under conditions of variable surface moisture and
fGV presence compared to the wavelengths of established crop residue indices. Ideally, the findings of this research effort will be useful for further informing SWIR band placements for the Landsat Next mission and developing a methodology useful for generalized spectral band selections for biophysical variables pertinent to other application areas.
2. Materials and Methods
To optimize the placement of Landsat Next SWIR bands for
fR estimation we used a database of agricultural field spectra from Dennison et al. (2019) [
39]. The Dennison et al. (2019) dataset contains spectra that were originally collected by Daughtry and Hunt (2008) [
30] and Quemada and Daughtry (2016) [
40] at the United States Department of Agriculture Beltsville Agricultural Research Center (BARC) in Beltsville, MD, USA. Spectra were collected using Analytical Spectral Devices (ASD) field spectrometers (Malvern Panalytical, Westborough, MA, USA). Native sampling intervals of these field instruments is approximately 2 nm in the SWIR2 region, with a coarser spectral resolution of up to 12 nm depending on the specific instrument [
39]. The instruments use cubic spline interpolation to resample spectra at a 1 nm interval.
Daughtry and Hunt (2008) collected 600 field spectra
in situ from seven different BARC agricultural fields, and included varying cover of crop residue, soil, and three live crops (corn (
Zea mays L.), soybeans (
Glycine max (L.) Merr.), and wheat (
Triticum aestivum L.)). Quemada and Daughtry (2016) collected field spectra over manually manipulated plots with varying crop residue cover and surface moisture. For both datasets, spectra were collected using an 18° foreoptic positioned 2.3 m above the surface with a 0° view zenith angle. A digital camera was positioned next to the foreoptic, and a photograph was taken of the field-of-view of each spectrum.
fR,
fS, and
fGV were determined for each spectrum by point sampling the corresponding photograph (Daughtry and Hunt, 2008; Quemada and Daughtry, 2016). Quemada and Daughtry (2016) also measured soil and crop residue relative water content (RWC) for each field-of-view, and a RWC threshold of 60% used by Dennison et al. (2019) provided a total of 316 field spectra from this experiment. More details on RWC categories are provided in
Section 2.4.
To assess
fR estimation performance, we applied an iterative wavelength shift approach to these agricultural spectra, hereafter referred to as the “BARC dataset” or simply “dataset”, computing generalized spectral indices, then using linear regressions to model index values as a function of field-measured
fR. We performed the iterative wavelength shift analysis on two version of the BARC dataset: (1) 10 nm interval and bandwidth spectra with Gaussian spectral response functions previously published in Dennison et al. (2019), hereafter referred to as the “10 nm dataset” and (2) 1 nm interval, 30 nm bandwidth spectra calculated by applying a 30 nm moving-average filter to the original 1 nm field spectra collected by Daughtry and Hunt (2008) and Quemada and Daughtry (2016), hereafter referred to as the “1 nm interval dataset”. The 10 nm dataset was processed to both surface reflectance (SR-processed) and surface reflectance with simulated sensor noise and atmospheric artifacts added (atm-processed). The atm-processed 10 nm spectra provide a general indication of atmospheric errors for Landsat Next
fR estimation since these errors were simulated for an imaging spectrometer with 10 nm bandwidths while Landsat Next will be a multispectral imaging system with ≥30 nm bandwidth for SWIR2 bands. Readers are directed to Dennison et al. (2019) [
39] for a more thorough description of formulation of the 10 nm datasets. The 1 nm interval dataset was only processed to surface reflectance.
For both the 10 nm and 1 nm interval datasets, we created a subset of the datasets based on each spectrum’s NDVI values, as abundant green vegetation has been found to impact
fR estimates. We computed NDVI from Landsat 8-simulated bands (Equation (1)) and selected the spectra with NDVI < 0.3 to represent low-vegetation conditions, producing 650 spectra for the 10 nm dataset and 643 spectra for the 1 nm interval dataset, with the difference in NDVI < 0.3 counts attributed to slight differences in band formation. The NDVI threshold of 0.3 was selected as this has been found to consistently represent a threshold for minimal green vegetation [
20,
31,
34]. This allowed us to assess green vegetation effects by comparing results from the full-NDVI and NDVI < 0.3 datasets. The NDVI formula used in this study is shown in Equation (1).
where OLI denotes reflectance simulated for Landsat 8 OLI bands 4 and 5 (visible red and near infrared) as subscripts.
For the iterative wavelength shift analysis, we implemented an approach similar to Serbin et al. (2009b) [
41], in which a two-band iterative generalized normalized difference index (gNDI) routine was used to determine which two reflectance wavelengths produced maximum correlation with ground-measured
fR. The Serbin et al. (2009b) gNDI approach was applied to several field spectroscopy studies conducted across the United States and results were aggregated to produce a composite
R2 value across sites. The original gNDI analysis was performed for all wavelengths from 400 nm to 2500 nm. In this study, we limited the iterative wavelength shift analysis to wavelengths between 2000 and 2350 nm as this portion of the SWIR region has been found to most consistently contain spectral variability related to the presence of lignocellulose absorption features present in NPV [
38,
41,
42]. We excluded wavelengths greater than 2350 nm that contained significant sensor noise. To assess
fR estimation performance using the iterative wavelength shift approach, we computed the coefficient of determination (
R2) and root mean squared error (
RMSE) (Equations (2) and (3)) across all unique wavelength combinations between 2000 and 2350 nm by computing a spectral index and using ordinary least squares regression to model
fR.
where
and
are observed (field-measured
fR) and predicted (index-estimated
fR) values, respectively,
is the average observed value, and
is the number of samples.
We performed the iterative wavelength shift analysis for generalized two-band indices (Equations (4) and (5)) and generalized three-band indices (Equations (11)–(13)). In performing this analysis across the 2000–2350 nm wavelength range, we seek to identify the wavelengths most useful for fR characterization with Landsat Next SWIR bands. R2 and RMSE are given equal consideration in performance assessments as maximizing explained variance and minimizing predictive error are both critical in selecting optimal wavelengths.
2.1. Two-Band Iterative Wavelength Shift Approach
The mathematical form of the gNDI spectral index from Serbin et al. (2009b) [
4] is shown in Equation (4).
where
R denotes reflectance, subscripts
i and
j denote wavelengths for bands 1 and 2 and subscript
s denotes a given spectrum. Each spectrum corresponds to a field-measured
fR value. The entire dataset of gNDI values was used to model
fR values (n = 916 for full-NDVI; n = 650/643 for NDVI < 0.3), resulting in an
R2 and
RMSE value for each
i, j wavelength in a two-dimensional spectral space.
In addition to implementing the two-band iterative gNDI approach, we also used a two-band generalized difference index (gDI) (Equation (5)), as Hively et al. (2021) [
37] found this form of SWIR spectral index to be less susceptible to influence from green vegetation when estimating
fR.
Two established crop residue indices that provide examples of two-band normalized difference and simple difference index forms are the Shortwave Infrared Normalized Difference Residue Index (SINDRI) and Shortwave Infrared Difference Residue Index (SIDRI) [
37,
41] (Equations (6) and (7)). Note gNDI and gDI will evaluate all specific wavelength combinations in the 2000–2350 range, including combinations identical to SINDRI and SIDRI.
where
R denotes reflectance, and the corresponding subscript denotes central wavelength for either a narrow band multispectral or hyperspectral sampling.
2.2. Three-Band Iterative Wavelength Shift Approach
We built on the two-band iterative wavelength shift approach from Serbin et al. (2009b) by including a third band. This modification was motivated by the fact that numerous studies have found three-band spectral indices to perform especially well for crop residue characterization and often better than two-band spectral indices [
30,
31,
43,
44]. We initially calculated two broad classes of indices using three-band generalized iterative approaches. These classes included three-band absorption-at-center indices, hereafter referred to as side peak indices, and three-band peak-at-center indices, hereafter referred to as center peak indices. The “peak” terms refer to a higher reflectance value in regions spectrally adjacent to absorption features in dry plant matter centered near 2100 and 2300 nm (
Figure 1). A well-established three-band side peak index is the Cellulose Absorption Index (CAI) [
43] (Equation (8)). A more recently established, yet illustrative example of a three-band center peak index is the Lignin Cellulose Peak Center Difference Index (LCPCDI) [
37] (Equation (9)). In this effort, we also test a second version of the LCPCDI with slightly shifted wavelengths (Equation (10)).
In the case of CAI, the spectral “side” terms
R2040 and
R2210 generally exhibit higher reflectance values than the subtracted spectral “center” term
R2100, with this later term corresponding to a lignocellulose absorption feature around 2100 nm for an NPV target [
38,
42]. In the case of LCPCDI, the spectral center term
R2210 generally exhibits higher reflectance than the
R2100 and
R2260 terms which overlap with lignocellulose absorption features at 2100 nm and 2300 nm, respectively, for an NPV target [
38,
42].
Figure 1 provides an illustration of these differences for example crop residue, soil, and green vegetation spectra from the BARC dataset. The 2040–2210 nm region/bands correspond to CAI with reflectance side peaks, while the 2100–2260 nm region/bands correspond to LCPCDI with a reflectance center peak for crop residue.
With the CAI and LCPCDI providing examples of side peak and center peak difference indices, respectively, we proceed noting that mathematically, side peak difference and center peak difference indices produce identical absolute values when computed with the same reflectance values for each band. Thus, for simplicity’s sake, figures and references will proceed with mention of the generalized Center Peak Difference Index (gCPDI) only (Equation (11)). In addition to the gCPDI, we also computed a generalized Center Peak Ratio Index (gCPRI) (Equation (12)) to compare three-band ratio indices to the more commonly implemented three-band difference indices, e.g., CAI and LCPCDI. Unlike the side peak and center peak difference indices, the ratio versions of these indices will not produce identical absolute values and thus, a generalized Side Peak Ratio Index (gSPRI) is computed and shown in Equation (13) to illustrate this is a unique index compared to gCPRI.
where
R denotes reflectance, subscripts
i, j, and
k denote wavelengths for bands 1, 2, and 3, respectively. The subscript
s denotes a given spectrum.
2.3. Iterative Wavelength Shift Approach Applied to BARC Spectra Datasets
We used the iterative wavelength shift approach to first analyze the 10 nm dataset processed with and without combined sensor noise and atmospheric artifacts (atm- and SR-processed, respectively). Leading with the 10 nm dataset wavelength shift analysis enabled us to determine whether atmospheric correction-based error sources, i.e., errors from atmospheric artifacts, were minimal enough to proceed with the wavelength shift analysis on the 1 nm interval dataset with surface reflectance processing only. While the atm-processed version of the 10 nm dataset only provided a limited comparison from one simulation of errors from a standard atmosphere and specific sensor, the comparison to the SR-processed dataset is assumed to be generally informative. After the 10 nm dataset analysis was performed and results demonstrated minimal differences between the atm- and SR-processed datasets (Results
Section 3.1 and
Section 3.3), we proceeded to apply the iterative wavelength shift approach to the 1 nm interval dataset (Results
Section 3.2 and
Section 3.4).
We created an additional modified version of the three-band iterative wavelength shift approach applied to the 1 nm interval dataset to better identify multiple spectral regions useful for fR estimation. While the results from the two-band wavelength shift analysis identified a single high performance (high R2, low RMSE) spectral region for fR estimation, the three-band analysis indicated the presence of multiple high R2/low RMSE clusters, hereafter referred to as “high correlation clusters”. To allow for the analysis of multiple high correlation clusters, we applied an empirical threshold of 2100 nm to band 1 to capture R2 and RMSE for the slightly lower-correlation clusters. In the proceeding analyses, the terms “gCPDI”, “gCPRI”, and “gSPRI” denote the best performing bands across the entire 2000–2350 nm range, while “gCPDI>2100”, “gCPRI>2100”, and “gSPRI>2100” denote best performing bands with a band 1 > 2100 nm constraint.
2.4. Assessment of Moisture and Green Vegetation Impacts on Crop Residue Estimation
The Quemada and Daughtry (2016) [
40] subset of the 1 nm interval BARC dataset was used for assessment of the impact of soil and crop residue RWC on
fR estimation for top-performing wavelength shift analysis identified wavelengths. This dataset was originally collected by Quemada and Daughtry (2016) as part of a study assessing spectral index-based
fR estimation performance under varying RWC conditions. The total spectra (n = 316) were split into three RWC categories: 0.0–0.1 (n = 135), 0.1–0.25 (n = 101), and 0.25–0.60 (n = 77) [
40]. These RWC classes were selected based on findings that crop residue spectral index performance was notably diminished after RWC exceeded 0.25. Quemada and Daughtry (2016) spectra contained no
fGV, meaning this dataset provides a largely controlled assessment of
fR estimation with
fS being the other cover type. We first assessed performance of the top-performing two- and three-band indices identified in the wavelength shift analysis (Equations (4), (5) and (11)–(13)) as a function of varying RWC using
R2 and
RMSE metrics. We then compared the performance of iterative wavelength shift indices to established crop residue indices.
In addition to established CAI, SINDRI, and LCPCDI, we evaluated several additional indices tested in Hively et al. (2021) [
37] including the Lignin-Cellulose Absorption Index (LCA), ratio version of CAI left peak (rCAI
LP), ratio version of CAI right peak (rCAI
RP), and the aforementioned heritage NDTI (Equations (14)–(17)).
where
R denotes reflectance, and the corresponding subscript denotes central wavelength for either a narrow band multispectral or hyperspectral sampling, and OLI denotes simulated reflectance from Landsat 8 OLI bands 6 and 7 (SWIR1 at 1610 nm and SWIR2 at 2200 nm, respectively) as subscripts.
Similar to the RWC analysis, the green vegetation analysis assessed the influence of varying
fGV levels on
fR estimation accuracy. For the green vegetation analysis, we used the Daughtry and Hunt (2008) [
30] subset of the 1 nm interval BARC dataset which contained all original spectra published in that study (n = 600). Like the RWC analysis, spectra were split into
fGV classes of 0.0–0.1 (n = 327), 0.1–0.3 (n = 136), 0.3–0.6 (n = 46), 0.6–0.9 (n = 44), and 0.9–1.0 (n = 47). These class ranges were chosen to keep a similar number of samples for the higher
fGV ranges where the total samples were fewer relative to the lower
fGV ranges. Like the RWC assessment, established crop residue indices were compared to top-performing iterative wavelength shift-identified indices and band wavelengths.
For our final analysis, we combined the RWC and green vegetation analyses to determine if the relative fR estimation of the top-performing bands changed under these combined conditions. We computed a composite R2 and RMSE for three RWC classes (0.0–0.6) and three fGV classes (0.0–0.6) to determine the best-performing bands for Landsat Next SWIR2 as these composites equally weight performance across a range of conditions expected to diminish fR estimation accuracy. These composite metric values were then compared to results from the 1 nm and 10 nm iterative wavelength shift analyses from the whole BARC dataset which skewed towards low fGV and low RWC conditions. Our final analysis identified top-performing band centers and established wavelength tolerances by identifying the top-performing wavelength ranges for each band.
4. Discussion
To evaluate optimal Landsat Next SWIR band placements for
fR estimation, we applied wavelength shift analyses to the 1 nm interval (30 nm bandwidth) and 10 nm BARC spectra datasets and assessed
fR estimation accuracy. For the two-band wavelength shift analysis applied to the 10 nm dataset, wavelengths similar to the 2210 and 2260 nm bands that formulate the well-established SINDRI index outperformed other spectral regions in
fR estimation. The
fR estimation accuracies of SINDRI with NDVI < 0.3 observed in this study fell between those previously established in Serbin et al. (2009b) [
41] with an
R2 of 0.741 for a U.S.-scale dataset and Hively et al. (2018) [
20] with an
R2 of 0.940 for a single-date, local-scale dataset. In the two-band wavelength shift analyses with gNDI, the top-performing bands were 2220 and 2270 nm with the NDVI < 0.3 dataset. When the two-band analyses were performed with the full-NDVI dataset, the 2220 and 2270 nm bands were again top-performing but with the gDI rather than gNDI.
For the 1 nm interval dataset analysis with NDVI < 0.3, gNDI was the top performer in
fR estimation with identified bands at 2226 and 2263 nm, but SINDRI offered very similar performance with
fR estimation differences less than 0.01 for
R2 and 0.0028 for
RMSE. For the full-NDVI 1 nm interval dataset analysis, gDI was the best performing index where it exhibited considerably higher
fR estimation performance than gNDI even with gDI having similar top-performing bands at 2227 nm and 2259 nm. The findings of both two-band analyses (10 nm and 1 nm interval datasets) indicate that the approximate band ranges of 2210–2230 nm for band 1 and 2260–2270 nm for band 2 provide a best overall solution for the case of Landsat Next SWIR2 being comprised of two bands. While gDI maintained more consistent performance for the different NDVI thresholds than gNDI, gDI was not the top performer in
fR estimation and further would be expected to be the least stable of all generalized indices tested in both the two- and three-band analyses. The expected lack of stability compared to normalized difference indices is due to the gDI, including SIDRI, being reliant on a simple reflectance difference between two bands and featuring no-scaling type adjustments that may partially compensate for variation in surface brightness, including ground-shading, surface anisotropy/bidirectional reflectance distribution function effects, and uncertainties/errors in surface reflectance retrievals [
46]. With the Landsat Next mission’s global mapping focus, this presents a challenge, as
fR estimation accuracy would vary considerably depending on
fGV cover. While multiple indices (including NDVI) could be used for pixel-level
fR estimation using two SWIR bands at 2200 nm and 2270 nm, this approach could produce inconsistencies in derived
fR products, and complicates product development compared to a single index approach.
The inclusion of an additional band for the three-band wavelength shift analyses (Results
Section 3.2 and
Section 3.4) improved
fR estimation performance while being less impacted by
fGV compared to the two-band indices in general. This finding comports with previous work by Serbin et al. (2009b) [
41] who demonstrated that the three-band CAI exhibited similar
fR estimation performance to SINDRI across a wide range of conditions but was notably less impacted by the presence of green vegetation. For the three-band wavelength shift analysis applied to the 10 nm dataset, the spectral regions associated with CAI bands (2030–2050 nm, 2080–2110 nm, and 2210–2220 nm) were found to be top performers for the NDVI < 0.3 dataset (
Figure 6) and the full-NDVI dataset (
Figure 7), indicating robust performance across a range of vegetation conditions. Wang et al. (2013) [
47] found CAI to be more correlated with vegetation dry matter content than both SINDRI and NDTI while also being less correlated with vegetation moisture content, partially explaining CAI’s high
fR estimation accuracy in this study compared to other indices. This is a critical performance difference between the three-band and two-band indices since crop residue surveys are often conducted during the spring season when green winter cover crops have reached maximum biomass and summer cash crops are emerging, meaning that satellite-based
fR estimation techniques would require resilience to
fGV effects. For the 10 nm analysis, the gCPRI with 2030, 2080, and 2220 nm bands was found to be top performing in
fR estimation for the NDVI < 0.3 dataset. For the full-NDVI dataset, gSPRI with 2030, 2110, and 2210 nm bands was found to be top performing. Only the central band 2 shifted by more than 10 nm in this comparison. The overall findings presented in
Table 3 indicate that for indices computed from CAI-type wavelengths (2040, 2100, and 2210 nm), there is a fair degree of latitude in spectral placement of band 2.
For the 1 nm interval dataset, gCPRI exhibited top performance with bands at 2031, 2085, and 2216 nm and an
R2 = 0.8397 and
RMSE = 0.1231. This was the top
fR estimation performance across all wavelength shift analyses (Results
Section 3.1,
Section 3.2,
Section 3.3 and
Section 3.4), and these wavelengths are nearly identical to the top-performing bands in the 10 nm dataset analysis. Also comparable to the 10 nm dataset analysis, for the 1 nm interval analysis with full-NDVI gSPRI was top-performing with three bands at 2036, 2111, and 2217 nm and an
R2 = 0.7581 and
RMSE = 0.1548. Compared to gSPRI, gCPRI performed quite comparably for the full-NDVI dataset in terms of
fR estimation performance while identifying the same band 1 wavelength of 2036 nm but identified different band 2 wavelengths (2100 nm vs. 2111 nm) and band 3 wavelengths (2169 nm vs. 2217 nm). This indicates that there is a fair degree of latitude in the placements of bands 2 and 3, while band 1 should ideally remain fairly fixed. Although CAI-type wavelengths were top-performing across the three-band wavelength shift analysis, ratio indices outperformed difference indices by
R2 values greater than 0.035 in certain cases. Further, difference indices were more prone to errors in estimation of
fR when both full-NDVI and atmospheric artifacts were present (
Figure 7 panels a–b vs. panels c–d). Assessment of index type was not the primary focus of this study, but considering these findings, a more in-depth investigation of index formation could provide critical information on development of
fR products suitable for regional and global scale mapping efforts.
To provide a more thorough assessment of the wavelength shift analysis findings in determining final band recommendations for Landsat Next SWIR2, we evaluated top-performing indices under conditions of varying RWC and
fGV. Nearly all narrow band multispectral indices comprised of multiple SWIR2 bands resolving lignocellulose absorption features exhibited
R2 values approaching or exceeding 0.9. NDTI, comprised of a single SWIR2 band, was the only index that had
R2 values well below 0.9. Further, NDTI exhibited a greater rate of decrease in
R2 values as a function of increasing RWC than other indices, indicating this index proves unreliable in
fR estimation under conditions of varying moisture, as has been demonstrated by analyses in Quemada et al. (2018) and Quemada and Daughtry (2016) [
32,
40]. The NDTI-
fR correlations of
R2~0.45 for the 0.25–0.60 RWC class were slightly lower, but in a similar range as those observed across sites with multitemporal Landsat imagery in Thoma et al. (2004) [
48]. Our findings indicate that RWC variability may partially explain lower performance in NDTI-based
fR estimation, as would be expected in analyses using multitemporal satellite imagery. Decreased
fR estimation performance of the high RWC class (0.25 to 0.6) was also observed for the two-band CAI type indices (
Figure 9) as would be expected for two-band indices with wavelengths of varying liquid water absorption strength. Comparatively, the performance of two-band SIDRI and SINDRI indicate that indices with 2210 nm and 2260 nm bands provide far better performance in
fR estimation in terms of robustness to RWC in the event of Landsat Next being limited to two SWIR2 bands. In the two-band case, SINDRI/SIDRI bands at ~2210 nm and 2260 nm perform much better than other two-band combinations, e.g., two-band CAI variants. For the green vegetation analysis, both two-band CAI indices performed somewhat poorly at higher
fGV levels. LCA and SINDRI performed moderately and SIDRI somewhat better than SINDRI. CAI exceeded all established indices in
fR estimation with increasing
fGV (
Figure 11).
In comparison to the wavelength shift generalized indices, (
Figure 10 and
Figure 12), CAI still maintains good performance relative to the generalized indices, but gSPRI-fNDVI is also a top performer across vegetation classes and is the highest performer for the 0.10–0.30 and 0.30–0.60 categories. The gSPRI-fNDVI bands (2036, 2111, and 2217 nm) were top performing in the RWC analysis. In the three-band wavelength shift analysis with the 1 nm interval BARC dataset, the wavelengths of the best performing band 1 were between 2031 and 2041 nm, indicating that this narrow spectral range represents an ideal band placement. The central wavelength of this range is 2036 nm, which was the best performing band in the top performing generalized index (gSPRI-fNDVI) across RWC and green vegetation analyses as shown by the across-class average
R2 and
RMSE in the last column of
Table 5, supporting our selection of the 2036 nm wavelength for band 1. The combined findings of the RWC and green vegetation analyses indicate that the recommendation of band 2 at 2097 (±14 nm) is ideal and well supported. For band 3, the top-performing wavelengths range from 2154 to 2225 nm. Although this a wide range, the two top-performing band 3 wavelengths were 2216 and 2217 nm. These top-performing wavelengths are less than a 20 nm shift compared to the Landsat 8 SWIR2 band center at 2200 nm, supporting some level of mission continuity with Landsat 4–9, albeit with a narrow band width. This slight increase in wavelength for band 3 was found to be advantageous for improving
fR estimation performance in general. This supports our final selection of 2214 nm for band 3 from a top-performing wavelength range of 2110 to 2217 nm. However, like band 2, we note there is a wide range of wavelengths that will represent good performance in
fR estimation for Landsat Next with a three-band configuration for SWIR2.
Overall, what was critical to this study’s focus was the consistent identification of high-performing bands at CAI-type wavelengths. The indices producing the lowest RMSE in fR estimation for the combined RWC and green vegetation analysis were all three-band indices with CAI-type wavelengths (including CAI itself). Our selection of final bands centered at 2036, 2097, and 2214 nm provides three bands well-suited for resolving the 2100 nm lignocellulose absorption feature of crop residue and other NPV over a range of conditions. The selected cutoff at 2350 nm in our analysis due to spectrometer noise may have limited our ability to fully examine the 2350 to 2500 nm spectral range. It is possible that clean spectra with high SNR measurements free from artifacts may reveal a different pattern in the wavelength shift analysis for two- or three-band indices; for example, a three-band index centered on the 2300 nm absorption feature that is evidenced in NPV spectra with high SNR. However, given lower radiance levels at longer wavelengths and the influence of atmospheric water vapor, clear satellite observations of the longward edge of the 2300 nm absorption feature may be difficult to obtain with broad band multispectral sensors. While our findings comport with former studies and establish well-evidenced band selections, it is critical to note the limitations of this study, the first of which is the limited geographic extent of this study, with all spectra being acquired from fields in the same region. This study was also limited to maize, soybean, and wheat crop residue spectra. Performing a similar analysis with a more globally representative distribution of spectra could greatly improve this analysis. Second, our analysis only compared SR- and atm-processed spectra from a single atmospheric correction simulation. Before establishing finalized band placements for Landsat Next, a more detailed assessment of atmospheric impacts on fR estimation performance is needed.