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Testing of the 4SM Method in the Gulf of California Suggests Field Data Are not Needed to Derive Satellite Bathymetry

Satellite-derived bathymetry methods over coastal areas were developed to deliver basic and useful bathymetry information. However, the process is not straightforward, the main limitation being the need for field data. The Self-calibrated Spectral Supervised Shallow-water Modeler (4SM) method was tested to obtain coastal bathymetry without the use of any field data. Using Landsat-8 multispectral images from 2013 to 2016, a bathymetric time series was produced. Groundtruthed depths and an alternative method, Stumpf’s Band Ratio Algorithm, were used to verify the results. Retrieved (4SM) vs groundtruthed depths scored an average r2 (0.90), and a low error (RMSE = 1.47 m). 4SM also showed, over the whole time series, the same average accuracy of the control method (40%). Advantages, limitations and operability under complex atmosphere and water column conditions, and high and low-albedo bottom processing capabilities of 4SM are discussed. In conclusion, the findings suggest that 4SM is as accurate as the commonly used Stumpf’s method, the only difference being the independence of 4SM from previous field data, and the potential to deliver bottom spectral characteristics for further modeling. 4SM thus represents a significant advance in coastal remote sensing potential to obtain bathymetry and optical properties of the marine bottom.


Introduction
Accurate bathymetry in the coastal area is one of the most basic yet fundamental sources of information for many purposes like navigation, military, resource exploitation, fisheries and tourism. Water depth is also a major factor in community zonation and is a fundamental variable to map and model benthic habitats, for research and conservation purposes. In marine sciences, acoustic, radar and optical systems have been used to assess bathymetry [1]. However, they require substantial time and effort to be deployed, operated and interpreted. Such an effort can be challenging, especially in developing countries. Furthermore, vast regions are too costly or difficult to reach for these conventional methods: this creates gaps in the knowledge of underwater habitats. Recently, satellite with those obtained using the Log Ratio method and with a depth sounding dataset. The potential of 4SM to retrieve depths from multispectral images without the use of field data is a significant advance in the exploration and monitoring potentials in coastal areas.

Study Area
The San Lorenzo channel (SLC) was chosen as study area for its morphology and for the variety of its shallow habitats [25,26]. The SLC is a shallow area that connects the Bay of La Paz to the Gulf of California (Figure 1). The communication between the Bay and the Gulf of California happens also through the "Boca Norte" (Northern mouth): this large opening reaches a depth of 350 m. The region has two contrasting seasons: a dry season (October-June) and a humid season (July-September); the latter is referred to as "Mexican monsoon" [27] and is associated with occasional significant precipitation, often through intense events like hurricanes. Hydrographic conditions in the bay, particularly in deeper areas, are strongly influenced by the seasonal variability of main thermohaline circulation of the southern Gulf of California [28]. Salinity ranges between 34‰ and 36‰ depending on the time of the year [29]. In particular, the deeper layers, are more influenced by the Gulf of California, while shallower ones are dominated by local processes like insolation, evaporation, precipitation and mixing [30]. Because of the high solar radiation during summer, a steep thermocline can form in the upper 20 m, and the intense evaporation cause the surface layer to be more saline. This situation can be reverted with strong monsoonal winds; during the end of the humid season, northerly colder winds promote vertical mixing of the water column. In particular, the SLC can show a vertical and horizontal variability of the water column caused by a combination of events that generate a very dynamic habitat. Among them, upwelling of colder waters from the Gulf of California can cause localized phytoplankton blooms ( [31] and references therein), and strong tidal currents [32] can transport bottom sediments and enhance turbidity of the bottom layers of the water column (author FF, personal observation); finally, during the monsoon season, sediment runoff increases due to intense episodic precipitations, decreasing water quality, while atmospheric conditions become more complex (see Appendix A).

Radiative Transfer Equation
4SM relies on the simplified radiative transfer equation (RTE) for optically shallow water (Equation (1)). The RTE has been discussed in detail by Philpot [33] and Maritorena et al. [34]. In this algorithm, the irradiance reflectance of shallow waters below the surface is equal to the deep water reflectance, plus the bottom substrate contrast attenuated by the depth effect. The simplified RTE [34] at the base of the atmosphere (BOA) is rewritten for nadir radiances [23]: it is inverted as: BOA : LB = Lw + (L − Lw)e (2KZ) (2) or at the sensor (Top of Atmosphere, TOA): where L is the spectral BOA radiance where the bottom substrate is at depth Z; Lw is the spectral BOA radiance of the sea where the bottom is optically deep, also defined as backscatter or water volume reflectance; LB is the spectral BOA radiance of the bottom substrate at null depth. By adding the atmospheric path radiance (La) to all BOA radiance terms, one gets the spectral TOA radiances at the sensor LsB, Ls and Lsw in Equation (3). 2K (or K for brevity) is an operational two-way diffuse attenuation coefficient, in units of m −1 , the sum of the down-welling and up-welling terms together (2K = Kdown + Kup) and Z is the actual depth of the seabed. The optical depth 2KZ, is dimensionless. Wavelength dependency subscripts of all L and K terms are omitted for brevity. This will finally allow for the linearization of the bottom contrast: 4SM is a "ratio method". For a pair of bands i and j, with K i < K j and suitable bottom contrast in band j, water column correction is achieved by increasing Z in Equation (2) until the ratio LB i /LB j matches the slope of the soil line (see the optical calibration section below), where LB i is the average of all bands with K i < K j and suitable bottom contrast. This process operates ratios among relative numbers, and therefore does not require radiance terms to be converted into units of calibrated reflectance. All radiance terms in the above equations represent the signal as measured by the sensor, and the terms digital numbers (DN), radiance and reflectance are used interchangeably and remain dimensionless in this article. This is the privilege of a "ratio method": the 4SM approach does not require formal atmospheric correction.

Image Resources Preparation
It was soon realized that the hydrological conditions of the La Paz area are complex and highly variable. Therefore, a time-series of Landsat-8 images have been downloaded from https: //earthexplorer.usgs.gov/; all scenes were searched with a less than 10% cloud cover condition. Preference was given to images from different months and seasons, avoiding duplicates from the same month, since such a time-detailed study was not the aim of the work. Nine images were selected to be processed and considered reasonably safe to be modeled (Table 1). We processed them using the 4SM method, then using the ENVI/SPEAR tool method.
As regards ENVI/SPEARS, the image preparation and preprocessing started with the creation of vector polygons to be used as masks for clouds and boats. Then, if necessary, the images were de-glinted following Hedley et al. [35]. The de-glinting process assumes a null penetration in water of the NIR-SWIR bands of the spectral images. Areas that are affected by glint are selected over deep water and then are used to calculate linear models of all bands against the NIR or SWIR band. The amount of glint is evidenced and then subtracted using the linear models. The images are then pansharpened using a modified version of the OrfeoToolbox algorithm in R-project in the Raster Package [36]. In this process, the generation of a high resolution image (PXS) is achieved through the fusion of the panchromatic (PAN) with the multispectral (XS) data. First, the two images need to be orthorectified by oversampling of the XS image, then a low pass filter is applied to the PAN band to equalize (in the Fourier domain) the spectral content with XS data. Once the spectral content is similar, XS are normalized with the low-pass filtered (PAN) and results are multiplied with the original panchromatic band. The whole process can be represented as: )PAN (5) As regards 4SM, the image preparation only consists in importing the raw data as digital numbers in a working database, and creating a few shapefiles for sampling glint, optically deep water, vegetation, and bright sandy beach. Deglinting and pansharpening in 4SM uses the same protocols as above; however, they are applied on the fly rather than as image pre-processing.

Optical Calibration of the Simplified RTE in 4SM
As presented by Morel and Favoretto [23] and at www.watercolumncorrection.com, it is possible to retrieve from the image all the information needed for the calibration of the simplified RTE. Solving for Z and LB in Equation (2) requires four spectral parameters which are estimated from the image itself: (1) the deep water reflectance Lsw; (2) the water column reflectance Lw; (3) the soil line; and (4) the brightest pixels line.
Estimating the TOA deep water reflectance Lsw requires the presence of an area in the image which is free of any glint (or de-glinted), and is optically deep in all wavebands. To estimate the soil line [37], the non-vegetated areas on the land part of the image are analyzed in order to provide the operational values of the ratios LB i /LB j of the bottom substrate at null depth for all possible pairs of wavebands i and j. These ratios are then assumed to apply to spectrally non-differentiated shallow water pixels.
Estimating the water volume reflectance Lw is done by visual inspection of the soil line in the optical calibration diagram, and using some commonsense knowledge. Therefore, the atmospheric path radiance La may be estimated as the difference La = Lsw − Lw. Please note that, by subtracting La from all Ls terms in Equation (3), a first order atmospheric correction of the imagery is achieved.
BPL is a radiometric model of the brightest shallow bottom over the whole depth range in the image. It assumes that the shallow water part of the image contains at least some stretches of the brightest bottom substrate that exists at the scene at various depths; it represents the exponential decay of the radiances as the bottom depth increases. The BPL is used to estimate the ratio K blue /K green of Sensors 2017, 17, 2248 6 of 23 the diffuse attenuation coefficients in the blue and green bands. Then this ratio is used to interpolate spectral K for all visible bands, using Table XXVII of Jerlov [12]; this dataset reports the diffuse attenuation coefficients for downwelling irradiance in oceanic and coastal waters worldwide. For two examples of straightforward optical calibration diagrams over apparently homogeneous waters (one oceanic water type, and one coastal water type), please refer to diagrams in Appendix B. For most scenes, the calibration diagrams exhibit a complex hydrologic situation, which we tentatively explain as follows: the clear deep oceanic waters are usually covered by a layer of slightly turbid coastal waters; the thickness of this upper layer varies across the scene, from just a very few meters to in excess of 30 m (see Appendix B). This vertical structure is illustrated in Figure 2 for a Landsat 8 scene acquired on 1 January 2015: X2, X3 and X5 are linearized Blue, Green and Red bands respectively Equation (4). For most scenes, the calibration diagrams exhibit a complex hydrologic situation, which we tentatively explain as follows: the clear deep oceanic waters are usually covered by a layer of slightly turbid coastal waters; the thickness of this upper layer varies across the scene, from just a very few meters to in excess of 30 m (see Appendix B). This vertical structure is illustrated in Figure 2 for a Landsat 8 scene acquired on 1 January 2015: X2, X3 and X5 are linearized Blue, Green and Red bands respectively Equation (4). This diagram exhibits two layered water types: • 0-5 m depth range: on that day, the BPL pixels in Figure  under-estimated accordingly, unless a stratified waters model is specified as shown in Figure 2 in the 0-5 m depth range; • In case of locally increased sediment turbidity (sediment resuspension), water leaving reflectance would be increased accordingly, therefore retrieved depth would be under-estimated, like shown between 4 and 5 km on Profile A in Figure 3.
Finally, through a series of interactive calibration steps, the practitioner now must progressively fine tune manually all these variables in the command line script, until satisfied that a sound consistency has been achieved: the calibration diagrams allow to take control of the calibration  Figure 1. (a) is the calibration diagram of linearized Blue (X 2 ) and Green (X 3 ) and reports estimated K 2 /K 3 values with Jerlov water types. (b) is the calibration diagram for Blue (X 2 ), Green (X 3 ) and Red (X 5 ) bands respectively. The backdrop in shades of gray represents the bi-dimensional histogram for all image pixels (white ROI in Figure 1). Blue dots are the actual pixels used for BPL calibration, each referenced to its row/line position in the image. Small white circles represent the scatter of averaged bare land pixels, as a proxy for the Soil Line. This diagram exhibits two layered water types: • 0-5 m depth range: on that day, the BPL pixels in Figure 2a clearly display along a straight line over the 0-5 m depth range for the pair Blue/Green. The ratio K blue /K green for this surficial layer is estimated at 0.95; this denotes a water type C1 + 0.17 of Jerlov. The BPL pixels in Figure  In case of locally increased attenuation coefficient K (phytoplankton), retrieved depth would be under-estimated accordingly, unless a stratified waters model is specified as shown in Figure 2 in the 0-5 m depth range; • In case of locally increased sediment turbidity (sediment resuspension), water leaving reflectance would be increased accordingly, therefore retrieved depth would be under-estimated, like shown between 4 and 5 km on Profile A in Figure 3. Finally, through a series of interactive calibration steps, the practitioner now must progressively fine tune manually all these variables in the command line script, until satisfied that a sound consistency has been achieved: the calibration diagrams allow to take control of the calibration process. This completes the set of parameters that are necessary for operating the inverted RTE (Equation (2)) without the need or use of any field data.

Depth Retrieval in 4SM
4SM is a ratio method, meaning that a band ratio is used to derive both Z and a spectral bottom signature. Let LB j be the water column corrected radiance in band j with suitable bottom contrast Ls-Lsw; Let LB i be the average water column corrected radiance of all available wavebands with K i < K j and suitable bottom contrast. The inversion of the model is achieved by increasing the Z term in Equation (2) until the ratio LB i /LB j matches that of the soil line. As detailed by Morel and Favoretto [23], for a Landsat-8 or WorldView-2 image, several solutions are available: the NIR solution, the Red solution, the Green solution, and the PAN solution. In practice, the PAN solution is preferred, as it carries several distinct advantages. The outputs are: (i) a raster DTM of the shallow water area in units of meter, and (ii) several rasters of water column corrected wavebands in units of relative radiance, ready for bottom typing (a "low-tide" view of the scene). Some seatruth data can be used for fine tuning the estimation of Z and for a tide correction. process. This completes the set of parameters that are necessary for operating the inverted RTE (Equation (2)) without the need or use of any field data.

Depth Retrieval in 4SM
4SM is a ratio method, meaning that a band ratio is used to derive both Z and a spectral bottom signature. Let LBj be the water column corrected radiance in band j with suitable bottom contrast Ls-Lsw; Let LBi be the average water column corrected radiance of all available wavebands with Ki < Kj and suitable bottom contrast. The inversion of the model is achieved by increasing the Z term in Equation (2) until the ratio LBi/LBj matches that of the soil line. As detailed by Morel and Favoretto [23], for a Landsat-8 or WorldView-2 image, several solutions are available: the NIR solution, the Red solution, the Green solution, and the PAN solution. In practice, the PAN solution is preferred, as it carries several distinct advantages. The outputs are: (i) a raster DTM of the shallow water area in units of meter, and (ii) several rasters of water column corrected wavebands in units of relative radiance, ready for bottom typing (a "low-tide" view of the scene). Some seatruth data can be used for fine tuning the estimation of Z and for a tide correction.

Combining Depths in 4SM
Single scenes are inevitably affected by alien features that impact the result (e.g., boats and their wakes, small clouds and their shadows, algal blooms, local variations of water optical properties, etc.). Therefore, a combined depth image can be produced by averaging all the retrieved depths that satisfy some quality criteria: for each shallow pixel, first an average depth is calculated; then depths that are outside the standard deviation range are excluded and a new average is calculated. This eliminates discrete artifacts without any smoothing. One can see for example in Figure 3 that, on 4 November 2013 (purple profile), a major depth under-estimation affects the southern half of the deep SLC between 4 km and 5 km on Profile A; an increase in turbidity possibly caused this artifact. These profiles also show that the depth combination reduces much of the noise without any smoothing.

Combining Depths in 4SM
Single scenes are inevitably affected by alien features that impact the result (e.g., boats and their wakes, small clouds and their shadows, algal blooms, local variations of water optical properties, etc.). Therefore, a combined depth image can be produced by averaging all the retrieved depths that satisfy some quality criteria: for each shallow pixel, first an average depth is calculated; then depths that are outside the standard deviation range are excluded and a new average is calculated. This eliminates discrete artifacts without any smoothing. One can see for example in Figure 3 that, on 4 November 2013 (purple profile), a major depth under-estimation affects the southern half of the deep SLC between 4 km and 5 km on Profile A; an increase in turbidity possibly caused this artifact. These profiles also show that the depth combination reduces much of the noise without any smoothing.

Groundtruthed DTM
The collection of ground truth depth soundings in the SLC was completed in two days by the use of a boat equipped with an Elite5x HDI fishfinder (Lowrance, Tulsa, Oklahoma,). The Transducer (TM260 1kW with 50 kHz wide 19o beam/200 kHz narrow 6o beam, Airmar, Milford, NH, USA), was set to read from the waterline. The offset between the antenna and the transducer position was automatically calibrated by the instrument, and the instrument flagged data output with an internal gyroscope in case of excessive wave action. However, during the whole groundtruthing process, sea conditions were excellent. Data have been collected at a constant speed of 10 knots on parallel transects. Up to eight depth readings were averaged for each UTM navigation point, then tide height was subtracted using open source tide data (http://predmar.cicese.mx/calendarios/). Finally, depth data were converted in a shapefile (n = 5004, red points in Figure 1), and a Digital Terrain Model (DTM) was created by spline interpolation of groundtruthed depths (Figure 4a). outside the standard deviation range are excluded and a new average is calculated. This eliminates discrete artifacts without any smoothing. One can see for example in Figure 3 that, on 4 November 2013 (purple profile), a major depth under-estimation affects the southern half of the deep SLC between 4 km and 5 km on Profile A; an increase in turbidity possibly caused this artifact. These profiles also show that the depth combination reduces much of the noise without any smoothing.

Groundtruthed DTM
The collection of ground truth depth soundings in the SLC was completed in two days by the use of a boat equipped with an Elite5x HDI fishfinder (Lowrance, Tulsa, Oklahoma,). The Transducer (TM260 1kW with 50 kHz wide 19o beam/200 kHz narrow 6o beam, Airmar, Milford, NH, USA), was set to read from the waterline. The offset between the antenna and the transducer position was automatically calibrated by the instrument, and the instrument flagged data output with an internal gyroscope in case of excessive wave action. However, during the whole groundtruthing process, sea conditions were excellent. Data have been collected at a constant speed of 10 knots on parallel transects. Up to eight depth readings were averaged for each UTM navigation point, then tide height was subtracted using open source tide data (http://predmar.cicese.mx/calendarios/). Finally, depth data were converted in a shapefile (n= 5004, red points in

Depth Retrieval in ENVI-SPEAR Tool
Eight scenes were processed with the ENVI-SPEAR tool over the same ROI as 4SM (Figure 1). This tool operates the Log Ratio Transform algorithm developed by Stumpf et al., [22]. It is integrated in the ENVI software (Exelis Visual Information Solutions, Boulder, CO, USA, v.5.3) as a Spectral Processing Exploitation and Analysis Resource (SPEAR) tool, from now ENVI-SPEAR tool. This tool is capable of retrieving relative depths from multispectral images which then are calibrated into meters using an existing depth sounding dataset. To this end, the groundtruthed DTM described above were used. An example of the output is shown in Figure 4c. Alien features were masked. Then an approximate atmospheric correction was applied on the whole image by Dark Pixel Subtraction. Images were pansharpened, then the Log Ratio Transform algorithm was applied. A 3 x 3 median filter was chosen to remove high frequency noise. Then all groundtruthed depth points (n = 5004) were used to calibrate relative depths into absolute depths. In the calibration tool ( Figure 5), it is possible to select a model that best fits data based on r 2 results (linear, exponential, polynomial model). To compare different results, a linear fitting ( Figure 5a) and the model with the highest r 2 were chosen for each scene (e.g. Figure 5b).

Depth Retrieval in ENVI-SPEAR Tool
Eight scenes were processed with the ENVI-SPEAR tool over the same ROI as 4SM (Figure 1). This tool operates the Log Ratio Transform algorithm developed by Stumpf et al., [22]. It is integrated in the ENVI software (Exelis Visual Information Solutions, Boulder, CO, USA, v.5.3) as a Spectral Processing Exploitation and Analysis Resource (SPEAR) tool, from now ENVI-SPEAR tool. This tool is capable of retrieving relative depths from multispectral images which then are calibrated into meters using an existing depth sounding dataset. To this end, the groundtruthed DTM described above were used. An example of the output is shown in Figure 4c. Alien features were masked. Then an approximate atmospheric correction was applied on the whole image by Dark Pixel Subtraction. Images were pansharpened, then the Log Ratio Transform algorithm was applied. A 3 × 3 median filter was chosen to remove high frequency noise. Then all groundtruthed depth points (n = 5004) were used to calibrate relative depths into absolute depths. In the calibration tool ( Figure 5), it is possible to select a model that best fits data based on r 2 results (linear, exponential, polynomial model).
To compare different results, a linear fitting (Figure 5a) and the model with the highest r 2 were chosen for each scene (e.g., Figure 5b).

Groundtruthing Regressions and Comparisons
As regards the accuracy of 4SM depths, pixels with both groundtruthed depths and satellite derived depths are selected and these depth pairs are assigned to bins in decimeters [23]. Bins with few data pairs are excluded as outliers and plotted as red points in the scatterplots of Figure 6. These outliers are generated by various alien features and must be excluded for a fair regression calculation. Then all the remaining bins are averaged into bins in meters. In Figure 6, all one-meter bins which are represented by a star symbol account for a total of 99% of all accepted depth pairs, while the remaining one-meter bins are represented by a white circle. Inside the two parallel gray lines in the scatterplot, satellite retrieved depths within ± 1 m of groundtruthed depths are included. A correlation coefficient (r 2 ) and a Root Mean Squared Error (RMSE) were calculated for each linear model: see Figure 6 and Table 1. Tide heights were adjusted manually and added to seatruth depths in order to minimize the RMSE result. Two scenes stand out with unrealistic tide heights (1.6 m and 1.7 m): this is possibly the result of a bad estimation of the soil line for these two scenes. In order to compare both 4SM and ENVI-SPEAR tool results versus the interpolated DTM of groundtruthed depth points, an accuracy index was estimated by calculating

Groundtruthing Regressions and Comparisons
As regards the accuracy of 4SM depths, pixels with both groundtruthed depths and satellite derived depths are selected and these depth pairs are assigned to bins in decimeters [23]. Bins with few data pairs are excluded as outliers and plotted as red points in the scatterplots of Figure 6. These outliers are generated by various alien features and must be excluded for a fair regression calculation. Then all the remaining bins are averaged into bins in meters.

Groundtruthing Regressions and Comparisons
As regards the accuracy of 4SM depths, pixels with both groundtruthed depths and satellite derived depths are selected and these depth pairs are assigned to bins in decimeters [23]. Bins with few data pairs are excluded as outliers and plotted as red points in the scatterplots of Figure 6. These outliers are generated by various alien features and must be excluded for a fair regression calculation. Then all the remaining bins are averaged into bins in meters. In Figure 6, all one-meter bins which are represented by a star symbol account for a total of 99% of all accepted depth pairs, while the remaining one-meter bins are represented by a white circle. Inside the two parallel gray lines in the scatterplot, satellite retrieved depths within ± 1 m of groundtruthed depths are included. A correlation coefficient (r 2 ) and a Root Mean Squared Error (RMSE) were calculated for each linear model: see Figure 6 and Table 1. Tide heights were adjusted manually and added to seatruth depths in order to minimize the RMSE result. Two scenes stand out with unrealistic tide heights (1.6 m and 1.7 m): this is possibly the result of a bad estimation of the soil line for these two scenes. In order to compare both 4SM and ENVI-SPEAR tool results versus the interpolated DTM of groundtruthed depth points, an accuracy index was estimated by calculating In Figure 6, all one-meter bins which are represented by a star symbol account for a total of 99% of all accepted depth pairs, while the remaining one-meter bins are represented by a white circle. Inside the two parallel gray lines in the scatterplot, satellite retrieved depths within ± 1 m of groundtruthed depths are included. A correlation coefficient (r 2 ) and a Root Mean Squared Error (RMSE) were calculated for each linear model: see Figure 6 and Table 1. Tide heights were adjusted manually and added to seatruth depths in order to minimize the RMSE result. Two scenes stand out with unrealistic tide heights (1.6 m and 1.7 m): this is possibly the result of a bad estimation of the soil line for these two scenes. In order to compare both 4SM and ENVI-SPEAR tool results versus the interpolated DTM of groundtruthed depth points, an accuracy index was estimated by calculating Depth_residual = (Depth_retrieved−Depth_measured). So a positive depth residual signals an overestimated depth, and vice versa. Depth residuals were classified in 5 classes of accuracy, and the percentage of pixels belonging to each class was calculated (Figure 7).

Results
This section first presents the results of the seatruth regressions ( Figures 5 and 6), then the results of the accuracy assessment for retrieved depth (Figure 7), and finally the depth residuals ( Figure 8).

Results
This section first presents the results of the seatruth regressions ( Figures 5 and 6), then the results of the accuracy assessment for retrieved depth (Figure 7), and finally the depth residuals ( Figure 8).

Seatruth Regressions
As regards 4SM results, linear relationships between retrieved depths and groundtruthed depths are shown for each scene in Figure 6. The regression lines do not account for all depth pairs; red outliers are excluded from the statistics. Linear regression model explained in excess of 80% of the depth variations. The 27 October 2016 scene reports the highest r 2 (0.99) although it also reports the highest RMSE (2.11 m). The 22 October 2014 scene scored the lowest RMSE. From Figure 6 it is also possible to see how combining depths improved linear fitting results and reduced the noise.
For ENVI-SPEAR tool results, please refer to Figure 5. In Figure 5a a linear model fitting is applied to the scatterplot, while in Figure 5b the best model that showed the higher r 2 is plotted. In particular, for eight ENVI-SPEAR scenes regression plots, the highest correlation coefficient r 2 was always achieved with a polynomial model.

Accuracy Assessment
Accuracy assessments are presented in Figure 7. The accuracy index allowed a visual estimation of overall accuracy of the retrieving methods applied for each scene. In terms of % of accuracy within ±1 m of groundtruthed depths, 4SM performed better in 4 out of 9 scenes; in the 3 remaining scenes, it scored similar results with ENVI-SPEAR with the exception of one scene: 22 October 2014 ( Figure 7A.1 and black bars in linked barplot chart) that is reported to be further discussed. In Figure 7B, 19 October 2013 scene is reported because 4SM scored its best results (50% of pixel within ±1 m of groundtruthed depths, Figure 7B.1 and black bars in linked barplot chart). Over shallow bright bottoms, 4SM performed better than ENVI-SPEAR ( Figure 7A,B white arrows); in particular, with a linear fitting model, ENVI-SPEAR tends to underestimate depth by more than 3 m over bright bottom areas ( Figure 7A.2,B.2). It is also observed, in Figure 5a, that linear fitting of ENVI-SPEAR results exhibits a detection limit: deeper than ~15 m, most retrieved depths are not correlated to real depths anymore; the polynomial model exhibits a better fit because of the curved shape of scatterplots above 0.8 Log Ratio results (Figure 5b). Moreover, in Figure 7A Figures A1-A3), accuracy of the methods is similar. Therefore, in spite of the adverse conditions of the SLC, and without the need of any field data, the 4SM method is comparable to the ENVI-SPEAR method, and equally valid.

Seatruth Regressions
As regards 4SM results, linear relationships between retrieved depths and groundtruthed depths are shown for each scene in Figure 6. The regression lines do not account for all depth pairs; red outliers are excluded from the statistics. Linear regression model explained in excess of 80% of the depth variations. The 27 October 2016 scene reports the highest r 2 (0.99) although it also reports the highest RMSE (2.11 m). The 22 October 2014 scene scored the lowest RMSE. From Figure 6 it is also possible to see how combining depths improved linear fitting results and reduced the noise.
For ENVI-SPEAR tool results, please refer to Figure 5. In Figure 5a a linear model fitting is applied to the scatterplot, while in Figure 5b the best model that showed the higher r 2 is plotted. In particular, for eight ENVI-SPEAR scenes regression plots, the highest correlation coefficient r 2 was always achieved with a polynomial model.

Accuracy Assessment
Accuracy assessments are presented in Figure 7. The accuracy index allowed a visual estimation of overall accuracy of the retrieving methods applied for each scene. In terms of % of accuracy within ±1 m of groundtruthed depths, 4SM performed better in 4 out of 9 scenes; in the 3 remaining scenes, it scored similar results with ENVI-SPEAR with the exception of one scene: 22 October 2014 ( Figure 7A.1 and black bars in linked barplot chart) that is reported to be further discussed. In Figure 7B, 19 October 2013 scene is reported because 4SM scored its best results (50% of pixel within ±1 m of groundtruthed depths, Figure 7B.1 and black bars in linked barplot chart). Over shallow bright bottoms, 4SM performed better than ENVI-SPEAR ( Figure 7A,B white arrows); in particular, with a linear fitting model, ENVI-SPEAR tends to underestimate depth by more than 3 m over bright bottom areas ( Figure 7A.2,B.2). It is also observed, in Figure 5a, that linear fitting of ENVI-SPEAR results exhibits a detection limit: deeper than~15 m, most retrieved depths are not correlated to real depths anymore; the polynomial model exhibits a better fit because of the curved shape of scatterplots above 0.8 Log Ratio results (Figure 5b). Moreover, in Figure 7A Figures A1-A3), accuracy of the methods is similar. Therefore, in spite of the adverse conditions of the SLC, and without the need of any field data, the 4SM method is comparable to the ENVI-SPEAR method, and equally valid.

Depth Residuals
Depth residuals are defined by the absolute difference between combined 4SM depths and DTM. Depth residuals are represented graphically in Figure 8. Most of the depth residuals were ≤0.5 m, especially over bright shallow and deeper (≈15 m) substrate, where 4SM showed more consistency. Conversely, higher residuals were found in two areas corresponding to darker bottoms (see also Figure 7A,B black arrows). Over time this area showed a change in bottom properties, when in 22 October 2014 a large portion of a low albedo patch on the northern side disappeared and wasn't recorded anymore. Finally, it is evident how areas below 20 m were the ones that showed higher residuals, where depth retrieval reaches its optical limit in this environment.

San Lorenzo Channel's Conditions
The results suggest that 4SM can be safely used on single scenes under reasonable conditions of low cloud cover, low glint effects, and homogeneous vertical and horizontal water optical properties. The SLC did not show any relevant variations in depth along the four years analyzed. However, the area was characterized by high seasonal variations in vertical and horizontal stratification of the waters; the same can be said for variations of spectral characteristic of the bottom, that are currently under investigation (Favoretto et al., unpublished data).
The application of 4SM not only allowed the retrieval of the bathymetry of the SLC that showed to be consistent with groundtruthed depths, but it generated a bathymetry model for the whole shallow area in the Bay of La Paz (Figure 9). In particular, the SLC showed a fair amount of layered waters with seasonal and spatial complexity, and 4SM does account to a limited extent for such layered waters while calibrating the simplified RTE. Overall, waters in the channel were vertically stratified, with common algal blooms events (red tides) in the complex hydrodynamic conditions in the Bay of La Paz ( [31] and references therein). In the 22 October 2013 scene for example, deep oceanic waters are covered by an upper layer of Coastal waters: in the San Gabriel bay (Figure 1, red square), this upper layer is~5 m thick, but it is~9 m thick in the SLC. Such heterogeneity is commonly found through the seasonal cycle for the scenes investigated. All of this considered, it is possible to obtain useful information even from low quality areas in the scenes, accounting for their limitations.

Depth Residuals
Depth residuals are defined by the absolute difference between combined 4SM depths and DTM. Depth residuals are represented graphically in Figure 8. Most of the depth residuals were ≤0.5 m, especially over bright shallow and deeper (≈15 m) substrate, where 4SM showed more consistency. Conversely, higher residuals were found in two areas corresponding to darker bottoms (see also Figure 7A,B black arrows). Over time this area showed a change in bottom properties, when in 22 October 2014 a large portion of a low albedo patch on the northern side disappeared and wasn't recorded anymore. Finally, it is evident how areas below 20 m were the ones that showed higher residuals, where depth retrieval reaches its optical limit in this environment.

San Lorenzo Channel's Conditions
The results suggest that 4SM can be safely used on single scenes under reasonable conditions of low cloud cover, low glint effects, and homogeneous vertical and horizontal water optical properties. The SLC did not show any relevant variations in depth along the four years analyzed. However, the area was characterized by high seasonal variations in vertical and horizontal stratification of the waters; the same can be said for variations of spectral characteristic of the bottom, that are currently under investigation (Favoretto et al., unpublished data).
The application of 4SM not only allowed the retrieval of the bathymetry of the SLC that showed to be consistent with groundtruthed depths, but it generated a bathymetry model for the whole shallow area in the Bay of La Paz (Figure 9). In particular, the SLC showed a fair amount of layered waters with seasonal and spatial complexity, and 4SM does account to a limited extent for such layered waters while calibrating the simplified RTE. Overall, waters in the channel were vertically stratified, with common algal blooms events (red tides) in the complex hydrodynamic conditions in the Bay of La Paz ( [31] and references therein). In the 22 October 2013 scene for example, deep oceanic waters are covered by an upper layer of Coastal waters: in the San Gabriel bay (Figure 1, red square), this upper layer is ~5 m thick, but it is ~9 m thick in the SLC. Such heterogeneity is commonly found through the seasonal cycle for the scenes investigated. All of this considered, it is possible to obtain useful information even from low quality areas in the scenes, accounting for their limitations.

Models Comparison
In Figure 7A,B, RGB color composite present the worst (A) and the best (B) scenes in terms of 4SM accuracy. It is important to note a major change in bottom composition from 2013 that clearly show a dark patch (black arrow Figure 7A) of what probably was macroalgae (Favoretto et al., unpublished data) that disappeared in 2014, and up to now it has not been detected again. This change may have been caused by Hurricane Odile in September 2014, that displaced significant amounts of sediments (Favoretto et al., unpublished data). This event allowed for a comparison between low-albedo bottom processing capabilities of 4SM and ENVI-SPEAR. The bottom albedo independent nature of ENVI-SPEAR (Stumpf's) algorithm should guarantee in some limits that dark bottoms are shown at the same depth as bright sand, when field data report so. However, the method applied in the SLC shows how depths over dark bottoms are overestimated within 5-10 m depth range ( Figure 7B.2,B.3). In particular, the linear model calibration of ENVI-SPEAR algorithm yields higher depth residuals than the polynomial model calibration. (Figure 7A.2,A.3). This limitation that was already pointed out in the introduction of this article about Stumpf's algorithm. As the results suggests, 4SM perform better over very bright shallow areas, but has the same problems as ENVI-SPEAR over very dark bottoms ( Figure 7B.1).
In the 3-10 m range, retrieved depths are over-estimated by 4SM: this means that bottom substrates are actually less green than assumed by the Soil Line in 4SM. In this depth range, dense red coralline algae formations, called rhodolith beds, characterize the area [25,26]. Coralline algae absorb additional wavelength over the green range for their photosynthetic activities, and their common presence in the area could in part explain a lower than expected green reflectance. This hypothesis is currently under investigation (Favoretto et al., unpublished data).
Over the 10-20 m range, most retrieved depths are under-estimated by 4SM: this means that bottom substrates are actually greener than assumed by the Soil Line in 4SM. This depth range is present in the SLC exclusively in its central portion, where tidal currents are supposed to merge in stronger bidirectional deeper currents. In this portion of the channel, where strong currents shape the sandy bottom: cyanobacterial biofilms can cover large portions of the seabed (Favoretto et al., in prep). These organisms, stretching for meters, can have a significant production and affect the green reflectivity of the substrate in the green band (see Appendix D).

The 4SM Method
In 4SM the detection of the shallow bottom in more than two wavebands allows for a better estimation of Z, and therefore yields a richer spectral bottom reflectance associated to the pixel. To this extent, and from many tests made in the development of 4SM (see www.watercolumncorrection.com, and [23]) it can be said that 4SM is not site-specific, and is capable of delivering both a bathymetric map and a water column corrected image in units of image's DN over many different water types, in different location of the world, when the high cost of collecting similar data in the field is simply not affordable. While an empirical method (e.g., [21]) explores the statistical relationship between image pixel values and field measured depths, 4SM operates a radiance inversion approach which does not use any field measured water depths for calibration. Using 4SM there is no need for a formal atmospheric correction since the spectral path radiance and the water volume reflectance are estimated through the calibration process. All of these advantages reduce artifacts and enhance operability, simplifying image processing and interpretation.
For each shallow pixel, the 4SM results are an estimate of water depth, and an acceptable fit of the water column corrected spectral bottom signature with the Soil Line, although contrasted bottom signatures entail potentially severe bias on retrieved depth. Another advantage of the 4SM method is the pansharpening adaptation that generates 15 m resolution images to be modelled. Using this modified pansharpening algorithm, pixels which are brighter than their surrounding in the PAN band get a boost in the multispectral band and vice versa. Other empirical methods use only multispectral bands, and this is applicable as long as there is enough contrast in colors (e.g., K blue < K green < K red ) like in clear oceanic waters. However, in coastal waters, this is not the case and there is hardly any color separation between K blue and K green . This actually is a fundamental limitation which precludes a reliable estimation of the model parameters for Coastal water types in methods like Lyzenga's and Stumpf's. The PAN solution offers a valuable alternative, as it will always generate enough color contrast, even with Coastal type waters. In the end, 4SM uses the image metadata to convert spectral water column corrected bottom signatures into calibrated reflectance (0−1), ready for bottom typing and time series studies. The method produces a low tide view of the shallow areas along with a DTM; this is a unique feature of 4SM, apart from semi-analytical methods [10].
Moreover, the application of combined depths improved model fitting results; however, it did not improve accuracy compared to other scenes. Strong depth residuals (>2 m) can hardly be interpreted in this case as caused by natural or anthropic events; they are likely noise in depth retrievals due to local perturbations like atmospheric or hydrological effects, but also phytoplankton blooms, turbid waters, wind or even boats wakes. Therefore, any pixel that shows this kind of variation should not be considered in the overall depth model. Combining depths is an important tool in reducing these types of noise (that are inevitable for the practitioner). The fact that most of the pixels depth residuals less than 0.5 m (Figure 8) in the 0 to 20 m depth range is supports 4SM as a robust depth retrieval method that can cope, to a limited extent, with a layered structure of the water column.

Conclusions
It is possible to conclude that: • 4SM is independent on field data to achieve the optical calibration; • it offers a simpler operational flowchart compared to previous methods (e.g., [16,19,22]); • its accuracy is equally valid, and in some case better, compared to the accepted and widely used Stumpf's algorithm; • it provides a priori important insight on the optical properties of the water column (spectral K, i.e., water quality), and also on the hydrological conditions; • it uses all bands with significant bottom detection and delivers computed depths, and water column corrected spectral bottom reflectance; • it provides all valuable information that allows to explore and monitor large coastal areas in a more efficient and cheaper way in terms of resources and time.
These results highlight the progress accomplished by 4SM as a band ratio method for satellite derived bathymetry, especially if considering its the independence from any field calibration, and show how the 4SM algorithm can be a relevant alternative to traditional ratio-methods.

Appendix B
Appendix B: two examples of clear-cut calibration diagrams. In Figures A4 and A5, X2, X3 and X5 denote the linearized Blue, Green and Red bands respectively (Equation (4)). The backdrop in shades of gray represents the bi-dimensional histogram for all image pixels. Blue dots are the actual pixels used for calibration of the BPL, each referenced to its row/line position in the image. Small white circles represent the scatter of averaged bare land pixels, as a proxy for the soil line.  Figure 1). Blue dots are the actual pixels used for BPL calibration, each referenced to its row/line position in the image. Small white circles represent the scatter of averaged bare land pixels, as a proxy for the Soil Line.
The 11 October 2016 scene offers a nice and straightforward optical calibration diagram for very clear waters. In Figure A4a, the BPL pixels (blue dots) display along a straight line over a depth range

Appendix B
Appendix B: two examples of clear-cut calibration diagrams. In Figures A4 and A5, X2, X3 and X5 denote the linearized Blue, Green and Red bands respectively (Equation (4)). The backdrop in shades of gray represents the bi-dimensional histogram for all image pixels. Blue dots are the actual pixels used for calibration of the BPL, each referenced to its row/line position in the image. Small white circles represent the scatter of averaged bare land pixels, as a proxy for the soil line.

Appendix B
Appendix B: two examples of clear-cut calibration diagrams. In Figures A4 and A5, X2, X3 and X5 denote the linearized Blue, Green and Red bands respectively (Equation (4)). The backdrop in shades of gray represents the bi-dimensional histogram for all image pixels. Blue dots are the actual pixels used for calibration of the BPL, each referenced to its row/line position in the image. Small white circles represent the scatter of averaged bare land pixels, as a proxy for the soil line.  Figure 1). Blue dots are the actual pixels used for BPL calibration, each referenced to its row/line position in the image. Small white circles represent the scatter of averaged bare land pixels, as a proxy for the Soil Line.
The 11 October 2016 scene offers a nice and straightforward optical calibration diagram for very clear waters. In Figure A4a, the BPL pixels (blue dots) display along a straight line over a depth range Figure A4. Plot of linearized calibration data (Equation (4)) for the whole of the 11 October 2016 scene. Bands 2, 3 and 5 are Blue, Green and Red, respectively. (a) is the calibration diagram of linearized Blue (X 2 ) and Green (X 3 ) and reports estimated K 2 /K 3 values with Jerlov water types. (b) is the calibration diagram for Blue (X 2 ), Green (X 3 ) and Red (X 5 ) bands respectively. The backdrop in shades of gray represents the bi-dimensional histogram for all image pixels (white ROI in Figure 1). Blue dots are the actual pixels used for BPL calibration, each referenced to its row/line position in the image. Small white circles represent the scatter of averaged bare land pixels, as a proxy for the Soil Line.
The 11 October 2016 scene offers a nice and straightforward optical calibration diagram for very clear waters. In Figure A4a, the BPL pixels (blue dots) display along a straight line over a depth range of~40 m; the slope of this line is the ratio K blue /K green = 0.47. In Figure A4b, the BPL pixels (blue and green dots) display along two straight lines over a depth range of~5 m, with slopes K blue /K red = 0.103 and K green /K red = 0.219. Please note that 0.103/0.219 = 0.47. Using this value to interpolate spectral K from Jerlov's data yields the following values in units of m −1 : K 1 = 0.075, K 2 = 0.083, K 3 = 0.174 and K 5 = 0.651. This case is misleading though, as the optical properties of the waters in this area exhibit much variability, both horizontally and vertically.   Figure 1). Blue dots are the actual pixels used for BPL calibration, each referenced to its row/line position in the image. Small white circles represent the scatter of averaged bare land pixels, as a proxy for the Soil Line.
The 29 January 2016 scene offers a nice and straightforward optical calibration diagram for Coastal waters of Jerlov. In Figure A5a, the BPL pixels (blue dots) display along a straight line over a depth range of ~30 m; the slope of this line is the ratio Kblue/Kgreen = 0.79. Using this value to interpolate spectral K from Jerlov's data yields the following values in units of m −1 : K1 = 0.191, K2 = 0.186, K3 = 0.234 and K5 = 0.878. Please note that, if Kblue = Kgreen, the ratio Kblue/Kgreen = 1.0 and there is no color separation at all by diffuse attenuation between these two bands: many shallow pixels would display as a function of noise. Therefore, unlike the Pan solution, which achieves good color separation [23], we can expect that the Green solution would yield bad depth results for coastal waters. In Figure A5b, the ratio Kblue/Kred = 0.33 and the ratio Kgreen/Kred = 0.37. Please note that 0.33/0.37 = 0.89: the upper layer in the 0-5 m depth range might be slightly less clear.

Appendix C
Eight ENVI-SPEAR calibration plots are displayed. Left is linear fitting, right is the best model fitting according to the coefficient of determination r 2 . Figure A5. Plot of linearized calibration data (Equation (4)) for the whole of the 29 January 2016 scene. Bands 2, 3 and 5 are Blue, Green and Red, respectively. (a) is the calibration diagram of linearized Blue (X 2 ) and Green (X 3 ) and reports estimated K 2 /K 3 values with Jerlov water types. (b) is the calibration diagram for Blue (X 2 ), Green (X 3 ) and Red (X 5 ) bands respectively. The backdrop in shades of gray represents the bi-dimensional histogram for all image pixels (white ROI in Figure 1). Blue dots are the actual pixels used for BPL calibration, each referenced to its row/line position in the image. Small white circles represent the scatter of averaged bare land pixels, as a proxy for the Soil Line.
The 29 January 2016 scene offers a nice and straightforward optical calibration diagram for Coastal waters of Jerlov. In Figure A5a, the BPL pixels (blue dots) display along a straight line over a depth range of~30 m; the slope of this line is the ratio K blue /K green = 0.79. Using this value to interpolate spectral K from Jerlov's data yields the following values in units of m −1 : K 1 = 0.191, K 2 = 0.186, K 3 = 0.234 and K 5 = 0.878. Please note that, if K blue = K green , the ratio K blue /K green = 1.0 and there is no color separation at all by diffuse attenuation between these two bands: many shallow pixels would display as a function of noise. Therefore, unlike the Pan solution, which achieves good color separation [23], we can expect that the Green solution would yield bad depth results for coastal waters. In Figure A5b, the ratio K blue /K red = 0.33 and the ratio K green /K red = 0.37. Please note that 0.33/0.37 = 0.89: the upper layer in the 0-5 m depth range might be slightly less clear.

Appendix C
Eight ENVI-SPEAR calibration plots are displayed. Left is linear fitting, right is the best model fitting according to the coefficient of determination r 2 .