F.J. Lopez Dekker
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25 records found
1
Encoding SAR ocean signatures into latent space
Capturing Multi-Scale Ocean Phenomena in SAR Imagery with Variational Autoencoders
Using 220,000 Sentinel-1 Wave Mode images co-located with ERA5 reanalysis data, VAE architectures were trained across four latent dimensionalities (32, 64, 128 and 256). The multi-scale complexity of SAR scenes introduced a strong frequency bias: standard pixel-wise losses such as Mean Squared Error failed to capture fine-scale detail, and conventional metrics such as PSNR and SSIM proved insufficient to measure this. Frequency Focal Loss (FFL) was incorporated to address reconstruction in the spectral domain, alongside a dynamic weight matrix that refocuses the loss on difficult-to-learn features. Dynamically annealing loss term weights had a striking effect on reconstruction quality, and subsequent hyperparameter optimisation using Optuna further confirmed that loss function tuning dominates over architectural choices. This sensitivity to loss function design is a central finding of this work.
VAEs successfully reconstructed large- and intermediate-scale ocean patterns at latent dimensions of 128 and 256. For air-sea flux estimation, three configurations were compared: a direct CNN regressor, a frozen VAE encoder with regression head, and a jointly trained VAE. All three underperform the physics-informed approach of O'Driscoll et al.\cite{o2023obukhov}, suggesting unsupervised deep learning alone cannot extract flux-relevant information, though task objectives incorporate ...
Using 220,000 Sentinel-1 Wave Mode images co-located with ERA5 reanalysis data, VAE architectures were trained across four latent dimensionalities (32, 64, 128 and 256). The multi-scale complexity of SAR scenes introduced a strong frequency bias: standard pixel-wise losses such as Mean Squared Error failed to capture fine-scale detail, and conventional metrics such as PSNR and SSIM proved insufficient to measure this. Frequency Focal Loss (FFL) was incorporated to address reconstruction in the spectral domain, alongside a dynamic weight matrix that refocuses the loss on difficult-to-learn features. Dynamically annealing loss term weights had a striking effect on reconstruction quality, and subsequent hyperparameter optimisation using Optuna further confirmed that loss function tuning dominates over architectural choices. This sensitivity to loss function design is a central finding of this work.
VAEs successfully reconstructed large- and intermediate-scale ocean patterns at latent dimensions of 128 and 256. For air-sea flux estimation, three configurations were compared: a direct CNN regressor, a frozen VAE encoder with regression head, and a jointly trained VAE. All three underperform the physics-informed approach of O'Driscoll et al.\cite{o2023obukhov}, suggesting unsupervised deep learning alone cannot extract flux-relevant information, though task objectives incorporate
In Search of Closure
Multiple Scattering Mechanisms in Synthetic Aperture Radar Interferometry
Since the coexistence of a geophysical component and phase noise is acknowledged, predicting the contribution of the phase noise and subsequently quantifying the significance of the geophysical closure phase help justify its non-negligibility and assess the feasibility of further investigating the underlying scattering mechanisms. Following this rationale, this research begins by characterizing the significance of closure phases through a statistical approach. The analysis is conducted over a large spatiotemporal scale using Sentinel-1 acquisitions, thereby providing a general perspective on the prevalence of significant closure phases.
With the aid of the current analytical understanding of the geophysical origins of closure phases, soil moisture variations, and volumetric scattering in combination with perpendicular baselines, we investigate the correlation between closure phases and these geophysical factors. Combined with the statistical significance, this approach allows us to quantify the explainable variance in the observations. The results indicate that a substantial portion of the observed signals remains unexplained by existing models, highlighting the limitations of current knowledge in explaining the observed signals.
The correlation between the unexplained variance in the observed closure phase and land use provides additional insights into their potential physical origins, particularly the high correlation with agriculture fields. This finding motivates a focused investigation into the geophysical closure phases related to vegetation. To this end, we selected croplands in southern Spain to examine vegetation-induced closure phases by qualitatively comparing Sentinel-1 observations with vegetation parameters, such as crop calendar and Leaf Area Index (LAI). The analysis reveals a clear signal associated with vegetation development. We proposed two models: one accounting for variations in vegetation water content and another considering line-of-sight (LoS) motion introduced by vegetation growth. Both models offer plausible explanations for the observed signatures and extend the analytical understanding of the individual scattering mechanisms contributing to geophysical closure phases. Building on these insights, we develop a composite model to integrate as many known mechanisms as possible, including soil moisture variations, ground surface scattering, and vegetation water content changes. Although the model predictions demonstrate an improved understanding and provide a partial analytical representation of the relevant processes, we remain in search of closure regarding the origins of geophysical closure phases. Future physical modeling efforts should therefore aim to capture the coupled effects arising from multiple scattering mechanisms.
Overall, this dissertation presents the prevalence of statistically significant closure phases, quantifies the extent to which the observed signals can be explained by current knowledge, identifies clear closure phase signatures associated with vegetation development, provides analytical representations of vegetation-related scattering mechanisms, integrates known processes within a composite analytical framework, and highlights that the coupled effects of multiple scattering mechanisms should be considered in future studies. ...
Since the coexistence of a geophysical component and phase noise is acknowledged, predicting the contribution of the phase noise and subsequently quantifying the significance of the geophysical closure phase help justify its non-negligibility and assess the feasibility of further investigating the underlying scattering mechanisms. Following this rationale, this research begins by characterizing the significance of closure phases through a statistical approach. The analysis is conducted over a large spatiotemporal scale using Sentinel-1 acquisitions, thereby providing a general perspective on the prevalence of significant closure phases.
With the aid of the current analytical understanding of the geophysical origins of closure phases, soil moisture variations, and volumetric scattering in combination with perpendicular baselines, we investigate the correlation between closure phases and these geophysical factors. Combined with the statistical significance, this approach allows us to quantify the explainable variance in the observations. The results indicate that a substantial portion of the observed signals remains unexplained by existing models, highlighting the limitations of current knowledge in explaining the observed signals.
The correlation between the unexplained variance in the observed closure phase and land use provides additional insights into their potential physical origins, particularly the high correlation with agriculture fields. This finding motivates a focused investigation into the geophysical closure phases related to vegetation. To this end, we selected croplands in southern Spain to examine vegetation-induced closure phases by qualitatively comparing Sentinel-1 observations with vegetation parameters, such as crop calendar and Leaf Area Index (LAI). The analysis reveals a clear signal associated with vegetation development. We proposed two models: one accounting for variations in vegetation water content and another considering line-of-sight (LoS) motion introduced by vegetation growth. Both models offer plausible explanations for the observed signatures and extend the analytical understanding of the individual scattering mechanisms contributing to geophysical closure phases. Building on these insights, we develop a composite model to integrate as many known mechanisms as possible, including soil moisture variations, ground surface scattering, and vegetation water content changes. Although the model predictions demonstrate an improved understanding and provide a partial analytical representation of the relevant processes, we remain in search of closure regarding the origins of geophysical closure phases. Future physical modeling efforts should therefore aim to capture the coupled effects arising from multiple scattering mechanisms.
Overall, this dissertation presents the prevalence of statistically significant closure phases, quantifies the extent to which the observed signals can be explained by current knowledge, identifies clear closure phase signatures associated with vegetation development, provides analytical representations of vegetation-related scattering mechanisms, integrates known processes within a composite analytical framework, and highlights that the coupled effects of multiple scattering mechanisms should be considered in future studies.
Fluxes and flows
Characterizing the air-sea interface with spaceborne radars
Like plenty of rumors, these, too, were grounded in some truth: SEASAT had shed light on many a mystery, though primarily in the field of physical sciences rather than Cold War conspiracies. Nonetheless, the value of spaceborne oceanography was now clear, and space agencies around the world did not stand idly by. Europe quickly followed suit with its own missions, launching in succession a series of high-resolution imagers, including ERS-1, ERS-2, ENVISAT, and, since 2014, the Sentinel-1 constellation.
Aided by these instruments and many others, the previous decades have been marked by continued scientific advances in the ever-growing field of radar oceanography. Building on that rich heritage, this dissertation aims to advance two distinct (but entwined) subdomains relating to either side of the air-sea interface.
In the first half of this dissertation, Chapters 2 and 3, we investigate the ubiquitous yet often overlooked atmospheric features present in most high-resolution radar images of the ocean. It may seem counterintuitive to study the atmosphere using ocean imagery, but much of the ocean’s surface variability is wind-driven, such that the ocean surface acts as a mirror for the wind field aloft. Till recently, the only systematic use for these atmospheric features had been in studies aiming to relate (an)isotropy to wind directions. But the information content is rich, and much more can be done.
In Chapter 2, we show that significant quantities of atmospheric information remain unexploited. And by using a domain-inspired encoding scheme, we transform high-dimensional radar images into a much lower-dimensional latent space, from which we extract substantially more atmospheric information than preexisting analytical methods.
Then in Chapter 3 we leverage the ever-increasing catalog of Sentinel-1 observations to go one step further. We illustrate that radar-derived atmospheric variables are complementary to state-of-the-art and reference atmospheric estimates. The challenge here is one of persuasion: how to argue that new estimates can complement state-of-the-art estimates when there are insufficient “ground truth” measurements to reconcile discrepancies between them? We aim to address this difficulty through a series of qualitative and quantitative assessments.
In the second half of the dissertation, Chapters 4 and 5, we switch to the other side of the air-sea interface, to investigate different methods of retrieving surface currents—a long-standing challenge in spaceborne oceanography. First, we investigate surface current retrieval for a proposed satellite modification, DopSCA, in Chapter 4. This system could be uniquely capable of retrieving surface current information, but its unorthodox design makes it susceptible to several additional noise sources. One of these noise sources, which we refer to as leakage—the undesired interaction between geometric Doppler, azimuthal backscatter gradients, and the antenna pattern—is investigated to assess its mission-compromising potential. Fortunately, this seems to be a comparatively minor issue.
Then, using a very different instrument in Chapter 5, we consider an alternative surface-current retrieval that incorporates polarimetry. Here we rely on the cross-correlation between wave motion, its radar cross section, and polarization to disentangle the convolved mixture of signals received by the satellite. Simulations and limited real observations illustrate that this approach may be a fruitful avenue towards the long-standing challenge of distinguishing between wave- and current motions. Future systems with additional polarimetric capabilities, such as Harmony or Sentinel-1 Next Generation, stand to gain from this approach in particular.
To summarize, this dissertation investigates radar-based retrieval of heat and momentum transport (from atmospheric convection and surface currents, respectively) by exploiting unique observational properties of a variety of radar satellites. We’ve made progress in both domains: providing the first quantitative and SAR-retrieved air-sea heat-flux estimates, and introducing a new method for surface-current retrieval. But fear not, enough work remains to entertain many radar oceanographers to come ;)
...
Like plenty of rumors, these, too, were grounded in some truth: SEASAT had shed light on many a mystery, though primarily in the field of physical sciences rather than Cold War conspiracies. Nonetheless, the value of spaceborne oceanography was now clear, and space agencies around the world did not stand idly by. Europe quickly followed suit with its own missions, launching in succession a series of high-resolution imagers, including ERS-1, ERS-2, ENVISAT, and, since 2014, the Sentinel-1 constellation.
Aided by these instruments and many others, the previous decades have been marked by continued scientific advances in the ever-growing field of radar oceanography. Building on that rich heritage, this dissertation aims to advance two distinct (but entwined) subdomains relating to either side of the air-sea interface.
In the first half of this dissertation, Chapters 2 and 3, we investigate the ubiquitous yet often overlooked atmospheric features present in most high-resolution radar images of the ocean. It may seem counterintuitive to study the atmosphere using ocean imagery, but much of the ocean’s surface variability is wind-driven, such that the ocean surface acts as a mirror for the wind field aloft. Till recently, the only systematic use for these atmospheric features had been in studies aiming to relate (an)isotropy to wind directions. But the information content is rich, and much more can be done.
In Chapter 2, we show that significant quantities of atmospheric information remain unexploited. And by using a domain-inspired encoding scheme, we transform high-dimensional radar images into a much lower-dimensional latent space, from which we extract substantially more atmospheric information than preexisting analytical methods.
Then in Chapter 3 we leverage the ever-increasing catalog of Sentinel-1 observations to go one step further. We illustrate that radar-derived atmospheric variables are complementary to state-of-the-art and reference atmospheric estimates. The challenge here is one of persuasion: how to argue that new estimates can complement state-of-the-art estimates when there are insufficient “ground truth” measurements to reconcile discrepancies between them? We aim to address this difficulty through a series of qualitative and quantitative assessments.
In the second half of the dissertation, Chapters 4 and 5, we switch to the other side of the air-sea interface, to investigate different methods of retrieving surface currents—a long-standing challenge in spaceborne oceanography. First, we investigate surface current retrieval for a proposed satellite modification, DopSCA, in Chapter 4. This system could be uniquely capable of retrieving surface current information, but its unorthodox design makes it susceptible to several additional noise sources. One of these noise sources, which we refer to as leakage—the undesired interaction between geometric Doppler, azimuthal backscatter gradients, and the antenna pattern—is investigated to assess its mission-compromising potential. Fortunately, this seems to be a comparatively minor issue.
Then, using a very different instrument in Chapter 5, we consider an alternative surface-current retrieval that incorporates polarimetry. Here we rely on the cross-correlation between wave motion, its radar cross section, and polarization to disentangle the convolved mixture of signals received by the satellite. Simulations and limited real observations illustrate that this approach may be a fruitful avenue towards the long-standing challenge of distinguishing between wave- and current motions. Future systems with additional polarimetric capabilities, such as Harmony or Sentinel-1 Next Generation, stand to gain from this approach in particular.
To summarize, this dissertation investigates radar-based retrieval of heat and momentum transport (from atmospheric convection and surface currents, respectively) by exploiting unique observational properties of a variety of radar satellites. We’ve made progress in both domains: providing the first quantitative and SAR-retrieved air-sea heat-flux estimates, and introducing a new method for surface-current retrieval. But fear not, enough work remains to entertain many radar oceanographers to come ;)
SAR-based Flood Monitoring
Comparison of Synthetic Aperture Radar sources on the Water-Land Boundary estimation for flood events in the Netherlands
Evaluation of the modeled results using an error matrix at the acquisition time showed that 67% and 68% of the pixels were correctly classified from the flood extents derived from Capella Space and Sentinel-1, respectively. The maximum flood extent from Sentinel-1 data decreased to 45% correct classification when compared to the modeled results at the peak of the flood. This is consistent with the acquisition times, which were taken before and two days after the flood peak, missing the peak flood moment. SAR-based water levels showed an overall precision of 0.141 m for Capella Space and 0.156 m for Sentinel-1. Agreement with water level gauge measurements was better in flatter, less vegetated areas and lower in steep, vegetated areas. Achieving consistent 20 cm water level accuracy (as required by the Dutch Ministry of Infrastructure and Water Management), across the study area remains complex. Both methods are prone to false positives and negatives, especially in areas with steep slopes, narrow canals, high vegetation, or roads. False classifications result in inaccurate flood extents, thus decreasing water level accuracy. Higher resolution of Capella Space images provided better alignment with the maximum flood extent, while Sentinel-1 images have wider coverage but missed the timing of the flood peak. In the end, the choice of SAR-system depends on timing, surface characteristics, and mapping extent needs. ...
Evaluation of the modeled results using an error matrix at the acquisition time showed that 67% and 68% of the pixels were correctly classified from the flood extents derived from Capella Space and Sentinel-1, respectively. The maximum flood extent from Sentinel-1 data decreased to 45% correct classification when compared to the modeled results at the peak of the flood. This is consistent with the acquisition times, which were taken before and two days after the flood peak, missing the peak flood moment. SAR-based water levels showed an overall precision of 0.141 m for Capella Space and 0.156 m for Sentinel-1. Agreement with water level gauge measurements was better in flatter, less vegetated areas and lower in steep, vegetated areas. Achieving consistent 20 cm water level accuracy (as required by the Dutch Ministry of Infrastructure and Water Management), across the study area remains complex. Both methods are prone to false positives and negatives, especially in areas with steep slopes, narrow canals, high vegetation, or roads. False classifications result in inaccurate flood extents, thus decreasing water level accuracy. Higher resolution of Capella Space images provided better alignment with the maximum flood extent, while Sentinel-1 images have wider coverage but missed the timing of the flood peak. In the end, the choice of SAR-system depends on timing, surface characteristics, and mapping extent needs.
Small Scales, Vast Ocean
Submesoscale Ocean Topography with Bistatic Synthetic-aperture Radar Interferometry
Synthetic-aperture radar (SAR) is a unique remote sensing instrument, particularly at C-band, capable of sensing the ocean surface at the submesoscales, with a wide swath, and in nearly all weather conditions. Harmony, the European Space Agency’s 10th Earth Explorer, features two SAR companion satellites. Two, out of a total of five, years of the mission’s life will be spent in a formation where the system will operate as a cross-track interferometer. Cross-track interferometry (XTI) is a technique that estimates the relative height of the surface from two SAR images of the same scene. Thus, Harmony could theoretically retrieve variations of the OST. In other words, the system could operate as a bistatic wide-swath ocean altimeter (WSOA). At the same time, Harmony will retrieve stress-equivalent wind fields, and instantaneous surface currents. Therefore, Harmony has the potential of providing an unprecedented wealth of co-located simultaneous data related to the ocean and the atmosphere. The aim of this thesis is to devise a method to estimate submesoscale ocean surface topography with a bistatic SAR interferometer, such as Harmony.
Assessing the design of a bistatic WSOA requires knowledge of the interferometric sensitivity, and temporal lag. The first obstacle that we encountered was that there is no model or analytical expression for these parameters that apply to a bistatic SAR with a squinted line of sight. The established relations found in the literature assume a zero-squint geometry. Hence, we use the Fourier Diffraction Slice Theorem to derive an analytical expression for the interferometric sensitivity, and the temporal lag. We show that forming an interferogram aligns the regions of support of the two images in the Fourier domain at each resolution cell, and that the temporal lag is the time offset that aligns the two regions. The sensitivity is equal to the vertical component of the aligned wave vectors projected on the elevation direction. We verify our results using simulations and confirm that our analytical expressions agree with the well-established relations for sensitivity and temporal lag for zero-squint systems.
We use the analytical expressions of sensitivity and temporal lag to build an interferometric performance model that computes the standard error of the height estimate for a formation-flying cross-track interferometer. The model considers the following random error sources: temporal decorrelation, thermal noise, spectral shift, volumetric decorrelation, and the effect of removing the phase due to motion of the surface using the individual phase centers of the instruments. Additionally, we derive a relation between the formation parameters that, when satisfied, minimizes the effective temporal lag, while maximizing the interferometric sensitivity. We then proceed to assess the performance over an orbit and along the 250 km-swath of an optimized formation.
Finally, we propose a data-driven algorithm to synchronize the signals of the independent SAR receivers. The algorithm achieves an unbiased root mean square error of 0.010◦ , reducing the phase synchronization error to within the error budget allocation.
Overall, the thesis presents how one can design, analyze, and retrieve relative ocean topography at the submesoscales with a bistatic SAR interferometer. It sets the foundations for an experimental OST product for the Harmony mission. Adding such a product to the mission would offer the first simultaneously acquired observations of wind field, current field, directional wave spectrum, and relative sea-surface height at high resolution and over a 250 km-wide swath. ...
Synthetic-aperture radar (SAR) is a unique remote sensing instrument, particularly at C-band, capable of sensing the ocean surface at the submesoscales, with a wide swath, and in nearly all weather conditions. Harmony, the European Space Agency’s 10th Earth Explorer, features two SAR companion satellites. Two, out of a total of five, years of the mission’s life will be spent in a formation where the system will operate as a cross-track interferometer. Cross-track interferometry (XTI) is a technique that estimates the relative height of the surface from two SAR images of the same scene. Thus, Harmony could theoretically retrieve variations of the OST. In other words, the system could operate as a bistatic wide-swath ocean altimeter (WSOA). At the same time, Harmony will retrieve stress-equivalent wind fields, and instantaneous surface currents. Therefore, Harmony has the potential of providing an unprecedented wealth of co-located simultaneous data related to the ocean and the atmosphere. The aim of this thesis is to devise a method to estimate submesoscale ocean surface topography with a bistatic SAR interferometer, such as Harmony.
Assessing the design of a bistatic WSOA requires knowledge of the interferometric sensitivity, and temporal lag. The first obstacle that we encountered was that there is no model or analytical expression for these parameters that apply to a bistatic SAR with a squinted line of sight. The established relations found in the literature assume a zero-squint geometry. Hence, we use the Fourier Diffraction Slice Theorem to derive an analytical expression for the interferometric sensitivity, and the temporal lag. We show that forming an interferogram aligns the regions of support of the two images in the Fourier domain at each resolution cell, and that the temporal lag is the time offset that aligns the two regions. The sensitivity is equal to the vertical component of the aligned wave vectors projected on the elevation direction. We verify our results using simulations and confirm that our analytical expressions agree with the well-established relations for sensitivity and temporal lag for zero-squint systems.
We use the analytical expressions of sensitivity and temporal lag to build an interferometric performance model that computes the standard error of the height estimate for a formation-flying cross-track interferometer. The model considers the following random error sources: temporal decorrelation, thermal noise, spectral shift, volumetric decorrelation, and the effect of removing the phase due to motion of the surface using the individual phase centers of the instruments. Additionally, we derive a relation between the formation parameters that, when satisfied, minimizes the effective temporal lag, while maximizing the interferometric sensitivity. We then proceed to assess the performance over an orbit and along the 250 km-swath of an optimized formation.
Finally, we propose a data-driven algorithm to synchronize the signals of the independent SAR receivers. The algorithm achieves an unbiased root mean square error of 0.010◦ , reducing the phase synchronization error to within the error budget allocation.
Overall, the thesis presents how one can design, analyze, and retrieve relative ocean topography at the submesoscales with a bistatic SAR interferometer. It sets the foundations for an experimental OST product for the Harmony mission. Adding such a product to the mission would offer the first simultaneously acquired observations of wind field, current field, directional wave spectrum, and relative sea-surface height at high resolution and over a 250 km-wide swath.
From InSAR Time-Series to Crop Growth
Machine Learning and Physics-Guided Models for Radar-Based Vegetation Analysis
The first part of this research evaluates the added value of Sentinel-1 InSAR coherence time series for land cover classification, using an agricultural region in São Paulo, Brazil, as a case study. This region is characterized by a mixture of crops, pastures, and sugarcane plantations, all managed asynchronously. The findings demonstrate that incorporating InSAR coherence alongside SAR backscatter improves classification accuracy, particularly during the dry season when the distinctions between vegetation and bare soil are more pronounced. The research employed machine learning approaches to analyze pixel-level and field-level classifications using different sampling schemes. It highlights how multi-looking strategies can be adjusted to improve the accuracy of the classification outcomes in agricultural settings. This research highlights the usefulness of coherence data for the detection of events such as harvesting, offering valuable insights for more dynamic agricultural monitoring. The sensitivity of the coherence to agricultural changes leads to the observed improvement in Land Use Land Cover (LULC) mapping.
Forward models, or observation operators, are essential for the interpretation of radar observations and for the development of assimilation frameworks. In particular, in this research, we are interested in forward modeling the relation between crop bio-geophysical parameters, such as Leaf Area Index (LAI), Above Ground Biomass (AGB), and soil moisture, the inputs to our data-driven model, and radar observables, the outputs.
In the second part of this research, we integrate an existing crop growth model, the Decision Support System for Agrotechnology Transfer (DSSAT), with machine learning techniques to train a forward model to predict SAR observables over silage maize fields in The Netherlands across multiple years. Using crop growth models circumvents the dependency on limitedly available field measurements. When we use training and validation data from the same growth season, we obtain accurate predictions, with a mean absolute error (MAE) of less than 1.23 dB. Some of the field-to-field variability is accounted for by including the mean backscatter intensity during a few acquisitions before crop emergence. The obtained performance suggests the potential of using this approach to generate observation operators for data assimilation frameworks or for anomaly detection, supporting large-scale agricultural monitoring. However, the results also highlight one of the main challenges: the resulting data-driven model fails to generalize when presented with input bio-geophysical parameters that fall outside the regions of the parameter space spanned by the training dataset, as can happen, for example, during a drought period.
In the final part, we develop a physics-guided machine learning approach to address the limitations of data-driven models: lack of generalizability, tendency to overfitting, and reliance on extensive training data sets. We introduce physical constraints in an artificial neural network (ANN) in two ways. First, by modifying the loss function, used to train the ANN, by including a penalty for unphysical behavior, in particular by penalizing negative values of the partial derivative of the predicted backscatter intensity with respect to the surface soil moisture, since we assume this should always be positive. Second, by mirroring the architecture of the widely used Water Cloud Model (WCM) in the network topology. The added physical term to the loss function improves the ANN performance in all cases considered, with an R2 increase of 3 percentage points (p.p). The WCM-inspired model performs slightly worse when trained and tested with data from the same year, but it generalizes better, producing significantly better results for unseen conditions. In addition, the WCM-inspired model also produces individual contributions to the observed intensity, such as the surface-scattering component and the vegetation backscatter component. ...
The first part of this research evaluates the added value of Sentinel-1 InSAR coherence time series for land cover classification, using an agricultural region in São Paulo, Brazil, as a case study. This region is characterized by a mixture of crops, pastures, and sugarcane plantations, all managed asynchronously. The findings demonstrate that incorporating InSAR coherence alongside SAR backscatter improves classification accuracy, particularly during the dry season when the distinctions between vegetation and bare soil are more pronounced. The research employed machine learning approaches to analyze pixel-level and field-level classifications using different sampling schemes. It highlights how multi-looking strategies can be adjusted to improve the accuracy of the classification outcomes in agricultural settings. This research highlights the usefulness of coherence data for the detection of events such as harvesting, offering valuable insights for more dynamic agricultural monitoring. The sensitivity of the coherence to agricultural changes leads to the observed improvement in Land Use Land Cover (LULC) mapping.
Forward models, or observation operators, are essential for the interpretation of radar observations and for the development of assimilation frameworks. In particular, in this research, we are interested in forward modeling the relation between crop bio-geophysical parameters, such as Leaf Area Index (LAI), Above Ground Biomass (AGB), and soil moisture, the inputs to our data-driven model, and radar observables, the outputs.
In the second part of this research, we integrate an existing crop growth model, the Decision Support System for Agrotechnology Transfer (DSSAT), with machine learning techniques to train a forward model to predict SAR observables over silage maize fields in The Netherlands across multiple years. Using crop growth models circumvents the dependency on limitedly available field measurements. When we use training and validation data from the same growth season, we obtain accurate predictions, with a mean absolute error (MAE) of less than 1.23 dB. Some of the field-to-field variability is accounted for by including the mean backscatter intensity during a few acquisitions before crop emergence. The obtained performance suggests the potential of using this approach to generate observation operators for data assimilation frameworks or for anomaly detection, supporting large-scale agricultural monitoring. However, the results also highlight one of the main challenges: the resulting data-driven model fails to generalize when presented with input bio-geophysical parameters that fall outside the regions of the parameter space spanned by the training dataset, as can happen, for example, during a drought period.
In the final part, we develop a physics-guided machine learning approach to address the limitations of data-driven models: lack of generalizability, tendency to overfitting, and reliance on extensive training data sets. We introduce physical constraints in an artificial neural network (ANN) in two ways. First, by modifying the loss function, used to train the ANN, by including a penalty for unphysical behavior, in particular by penalizing negative values of the partial derivative of the predicted backscatter intensity with respect to the surface soil moisture, since we assume this should always be positive. Second, by mirroring the architecture of the widely used Water Cloud Model (WCM) in the network topology. The added physical term to the loss function improves the ANN performance in all cases considered, with an R2 increase of 3 percentage points (p.p). The WCM-inspired model performs slightly worse when trained and tested with data from the same year, but it generalizes better, producing significantly better results for unseen conditions. In addition, the WCM-inspired model also produces individual contributions to the observed intensity, such as the surface-scattering component and the vegetation backscatter component.
A new perspective on vegetation water dynamics
Assimilating ASCAT observations to constrain soil and vegetation states using a data-driven observation operator
In order to assimilate ASCAT observables, an observation operator is needed to link between LSM states to radar observations. Radiative transfer models (RTMs) are often used to assimilate radar backscatter into LSM [8, 9]. However, RTMs require moisture content or dielectric properties of soil and vegetation cover which are not simulated by the LSM. Therefore, to directly link land surface states and ASCAT observables, a Deep Neural Network (DNN) was trained and validated in Chapter 3. The performances and sensitivity of theDNNwere evaluated tomake sure the observation operator is physically plausible... ...
In order to assimilate ASCAT observables, an observation operator is needed to link between LSM states to radar observations. Radiative transfer models (RTMs) are often used to assimilate radar backscatter into LSM [8, 9]. However, RTMs require moisture content or dielectric properties of soil and vegetation cover which are not simulated by the LSM. Therefore, to directly link land surface states and ASCAT observables, a Deep Neural Network (DNN) was trained and validated in Chapter 3. The performances and sensitivity of theDNNwere evaluated tomake sure the observation operator is physically plausible...
With recent developments, the ASCAT variables slope and curvature have become of increasing interest in structural vegetation monitoring. These variables are a second-order Taylor polynomial’s first and second derivatives used to normalise the ASCAT backscatter-incidence angle relationship. This study explored the possibility to use these novel variables in forest fire research.
The focus was to discover to what extent the variables responded to a major forest fire.
To do so, grid points affected during the 2009 Australian Black Saturday Fires are compared to unaffected control grid points utilizing Z-scores. These control grid points have been selected based on time series similarity in the two years before the fire. Time series from 2007 to 2021 are used to investigate fire impact and recovery. The ASCAT variables are compared to a similar
NDVI time series to aid in interpreting the results.
The findings show that both slope and curvature are sensitive to the major forest fire. Both variables show an impact shortly after the fire, which can be explained by the loss of scattering elements in the vegetation due to the fire. In the following years, there is a notable recovery which can be explained by the vegetation regrowth forming new scatterers. The NDVI showed similar
behaviour but the recovery was differently timed, suggesting that the signal recovery is driven by something else or that the regrowth of leaves is different from the regrowth of the structural elements that the ASCAT variables represent.
The results help in understanding the ASCAT variables and their interpretation in terms of vegetation scatterers. Especially for the curvature, the clear change in signal deflects the discussion of whether the variable has information potential. Nevertheless, for the ASCAT variables to be applicable in forest fire research, they need to be better understood and additional research is necessary. Suggestions are for example a ground validation study or a global forest fire study, which would suit the coarse resolution of the ASCAT variables better and improve the understanding of the interaction between forest fires and the variables.
Although using the ASCAT variable for forest fire research is in its infancy, the results about its suitability are promising, both for ASCAT product development, as well as for the forest fire research field. Exploring the possibilities further is worthwhile, especially considering the fact that the slope and curvature time series cover a long continuous period starting as early as 1991. This long time series makes the ASCAT variables suitable for long-term forest fire monitoring, and the daily nature of the data might also make them interesting for short-term monitoring. ...
With recent developments, the ASCAT variables slope and curvature have become of increasing interest in structural vegetation monitoring. These variables are a second-order Taylor polynomial’s first and second derivatives used to normalise the ASCAT backscatter-incidence angle relationship. This study explored the possibility to use these novel variables in forest fire research.
The focus was to discover to what extent the variables responded to a major forest fire.
To do so, grid points affected during the 2009 Australian Black Saturday Fires are compared to unaffected control grid points utilizing Z-scores. These control grid points have been selected based on time series similarity in the two years before the fire. Time series from 2007 to 2021 are used to investigate fire impact and recovery. The ASCAT variables are compared to a similar
NDVI time series to aid in interpreting the results.
The findings show that both slope and curvature are sensitive to the major forest fire. Both variables show an impact shortly after the fire, which can be explained by the loss of scattering elements in the vegetation due to the fire. In the following years, there is a notable recovery which can be explained by the vegetation regrowth forming new scatterers. The NDVI showed similar
behaviour but the recovery was differently timed, suggesting that the signal recovery is driven by something else or that the regrowth of leaves is different from the regrowth of the structural elements that the ASCAT variables represent.
The results help in understanding the ASCAT variables and their interpretation in terms of vegetation scatterers. Especially for the curvature, the clear change in signal deflects the discussion of whether the variable has information potential. Nevertheless, for the ASCAT variables to be applicable in forest fire research, they need to be better understood and additional research is necessary. Suggestions are for example a ground validation study or a global forest fire study, which would suit the coarse resolution of the ASCAT variables better and improve the understanding of the interaction between forest fires and the variables.
Although using the ASCAT variable for forest fire research is in its infancy, the results about its suitability are promising, both for ASCAT product development, as well as for the forest fire research field. Exploring the possibilities further is worthwhile, especially considering the fact that the slope and curvature time series cover a long continuous period starting as early as 1991. This long time series makes the ASCAT variables suitable for long-term forest fire monitoring, and the daily nature of the data might also make them interesting for short-term monitoring.
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Sensitivity Assessment of Sentinel-1 SAR Closure Phase to Vegetation and Soil Moisture Dynamics
A Case Study for Regions in Southern France
This thesis aims to study the feasibility of using time series Interferometric Synthetic Aperture Radar (InSAR) as a means to monitor differential settlement in greenhouse structures. The analysis was primarily done using RADARSAT-2 data. In case of translucent surfaces of greenhouses, it was important to firstly identify the physical targets that are associated to scattering centres. This was done by analysing the statistics of the heights of the scatterers which helps in ascertaining where the radar signal is getting back-scattered from. It was inferred that the persistent and distributed scatterers are primarily identified from objects on the roof and outer walls of the greenhouses.
Moreover, the magnitude of deformation estimated from the scatterers have been corroborated with geotechnical data. It was seen that higher magnitudes of deformation was seen in locations with compressible soil types such as clay and peat close to the ground surface. It was also seen that greenhouse structures are prone to differential settlement when the depths of the piles are insufficient in areas with varying soil types. The effect of thermal contributions has also been studied and it was found that the estimation of thermal expansion does not significantly affect the estimated deformations.
From the study, it is evident that time series InSAR offers an effective means to monitor differential settlements in greenhouses. In order to check for differential settlement in individual greenhouses, it is proposed that a persistent scatter interferometric analysis be done initially and if it is seen that the density of these scatterers is insufficient, the analysis can be followed up with time series interferometry of distributed scatterers. Incorporating multiple track directions of radar data increases the number of greenhouses that can be monitored. Moreover, it was also seen that persistent scatterers were identified from additional greenhouses when Sentinel-1 data was used, despite its poorer spatial resolution. For further study, it is recommended that corner reflectors are used to validate the positions of the targets that are identified as persistent and distributed scatterers.
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This thesis aims to study the feasibility of using time series Interferometric Synthetic Aperture Radar (InSAR) as a means to monitor differential settlement in greenhouse structures. The analysis was primarily done using RADARSAT-2 data. In case of translucent surfaces of greenhouses, it was important to firstly identify the physical targets that are associated to scattering centres. This was done by analysing the statistics of the heights of the scatterers which helps in ascertaining where the radar signal is getting back-scattered from. It was inferred that the persistent and distributed scatterers are primarily identified from objects on the roof and outer walls of the greenhouses.
Moreover, the magnitude of deformation estimated from the scatterers have been corroborated with geotechnical data. It was seen that higher magnitudes of deformation was seen in locations with compressible soil types such as clay and peat close to the ground surface. It was also seen that greenhouse structures are prone to differential settlement when the depths of the piles are insufficient in areas with varying soil types. The effect of thermal contributions has also been studied and it was found that the estimation of thermal expansion does not significantly affect the estimated deformations.
From the study, it is evident that time series InSAR offers an effective means to monitor differential settlements in greenhouses. In order to check for differential settlement in individual greenhouses, it is proposed that a persistent scatter interferometric analysis be done initially and if it is seen that the density of these scatterers is insufficient, the analysis can be followed up with time series interferometry of distributed scatterers. Incorporating multiple track directions of radar data increases the number of greenhouses that can be monitored. Moreover, it was also seen that persistent scatterers were identified from additional greenhouses when Sentinel-1 data was used, despite its poorer spatial resolution. For further study, it is recommended that corner reflectors are used to validate the positions of the targets that are identified as persistent and distributed scatterers.
surface melt on blue ice. This is done via interferometry (and the corresponding coherence) and with the backscatter coefficient. Coherence turns out the be an unreliable method to detect surface melt, since the influence of wind and precipitation on the decrease of coherence is dominant. Thus, surface melt detection via this method is difficult. Backscatter showed some potential to detect surface melt on blue ice, but due to the larger standard deviation than the actual decrease of backscatter (assumed due to surface melt), a clear distinction between blue ice and surface melt can not be made. Melt features, such as rivers, lakes and ponds are detectable with the backscatter, due to their distinctive shape. Since these melt features are linked to surface melt, backscatter can indirectly be used to detect surface melt on blue ice. ...
surface melt on blue ice. This is done via interferometry (and the corresponding coherence) and with the backscatter coefficient. Coherence turns out the be an unreliable method to detect surface melt, since the influence of wind and precipitation on the decrease of coherence is dominant. Thus, surface melt detection via this method is difficult. Backscatter showed some potential to detect surface melt on blue ice, but due to the larger standard deviation than the actual decrease of backscatter (assumed due to surface melt), a clear distinction between blue ice and surface melt can not be made. Melt features, such as rivers, lakes and ponds are detectable with the backscatter, due to their distinctive shape. Since these melt features are linked to surface melt, backscatter can indirectly be used to detect surface melt on blue ice.