Figure 2. The overall overflow of KappaMaskv2.

As the general overflow has stayed the same as in KappaMask, more details can be found here.

KappaSet development

KappaMaskv2 is an AI-based cloud and cloud shadow processor whose quality highly depends on the training dataset. There are only a few datasets publicly available. Therefore, KappaZeta went through deserts and oceans, mountains and rainforests to create the one and only, KappaSet, a novel and diverse cloud and cloud shadow dataset. Check out the dataset distribution in Figure 3.

Figure 3. KappaSet train set distribution

KappaSet's main features include:

• Five classes: cloud, cloud shadow, semi-transparent clouds, clear, and missing.
• Different surface types :  deserts, snow/ice cover, water bodies, cities, farmlands, mountains, rainforests.
• Different types of clouds: cumulus, cirrus, stratus.
• Various weather conditions

Figure 4. KappaSet test set distribution

KappaMaskv2 was compared to other cloud masking processors, including Sen2Cor, Fmask, MAJA, IdePix and S2Cloudless. In Figure 5, you can see that KappaMaskv2 generally performs better in every class. Fmask prediction is close to the KappaMask prediction, except for water being classified as a cloud. Sen2Cor and IdePix correctly identified cumulus clouds when cloud shadows and semi-transparent clouds are underestimated. Sen2Cor example shows that some semi-transparent clouds and cloud shadows are detected as missing class.

S2Cloudless prediction can be defined as "close to the ground truth label" if semi-transparent clouds and cloud shadows are considered. The general picture shows that clouds are overestimated. However, if the semi-transparent class is counted as a cloud, the prediction looks more accurate. MAJA prediction is similar to S2Cloudless, although some pixels are misclassified as clear.

Figure 5. Comparison of L1C prediction output for a 512 × 512 pixels sub-tile in the test dataset. By design, Fmask and S2Cloudless do not have semi-transparent class included. S2Cloudless does not have a cloud shadow class.

We used Dice Similarity Coefficient as an evaluation metric. Note that evaluation was performed on cloud, cloud shadow, semi-transparent cloud and clear classes.

Figure 6. Dice coefficient evaluation performed on the KappaSet test set for KappaMaskv2 Level-1C, Sen2Cor, Fmask, IdePix, MAJA and S2Cloudless.

KappaMaskv2 L1C yielded the highest Dice coefficient for each class. The significant improvement of KappaMaskv2 L1C compared to other cloud masking approaches is more accurate cloud shadow and semi-transparent cloud detection with Dice coefficients of 67% and 75%, respectively. KappaMaskv2 L1C reached the Dice coefficient of 84% for cloud class, followed by IdePix and Sen2Cor with 60% each.

Running time comparison

As we mentioned before, changing cloud detector architecture allowed us to speed up the running time of KappaMaskv2. We compared how fast KappaMaskv2 was on both GPU and CPU in comparison to Sen2Cor, Fmask, IdePix, and S2Cloudless. MAJA is not presented as it was run in the backward mode meaning that the running time for MAJA depends on the number of valid products in the time series.

Figure 7. Time comparison (in minutes) was performed on the single Sentinel-2 Level-1C product inference. KappaMaskv2 L1C with GPU and CPU, Sen2Cor, Fmask and S2Cloudless on generating 10 m resolution classification map. IdePix classification map is at 20 m resolution mask.

KappaMaskv2 with GPU is almost two times faster than Sen2Cor or Fmask and five times faster than IdePix. In turn, Sen2Cor is faster by 10 seconds compared to KappaMaskv2 if the latter uses CPU instead. In turn, S2Cloudless inference time is around 18 minutes which is 6 times slower than KappaMaskv2. KappaMaskv2 is available here: https://github.com/kappazeta/km_predict

Summary

• We compiled diverse cloud and cloud shadow dataset, named KappaSet. It consists of 9251 labelled sub-tiles at 10 m resolution, from Sentinel-2 Level-1C products. We believe that KappaSet will benefit the research on cloud masking. KappaSet can be found here.
• We presented KappaMaskv2, an AI-based cloud and cloud shadow processor for Sentinel-2, which operates at the global scale. It was compared to other cloud masking approaches on the carefully selected test set. The results showed that KappaMaskv2 significantly improved cloud shadow and semi-transparent cloud detection. KappaMaskv2 is available here. Feel free to try it out and share your experience with us!

Local methods

The design of efficient despeckling filters is a long-standing problem that has been the object of intense research since the advent of SAR technology. The most straightforward way to reduce these fluctuations and estimate the values of the physical parameters is to average several independent samples from the data. This operation, called multilooking, was applied in various forms from the very beginning of the SAR era. However, such averaging that applies equally to every region of the image, regardless of the local heterogeneity, strongly degrades the spatial resolution.

In the beginning of 2000s, Lee et al. proposed to use adaptive filtering for polarimetric and interferometric SAR denoising. Instead of estimating the parameters over a rectangular sliding window, a directional window is locally selected among eight edge-aligned windows according to the local gradient of the amplitude images. Lee’s method preserves the edge structures since values of pixels on each side of the edge are never combined together, avoiding the smoothing effects. Unfortunately, this method tends to leave a high variance in homogeneous areas and create some undesired artifacts.

The intensity-driven adaptive-neighborhood (IDAN) technique was proposed for the polarimetric and interferometric SAR parameter estimation. Following the idea of filtering over directional windows, the IDAN performs a complex multilooking operation on an adaptive neighborhood. This adaptive neighborhood is constructed with a region-growing algorithm where the most similar adjacent pixels are selected iteratively according to their intensity values. The adaptive neighborhood aims to select as many pixels as possible, all following the same statistical population as the considered pixel. This decreases the resolution loss in the estimation since noisy values coming from other populations are rejected. Due to its window-shaped adaptivity, the IDAN achieves the best trade-off between the residual noise and resolution loss among window-based methods. However, due to its connectivity constraint, the IDAN leaves a high variance in regions where there are only few adjacent similar pixels.

The following generation of filtering approaches introduced stronger priors to guide the solution. The first family includes the variational-based methods which have gradually been utilized for SAR image despeckling. Those methods are stable and flexible and break through the traditional idea of filters by solving the problem of energy optimization. Although these methods have achieved good reduction of speckle noise, the result is usually dependent on the choice of the model parameters and prior information, and is often time-consuming. In addition, the variational-based methods cannot accurately describe the distribution of speckle noise, which also constraints the performance of speckle noise reduction.

The second large family of approaches is based on wavelet transforms. Due to their spatially localized and multiresolution basis functions, wavelets yield sparse yet accurate representations of natural images in the transform domain. Sharp discontinuities and pointlike features, so common in SAR images, are well described by a small number of basis functions, just like the large homogeneous regions between them. The major weaknesses of this type of approach are the backscatter mean preservation in homogeneous areas, details preservation, and producing artificial effect into the results such as ring effects.

Non-local methods

The non-local means (NLM) algorithm has provided a breakthrough in detail preservation in SAR image despeckling. During the recent years, powerful and widespread methods such as PPB, NL-SAR and SAR-BM3D have been created. In the following paragraph, we will describe the essentials of the algorithm. Figure 1 summarizes the processing steps. 

Figure 1. Non-local estimation in action: processing at pixel x.

Non-local estimation methods generally follow a three-step scheme with many possible variations at each step and, possibly, preprocessing steps and/or iterative refinement of results by repeated non-local estimations. The first step identifies similar patches (patch size is generally set from 3x3 to 11x11 pixels). It must reliably find, within an extended search window (typically 21x21 to 39x39 pixels), patches that are close to the reference central patch. Recurring patches are found in smooth regions, but just as well around region boundaries, textures, artificial structures, etc., as shown in figure 2. Once several patches have been selected, they are assigned relative weights.

Figure 2. Fragments of SAR images: (a) homogeneous region, (b) line, (c) texture, (d) structure. For each target patch (green) several similar patches (red) are found in the same fragment [1].

The second step combines patches, according to their weights, to form an estimate of either the central pixel (pixel-wise estimation), the central patch (patch-wise estimation), or all selected patches (stack-wise estimation). The estimates computed from all possible reference patches are then merged in a last step to produce the final image.

The most straightforward way to combine patches is to use pixel-wise filtering. Within this approach, a weight is assigned for the central pixel of all the patches. By using those weights, the estimation for the central pixel in a target patch is calculated.

The difference in patch-wise filtering is that all pixels in the patch, not just the central one, are estimated at once. Since each pixel is estimated several times, a suitable aggregation phase is necessary to combine all such estimates. The simplest form of aggregation is to consider uniform weights for all the estimated pixels. Another strategy is to set the weight associated with each estimate as inversely proportional to its variance.

To illustrate why patch-wise estimation improves performance, let us consider the special case of a pixel near the boundary between two homogeneous regions. Since the patch centered on it is strongly heterogeneous, most other patches of the search area, coming from homogeneous regions on either side of the boundary, are markedly dissimilar from it, and contribute very little to the average. The estimate, thus, involves only a small effective number of predictors, those along the edge, which results in a high variance. As a result, a visible “halo” of residual noise is observed near the edges, a phenomenon well-known in NLM, also referred to as the rare patch effect. The target pixel, however, belongs to a large number of patches, not just the patch centered on it, many of them drawn from the homogeneous region to which the pixel belongs. In patch-wise reprojection, all of these patches are included in the average reducing the estimate variance, especially if suitable weights are used to take into account the reliability of each contribution.

Let us now consider the third strategy, with stack-wise filtering. The first difference with regard to patch-wise filtering is that now all patches collected in the stack are collaboratively filtered before reprojecting them to their original position. The major improvement is that the stack is filtered in three dimensions, i.e, not only along the stack but also in the spatial domain. In SAR-BM3D, the whole stack, formed by just a limited number of similar patches, is wavelet transformed, Wiener filtered, and back transformed. By so doing, strong spatial structures are emphasized through filtering while random noise is efficiently suppressed. As a matter of fact, these techniques exhibit significant improvements especially in highly structured areas (edges, point reflectors, textures). The efficiency of collaborative filtering comes from the full exploitation of the redundancy of information in a stack of similar patches.

The performance of NLM methods depends on the setting of several parameters, like patch size and search area size, which should be related to image resolution, smoothing strength, and balance between original and pre-estimated data. In most of the non-local approaches these parameters are set by hand. Few works have considered semisupervised setting or automatic setting with spatial adaptation. NL-SAR is one of such publicly available methods that automatically tunes patch and search window sizes and prefiltering strengths to provide improved results.

Speckle filtering in KappaZeta

In KappaZeta we analyzed, modified and combined multiple published methods when designing a custom speckle filter for KappaOne service. For details, take a look at our newsletter from April 2022.

The Sentinel-1 data is different than most other satellite data because it is not dependent on weather or daylight, and thus is able to provide data on days where other satellites cannot because of clouds. 

As Sentinel-1 is a great data source acquiring large quantitites of Synthetic Aperture Radar data with global coverage, which is valuable for numerous Earth Observation applications, we have decided to make it accessible and easy to use for a wider audience.  

Figure 1. Example of standard Sentinel-1 GRD backscatter image

There are some services on the market, which make optical satellite data, like Sentinel-2 or Landsat easy to use and analyse. However, there is no application that utilizes the Sentinel-1 data in its full potential. Therefore, KappaZeta team decided to resolve this issue by establishing the KappaOne service, where S1 data will be processed and prepared for the user in analysis ready data (ARD) format.  

What is KappaOne?

KappaOne stands for one-click or one API command integration. There are six Sentinel-1 ARD products available, which are presented in human-friendly as well as machine-readable form, providing value for a long list of end-user applications. 

Provided Sentinel-1 ARD layers are the following:

• Time series of small geographical region – parcel, statistics (mean, median, min, max, stddev) of Vertical-Horizontal (VH) and Vertical-Vertical (VV) backscatter, VH/VV backscatter ratio, VH and VV 6-day repeat pass coherence (phase difference changes);

• Calibrated high-resolution VH and VV repeat pass interferometric coherence rasters;

• Calibrated high-resolution VH and VV backscatter and VH/VV ratio rasters;

• Multi-polarisation backscatter image for visual use as a WMS service;

• Synthetic Sentinel-2-like natural colours image based on Sentinel-1 and -2 time series with AI-modelling;

• Synthetic NDVI-like raster based on Sentinel-1 and -2 time series with AI-modelling. 
  

You can have an overview of our service here. This is a web-map, where you can choose the layer which you are interested in. Moreover, you can scroll the dates in the calendar to see how the area of interest looked in a particular time.  

Figure 2. KappaOne web-map

The other convenient feature of our webpage is the one-click command with which you can download a pre-set QGIS project for the layer and date you are interested in. You can open the setup file in QGIS, where you will see the WMS layer with the chosen product for a particular date. 

Another asset of the KappaOne service, is a visualisation of the time series of parcel-level statistics. By clicking on the parcel of interest, the chart of the area becomes visible, where you can browse the time series of various Sentinel-1 and Sentinel-2 parameters.

Who can use it and where?

There are numerous applications where Sentinel-1 Analysis Ready Data could be used. For example, this service can be used by the EO or GIS companies without Synthetic Aperture Radar expertise for Mapping/GIS analysis tasks, where frequent and systematic data is needed. 

Sentinel-1 ARD is vital also for the agricultural subsidy checks, where on-spot checks conducted by the inspectors are gradually replaced by satellite monitoring. The grassland maintenance checks can be very slow and expensive if done manually. Therefore, for this kind of task, the usage of satellite monitoring is a great way of saving time and money. 

With Sentinel-1 data many more tasks can be solved. As it was underlined before, satellite monitoring is an efficient tool for resolving various measurement and assessment tasks, where instead of gut feeling decisions could be done based on actual data. It can be used for the greenhouse gas fluxes modelling, as well as flood risk assessments or the landscape dynamics based on historical data and damage mapping near real time. Also, the monitoring of the seaports could be performed, which would reflect the flow of the sea containers. 

The Figure below shows Sentinel-1 multiband image for the port area in Rostock, Germany. Yellow areas on the image represent big metallic constructions, which are the sea containers transported with ships. It is visible that on 29th of May 2021, the ship was leaving or entering the port and ships had changed their location in Rostock port and its surrounding in the sea by 4th of June.

Figure 3. Example of changes in the port, visible on S1 multiband image, a) 29.05.2021, b) 04.06.2021

Figure 4 illustrates the ploughing example on the Synthetic NDVI layer, which is computed from Sentinel-1 raster with usage of historical Sentinel-2 data. It is visible that the vegetation index before ploughing on the parcels is significantly higher than after ploughing, as the color changes rapidly from yellow to dark orange.  

Figure 4. Example of ploughing event, visible on S1 sNDVI, a) 29.05.2021, b) 04.06.2021

Olga Wold

Geospatial data quality specialist

olga.wold@kappazeta.ee

Sentinel-2 is a beautiful European data factory, producing tons of valuable imagery every day. Its full potential is yet to be exploited. The first Sentinel-2 satellite was launched in 2015 and after launching the second satellite (2B) the system reached its full data production capacity in the second half of 2017. One of the factors limiting the usage of Sentinel-2 data is clouds. There is a need for an accurate mask for separating the clear pixels from the corrupted ones. Figure 1 illustrates it well – not only the cloud covered areas are unusable for great majority of EO applications, but also the cloud shadows cause trouble. If you run e.g. a crop classification algorithm on these regions you cannot expect an adequate result.

While Sentinel-2 system, functioning as a data factory, is beautiful and undeniably a huge game changer, then the official Sen2cor cloud mask incorporated to the L2A data products can be insufficient in terms of accuracy when used in fully automatic processing chains. The issues rise with underestimating the cloud shadows and small fragmented clouds. While feeding an operational processing chain (such as the grassland mowing detection system of KZ) with this data a lot of corrupted pixels are passed through, deteriorating the accuracy of the end result. In practice we have ended up with aggressive outer buffering and few other post-processing steps to reduce the errors. But obviously these are all just work-arounds without solving the underlying problem. The cloud mask itself, out-of-the-box, should be accurate enough without thinking about it during the work processes.

When digging deeper, you find that the Sen2cor cloud mask processor has a rule-based thresholding decision tree with some post-processing steps (e.g. morphological filtering to reduce the noise). On one hand it is impressive how accurate results this decision tree is able to produce in a global scale, but after the revolution of AI and deep learning one knows that the same task can be solved much better with a different – more modern design.

Leaving the Sen2cor cloud mask as it is, the proposal of KappaZeta was convincing enough that we were given a chance to develop an AI-based Sentinel-2 cloud mask for ESA and we are very grateful for it.

Which other cloud masks are out there?

Firstly, we would like to outline how import is to develop open source cloud masks. There are a few privately developed cloud masks, raising the first question about accuracy figures. If these details are not public, it is also hard to assess how good the offered product really is and that raises many other questions. Furthermore, this adds to the unnecessary amount of time spent on something that could be shared openly, reducing duplication, and contributing to improved products. Therefore, everybody would win time-wise and quality-wise from more open approach and sharing. This is what we believe in and hope that more and more companies over time will come to the same conclusion.

One of the best open source cloud masks is probably s2cloudless by Sinergise. Find more information from here, here and here.

There is just one thing we would like to question and open for discussion. They write that: “We believe that machine learning algorithms which can take into account the context such as semantic segmentation using convolutional neural networks (see this preprint for overview) will ultimately achieve the best results among single-scene cloud detection algorithms. However, due to the high computational complexity of such models and related costs they are not yet used in large scale production.” So CNNs are great, but too heavy to be practical? Let us put this claim in doubt, at least in 2020. One thing is CNN model fitting, which for a complex model can be computationally expensive, that is true. But the other thing is running a prediction with a pre-trained model. This is much cheaper – and this is what you need to do when you put a CNN into production.

One of the best research papers on using deep learning for cloud masking is probably by DLR. We are taking this as one of the starting points for our development. They claim higher accuracies than Fmask (which is roughly on the same level with Sen2Cor) at a reasonable computational cost (2.8 s/Mpix on a NVIDIA M4000 GPU).

There are also several CNN-based cloud masking research papers by the University of Valencia. E.g. by Mateo-García and Gómez-Chova (2018) and Mateo-García, Gómez-Chova and Camps-Valls (2017).

All in all – deep learning as a universal mimicking machine has proven to be at least as accurate in recognizing objects from images and segmenting them semantically as human interpreters. Deep learning has been proven in various domains with image interpretation, speech recognition and, text translation. Computer Vision, which focuses particularly on digital images and videos, has enormous success in medical field, where data labelling is an expensive procedure or rapidly developing autonomous driving cars field, where huge amount of data should be processed in real time. There is every reason to believe that it will excel also in detecting clouds and cloud-shadows from satellite imagery. What determines the success is the quality and variety of the model fitting reference data set.

We believe that cloud masking is such an universal pre-processing step for satellite imagery that sooner or later someone will develop an open source deep learning cloud mask and all the closed source cloud masks become obsolete. Let us then try to be among the first and help the community further.

How?

The goal of the project is to develop the most accurate cloud mask for Sentinel-2. We know it is going to be hard and to avoid going crazy by trying to solve everything at once, we are limiting the scope of the project. We concentrate on Northern European terrestrial summer season conditions. With Northern Europe we mean the area north from the Alps, which has relatively similar nature and land cover. Summer season means the vegetative season – from April to October. We start from terrestrial conditions (with all due respect to the marine researchers), because we believe it has higher impact for developing operational services that make clients happy, for example in the agricultural and forestry sectors.

Everyone, who has worked on machine learning projects, know that the most critical factor for success is the quality and variety of input data. In our case it is the labelled Sentinel-2 imagery following the classification schema agreed in CMIX. Eventually each pixel should have a label, one out of four: 1) clear, 2) cloud, 3) semi-transparent cloud, 4) cloud shadow. For labelling we are using CVAT with a few scripts for automation and thanks to the hard work of our intern Fariha we have already labelled more than 1500 Sentinel-2 cropped 512x512 pixels tiles. The work goes on to have a large and accurate reference set for CNN model fitting.

To be more effective, there are several machine learning techniques we are going to apply:

1) Active learning. To select only the tiles and pixels, which have the highest impact for increasing the accuracy of the model. Labelling is a time-consuming process, and it is critical to do only work that matters.

2) Transfer learning. The idea is to use all possible open sources labelled Sentinel-2 images to train the network and then fine-tune it on our smaller focused dataset.

The initial literature review is completed and we plan to start with applying U-Net on our existing labelled dataset. We still have many open questions, e.g. should we use one of the rule-based masks as an input feature; is the improvement worth the fear that the network can possibly capture the same errors; to what extent we can augment existing features in terms of brightness and angles; can certain calculated S2 coefficients help the network, such as NDVI, NDWI etc?

Last, but not least, it is an open source project. All our results, final software and source code will be freely and openly distributed in GitHub. Openness and accessibility of our software should directly translate into greater usage. We are also intending to learn from the community and take advantage of the existing open source projects and labelled cloud mask reference data sets.

If you have any good suggestions how we could improve our cloud mask or be aware of some parallel developments for cooperation, please let us know. Our project runs from October 2020 to September 2021.

Further information:
Marharyta Domnich
marharyta.dekret@kappazeta.ee

Mowing detection

One of the examples where we meet the splitting challenge is the mowing detection task. The goal of mowing detection is to predict the time at which the grass on the field was cut. Thus, as part of our mowing detection project, each year we collect field books from farmers and field reports from the inspectors of the local paying agency. The received data is converted and reviewed manually, and some of the ground truth is produced from the manual labelling.

The labels would differ in trustworthiness, depending on the source (farmer field books, inspector field reports, any of the former with manually adjusted dates, or fully manual labelling). Since inspector field reports are the most reliable source, we would use most of them for the validation and test set. However, we would need at least some of them to be present in the training dataset as well. Additionally, each dataset is expected to have as well balanced classes distribution as possible, perhaps with additional filtering to randomly drop least trustworthy samples from the over-represented class.

Considering the aforementioned conditions, let’s say we would like to have 70% of the labelled data for training, 20% for validation and 10% for testing. For validation and testing, we would only use instances from inspector field reports and farmer field books with tweaked dates. For training, we would use data from all sources, including the ones from inspector field reports and tweaked field books which were left over from the test and validation datasets.

Crop classification

Another task we are dealing with is crop classification. We would like to detect the crop type of agricultural fields out of 28 possible classes. Similarly to the mowing detection we have different sources for labels, some of which have been provided by the local Agricultural Registers and Information Board, some from drone observations. For crop classification, class balance distribution plays the core role. In order to mitigate the issue of an unbalanced dataset, undersampling and oversampling can be used. Undersampling and oversampling should be available for the training subset, while for testing we would use some of the fields with labels of high confidence. Some of the classes might have a poor representation, due to which general split ratios might leave the validation or test dataset without any samples, whereas we need to ensure that all datasets have enough samples.

Thus, the requirements for splitting are the following. We would like to have 70% / 20% / 10% splits, ensuring that for smaller representing classes at least one instance is present in all sets. Additionally for the test set we would like to have the list of high confidence instances together with random leftover samples that added up to 10% of the whole data.

Generic and configurable

While such processing chains can be implemented, we have found it tricky to have it generic and configurable enough to cater for all sorts of projects with different (and sometimes rapidly changing) requirements.

Current solution

Currently we have separate implementations for mowing detection and crop classification, both of which take input parameters from a config file. The config file is basically python code and supports the definition of custom filter functions for datasets. For each dataset, the current solution invokes custom filters (if any) and then performs random sampling of data indices, leaving the rest of the samples for the next datasets. The samples which have been filtered out, are also left for the next datasets, for each dataset might have a different filter.

The reason why we prefer to use data / sample indices instead of data directly, is to have a layer of abstraction. This way the splitting logic could be agnostic of data type. It would not matter whether a single sample / instance is a raster image, an image time-series or time-series of parameter values which have been averaged over a pre-defined geometry.

For multiclass applications such as crop classification, data indices are sampled separately for each class within each dataset. The splitting also supports capping of samples for classes which are represented too well. However, if there are too few samples per class, a low threshold can be applied such that a different split ratio would be used. For instance, in the case of 70% training, 20% validation and 10% testing dataset with just 9 samples in one of the classes, we might end up with 7 samples in the training dataset, 2 samples in validation and 0 in the test set. To mitigate the issue, we could have the ratios adjusted to 40% training, 30% validation and 30% testing for classes with less than 100 samples.

Ideas for future developments

Instead of project-specific implementation of the splitting logic, we would prefer to have a generic framework for graph-based data splitting with support for cross-validation and bagging. Please let us know if there is such a framework already out there, or if there would be community interest in developing the framework.

Using machine learning in crop type classification is not new, and definitely not a revolutionary breakthrough - already for decades different classifiers (Support Vector Machine, Decision Trees, Random Forest and many more) have been used in land cover classification. Recently also neural networks, the wunderkind of machine learning and image recognition, are widely used in crop discrimination. Satellite data, as the main input to classification models, has no serious alternatives, since our aim is to implement it on worldwide scale and in applications, which run near real time. So, why even get excited about another crop type classification study, which exploits same methods and datasets as tens of previous studies?

I can give you one reason. Estonia has been very successful in following European Commission (EC) guidelines and rules in modernizing the EU Common Agricultural Policy. In 2018 EC adopted new rules that allow to completely replace physical checks on farms with a system of automated checks based on analysis of Earth observation data. The same year Estonian Agricultural Registers And Information Board (ARIB) launched the first nation-wide fully automated mowing detection system, which uses Sentinel-1 and Sentinel-2 data and where the prediction model inside the system is developed by KappaZeta. The system has been running for 3 years, it has significantly reduced the amount of on-site checks and increased the detection of non-compliances. In short – saved Estonian and EU taxpayers’ money. Automated crop discrimination is the next step in pursuing the above-mentioned vision and will probably become the foundation of all agricultural monitoring. With proved and tested methodology, it’s highly likely that Estonia will take this next step in the very near future and launch it again on the nationwide level. This is definitely a perspective to be excited about.

Now, let’s see how we tackled “the good old” crop classification task.

Input data

Although algorithms and methods are important to make a difference in prediction model performance, the training data is the most valuable player in this game. In Estonia all farmers who want to be eligible for subsidies need to declare crops online (field geometry + crop type label). This open dataset is freely accessible to everyone and has the permission to re-use and redistribute both commercial and non-commercial purposes. Since the crop type labels are defined by farmers and most of them are not double-checked by ARIB, there can be mistakes (according to ARIB’s estimations, less than 5%). Therefore, for additional validation we ran our own cluster analysis on time-series to filter out obvious outliers in each class.

For Sentinel-1 images preprocessing we have developed our own processing chain to produce reliable time-series for several features. From the previous studies it’s known that features (channel values and indexes) from Sentinel-2 images combined with features from Sentinel-1 images (coherence, backscatter) give better classification results than any of these features separately.

We used data from 2018 and 2019 seasons (altogether more than 200 000 parcels) and aggregated all crop type labels into 28 classes which were defined by the need of the ARIB.

Model architecture was rather simple – input layer, flatten layer, three fully connected dense layers (two of them followed by batch normalization layer) and output (Figure 3). Our experiment with adding 1D CNN layer after input didn’t improve results significantly. More complicated ResNet (residual neural network) architecture increased training time by approx. 30%, but results were similar to a linear neural network.

Classification results

Some features are more important than others

They are not. We found that the 5 most important features are Sentinel-1 backscatter (s1_s0vh, s1_s0vv), NDVI, TC Vegetation and PSRI from Sentinel-2. To our surprise, soil type and precipitation sum before satellite image acquisition had low relevance.

What next?

If you are more interested about this study, our Sentinel-1 processing pipeline or machine learning expertise, then feel free to get in touch. We have the mentality to share not hide our experience and learn together on this exciting journey.

The Japanese space and satellite program consist of two series of satellites – those used mainly for Earth observation and others for communication and positioning. There are 3 Earth Observation satellites in nominal phase, 3 in latter phase in operation and 3 more under development.

Greenhouse gases Observing SATellite-2 "IBUKI-2" (GOSAT-2) is measuring global CO₂ and CH₄ distribution of lower and upper atmosphere. Climate "SHIKISAI" (GCOM-C) satellite carries an optical sensor capable of multi-channel observation at wavelengths from near-UV to thermal infrared wavelengths (380nm to 12µm) to execute global, long-term observation of the Earth’s environment. Advanced Land Observing Satellite-2 "DAICHI-2" (ALOS-2) aims are to monitor disaster areas, cultivated areas and contribute to cartography.  

ALOS-2, which is specifically interesting for radar enthusiasts, is a follow-on mission from the ALOS “DAICHI”. Launched in 2006, ALOS was one of the largest Earth observation satellites ever developed and had 3 different sensors aboard: PRISM (Panchromatic Remote-sensing Instrument for Stereo Mapping) for digital elevation mapping, AVNIR-2 (Advanced Visible and Near Infrared Radiometer type 2) for precise land coverage observation and PALSAR (Phased Array type L-band Synthetic Aperture Radar) for day-and-night and all-weather land observation. ALOS operations were completed in 2011, after it had been operated for over 5 years.  

ALOS-2 was launched in 2014 and carries only radar instrument aboard. New optical satellite, ALOS-3, which will improve ground resolution by approx. three times from that of ALOS (2.5 to 0.8 m at nadir, wide-swath of 70 km at nadir), is already under development together with ALOS-4, which will take over from ALOS-2 to improve the functionality and performance.  

Let’s come back to present day. The state-of-the-art L-band Synthetic Aperture Radar (PALSAR-2) aboard ALOS-2 have enhanced performance compared to its predecessor. It has a right-and-left looking function and can acquire data in three different observation modes:

• Spotlight – spatial resolution 1x3 m, NESZ -24, swath 25 km. 
• Stripmap – spatial resolution 3-10 m, swath 30–70 km. Consist of Ultrafine (3 m), High sensitive (6 m) and Fine (10 m) modes. 
• ScanSAR – spatial resolution 60-100 m, swath 350–490 km.  

Emergency observations have highest priority for ALOS-2, but for systematic observations Basic Observation Scenario (BOS) has been developed. This ensures spatial and temporal consistency at global scales and adequate revisit frequency.  ALOS-2 BOS has separate plans for Japan and for the rest of the world, success rate for these acquisitions is 70–80 %.  

Basic observations over Japan are mostly undertaken in Stripmap Ultrafine mode and sea ice observations during winter in ScanSAR mode.

Stripmap Fine and ScanSAR modes are used for global BOS. There are several areas of interest, where ALOS-2 is putting more focus, for example:

• Wetlands and rapid deforestation regions in ScanSAR mode
• Crustal deformation regions both in Stripmap Fine and ScanSAR mode
• Polar regions both in Stripmap Fine and ScanSAR mode

In addition to those special regions global land areas are observed in Stripmap Fine mode at least once per year.

We made a little experiment to test, how many acquisitions we get over city of Tartu per year. Here are the results (platform for viewing and ordering data is here):

So, compared to Sentinel-1 radar-satellite, ALOS-2 acquisitions frequency is much lower over Europe, and its difficult to develop agriculture monitoring services only on this platform. For forestry and other environmental monitoring, where changes are not happing that often as in agriculture, ALOS-2 can be very useful due to its better spatial resolution than Sentinel-1. Being an L-band satellite it can also penetrate deeper into vegetation and provide information about the lower layers of the canopy. JAXA is already developing ALOS-4 with PALSAR-3 aboard, which will aim broader observation swath compared to the predecessor.

RCM is a combination of three identical and equally spaced satellites, flying in the same orbit plane 32 minutes apart at an altitude of 600 km. Each of the spacecraft carries Synthetic Aperture Radar (SAR) aboard, plus a secondary sensor for Automatic Identification System (AIS) for ships. When RADARSAT-2 has left- and right-looking operation, then RCM is only right-looking, because multiple satellites increase revisit times and eliminate the need to look both ways. The SAR device aboard RCM satellites is quite similar to RADARSAT-2 – C-Band antenna, 100 MHz bandwidth, 4 regular polarization modes (HH, VV, HV, VH) plus compact polarimetry.  Polarization isolation is slightly better: >30 dB. See detailed comparison of RADARSAT satellites here.

The constellation system provides better coverage with smaller and less expensive satellites. This configuration allows for daily revisits of Canada’s territory, as well as daily access to 90% of the world’s surface. RCM can provide a four-day exact revisit (3 satellites equally phased in a 12 day repeat cycle orbit), allowing coherent change detection with InSAR. For specific applications (ship detection, maritime surveillance) data latency from acquisition to delivery can be only 10-30 minutes, but in general it will be from hours to 1 day.

• Low resolution (100 m), swath 500 km, NESZ -22 dB
• Medium resolution (16, 30, 50 m), swath 30-350 km, NESZ -25…-22 dB
• High and very high resolution (3-5 m), swath 20-30 km, NESZ -17..-19 dB
• Spotlight (1x3 m), swath 20 km, NESZ -17 dB