the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
An improved sea ice detection algorithm using MODIS: application as a new European sea ice extent indicator
Joan Antoni Parera-Portell
Raquel Ubach
Charles Gignac
The continued loss of sea ice in the Northern Hemisphere due to global warming poses a threat to biota and human activities, evidencing the necessity of efficient sea ice monitoring tools. Aiming at the creation of an improved sea ice extent indicator covering the European regional seas, the new IceMap500 algorithm has been developed to classify sea ice and water at a resolution of 500 m at nadir. IceMap500 features a classification strategy built upon previous MODIS sea ice extent algorithms and a new method to reclassify areas affected by resolution-breaking features inherited from the MODIS cloud mask. This approach results in an enlargement of mapped area, a reduction of potential error sources and a better delineation of the sea ice edge, while still systematically achieving accuracies above 90 %, as obtained by manual validation. Swath maps have been aggregated at a monthly scale to obtain sea ice extent with a method that is sensitive to spatio-temporal variations in the sea ice cover and that can be used as an additional error filter. The resulting dataset, covering the months of maximum and minimum sea ice extent (i.e. March and September) over 2 decades (from 2000 to 2019), demonstrates the algorithm's applicability as a monitoring tool and as an indicator, illustrating the sea ice decline at a regional scale. The European sea regions located in the Arctic, NE Atlantic and Barents seas display clear negative trends in both March (−27.98 ± 6.01 × 103 km2yr−1) and September (−16.47 ± 5.66 × 103 km2yr−1). Such trends indicate that the sea ice cover is shrinking at a rate of ∼ 9 % and ∼ 13 % per decade, respectively, even though the sea ice extent loss is comparatively ∼ 70 % greater in March.
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The Arctic sea ice cover has been changing rapidly over the last decades, with its overall extent declining steadily since the first satellite observations in the late 1970s (e.g. Cavalieri and Parkinson, 2012; Massonnet et al., 2012; Meier et al., 2014; Parkinson, 2014; Serreze and Stroeve, 2015; Comiso et al., 2017), reaching its historical minimum on September 2012. The same decreasing trends are also evidenced by other parameters such as sea ice thickness (Kwok, 2018; Liu et al., 2020), which has decreased as much as 65 % in the period extending from 1975 to 2012 (Lindsay and Schweiger, 2015). This massive loss of ice is unprecedented in the last few thousand years (Polyak et al., 2010) and is attributed both to climatic variability and to external forcing caused by the anthropogenic release of greenhouse gases (e.g. Myhre et al., 2013; Stroeve and Notz, 2018). All projection models agree that Arctic sea ice will continue shrinking and thinning, eventually leading to ice-free summers in the upcoming decades (Massonnet et al., 2012; Stroeve et al., 2012; Collins et al., 2013; Notz and Stroeve, 2016; Stroeve and Notz, 2018) and even as soon as in the late 2030s (AMAP, 2017).
The dynamism of the sea ice and the effect it has on climate, biota and human activities make the regular monitoring of its properties (e.g. extent, concentration, thickness) necessary. Today sea ice data are continuously obtained from several satellite-borne instruments (e.g. Spreen and Kern, 2016), among which microwave sensors stand out for their ability to acquire data regardless of the lighting and weather conditions. Passive microwave sensors typically provide data at resolutions above 15 km, hindering their use for local and regional sea ice studies. On the other hand, active microwave and visible-infrared sensors can acquire data at much higher spatial resolutions. For instance, ESA's satellites Sentinel-1 (synthetic aperture radar) and Sentinel-2 (visible-infrared) achieve resolutions of 5–100 m in the first case and 10–60 m in the latter. However, such high-resolution sensors render data with sparse spatial and temporal coverage due to their small swath size and long revisit times, although this effect is minimized at the poles. Instead, MODIS visible and infrared imagery offers a balanced trade-off between temporal and spatial coverage. MODIS is an imaging sensor on board NASA's sun-synchronous satellites Terra and Aqua, launched in 1999 and 2002, respectively. It acquires data in 36 spectral bands, ranging from the visible spectrum to the thermal infrared. Spatial resolution at nadir varies from 250 m (bands 1 and 2) to 500 m (bands 3–7) and 1 km (bands 8–36) and has a large swath width of 2330 km. The MODIS Terra and Aqua MOD29 and MYD29 datasets (Hall et al., 2015a, b) provide daily global sea ice extent coverage at 1 km but frequently fail to map the sea ice edge at this level of detail. This is caused by the MODIS MOD35_L2 cloud mask product (Ackerman et al., 2010; MODIS Atmosphere Science Team, 2017), the accuracy of which depends on the correct identification of background sea ice at 25 km resolution (Riggs and Hall, 2015). Therefore, sea ice beyond this background is finally labelled as cloud instead of clear, eventually preventing the products which rely on this cloud mask from accurately mapping the sea ice cover.
In this context, a new 500 m resolution MODIS sea ice detection algorithm (IceMap500) was developed, aiming at the improvement of existing European sea ice extent indicators based on passive microwave observations (EEA, 2020) by providing additional and higher-resolution data. IceMap500 is heavily influenced by the cloud masking and classification approaches of the previous IceMap250 algorithm (Gignac et al., 2017), which nonetheless is still vulnerable to the MOD35_L2 background effects. The new algorithm is optimized to minimize classification errors and improves the quality of the maps by introducing a five-step workflow to prevent MOD35_L2 from breaking the 500 m resolution.
To test the usefulness of IceMap500 as a European sea ice extent indicator, we analyse the sea ice trends in the European regional seas from 2000 to 2019 using MODIS Terra data. The analysis covers the northernmost European sea regions defined by the European Union's Marine Strategy Framework Directive (MSFD) where sea ice might occur (EEA, 2018) and is restricted to the months when the maximum and minimum sea ice extents are reached in the Northern Hemisphere, that is, March and September, respectively.
2.1 Study area
This work focuses on the European regional seas established by the MSFD (EEA, 2018). As sea ice only occurs in the northernmost oceanic sea regions or in enclosed, low-salinity water bodies such as the Baltic Sea, spatial coverage has been significantly reduced to avoid the processing of uninformative data. The final study area extends over the sea regions in Fig. 1, covering an area of roughly 4 ×106 km2. With the inclusion of a 400 km buffer to coherently join all the target regional seas in a single study region, the totality of the processed area sums up to approximately 8 ×106 km2.
Oceanic sea ice in the Northern Hemisphere has both a perennial and a seasonal fraction. Typically, maximum and minimum sea ice extent are reached in March and September (e.g. Stroeve et al., 2008), respectively, with the perennial fraction being mostly enclosed in the Arctic basin (Comiso, 2009). The ice cover in the Baltic Sea, however, has no perennial fraction and can be highly variable due to the milder climate, often resulting in different freezing and melting periods during the same winter (Granskog et al., 2006). The sea ice season usually lasts for 6 to 8 months, starting in October or November in the Bothnian Bay and the Gulf of Finland. Maximum extent is also normally reached in March (Haapala et al., 2015). Therefore, given the particular characteristics of the Baltic Sea, the sea ice extent analysis is done by splitting the study area in two regions: the NE Atlantic–Barents region (completely including the Iceland, Norwegian, Barents and White seas) and the Baltic region.
2.2 Selected data
Data used in this work consist of MODIS Terra level 1B top-of-atmosphere (ToA) radiance products MOD021KM (MODIS Science Team, 2017a), MOD02HKM (MODIS Science Team, 2017b) and the MOD35_L2 cloud mask (MODIS Atmosphere Science Team, 2017), as summarized in Table 1. Swath data are resampled to 500 m resolution if necessary, converted to GeoTIFF format and projected to North Pole Lambert azimuthal equal area using HDF-EOS to GeoTIFF Conversion Tool (HEG) v2.15 (NASA, 2019). No stitching is applied, as each scene is processed individually. However, scenes are clipped according to the selected study area. IceMap500 uses ToA radiance as input data, which are later converted to ToA reflectance or ToA brightness temperature, so there is no atmospheric correction. Note that the objective of the algorithm is to map sea ice presence rather than using reflectance as a proxy to get other physical variables such as sea ice concentration, so the absence of atmospheric correction reduces processing time, facilitates the algorithm's replicability and ensures the consistency of the dataset.
2.3 Overview of previous MODIS sea ice extent algorithms
IceMap500 is fundamentally based on the previous IceMap (Riggs et al., 1999; Hall et al., 2001) and IceMap250 (Gignac et al., 2017) algorithms and inherits many of their features. Both algorithms feature a classification strategy based on threshold tests but differ on the cloud masking approach. IceMap uses the Normalized Difference Snow Index (NDSI, Eq. 1) as the main criterion to classify sea ice, followed by a ToA threshold test using MODIS B4 (545–565 nm). To prevent misclassification of clouds as sea ice, this algorithm uses the MOD35_L2 cloud mask as an input and outputs sea ice extent at 1 km resolution.
Instead, IceMap250 uses the Normalized Difference Snow and Ice Index 2 (NDSII-2, Eq. 2) (Keshri et al., 2009), as well as the same ToA reflectance threshold at 545–565 nm to classify sea ice and water. The threshold value of the NDSII-2 is determined by splitting data in two groups with a Jenks natural breaks optimization (Jenks, 1967), which maximizes inter-class variance and minimizes intra-class variance. This algorithm features a hybrid cloud masking approach designed to minimize error while maximizing the mapped area, using the MOD35_L2 cloud mask alongside an additional visibility (VIS) mask, both at 1 km resolution.
The VIS mask in IceMap250 is intended to identify areas where visibility is sufficient to perform a classification, for the sole goal of detecting open water. It uses the normalized difference between the MODIS thermal bands B20 and B32 as in Eq. (3).
The standard score of is then calculated, as seen in Eq. (4), where μ and σ are the mean and standard deviation of of the swath data to be classified. Pixels where VIS < 0.5 are tagged as having enough visibility. The masking produces the MOD35 and the VIS datasets, which are classified separately and later combined following the set of rules in Table 2.
Although masking in IceMap250 is done at a resolution of 1 km, the algorithm maps sea ice and water at 250 m within the masked area. This is accomplished by means of a downscaling technique by Trishchenko et al. (2006).
2.4 IceMap500: challenges and improvements
Both IceMap and IceMap250 face some challenging limitations which IceMap500 tries to address. The most important issue arises from the MOD35_L2 cloud mask, as it occasionally features resolution-breaking square artefacts of 25 km side length along the ice edge (Fig. 2) that prevent its accurate mapping. Such artefacts originate in the setting of the snow/ice background flag during the production process of the mask (Riggs and Hall, 2015), in which NSIDC's Near-real-time Ice and Snow Extent (NISE) product (Brodzik and Stewart, 2016), based on SSM/I-SSMIS passive microwave data with a cell size of 25 km, is used to determine the flag's state. Therefore, as the cloud detection algorithm takes different paths depending on the background flag, sea ice falling outside the footprint of the NISE classification is ultimately tagged as cloud in MOD35_L2. These 25 km artefacts can occupy extensive areas in some scenes, causing the loss of many cloud-free classifiable pixels.
Another notable source of classification errors, this time only in IceMap250, arises from the NDSII-2 test, which uses the Jenks natural breaks optimization to split pixels in two groups, regardless of the surface classes present in a scene. When batch processing MODIS data it may be likely to run into scenes lacking either ocean water or sea ice, and, consequently, the Jenks optimization splits pixels into both surface classes erroneously. Clouds that are undetected by the MOD35_L2 cloud mask algorithm (Ackerman et al., 2010) and sun glint over ocean water may also be common error sources due to the similar reflectance characteristics to sea ice, in both IceMap and IceMap250. Additionally, as stated in Gignac et al. (2017), bare ice and melt ponds may also fail the classification tests due to the similarity with ocean water.
To mitigate those potential classification errors, IceMap500 features changes in the data masking and the classification rules. The new algorithm uses the dual masking approach and the NDSII-2 and B4 ToA reflectance tests as IceMap250 but increases the restrictiveness of the masking and the classification. It also introduces an additional sea surface temperature (SST) test and a new MOD35 correction workflow to minimize the effect of the NISE footprint and enlarge the mapped area (see the structure in Fig. 3). The downscaling technique used in IceMap250 is not applied for various reasons: (I) simplicity, (II) reduced processing times, (III) MODIS Aqua band to band registration errors which may be even larger than the 250 m cell size itself (Xiong et al., 2006; Khlopenkov and Trishchenko, 2008), and (IV) spectral integrity of the imagery (since no downscaling is applied). IceMap500 swath maps can be aggregated at any desired timescale. We use a map aggregation approach which is sensitive to spatio-temporal variations in sea ice and which can be used to filter out unreliable sea ice classifications. The next sections give a more in-depth explanation of the IceMap500 workflow.
2.4.1 The masking
IceMap500 uses the same hybrid cloud masking approach as IceMap250. The VIS mask is used and calculated as in IceMap250, using the same VIS < 0.5 threshold value. Therefore, IceMap500 also generates the MOD35 and the VIS datasets. Nevertheless, the MOD35 mask includes additional constraints so not only cloud cover is considered but also the lighting conditions, sun glint and presence of land. This information is contained within the MODIS product MOD35_L2, which provides multiple quality assessment flags (Strabala, 2004; Ackerman et al., 2010). We use the following flag states:
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Unobstructed FOV selects only pixels identified as confident clear, with a confidence of 99 % (Ackerman et al., 2010).
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Day/Night selects only pixels identified as day. This flag is of special importance during the winter months, when the polar twilight zone reaches the lowest latitudes, and, therefore, the available daytime area becomes scarcer.
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Sun glint selects only pixels identified as no sun glint. This way, areas with sun glint caused by the reflection angle of the sun being between 0 and 36∘ are discarded. Other potential sun glint sources are not considered (Ackerman et al., 2010).
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Land/Water selects only pixels identified as water. Land masking is crucial to ensure the quality of the resulting classification because, as already pointed out in Gignac et al. (2017), an incorrect masking may generate sea ice false positives due to the reflectance contrast of land with water.
2.4.2 The classification tests
In IceMap500 three different threshold tests are included.
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NDSII-2 test (tndsii2). Same as in IceMap250. The threshold value k is determined by slicing the NDSII-2 (Eq. 2) with the Jenks natural breaks optimization. Pixels in the first group (i.e. NDSII-2<k) are classified as sea ice. This test was shown to discriminate 96 %–100 % of sea ice even during the melting periods in Gignac et al. (2017).
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Green ToA reflectance test (tb4). Same as in both IceMap and IceMap250. A pixel is tagged as sea ice if its reflectance is ⩾ 17 % at 545–565 nm (B4). This threshold is based on the contrast in reflectance between ice and water at visible wavelengths and was first used in Riggs et al. (1999) and later validated in Gignac et al. (2017). Gignac et al. (2017) demonstrated that a B4 ⩾ 17 % threshold resides slightly into the upper standard deviation of the water class reflectance, so the risk of misclassifying melt ponds, leads, polynyas and low-albedo sea ice is low.
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Mid-range infrared temperature test (tb20). This new threshold is based on the sea surface temperature (SST) using B20 (3.660–3.840 µm). It is always used in conjunction with tb4, although only in the MOD35 dataset classification. Therefore, sea ice is classified only when both B4 ⩾ 17 % and SST < 1 ∘C. The tb20 test is used as a sort of mask to confirm that a pixel tagged as sea ice really belongs to sea ice, as unmasked sun glint, turbid water and aerosols may raise water reflectance past the tb4 threshold. To perform this test B20 is temporarily atmospherically corrected with a straightforward equation used in the MODIS SST algorithm (Brown and Minnett, 1999) for mid-range infrared SST derivation (Eq. 5):
where TB20 is the brightness temperature of B20. The 1 ∘C threshold is designed to include leads, cold water, new sea ice and melt ponds (which according to Zhang et al. (2017) typically stay below 0.3 ∘C) to prevent breaking the 500 m resolution, while still discarding most open water (refer, for instance, to global SST products such as NOAA High Resolution SST by NOAA/OAR/ESRL PSL, Boulder, Colorado, USA, available at https://psl.noaa.gov/data/gridded/data.noaa.oisst.v2.highres.html, last access: 26 April 2021). Moreover, B20 may be contaminated by reflected solar radiation, causing TB20 to increase and therefore making the exclusion of sun glint easier.
In addition, IceMap500 features restrictive classification rules to compensate for the output of tndsii2 in scenes with a single surface class, as the Jenks optimization will still split data into two groups. The classification rules depend on the dataset that is being classified, as when merging the MOD35 and VIS maps changes in a single dataset classification, ultimately affecting the whole outcome. The classification rules are shown in Table 3: sea ice is only mapped in the MOD35 dataset when there is consensus between the tests, while in the VIS dataset it is mapped whenever tb4 is positive. A downside of this method is that it may leave some melt ponds as NoData, since in the most advanced melting states they tend to show NDSII-2 values similar to water (Gignac et al., 2017). Note that while masking is done at 1 km resolution, the swath data that are classified are at 500 m, so sea ice and water are mapped at 500 m within the mask limits.
2.4.3 MOD35 correction
Once the MOD35 map is created, an additional set of tests is introduced to attenuate the effects of the NISE footprint present in the MOD35_L2 mask, which propagate to the MOD35 classification and ultimately to the composite maps. Although the inclusion of this correction increases the chances of classification errors, it greatly improves the sea ice edge delineation and increases the classified area. The MOD35 correction is designed to reclassify NoData pixels within a buffer zone surrounding clusters of sea ice. Within this buffer the MOD35_L2 cloud mask is ignored during the classification. Instead, MODIS B7 (2.105–2.155 µm) is used to detect clear areas by taking advantage of the very low reflectance values that water, snow and ice display at such wavelengths, allowing cloud discrimination (e.g. Platnick et al., 2001; Thompson et al., 2015). To avoid error amplification, sea ice clusters below 100 pixels are deleted before the correction: if those clusters are found far from the ice edge, it is likely that they originate from sun glint or unmasked clouds, while those found close to large clusters of sea ice are ultimately classified again as such. The MOD35 correction includes five tests, as illustrated in Fig. 4.
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NoData test. NoData pixels pass the test, while classified areas remain the same. All pixels set as NoData during the MOD35 classification also undergo the tests and may finally be labelled as sea ice or water.
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Euclidean distance test. NoData pixels found at 35 km or closer to a cluster of sea ice pass the test; otherwise they are set as NoData. This distance is roughly equal to the diagonal of NISE's 25 km cells and is used to reduce the chances of misclassifying clouds as sea ice by setting a buffer along the ice edge.
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Short-wavelength infrared ToA reflectance test (tb7). Pixels below 3.5 % ToA reflectance at 2.105–2.155 µm (B7) pass the test, otherwise they are set as NoData. This threshold is based on the low reflectance that water, snow and ice display around 2 µm: spectral signatures in Fig. 5 indicate a maximum reflectance of ∼ 10 % for ice within the B7 bandwidth, while the reflectance of snow and water is always below 5 %. This test is used as a cloud filter, as it is expected that clouds show higher reflectance values. Figure 5 also shows the threshold includes only 45.3 % of clear areas according to our sampling, although most of the remaining samples belong to sea ice far from the ice edge, which is of no interest in the MOD35 correction. However, by setting such a restrictive threshold only a small fraction of clouds are included (1.5 %), which is preferred over including all sea ice while increasing sea ice false positives due to the cloud cover.
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tndsii2. They are the same as in the MOD35 classification. Pixels where NDSII-2 <k pass the test, otherwise they are set as NoData. In this case, the Jenks optimization is not performed using all the clear pixels in the scene but rather only those within the 35 km buffer zone set as clear by tb7.
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tb4 and tb20. They are the same as in the MOD35 classification. Pixels where B4 ⩾ 17 % and SST < 1 ∘C are classified as sea ice, otherwise they are set as NoData.
Finally, the MOD35 map and the result of the MOD35 block correction are merged and later combined with the VIS map according to the compositing rules in Table 2. A visual example of the workflow in IceMap500 is given in Fig. 6, illustrating each intermediate result of the algorithm.
2.4.4 Map aggregation and calculation of sea ice extent
The corrected MOD35 and VIS maps created for each scene are combined to take advantage of the strengths of both the MOD35 and the VIS classification methods, following the criteria seen in Table 2. The extensive cloud cover found in most scenes and the restrictiveness of the classification imply that only a small area is finally mapped, although the new correction reduces the impact of the cloud mask. In any case, many scenes are required to map large expanses of the sea ice cover. In IceMap500 a map aggregation method based on the number of coincident sea ice classifications achieved in each pixel is used, meaning that pixels classified as sea ice in a large number of scenes will have higher reliability. The aggregated maps are generated by calculating the sum of composite maps where ice = 1 and water = 0 and later normalizing the results according to the maximum number of coincident sea ice observations achieved. With MODIS Terra the maximum number of observations typically reaches ∼ 50 in March and ∼ 60 in September, so using both Terra and Aqua, this number could double and significantly increase the usefulness of this method. The output provides information about where sea ice is more likely to be found; thus we appropriately refer to the resulting maps as sea ice presence likelihood maps (Fig. 7). This approach allows users to detect the places where sea ice has been more unstable during a given time period, as the sea ice presence likelihood will drop in such cases. Likelihood maps even allow the detection of cracks in the sea ice, and of course if sea ice has moved significantly the sea ice presence likelihood will be lower.
Sea ice extent is obtained from the likelihood maps by selecting a likelihood threshold, in this case 10 %. Then, pixels where sea ice presence is >0 % and <10 % (0 % is water) are discarded because such observations might not be reliable enough. By eliminating such observations, a small NoData buffer zone along the ice edge is generated. IceMap500 then takes advantage of the pixels set as water and fills the NoData gaps using a Euclidean distance allocation method. This way a clearer and smoother sea ice edge is obtained, which nonetheless does not ignore the information carried by pixels where likelihood falls below the selected threshold. This procedure acts as an additional post-classification error filter and produces a sea ice extent map, as the constant motion of the ice tends to hide the presence of features such as leads, cracks, polynyas and ice floes.
It is worth noting that the aggregation procedure eventually sets either NoData pixels that were never really classified by the algorithm during the entire time period as sea ice or water. Although the dual masking approach and the use of the MOD35 correction greatly improve the final classified area, NoData gaps still tend to appear in the regions closer to the pole in the March monthly maps as a consequence of the poor lighting conditions. This also makes sea ice presence likelihood to drop. September has no such lighting limitations, so NoData gaps appear more randomly. Fortunately, the average NoData area fraction of our monthly time series only reaches 1.0 % in March and 0.7 % in September.
We use the new IceMap500 algorithm to obtain swath and daily maps during the months of March and September of the 2000–2019 period, using only MODIS Terra data. The resulting maps have been aggregated at a monthly scale to obtain the time series of sea ice extent, from which sea ice extent trends have been calculated. The performance of the algorithm is assessed with confusion matrices by manually validating swath maps.
3.1 Sea ice extent evolution and trends
Monthly sea ice extent maps have been used to determine the sea ice extent trends between 2000 and 2019 in the NE Atlantic–Barents region and the Baltic Sea separately. Both March and September trends have been obtained for the NE Atlantic–Barents, that is, the trends of the maximum and minimum sea ice cover, respectively. Since there is no perennial sea ice fraction in the Baltic Sea, only the March trend is available in this case, also corresponding to the maximum sea ice cover. The resulting trend lines, represented in Fig. 8, have been obtained via least-squares linear regression.
Results indicate that in the NE Atlantic–Barents region the sea ice decline is ∼ 70 % faster in March than in September. Although September's extent is comparatively smaller, the standard error of the trends is similar in both months ( km2yr−1), with R2 being lower in September. Nevertheless, both trends have been found to be statistically significant when considering a significance level of 99 %. In particular, the March trend displays a very low p value, indicating a significance level of ∼ 99.98 %. In contrast, the Baltic Sea displays no clear tendency and a large variability. This causes R2 to be very low and the standard error of the trend to be almost equal to the trend itself. If the 99 % significance level criterion is followed, then H0 can not be rejected in the Baltic Sea.
3.2 Accuracy assessment
We randomly selected 8 years to perform the quality assessment, from which a total number of 32 scenes have been used, that is, two scenes per month to allow comparison. As a prerequisite, each validation scene must have both sea ice and water pixels. Validation has been carried out with confusion matrices by generating 1500 random points per scene over the classified areas. Those points have been manually tagged as either sea ice, water or cloud, with the help of the corresponding RGB swath. Although no clouds are mapped in the algorithm, points found over clouds opaque enough to avoid the identification of the surface below add to the total sea ice commission error.
Accuracy assessment results are summarized in Table 4. All scenes achieved overall accuracies above 90 %, resulting in an average accuracy of 96.0 %. The average kappa coefficient of 0.85 indicates a strong agreement between classification and ground truth, despite being affected by scenes with few water validation points, causing the kappa coefficient to drop due to the disproportion between classes. Individually, only 5 out of 32 computed kappa coefficients are found below the 0.80 value, while 10 are found between 0.80–0.90 and 17 above 0.90, indicating very strong agreement. The primary source of error affecting the classification is sea ice commission, with its mean value alone adding up to 7.3 %, that is, more than sea ice omission, water commission and water omission combined.
By separately analysing both months, mean accuracy is found to be higher in March than September, differing by 1.9 %. Accuracy results in September are also slightly more variable, showing a σ of 2.8 % versus 2.5 % in March. On the contrary, the mean kappa coefficient is lower in March than in September. This is linked to the much greater sea ice area covered in March, which occasionally causes some scenes to have very few water validation points, making the kappa coefficient drop due to the disparity in validation points between classes. The standard deviation of kappa greatly illustrates this issue, being 0.23 in March and 0.06 in September.
Nevertheless, the difference in accuracy between months does not arise from validation artefacts but mainly from the disparity in sea ice commission. With a mean sea ice commission error of 2.5 %, March classifications outperform those for September, which show a mean error of 12.2 %. Since there are only two classes, high water omission error should be expected. However, it is very low in both cases, 0.3 % in March and 0.04 % in September, revealing the dominance of sea ice commission is not caused by the misclassification of water as sea ice but of clouds as sea ice. Instead, sea ice omission error is similar in both months, being 2.7 % in March and 3.3 % in September, while water commission is 2.5 % and 1.9 %, respectively. Thus, globally, the major error contribution is due to the misclassifications of clouds as sea ice, especially in September, while misclassification of sea ice as water and water as sea ice remain lower in the first case and minimal in the latter.
According to Chan and Comiso (2013), the MOD35_L2 cloud mask tends to underestimate the cloud cover over sea ice, whereas over open water it is overestimated but closer to reality. Indeed, most sea ice commission error in our validation is due to the misclassification of clouds as sea ice within the limits of the sea ice cover; in fact, despite the cloud fraction being much larger over open ocean than over sea ice, in the first case sea ice commission errors are uncommon. Some of the clouds that are commonly left undetected by the MOD35 cloud mask include low-level (top below 2 km), high-level (top above 6 km) and thin clouds less than 2 km thick (Chan and Comiso, 2013). Additionally, our validation showed that multilayered clouds cast shadows which can be finally tagged as sea ice. The rise of sea ice commission error during September may be explained by the fact that, as shown by Chan and Comiso (2013), late summer in the Arctic is considerably cloudier than winter, as lower sea ice concentration relates to a larger cloud fraction.
Since sun glint issues have been mostly solved, as evidenced by the minimal impact of water omission error, and most sea ice commission is generated within the sea ice cover, there are few clusters of sea ice false positives over open ocean, most of which are removed during the MOD35 block correction. Thus, few of those errors are propagated to the sea ice presence likelihood maps, allowing the selection of low threshold values to obtain sea ice extent.
3.2.1 Agreement with NSIDC's Sea Ice Index
The Sea Ice Index (SII; Fetterer et al., 2017) is a widely used global sea ice extent and concentration product distributed by the NSIDC, which is derived from satellite passive microwave data at 25 km spatial resolution. It covers from 1978 to the present, is updated on a daily basis and provides monthly median sea ice extent maps. In the Sea Ice Index (SII), extent is derived from sea ice concentration by setting where concentration is 15 % or above as sea ice pixels. In spite of the difference in spatial resolution between the SII and IceMap500, measuring the agreement or similarity between both datasets can act as an estimator of the quality and consistency of IceMap500's monthly aggregates. Thus, SII maps have been reprojected to North Pole Lambert azimuthal equal area and resampled down to a 500 m cell size. Then agreement has been calculated as the coincident sea ice area fraction between both datasets, compared to the total sea ice extent including coincident and non-coincident area (Eq. 6).
where A is an IceMap500 monthly aggregate and B the corresponding SII. Figure 9 illustrates the agreement for both March and September from 2000 to 2019. Mean agreement in March is 89.5 % with a standard deviation of 1.1 %, whereas in September mean agreement is lower, 85.5 %, and displays higher variability, with a standard deviation of 3.1 %. Only in a single case does the agreement fall below 80 %, corresponding to September 2013 (74.7 %).
An example of both datasets is shown in Fig. 10 for visual comparison: even though the difference in spatial resolution is not compensated for, both numerical and visual analyses suggest that IceMap500 monthly aggregates are coherent with existing data even considering the different sea ice extent calculation approach.
4.1 Sea ice trends
Sea ice trends obtained from our monthly extent maps in the NE Atlantic–Barents region are consistent with previous observations, and both are statistically significant when considering a significance level of 99 %. The trends obtained in this study are regional and therefore do not reflect the overall Arctic sea ice extent tendencies, although they can be compared to studies in which regional trends are also analysed. In Cavalieri and Parkinson (2012) the summation of sea ice trends (1979–2010) in the Greenland Sea and the Barents–Kara seas, roughly corresponding to our study area, shows a greater loss of sea ice extent during winter (−21.7 ± 3.1 × 103 km2yr−1) than during summer (−18.6 ± 3.2 × 103 km2yr−1). This is in accordance with our results, and both trends are within the error range of the trend lines in Fig. 8. Similarly, the summation of the Greenland–Barents–Kara trends in Peng and Meier (2017), covering from 1979 to 2015, indicates a trend of −19.0 ± 4.4 × 103 km2yr−1 for the maximum sea ice extent and −14.9 ± 5.7 × 103 km2yr−1 for the minimum. This behaviour is also reported in the Barents Sea in Kumar et al. (2021), spanning the 1979–2018 period. Nevertheless, the sea ice extent loss is proportionally smaller in winter than in summer: in our study area the decadal sea ice loss is approximately 9 % in March and 13 % in September. Peng and Meier (2017) report sea ice losses of 10.1 % and 10.8 % per decade in the Greenland and Barents seas in winter, closely matching our results.
In the case of the Baltic Sea, no statistically significant trend can be inferred due to high interannual variability and the limited lifespan of MODIS. This, however, does not imply that H0 (i.e. that the Baltic ice cover is stable) is true: previous research (Jevrejeva et al., 2004) based on data from coastal observatories covering the years 1900 to 2000 reveals a significant decreasing trend in sea ice occurrence probability in the southern Baltic Sea, while in the northern half ice occurs every winter. Moreover, it shows a shortening of the sea ice season and an advance in the date of break-up, especially in the northern areas. More recent analyses (Vihma and Haapala, 2009; Haapala et al., 2015) also indicate that over the last century the sea ice season has shortened and the occurrence of severe winters has fallen. Thus, although IceMap500 may not be suitable for Baltic sea ice monitoring at a monthly scale due to the large variability, both interannually and within a same freezing period (Granskog et al., 2006), it can be useful for detailed sea ice studies spanning shorter time periods.
4.2 Applicability of IceMap500
Accuracy assessment shows that the major source of error in IceMap500 is sea ice commission, mostly caused by undetected clouds. This is especially true in September due to the cloudier atmospheric conditions during the Arctic summer. This issue is also reflected in the agreement with NSIDC's SII, with the September agreement being lower than in March in all but 2 years and occasionally falling down to 75 % (September 2013). The larger number of scenes available during that month alongside the larger sea ice commission error make the September monthly aggregates potentially affected by sea ice false positives to a greater extent, so a possible way of dealing with this situation is to increase the sea ice presence likelihood threshold. In the case of September 2013, a small change in the threshold value (from 10 % to 11 %) translates into an increase in IceMap500-SII agreement from 75 % to 80 % (see Fig. 11 for visual comparison). An additional source of disagreement between SII and IceMap500 in the summer months is the greater fragmentation of the ice cover, leading to the formation of sea ice floes, alongside the coastline discrepancy. However, these two sources are intrinsically linked to the difference in spatial resolution between both products. In the case of September 2013, the fragmentation of sea ice (notice the water pixels within the SII edge in Fig. 11) in combination with high sea ice commission due to unmasked clouds led to an unusually low agreement score.
Overall, both the accuracy assessment of IceMap500 and the generally high agreement values with the SII suggest that the new algorithm is well suited for sea ice studies and monitoring. Its processing time also allows near-real-time mapping: it takes around 50 min to generate a full daily map covering our study area (i.e. 16 scenes) using a modest machine with an Intel Xeon X5550 (4×2.67 GHz) processor and 12 GB RAM. Therefore, IceMap500 may represent an improvement towards local and regional sea ice studies, especially taking into account the spatio-temporal information carried by the sea ice presence likelihood maps. Additionally, the inclusion of the MOD35 correction allows IceMap500 to map the sea ice edge more accurately than the MOD29 product (see the comparison in Fig. 12), which is visibly affected by the NISE footprint. This increase in mapped area is also advantageous when aggregating maps at any timescale, as sea ice presence likelihood rises and the presence of NoData gaps is minimized. Instead, in Fig. 12 the IceMap500 result is closer in terms of both mapped area and spatial resolution to the VIIRS/NPP sea ice cover (375 m) swath product (Tschudi et al., 2017). It is worth noting, however, that VIIRS products may also be affected by the VIIRS cloud mask in the same way that MODIS is, because NISE is also used to detect background sea ice in the VIIRS cloud mask algorithm (Frey et al., 2019).
Even though IceMap500 is designed to work with MODIS, it could also be used with other optical and infrared sensors, as long as the selected sensor has equivalent bands to those used by this algorithm. Nevertheless, the application of the MOD35 correction, which would have to be adapted, depends on the characteristics of the cloud mask to be used, and may not even be necessary. In the case of VIIRS the MOD35 correction may be advantageous due to the potential effect of the NISE background, but there is no direct equivalent to MODIS B7, which is used to identify clouds during the correction. Therefore, the potential of the closest match (VIIRS band M11, with a 2.20–2.30 µm bandwidth) to discern clouds from the ice cover should be assessed in this context. However, the application of the IceMap500 algorithm to both other sensors or other study regions might yield different accuracy assessment results, so the threshold tests or the classification restrictiveness might need to be revised in each particular case to improve its performance.
The new IceMap500 algorithm is shown to generate high-quality sea ice maps by systematically achieving accuracies above 90 %. Quality assessment revealed the most common error is sea ice commission caused by unmasked clouds, manifesting the key role that cloud masking plays on the overall accuracy of the algorithm. The addition of the MOD35 correction substantially improves the delineation of the ice edge, preventing the propagation of the NISE footprint, and increases the mapped area, which is of capital importance when deriving daily and monthly maps due to the restrictiveness of the classification and the weather dependence of MODIS visible and infrared data. High agreement between our monthly sea ice extent maps and NSIDC's Sea Ice Index, especially in March, demonstrates the consistency of the map aggregation method and further exemplifies the overall good performance of the algorithm. Data produced by IceMap500 have proven useful to evaluate sea ice extent trends in the NE Atlantic–Barents region and the Baltic Sea. Significant negative trends have been observed in both March and September in the NE Atlantic–Barents region, while the Baltic Sea displays much more variability, and no trend can be inferred from it. Given the high accuracies achieved and the coherence with existing data, we find that IceMap500 is a useful tool for sea ice studies and monitoring, particularly at local and regional scales.
The source code is hosted at https://doi.org/10.5281/zenodo.4973715 (Parera-Portell, 2021). Monthly March and September sea ice extent maps from 2000 to 2019 are available at https://doi.org/10.5565/ddd.uab.cat/233396 (Parera-Portell and Ubach, 2020).
RU and JAPP conceptualized the study. JAPP developed the methodology and software, analysed the dataset, and wrote the original draft. RU and CG supervised research and reviewed and edited the manuscript.
The authors declare that they have no conflict of interest.
The authors thank the two anonymous referees and the editor Melody Sandells for their useful comments, which greatly improved the manuscript. Work on software QGIS and the HDF-EOS to GeoTIFF Conversion Tool (HEG) is acknowledged. Special thanks go to Jaume Fons-Esteve at the Department of Geography, Universitat Autònoma de Barcelona.
This paper was edited by Melody Sandells and reviewed by two anonymous referees.
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