Due to its large extent, the surveying of ice masses in the CHPS has been of great importance to understand its development over the past and especially recent years to understand the impact of climate change [
3,
4]. The CHPS is the largest freshwater reservoir in South America [
1], providing fresh water to a large part of the dry Patagonian Argentina. The ice mass fed 154 major outlet glaciers until 2011 [
5]. Some studies were already carried out on the development of the glacier extent and mass balance through a combination of digital elevation models and optical data [
1,
6]. However, apart from the knowledge of the glacier extent, the understanding of the land cover types (i.e., the snow and ice types) of the glaciers is of significance, as the variability of seasonal snow cover is an important parameter in the climate system. The type of snow and ice cover of a certain region gives information not only about energy and moisture budgets within the glacier but also is an indicator for surface temperature and precipitation changes [
7].
1.1. Contribution
In the scope of our study, the land cover composition on the glacier surface is defined through classification of the snow and ice types on the surface of the glaciers. To investigate the change in glacier extent and surface composition, an evaluation of a time series of specific years is conducted.
This paper extends our previous work [
8], where we rely on a pixel-wise classification of Sentinel-2 data with respect to different snow and ice classes. The straightforward approach for this is given by a supervised classification [
9]. However, no reference data (i.e., training examples) are available for the different snow and ice cover types in the investigated area. Consequently, suitable reference data need to be obtained, for which we rely on theoretical knowledge [
10] to simulate labeled Sentinel-2 compliant data from densely sampled spectral reflectance curves representing different snow and ice cover types [
11,
12,
13]. On this basis, we apply four different classification approaches, thereof two unsupervised approaches (k-means clustering [
14] and rule-based classification via snow and ice indices [
15,
16]) and two supervised approaches (Linear Discriminant Analysis [
17] and Random Forest classifier [
18]). In this paper, our contributions are twofold: (1) We evaluate the given methodology in detail and thereby also deeper analyze the quality of the given reference data; (2) We conduct a multi-temporal analysis to assess changes in glacier extent and surface composition.
Accordingly, we first focus on the pixel-wise classification of Sentinel-2 imagery available for the Tyndall Glacier area, and we then use the best-performing approach for a multi-temporal analysis. Here, the year 2019 is examined more closely as a representative to demonstrate the findings of the change in glacier surface composition within one year. The dates of the end of ablation and end of accumulation time are investigated subsequently. These dates reveal significant information about the glacier state over the explored timeline of the years 2016 to 2020. The plausibility of the findings is independently evaluated by comparison with temperature and precipitation data. These data mainly influence the glacier’s snow and ice state. Several metrics are applied to demonstrate the classification findings in an intuitive way: Area statistics for each snow and ice class are calculated. Finally, the change in glacier snout extent is described.
1.3. Background
Glaciers play an important role in their influence on climate. According to the Global Climate Observing System (GCOS), glaciers belong to the Essential Climate Variables (ECVs) [
19], as glacier changes are key indicators of climate change [
20]. Their melting will significantly impact the sea-level rise over the next 100 years [
21].
In the context of glacier monitoring, the multi-temporal analysis of a glacier concerning different snow and ice types is relevant to detect changes in the glacier’s surface composition. The glacier influences its environment in different ways through melting or refreezing on the glacier [
22,
23]. Its surface composition gives information about energy and moisture budgets within the glacier and is an indicator for surface temperature and precipitation changes [
7]. This influence can be estimated from the extent of snow and ice classes on the glacier’s surface, which demonstrates the state of melting or refreezing.
To analyze the extent of different snow and ice classes on the glacier’s surface, corresponding target classes for the classification task need to be defined. There exist different definitions of snow or ice types [
24] or glacier zones [
25], which have been derived according to several physical properties. Therefore, the task of snow and ice type definition is essential to delimit possibly distinguished classes. The characteristics of the snow and ice types alter the spectral signature of the different snow and ice types in the multi-spectral satellite imagery and can therefore be detected through classification of the optical imagery [
8]. The definitions used in our work rely on the classes used in [
10,
26,
27,
28] and specified by one spectral signature per class, covering wavelengths between about 0.4 μm and 1.2 μm. However, these classes do not correspond with other snow and ice class definitions like, for example, given in [
29,
30], since definitions there rely on radar systems and thus different wavelengths, resulting in different characteristics that are revealed by the acquired data. The classes considered in the scope of our work can be briefly described as follows:
Glacier Ice: This ice type is formed when fallen snow is compressed and slowly turning into ice. This process occurs, where the accumulation of snow and ice exceeds ablation and where different geological criteria are met. Glacier ice typically exists in the lower parts of a glacier;
Refreezing Ice: This ice type occurs when snow falls on already existing ice. The fresh snow is compressed and becomes part of the glacier. Compared to glacier ice, refreezing ice typically exists in the upper parts of a glacier and is newer ice;
Dirty Glacier Ice: This ice type contains small impurities within the ice. These impurities are mostly bare soil or rock material debris lying on the glacier or adjacent to the glacier, and even small impurities of soil can cause a different spectral reflectance of the ice;
Firn: This snow type is characterized by being melted and refrozen. Therefore, it contains a higher water content than
Fresh Snow and more impurities. More specifically, due to changes in incident solar radiation and temperature, fallen snow melts and refreezes in certain intervals. Snow that traversed this process once or several times is commonly defined as
Firn [
25,
26,
27,
28,
29], but sometimes also as
AgedSnow [
10];
Fresh Snow: This snow type represents newly fallen snow that did not go through the process of melting and refreezing. It has lower water content and contains fewer impurities in comparison to Firn.
Note that these classes only describe transient states of the snow and ice, which can quickly transform into other states (and therefore classes), depending on several natural conditions. Some of these classes (
FreshSnow,
Firn,
Refreezing Ice) might therefore quickly lose their distinguishing characteristics that influence the spectral reflectance. However, these classes are of great interest for glacier monitoring, and the motivation for using these classes seems intuitive: The deeper the snow depth, the bigger the delay in time to reach isothermal conditions, which allows the snow cover on the glacier to persist longer [
31]. Thus, it prevents more melting and water run-off from the glacier. The separation into the classes of
Fresh Snow and
Firn allows statements about the snow wetness, one of the main physical properties of snow. Snow wetness accordingly allows statements about the location of zones of accumulation areas on the glacier. Concerning the ice classes, three classes are distinguished. On the one hand, the performed separation allows reasoning about the extent of debris cover on the glacier surface. Debris cover influences the glacier behavior, as surface debris affects the rate of glacier melting [
32]. On the other hand, the separation of
Refreezing Ice is relevant, as the refreezing of meltwater may prevent immediate run-off of meltwater and therefore also influences glacier ablation in another way than
Glacier Ice [
33].
Several approaches exist to apply remote sensing techniques for glacier observation. In this context, numerous studies focused on the development of the glacier extent and mass balance of glaciers in general. The extent of glaciers was, for instance, investigated in [
34,
35,
36]. Mass balance can be estimated through optical remote sensing [
37] and the combination of digital elevation models and optical remote sensing data, which is quite commonly applied [
6,
38,
39,
40]. Some studies were carried out on the mass balance of the here investigated Tyndall Glacier [
1,
41].
Other studies suggest several different approaches for glacier observation. These can employ different sensors that make use of other segments of the electromagnetic spectrum. Taylor et al. [
42] give an overview of several innovations of usable sensors. Besides optical remote sensing, SAR remote sensing can be used for snow and ice cover investigations [
43,
44,
45,
46], alike thermal infrared remote sensing [
47,
48].
Using only optical satellite data, a diversity of techniques may be applied for glacier monitoring. Dietz et al. [
10] highlight remote sensing methods considering snow properties in different wavelengths. Rabatel et al. [
49] present three different methods for mass balance determination: the ELA (equilibrium-line altitude) approach, the albedo approach and the snow map approach. Few studies focus on the categorization of specific snow and ice classes on the glacier area. The albedo approach and the snow map approach proposed by Rabatel et al. [
49] belong to these studies. The albedo approach is based on the principle of the evocation of different spectral responses by distinct snow and ice classes. Therefore, the specific spectral reflectances of the distinct snow and ice classes need to be known. Dietz et al. [
10] give an overview of the reflectances of different surface types related to snow cover in a different wavelength. The reflectances of several different glacier states and locations and other large ice accumulations, where the classification into snow and ice classes might be advantageous (e.g., Antarctica), vary a lot [
50]. Takeuchi et al. [
51] show the specific surface albedo on the Tyndall Glacier, which is also the area of interest in our study, but without an assignment of specific classes to certain albedo values. Baraka et al. [
52] propose a deep learning approach to categorize the classes of clean and debris-covered ice. Similar works focused on the mapping of debris-covered glaciers [
53,
54] or the identification of rock glaciers [
55] for Himalayan areas.
Besides supervised approaches, rule-based approaches and unsupervised approaches are already applied for snow cover classification. Wang and Li [
56] use the Normalized Difference Snow Index (NDSI) in combination with supervised approaches. Another snow mapping method is based on regional snow maps from daily optical satellite images, where the first step also consists in calculating the NDSI [
49]. Combinations of three different snow indices to distinguish four classes allow an even more sophisticated separation [
15]. Here, a thresholding is applied to assign each pixel to either class. Gupta et al. [
57] use only the NDSI and thresholding. Paul et al. [
16] and Zhou et al. [
58] use band ratios and thresholding for glacier extent mapping. DeAngelis et al. [
2] use an unsupervised (k-means and ISOdata clustering) and supervised (max likelihood) approach for a classification with respect to the classes of
Bare Ice,
Debris-covered Ice,
Slush,
Snow-1,
Snow-2 and
Shadows.
Overall, many studies have been carried out to map glacier extent and obtain mass balance. In contrast, a classification into snow and ice classes was rarely realized. Considering all possibilities optical remote sensing data offer to carry out this study, we decided to use Sentinel-2 data and four different classification approaches, two supervised and two unsupervised ones (according to [
8]). These approaches are used as the basis for further investigations and development in our study.
Multi-temporal analyses have been widely used for change detection over several years in all fields based on remote sensing data. In this regard, many studies (see, for example, [
59,
60]) focus on land cover change detection with Sentinel-2 data. Specialized in the field of study on glacier change detection, Cao et al. [
61] conduct a multi-temporal analysis on the changes in glacier volume, and others on the development of the glacier extent over time [
62,
63]. Asokan et al. [
64] give an overview of different change detection techniques in general.
Several studies consider the same area of investigation as in this study [
2,
65]. The Patagonian Icefield and its glaciers are of major interest as they have been significantly retreating for some years [
1] and may contribute significantly to sea-level rise [
3,
4]. We specifically focus on one glacier in the CHPS, the Tyndall Glacier. It already has been investigated in particular in several studies [
6,
41].