CHAPTER 30 Monitoring glacier changes on the Antarctic Peninsula Jorge Arigony-Neto, Pedro Skvarca, Sebastián Marinsek, Matthias Braun, Angelika Humbert, Cláudio Wilson Mendes Júnior, and Ricardo Jaña ABSTRACT 30.1 INTRODUCTION The Antarctic Peninsula has exhibited some of the most spectacular changes observed in glacial systems in recent decades. The events include disintegration of ice shelves, acceleration and thinning of glaciers, variations in the limits between glacier facies, and retreat of glacier fronts. However, due to the lack of both consistent systematic observations of the glacial systems and information on their boundary conditions, it is difficult to accurately predict the contribution of Antarctic Peninsula glaciers to sea level rise and further responses of these ice masses to climatic and oceanographic changes. In this context, the activities of the GLIMS Regional Center for the Antarctic Peninsula and its network of international collaborators are based on the use of various types of Earth observation imagery, mainly optical and radar data. Although a complete glacier inventory is still lacking, we present the results of changes in glacier frontal positions and boundaries of glacier facies as well as links to dynamical adjustments for various locations in the Antarctic Peninsula’s ice masses. Evaluation of Advanced Spaceborne Thermal Emission and reflection Radiometer (ASTER) digital elevation models generated for the Antarctic Peninsula is also discussed. The Antarctic Peninsula (AP; Fig. 30.1) has undergone rapid climatic warming during the last 50 years (Vaughan et al. 2003). As a consequence, the glacial systems of this region have reacted with drastic changes, such as retreat, breakup, and disintegration of ice shelves (Skvarca 1993, Rott et al. 1996, 1998, Skvarca et al. 1999, Skvarca and De Angelis 2003, Rack and Rott 2004, Braun et al. 2009), acceleration and thinning of glaciers (De Angelis and Skvarca 2003, Rignot et al. 2004, Scambos et al. 2004, Pritchard and Vaughan 2007), variation in the limits between glacier facies (Rau and Braun 2002, Arigony-Neto et al. 2007, 2009), and retreat of glacier fronts (Skvarca et al. 1995, Simões et al. 1999, Rau et al. 2004, Cook et al. 2005). Glacial response times in the AP range widely, as do climatic and oceanographic components of the system, and so glacier dynamics differ considerably in the region. Climate change is often considered a major cause of glacier changes in the AP (Skvarca et al. 1999, Skvarca and De Angelis 2003, Vaughan et al. 2003). However, due to the lack of both data on the boundary conditions of glaciers and consistent systematic observations of glacier dynamics to feed more complex models of glacier mass balance, it is 718 Monitoring glacier changes on the Antarctic Peninsula Figure 30.1. Overview map of the Antarctic Peninsula showing the location of the study areas. Black boxes correspond to areas analyzed with satellite sensor data. Glaciers discussed in the text are labeled as follows: BS ¼ Boydell and Sjögren; DBE ¼ Dinsmoor, Bombardier, and Edgeworth; D ¼ Drygalski; HGE ¼ Hektoria, Green, and Evans; and JCMM ¼ Jorum, Crane, Mapple, and Melville. Regional context 719 difficult to predict accurately the contribution of AP glaciers to changes in sea level (Rignot et al. 2004, 2005, Pritchard and Vaughan 2007) and further responses to climatic change and variation in oceanographic parameters (Vaughan 2006, Arigony-Neto et al. 2007). Work done within the framework of the GLIMS Regional Center for the Antarctic Peninsula and its network of international collaborators aims not only to promote the use of optical imagery to monitor ice masses of this region, but also to investigate the possibility of adapting products, based on analyses of SAR data, to the GLIMS concept in a synergistic way. In this chapter, we briefly present some of the indicators of climatic and glaciological changes observed in the AP, and evaluate ASTERderived products’ ability to represent the topography of AP ice masses. We also present three case studies in which variations in dynamical parameters of a subset of AP glaciers are measured using methods related or complementary to GLIMS analyses. 30.2 REGIONAL CONTEXT 30.2.1 Geologic context The AP is vast, stretching southward from 60 S for more than 1,500 km down to 75 S. The region is widely glaciated, interrupted only by sparse rock outcrops. The AP’s early development was as an Andean-type oceanic/continental plate margin of Gondwanaland. Construction of the plate margin—started in the Paleozoic and continued through the Mesozoic—involved compressional folding, uplift, and metamorphism of marine sediments (including thick sedimentary sequences shed from Gondwanaland into the marine environment), anatexis (partial melting of the crust), igneous intrusions, and volcanism (mainly silicic). Hence, the AP’s basement rocks, widely exposed by uplift and erosion, are primarily high-grade metamorphic rocks, such as granite gneiss, and silicic igneous rocks (Harrison et al. 1979, Birkenmaier 1994, Millar et al. 2002). Starting in the Late Cretaceous, marine sedimentary deposition in a back-arc basin produced a 6,000 m thick sequence preserved on James Ross Island (Smellie et al. 2007). The sedimentary platform sequence was uplifted and partly eroded, and subsequently overprinted by a massive, mainly subglacial basaltic shield volcano and many subsidiary volcanic structures over the past 9.2 million years. Glacial erosion of the lava-capped sedimentary edifice has produced the peculiar shape of James Ross Island, as shown below (see Fig. 30.5 on p. 726). Primarily basaltic, subglacial volcanism also occurred elsewhere in the northern part of the AP region in Late Cenozoic times, thus producing many rock deposits bearing the imprint of lava– ice interactions, particularly on Alexander and Vega Islands as well as James Ross Island (Smellie et al. 1993, Hambrey et al. 2008). This late episode of volcanism is thought to have begun beneath an Antarctic Peninsula ice sheet and to have occurred more recently beneath small ice caps. This activity produced interspersed lavas, tuff cones, and glaciodeltaic, glaciofluvial, and diamictite sequences. Volcanic eruptive episodes on James Ross Island are probably not finished, but they occur only once every 10 5 years on average (Smellie et al. 2007), and so eruptions are improbable anytime soon. Active plate subduction, rifting, and volcanism still occur in the nearby Shetland Islands region (Lawyer 2009). In general, however, the AP is not considered volcanically very active. AP history indicates that most rocks now undergoing glacial erosion in the AP consist of a wide variety of igneous and high-grade metamorphic rocks. 30.2.2 Climatic context The Antarctic Peninsula has a polar to subpolar maritime glacial climate; as such, it experiences considerable summer rainfall and winter snow. It is dominated by a rugged, though not particularly high mountain range, attaining over 2,000 m in elevation in places but less than 1,000 m along most of its length. The spine of the AP is high enough to impose a strong orographic effect, with the east to southeast side being in the precipitation shadow of prevailing winds and precipitation sources that are based mainly in the Bellingshausen Sea (Fig. 30.1). The maritime glacial climate and its dominant wet-based temperate and polythermal glaciers and ice caps differ from the severe polar climate and cold-based glaciers and thick ice sheets dominating most of Antarctica. Unlike most of Antarctica, most of the AP has a distinct summer melting season, especially in its northern reaches. Glaciers in the AP mainly have low supraglacial debris loads because the ice cover is so extensive and rock outcrops are comparatively few; hence, erosion of glacial valleys must occur mostly by subglacial abrasion and not much at all by landsliding and 720 Monitoring glacier changes on the Antarctic Peninsula mass wasting, bearing little resemblance to the case in Patagonia and Alaska, for instance. A statistically significant warming trend was detected in the AP using different datasets, measured both locally in situ and regionally via remote sensing. Turner et al. (2005) gave the warming rate of the Antarctic Peninsula at Faraday/Vernadsky Station (65 14 0 S, 64 15 0 W) as 0.056 0.043 C yr1 over the year and 0.109 0.088 C yr1 during the winter for the period between 1951 and 2000. Moreover, radiosonde temperature observations complemented by NCEP/NCAR reanalysis data revealed a mean annual tropospheric (850–300 hPa) warming of 0.027 0.022 C yr1 above Faraday/Vernadsky between 1956 and 1999 (Marshall et al. 2002). Finally, a database of more than 500 mean annual temperatures derived from measurements of snow temperature at around 10 m depth and air temperature measured at meteorological stations and automatic weather stations allowed Morris and Vaughan (2003) to estimate the increase in temperature for the whole AP to be 0.035 0.010 C yr1 over the period 1904–2000. In addition to atmospheric warming, a statistically significant rise in the number of precipitation events during winter was reported from observations at Faraday/Vernadsky from 1956 to 1994 (Turner et al. 1997), resulting in the records of precipitation per season at the end of the time series increasing by 50%. This appears to be related to the more frequent arrival of cyclones from the Bellingshausen Sea (Turner et al. 1995), where this precipitation originates (Turner et al. 1998). Furthermore, data from ice cores (Peel 1992, Thompson et al. 1994, Raymond et al. 1996, Thomas et al. 2008) indicated an increase in accumulation on the plateaus of the AP in the last four decades. A rising trend in the duration of melt periods in the AP was detected using two different methods. Ridley (1993), Fahnestock et al. (2002), and Torinesi et al. (2003) examined the duration of melt seasons over 13 (1978–1991), 22 (1978–2000), and 20 (1980–1999) year periods, respectively, using satellite-based passive microwave data. All three studies found high variability in the duration of the melt season as well as a positive trend in melt season length, although Ridley (1993) and Fahnestock et al. (2002) analyzed the area of the AP ice shelves only and Torinesi et al. (2003) considered the whole AP. Vaughan (2006) used an approach based on positive degree-days (PDDs) to predict ablation conditions. By using temperature trends from Morris and Vaughan (2003), annual PDDs were calculated for the whole AP over the period 1950–2050. Results indicated a strong positive trend in annual PDDs, mainly concentrated in the northeastern sector of the AP. 30.2.3 Summary of known glacier dynamics According to analyses of recent Gravity Recovery and Climate Experiment (GRACE) data for the period 2002–2009, which allows estimation of glacier mass change, the northern AP has the continent’s second largest negative mass balance rate (Chen et al. 2009). However, such low-resolution data belie the geographic complexity and rapidity of some glacier dynamics in the region. The successive breakup and retreat of ice shelves occurring in the AP over the last two decades has received extensive attention from the general public and media. After the retreat of Wordie Ice Shelf in the late 1980s (Doake and Vaughan 1991, Vaughan and Doake 1996), pronounced retreat and breakups were also detected at the northern margins of George VI Ice Shelf and Wilkins Ice Shelf (Lucchitta and Rosanova 1998, Scambos et al. 2000), followed by a rapid sequence of breakup events on the northeastern side of the peninsula: Prince Gustav Ice Shelf and Larsen A Ice Shelf disappeared in 1995 (Skvarca 1993, Rott et al. 1996, 1998, 2002). Larsen B Ice Shelf started calving in 1995 and collapsed almost completely in 2002 (Skvarca et al. 1999, Rack and Rott 2004). Moreover, new breakup events and retreat were detected in 2008 and 2009 at Wilkins Ice Shelf, when almost 40% of the ice shelf connecting the two islands broke off (Braun et al. 2009, Humbert et al. 2010). Progressive thinning (Shepherd et al. 2003, Skvarca et al. 2004), the formation of melt ponds (Scambos et al. 2000, 2003), changes in structure (Glasser and Scambos 2008, Braun et al. 2009) and extended melt seasons (Fahnestock et al. 2002, Van den Broeke 2005) linked to the breakup of ice shelves are strong indications that some of these events occurred in response to changing climatic and oceanographic conditions, at least in the case of Prince Gustav Ice Shelf and Larsen Ice Shelf. In this context, Morris and Vaughan (2003) proposed the 9 C isotherm of mean annual temperature as the new limit of ice shelf distribution in 2002, updating the 5 C limit previously proposed by Reynolds (1981). Hence, further warming might Methodology shift the viability limit of ice shelves in the AP farther south. An overall trend of glacier front recession was detected in the AP (Rau et al. 2004, Cook et al. 2005), on James Ross Island (Skvarca et al. 1995, Skvarca and De Angelis 2003) and on the South Shetland Islands (SSI; Park et al. 1998, Calvet et al. 1999, Simões et al. 1999, Braun and Goßmann 2002). As suggested by Cook et al. (2005), floating glaciers and most ice shelves may be reacting to progressive atmospheric warming detected in the AP (Vaughan et al. 2003, Morris and Vaughan 2003, Scambos et al. 2003). However, as they are influenced by other external factors (e.g., oceanic temperature and circulation), it is difficult to isolate a clear climate cause (Rau et al. 2004). Tidewater glaciers with their fully grounded marine termini are influenced by a complex set of forcing mechanisms composed of atmospheric temperature and oceanographic parameters as well as subglacial topography (Van der Veen 2002, Benn et al. 2007), and hence their retreat rates cannot be linearly linked to short-time climate change on ice masses (Pfeffer 2003). Thus, for all types of glaciers in the AP, climate change, oceanographic conditions, and glacier/ice shelf dynamics are complexly coupled, with climate change pretty obviously a key driving factor. However, the system has strong forcings other than climate change. Hence, prediction of glacier and ice shelf dynamics in the AP is hazardous at best, and clear attribution of recent dynamics to climate change alone is not warranted. 30.3 METHODOLOGY 30.3.1 Evaluation of ASTER-derived DEMs for the Antarctic Peninsula High-quality digital elevation models are only available for selected regions. However, measurement of morphometric glacier parameters such as length, width, area, glacier front position, basin boundaries, among others, where 3D coordinates are needed, requires a consistent spatial frame of reference. Some methods that use spaceborne optical sensor data to retrieve such parameters have been tested mainly for alpine and temperate glacier regions (Paul 2001, Paul et al. 2002). Nevertheless, in the AP some factors related to the specific characteristics of this polar environment (e.g., frequent high cloudiness, high reflection of snow-covered 721 surfaces, morphology of the terrain, etc.) render application of these digital image–processing methods difficult. Consequently, investigation, testing, and adaptation of these traditional algorithms for application in the AP are required. With this focus, we have investigated the use of near-infrared stereo pairs acquired by ASTER for topographic data generation along the AP. The ASTER visible/near-infrared band subsystem (VNIR) offers 15 m spatial resolution (images were provided through the GLIMS project). An area of roughly 600 km 2 , located on the western side of the AP in the region of Marguerite Bay, was chosen as the test site (Fig. 30.1). The area is almost completely covered by ice and snow, having a geographical setting inclusive of many of the ice forms that occur in Antarctica. Topography rises rapidly from the heads of glaciers to the central plateau. The best independently available terrain representation for the area is provided by the Darmstadt University of Technology Model (TUD DTM; Fig. 30.2) and the complementary Base General San Martin aerial photo map (TUD Karte; Fig. 30.2). This dataset was created from black and white aerial photography taken by the Bundesamt für Kartographie und Geodäsie (BKG) in February 1989 (Wrobel et al. 2000). Generated by means of semiautomatic processing from aerial photo coverage, the TUD DTM has a 30 m grid cell size and the following accuracies: 3–10 m, mountain ranges, rock areas, snow-free zones; 10–20 m, crevasses, ice faults, structured snow-covered terrain; 50 m or more, monotonous snow-covered areas without structures, clearly visible in the central part of the DEM on McClary Glacier (Fig. 30.2). To derive a DEM for our test site, eight ASTER L1A scenes with acceptable cloud coverage were used from a total of 32 scenes acquired between November 2000 and September 2005. The process chain to derive a multitemporal median DEM (MT DEM) was computed following the flow diagram shown in Fig. 30.3. A breakdown of this process is given in Sections 30.3.1.1–30.3.1.3. 30.3.1.1 DEM generation DEMs were derived for all available scenes using a fixed combination of parameters with 15 m output pixel size, a 3 3-pixel correlation matrix size, no ‘‘water detection’’ or ‘‘extended correlation’’. Terrain geometric correction for each ASTER 722 Monitoring glacier changes on the Antarctic Peninsula Figure 30.2. (Top) Digital elevation model (IfPK TUD 1999) of the test site located in the surroundings of the Base General San Martin, Marguerite Bay. Lambert Conformal Conic (WGS 72) cartographic projection. (Bottom) Base General San Martin aerial photo map (TUD Karte). Sources: aerial photography (1988/1989) by Bundesamt für Kartographie und Geodäsie (BKG, formerly IfAG); stereo modeling and DEM production by the Technical University of Darmstadt (TUD); topographic features by the Institute of Physical Geography, University of Freiburg (IPG) (see Wrobel et al. 2000). Figure can also be viewed in higher resolution as Online Supplement 30.1. Methodology 723 Figure 30.3. Flow diagram for the multitemporal ASTER scenes processing approach, showing the production of an averaged DEM by pixel-based median filtering within a layer stack. L1B scene was performed using the DEM derived to produce the corresponding orthorectified image. 30.3.1.2 DEM registration A registration process was carried out in two steps to register each ASTER-derived DEM with the reference TUD model. Because of difficulties and inaccuracies in image-to-image registrations based on just two DEMs, registration of the orthorectified L1B image with the TUD Karte image was first performed. This step provided the GCPs and coefficients for first-degree polynomial correction applied in each registration. Finally, image-to-map registration using the GCPs and coefficients calculated in the previous step was carried out for each DEM. 30.3.1.3 Stacking and filtering Co-registered DEMs were added to a layer stack. Within this step we masked seawater areas and resampled the data from 15 to 30 m using the 724 Monitoring glacier changes on the Antarctic Peninsula nearest neighbor method. Finally, the median value of stacked pixels was calculated to filter out extreme pixel values in the derivation of the multitemporal median DEM (MT MED model). In order to describe errors that can occur in ASTER-derived models we compared the altitudes of each model with the TUD reference model pixel by pixel. We also considered the Radarsat Antarctic Mapping Project (RAMP) DEM (Liu et al. 2001), which provides an independent comparison and a measure of the magnitude and spatial distribution of the DEM’s error in this area. RAMP models and ASTER-derived models were each subtracted from the TUD reference model. Map algebra operations (i.e., subtraction and masking) were applied to generate three altitude deviation maps. The resulting maps (Fig. 30.4) are shown in a blue–red bipolar color schema used to represent the magnitude and sign of altitude deviation values. In addition, Table 30.1 shows the distribution of altitudinal deviations between different elevation models. In Fig. 30.4 blue represents an elevation of ASTER or RAMP models higher than the corresponding TUD elevation; red represents an elevation of ASTER or RAMP models lower than the corresponding TUD elevation. White represents altitude deviation less than 10 m. Comparing the altitude deviations of ASTER and RAMP models from the TUD DEM, we can observe on the MT MED the preponderance of altitude differences smaller than 20 m (Fig. 30.4; Table 30.1). In this range, the distribution of errors is more concentrated and they are smaller than shown on the MED MED map. Accordingly, the MT MED model represents the best fit with the reference TUD model. This indicates that ASTER DEMs can achieve higher accuracy using the multitemporal approach than using the alternative single-scene schema. The digital elevation model derived within RAMP did not provide the accuracy necessary for deriving morphometric glacier parameters as required for the GLIMS project. This was due to data source compilation and the scale of the RAMP DEM (i.e., 200 m spatial resolution). Furthermore, the accuracy parameters of the RAMP model found at our test site were less acceptable than those reported in the literature (Liu et al. 1999, Bamber and Gomez-Dans 2005). The accuracy parameters of our ASTER-derived digital elevation models based on the doublemedian filtering scheme (MED MED) and on the Figure 30.4. Altitude deviations between the TUD reference model versus ASTER-derived and RAMP models. (Left) MED MED model, digital elevation model using only one ASTER scene (SC:AST_ L1A.003:2030971130, September 19, 2005, 13:33:26). (Middle) MT MED model. (Right) RAMP DEM. Blue represents an elevation of ASTER or RAMP models higher than the corresponding TUD elevation; red represents an elevation of ASTER or RAMP models lower than the corresponding TUD elevation. White represents an altitude deviation less than 10 m. Location of test site indicated in Fig. 30.2’s caption. Case studies and special topics 725 Table 30.1. Distribution of altitude deviations between different elevation models (TUD– RAMP, TUD—MED MED and TUD–MT MED): absolute and relative frequencies of the classes used in Fig. 30.4. Rows in gray represent high-accuracy classes. Deviation ranges TUD–RAMP TUD–MT MED (m) (pixels) (%) (pixels) (%) (pixels) (%) 800 to 100 178,896 28.7 58,645 9.4 7,016 1.1 100 to 50 61,474 9.97 8,595 12.6 51,427 8.3 50 to 20 48,063 7.7 179,356 28.8 173,244 27.8 20 to 10 16,116 2.6 87,901 14.1 100,601 16.2 10 to 10 40,177 6.5 123,960 19.9 161,628 26.0 10 to 20 25,242 4.1 28,907 4.6 36,700 5.9 20 to 50 68,084 10.9 35,365 5.7 48,472 7.8 50 to 100 77,576 12.5 18,513 3.0 26,163 4.2 >100 106,715 17.1 10,862 1.7 16,934 2.7 multitemporal median scheme (MT MED) were higher than reported in the literature for the same type of surface (i.e., between 31 and 70 m root mean square with maximum errors of 200 and þ500 m; Kääb, 2005). Double-median filters, made up of a spatial median and a multiprocess median, were capable of suppressing artifacts in a single scene. For each point the multitemporal median (MT MED) used altitude values unaffected by artifacts. 30.4 TUD–MED MED CASE STUDIES AND SPECIAL TOPICS 30.4.1 Monitoring glacier change in the northeastern Antarctic Peninsula GLIMS objectives include measurements of changes in glacier extent with the aim of establishing a digital baseline for future comparisons. Our monitoring of glacier change using ASTER images covers the northeastern side of the AP extending between 63.8 S and 65.5 S (Fig. 30.1), and comprises different types of glaciers on Vega Island and James Ross Island, Boydell Glacier and Sjögren Glacier calving into Prince Gustav Channel, Dinsmoor-Bombardier-Edgeworth and Drygalski outlet glaciers calving into Larsen A embayment, and Hektoria-Green-Evans, Jorum, Crane, Mapple and Mellville Glaciers discharging presently into Larsen B embayment (Fig. 30.1). The first usable ASTER images of the northeastern AP were acquired in early 2001 and used since then to document the drastic glacier retreat and ice loss in this region until 2008–2009. Of particular importance is the monitoring of glacier retreat behind the grounding line (GL) because of its contribution to global sea level rise. The position of the GL was derived by means of different InSAR interferograms (Rott et al. 2002, Rack and Rott 2004). ASTER images were co-registered with the Landsat ETMþ mosaic of 21-Feb-2000 covering the northeastern Antarctic Peninsula. This mosaic was georeferenced to characteristic ground features using GPS. Co-registration error was of the order of 0.5 pixels (i.e., 7.5 m). All areas and glacier retreat measurements were performed manually by means of commercial GIS software. 30.4.2 Glaciers of Vega Island and James Ross Island 30.4.2.1 Vega Island (VI, Fig. 30.5) Field measurements carried out on two glaciers with termini on land—Glaciar Bahı́a del Diablo (GBD) and Glaciar Cabo Lamb (GCL); Fig. 726 Monitoring glacier changes on the Antarctic Peninsula Figure 30.5. ASTER image mosaic (bands 3, 2, 1) assembled with three L1B scenes acquired 03-Mar-2009, showing Vega Island and James Ross Island. Blue indicates glacier retreat from 1988 to 2001 derived from Landsat TM and ASTER images. Red and green indicate, respectively, retreats and advances from 2001 to 2009 derived only from ASTER imagery. Pink shows the area of ice shelf disintegration in Röhss Bay between 2001 and 2009. Figure can also be viewed as Online Supplement 30.2. 30.5—reveal major thinning rates of about 1.0 m yr1 since the early 1980s (Skvarca and De Angelis 2003). Furthermore, detailed annual mass balance measurements of GBD carried out as a contribution to the World Glacier Monitoring Service (WGMS) show negative values from 1999 to 2008, with an average of 0.31 m water equivalent. An early ASTER image acquired on 08-Jan-2001 with the aid of a contour map derived from kinematic GPS was used to help define the drainage area of GBD. 30.4.2.2 James Ross Island (JRI, Fig. 30.5) The baseline for glacier extent on JRI had already been established in 1975 from Kosmos KATE-200 space photos (Skvarca et al. 1995). In total, 39 outlet glaciers draining JRI were analyzed, of which 33 were tidewater calving, one was freshwater calving into a lake, and 5 were terminating on land. As shown by Kosmos, Landsat, and ASTER images the retreat rate of JRI glaciers has increased considerably from 1.8 km 2 yr1 during the period Case studies and special topics 1975–1988 to 2.9 km 2 yr1 in 1988–2001. Glacier/ ice shelf frontal positions and their change for the latter period were also reported by Rau et al. (2004) and Kargel et al. (2005), though they considered fewer glaciers. Here we extend the study from 2001 to 2009, investigating the same glaciers as in the earlier period. Further analysis is based on ASTER images acquired on 08-Jan-2001 and 03Mar-2009 revealing a similar decrease rate of 2.6 km 2 yr1 and an ice loss of 21 km 2 . During the overall period 1975–2009 the total glacier area of JRI decreased by 81.3 km 2 . An additional 101 km 2 were lost from 2001 to 2009 due to disintegration of a small ice shelf in Röhss Bay (Fig. 30.5). Overall, our extended record shows sustained and accelerating retreat as well as drastic ice shelf breakup similar to that which has affected the larger ice shelves of the peninsula’s mainland. 30.4.3 Former tributaries of Prince Gustav Channel (PGC) Ice Shelf 30.4.3.1 Boydell Glacier and Sjögren Glacier (B-S) Both glaciers fed the former ice shelf within PGC, which disintegrated in 1994/1995. The ASTER image of 26-Sep-2001 revealed characteristic features such as surge waves, looped moraine, and marginal crevasses, indicating an active surging phase of B-S glaciers (De Angelis and Skvarca 2003). Evidence for strong glacier acceleration and significant surface lowering/thinning after the ice shelf collapse were the remnant ice terraces detected at glacier margins. Further retreat from late 2001 to early 2009 (Fig. 30.6) was derived using a co-registered series of ASTER images, which allowed us to compute major retreats of 7.8 km (B) and 10.8 km (S), with significant total area loss of 69.5 km 2 behind the grounding line derived by interferometry. 30.4.4 Former tributaries of Larsen A Ice Shelf 30.4.4.1 Dinsmoor-Bombardier-Edgeworth (D-B-E) glaciers This glacier system fed the former Larsen A Ice Shelf before its collapse in early 1995. Surge waves and looped moraines, characteristic features of an active surging phase, had already been detected on Bombardier Glacier and Edgeworth Glacier (Fig. 30.7) from the ASTER image of 26-Sep-2001 (De 727 Angelis and Skvarca 2003). However, this early surge only affected these glaciers, which have advanced 1.6 km with net areal gain of 6.5 km 2 . A recent ASTER image acquired on 09-Dec-2008 together with ice front positions mapped using GPS during aerial surveys carried out along the northeastern AP in early 2007 and 2008 reveal another surging phase of the D-B-E glacier system, which has advanced 1.8 km. This indicates that strong dynamic perturbations are still affecting the former tributaries 14 years after the removal of the ice shelf. A recent surging event has also affected Dinsmoor Glacier, which advanced with a net areal increase of 5.1 km 2 from 11-Mar-2007 to 09-Dec2008 (Fig. 30.7). In this period, the B-E glaciers surged by 6.5 km 2 (i.e., the same net areal gain as during the 2000–2001 surge). By early December 2008, the three glaciers had lost an area of 39.5 km 2 behind the GL. 30.4.4.2 Drygalski Glacier (D on Fig. 30.1) The first available ASTER image of Drygalski Glacier after the disintegration of Larsen A was acquired on 22-Nov-2001. The most recent ASTER image allowed computation of an area loss of 34.5 km 2 behind its grounding line up to 09-Dec-2008. Three smaller glaciers also draining into the Larsen A embayment had lost an additional 36.5 km 2 behind their grounding lines by 09-Dec-2008. Both areas represent a contribution to sea level rise. 30.4.5 Former tributaries of Larsen B Ice Shelf 30.4.5.1 Hektoria-Green-Evans (H-G-E) The H-G-E glacier system has been subject to continuous retreat since early 2002 (as sequential ASTER images reveal); about 115.1 km 2 of its area inland of the grounding line had been lost by 25Feb-2008 (Fig. 30.8). 30.4.5.2 Jorum-Crane-Mapple-Melville (J-C-M-M) Farther south, five ASTER images provide information on the glacier extent of Crane, Mapple, and Melville, the three southernmost glaciers that fed the former Larsen B Ice Shelf and calve at present into its embayment (Fig. 30.9). Crane Glacier with 60 km in length is the longest in the AP and retreated 10.8 km between late 2002 and early 2008 with an area loss of 57.5 km 2 , 35.0 km 2 of 728 Monitoring glacier changes on the Antarctic Peninsula Figure 30.6. Section of ASTER image of 28-Oct-2006 (bands 3, 2, 1) showing the retreat of B-S glaciers behind the grounding line (GL) since 26-Sep-2001 (PGC ¼ Prince Gustav Channel). Figure can also be viewed in higher resolution as Online Supplement 30.3. which was behind the GL. Farther south, Mapple is the only glacier whose ice front is still flowing outward from the grounding line, hence is not yet contributing to sea level rise, while Melville Glacier had lost by early 2008 an area of about 1.9 km 2 behind the GL. Jorum Glacier and two small neighboring glaciers located north of Crane have also retreated behind the GL (losing an area of 26.5 km 2 ). In total, all glaciers calving into the Larsen B embayment had lost by early 2008 about 178.5 km 2 of their area behind their grounding lines, representing a contribution to global sea level rise. 30.4.6 Monitoring changes and breakup events on the Wilkins Ice Shelf 30.4.6.1 Areal changes and breakups between 1986 and 2009 Wilkins Ice Shelf (WIS) is located in the southwestern part of the AP. It is currently the southern- most ice shelf on the peninsula to show breakup events according to the definition given by Braun et al. (2009). We define breakup as a sudden fast release of fragments of variable size, happening on a timescale of hours to days; in contrast to disintegration where the complete ice shelf is lost. Calving is seen as an ordinary process of mass loss of an ice shelf on a timescale of months or years; while retreat is a reduction in size on a timescale of months or years. WIS is confined by several islands—namely, Alexander, Rothschild, Charcot, and Latady (Fig. 30.10). Additionally, numerous ice rises intersect the ice shelf. The primarily remote sensing–based analysis of Vaughan et al. (1993) suggested that the mass balance of WIS was dominated by surface accumulation and basal melting, and that as a consequence it might be particularly prone to variations in atmospheric and oceanic boundary conditions. Some inflow occurs from Lewis Snowfield and into Schubert Inlet and Haydn Inlet. However, Case studies and special topics 729 Figure 30.7. Section of the ASTER image acquired 02-Dec-2008 (bands 3, 2, 1) showing recent surge and D-B-E ice front fluctuations since 2001 and retreat inland behind the GL. Front positions on 11-Feb-2006, 11-Mar-2007, and 03-Mar-2008 are from GPS surveys, while the 26-Sep-2001 and 02-Oct-2003 front positions are from ASTER. Figure can also be viewed in higher resolution as Online Supplement 30.4. Figure 30.8. Retreat of Hektoria-Green-Evans (H-G-E) glaciers shown on a section of the ASTER image acquired 27-Sep-2004 (bands 3, 2, 1). Figure can also be viewed in higher resolution as Online Supplement 30.5. 730 Monitoring glacier changes on the Antarctic Peninsula Figure 30.9. Section of ASTER image acquired 25-Feb-2008 (bands 3, 2, 1). Numbers in circles indicate ice front positions on (1) 07-Nov-2002; (2) 02-Feb-2003; (3) 13-Jan-2004; (4) 27-Sep-2004 and (5) 25-Nov-2006. Figure can also be viewed in higher resolution as Online Supplement 30.6. the flow from these inlets into the main ice shelf is considerably blocked by ice rises. While the situation between 1986 and 1990 indicated a stable ice shelf (observed in Landsat imagery), by 1993 the northern ice front was reported to have retreated several times by Lucchita and Rosanova (1998). A further massive area loss occurred during February 1998, when approximately 1,100 km 2 were lost (Scambos et al. 2000). Up to February 2008 the extent of the ice shelf remained almost constant and the area amounted to about 13,000 km 2 . However, there was a considerable increase in the number of fractures arising from tensile stresses in the vicinity of ice rises. A review of the state of WIS by Braun et al. (2009) revealed that several distinct breakup events in contrast to frequent calving (including the abovementioned) occurred prior to 2008. The authors concluded that increasing basal melt rates due to variations in the ocean regime and changes in the properties of materials comprising WIS due to atmospheric and ocean changes could be two possible factors responsible for reducing the integrity of the ice shelf. In the course of 2008, WIS underwent considerable changes, including three distinct breakup events (Humbert and Braun 2008; Braun and Humbert 2009; Scambos et al. 2009). On February 28, 2008 the first breakup event started along the northwestern ice front between Charcot Island and Latady Island. The signature of Envisat C-band SAR (synthetic aperture radar) data revealed a moist or wet surface. In contrast, during the second breakup event on May 30/31, 2008 the bright SAR backscatter indicated frozen conditions. The hypothesis of meltwater from melt pools draining into crevasses was hence ruled out as a potential explanation. A third breakup event followed in July Case studies and special topics during austral winter, leaving a fragile connection to Charcot Island only 900 m wide at its narrowest point. The remaining ice shelf bridge finally collapsed in the first days in April 2009 (Humbert et al. 2010), followed by destabilization of the northern ice front. An overview of ice fronts from 1990 to the various stages is shown in Fig. 30.10. Scambos et al. (2000) and Cook and Vaughan (2010) based their analyses on historic maps and declassified satellite imagery, which showed that the ice front of WIS did not change between 1947 and 1986 in any considerable way. Table 30.2 summarizes the respective area losses. The numbers differ slightly from the data given by Cook and Vaughan (2010) in their overview of Antarctic Peninsula ice shelf areal changes as a result of differences in image dates and potential differences in interpretation of the heavily fractured ice shelf front. WIS has lost a total of about 5,624 km 2 of its area since 1986, which amounts to about 43% of its size before the onset of breakups. 30.4.6.2 A three-step process chainfor breakups In the past, various explanations for ice shelf breakup and retreat have been proposed. They cover individual factors or distinct mechanisms leading to failure. We propose a general three-stage process chain consisting of a cause, a trigger, and a consequence (Fig. 30.11). It can be applied independently of the specific mechanisms of each step and structures the breakup process along a timeline. The primary process leads to fracture formation, the secondary step triggers propagation of the crack through the entire ice shelf, and the tertiary process involves the release of icebergs. Identifying the mechanisms involved in the first two steps is particularly in need of improvement in order to understand what lies behind breakup processes and what their potential consequences are. A known primary process is the formation of crevasses by flowinduced stresses, like shear margins or crevasses in the vicinity of ice rises (Doake and Vaughan 1991, Glasser and Scambos 2008). For WIS, Braun and Humbert (2009) proposed that fracturing was caused by bending stresses resulting from buoyancy forces induced by an ice thickness gradient. This gradient arose presumably from inhomogeneous basalt melt rates, where the seaward margin of the ice plate experienced more basal melt than areas farther inward. Scambos et al. (2009), on the other hand, proposed a plate bending stress model 731 induced by buoyancy forces due to tides and the stress boundary condition at the seaward margin, similar to stress fields along calving fronts. Perhaps the most prominent secondary process is the drainage of surface melt ponds into crevasses, which increases stress at the crack tip. Subsequently, cracks propagate vertically through the entire ice shelf (Weertman 1973, Van der Veen 1998, Scambos et al. 2000, 2003). This secondary process is widely acknowledged to have taken place during the breakup of Larsen B. Scambos et al. (2009) propose a model that replaces surface melt water by brine for the February 2008 WIS breakup. However, as the May and June/July 2008 breakups occurred during austral winter, when the availability of liquid was unlikely, further secondary processes likely exist. Tertiary processes—such as the release of ice fragments—may include icebergs that capsize, as shown by MacAyeal et al. (2003) for the breakup of Larsen B. The fast rotation of icebergs as they capsize leads to a rapid massive area increase. For all three breakups of WIS in 2008, the failure of the ice bridge, and the subsequent mass loss at the northern ice front, this process took place. This tertiary process releases a large amount of energy (MacAyeal et al. 2009), as the capsizing of icebergs decreases potential energy. Guttenberg et al. (2011) presented computations on this conceptual model that was not tied to a specific ice shelf or observation data. They also investigated how the aspect ratio of icebergs and its variance influence breakup conditions. It is important to link this tertiary process to fracture patterns observed before breakup. The failure of the ice bridge on WIS in 2009 liberated energy of the order of 10 14 J (as shown by Humbert et al. 2010). 30.4.7 Variation of radar glacier zone boundaries in the northeastern Antarctic Peninsula One of the biggest problems in building a time series of GLIMS analyses for the AP is the lack of a consistent spatiotemporal series of optical datasets. An alternative is to use the database of SAR images available for this region. This case study involves using a time series of ERS-1/2 SAR images to ascertain the boundaries between radar glacier zones such as the bare ice radar zone (BIRZ), wet snow radar zone (WSRZ), frozen percolation radar zone (FPRZ), and dry snow radar zone (DSRZ), which can be used as proxies for GLIMS-related param- 732 Monitoring glacier changes on the Antarctic Peninsula Figure 30.10. (Upper) Overview map of Wilkins Ice Shelf based on a Landsat mosaic from 1990 (& USGS 1990). The features labeled are B ¼ Burgess Ice Rise, P ¼ Petrie Ice Rises, V ¼ Vere Ice Rise. The purple line indicates the present extent, the black line the grounding line. (Lower) The situation as depicted by a TerraSAR-X ScanSAR image on 02-Nov-2009 (& DLR 2009) superimposed on two Envisat ASAR wideswath images from 26-Jun-2009 and 30-Jun-2009 (& ESA 2009). Ice front positions on specific dates are given in color, the black line shows the grounding line. Figure can also be viewed in higher resolution as Online Supplement 30.7. Case studies and special topics 733 Table 30.2. Compilation of the retreat area of Wilkins Ice Shelf since 1986. Northern ice front Northwestern ice front Southern ice front Period/year Retreat area (km 2 ) Period/year Retreat area (km 2 ) Period/year Retreat area (km 2 ) 1986–1990 97 1990–1993 57 1990–2004 196 1990–1991 655 1993–1998 0 1991–1992 0 1998–1999 20 1992–1993 544 1999–2000 87 1993–1998 0 2000–2001 0 1998–1999 1,100 2001–2003 52 1999–2008 0 2003–2004 51 2004–2009 74 2008 1,220 2004–2007 0 2008 585 Sum 948 Sum 270 2009 790 Sum 4,406 eters such as snowline position, area of the ablation zone, etc. The concept of radar glacier zones used here corresponds to the classification scheme proposed by Rau et al. (2000) and further discussed by Braun et al. (2000) and Arigony-Neto et al. (2007, 2009). The satellite data used for analysis consisted of eight images acquired on the northeastern part of the AP (frame 4,923, tracks 109 and 381) from 1993 to 2000 by ERS-1/2 SAR (Fig. 30.12) C-band VVpolarization instruments. Normalized backscattering coefficients (0 ) were calculated using the Basic Envisat and ERS SAR Toolbox (BEST) from the European Space Agency (ESA). BEST uses the SAR calibration algorithm developed by Laur et al. (2004), who estimated that resulting values of 0 have an accuracy of 0.4 dB. The excellent stability of SAR sensors enables direct comparison of calibrated data (Meadows et al. 1998). To reduce the speckle effect, a 5 5 median filter was applied. Finally, speckle-filtered images were orthorectified using the DEM from RAMP (Liu et al., 2001). Image analyses were carried out automatically by means of a knowledge-based image analysis algorithm modified from Arigony-Neto et al. (2007). These authors developed an approach based on classifying areas located in a 600 m buffer along glacier centerlines. In this study, we adapted this method so that it considered whole glacier basins. Rules used for pixel classification were mainly based on backscattering thresholds determined by Rau et al. (2001) and altitude thresholds discussed in Arigony-Neto et al. (2009) (Table 30.3). Elevation information was derived from the RAMP DEM. Rocks and ocean areas were masked by rock outcrops and the coastline according to the Antarctic Digital Database (ADD; SCAR 2010). Misclassified pixels usually corresponded to steep slopes where AP plateaus break down to become glaciers or crevasse fields inside major classes such as the wet snow radar zone. These pixels were eliminated using a focal majority 5 5 filter. Fig. 30.12 shows the resulting distribution of radar glacier zones during the time period of image acquisitions. Analyses using images acquired on track 381 were restricted to the area common to track 109. In general, the boundaries of radar glacier zones presented enormous variation in the time period of study. This can be explained by the fact that the development of superficial zones or 734 Monitoring glacier changes on the Antarctic Peninsula Figure 30.11. Schematic of the three-step process during ice shelf breakups using the ice bridge on WIS as an example. While the upper panel illustrates a vertical view of the ice bridge with initial rifts formed during July 2007, the middle and lower panels represent cross-sections through the ice bridge along the thick black line of the upper panel. In the middle part the dotted lines denote perforation of the complete ice plate during this process, while the lower panel illustrates the area gain by sliver icebergs capsizing. facies on glaciers is greatly influenced by local and regional climatic and meteorological settings (Braun et al. 2000, Rau et al. 2000, Arigony et al. 2007, 2009). Indeed, the boundaries and extensions of radar glacier zones do not correspond to images acquired in the same period of the year, as in 13Feb-1993 and 11-Feb-1997 (Fig. 30.12B and 30.12F). For example, in the image acquired on 13-Feb-1993, major extensions of the wet snow radar zone (WSRZ) were observed in the coastal regions of Trinity Peninsula and James Ross Island, while the image from 11-Feb-1997 shows the WSRZ restricted to the northwestern tip of Trinity Peninsula. From analysis of the development of radar glacier zones during austral summer 1996/ 1997, it is possible to observe evolution of the BIRZ from the previous year (Fig. 30.12C) in the FPRZ after the first melt–freeze spring events (Fig. 30.12D). Subsequently, melt occurs in the snowpack covering most low-altitude areas along the east coast of the AP and parts of James Ross Island and Vega Island, and at the end of the summer (Fig. 30.12H) it is possible to record the maximum extension of the BIRZ for that balance year. Such variations indicate that great expanses of saturated snowpack melt during the summer. This event is probably related to the high frequency of days with positive temperatures recorded for the period between 29-Oct-1996 and 18-Mar-1997 at meteorological stations located in the region (72, 30, and 74 days, respectively, for Esperanza, Marambio, and O’Higgins Stations). Furthermore, long periods with positive temperatures during summer 1996/ 1977 are confirmed by the relatively high mean summer temperatures recorded for Esperanza (0.9 C), Marambio (1.46 C), and O’Higgins (0.5 C). Skvarca and De Angelis (2003) also confirm the relationship between summer mean air temperatures and mass balance for this region. The small area of the BIRZ detected on 03-Oct2000 is arguably an underestimate of the total extension of this radar glacier zone at the end of the balance year 1999/2000, because records of mean temperatures for austral summer 1999/2000 appeared to be higher at the meteorological stations mentioned above. Case studies and special topics 735 Figure 30.12. Area corresponding to footprints of ERS-1/2 SAR imagery acquired on frame 4,923, track 109 (area 1 in A) and track 381 (area 2 in A). The coastline is represented by the black continuous line and rocks are represented by light-gray polygons (B-I ¼ thematic maps resulting from image classification; BIRZ ¼ bare ice radar zone; WSRZ ¼ wet snow radar zone; and FPRZ ¼ frozen percolation radar zone). Figure can also be viewed in higher resolution as Online Supplement 30.8. 736 Monitoring glacier changes on the Antarctic Peninsula Table 30.3. Thresholds for backscattering coefficients ( 0 ) and altitude used for the classification of radar glacier zones on the Antarctic Peninsula. Radar glacier zones Dry snow radar zone Frozen percolation radar zone Wet snow radar zone Bare ice radar zone 30.5 REGIONAL SYNTHESIS The stereoscopic capability of the ASTER sensor offers the opportunity to produce medium-scale spatial resolution digital elevation models of the AP compatible with the requirements of GLIMS. Application of spaceborne optical imagery from the AP, in particular, is often hindered by frequent cloud cover. The incomparably large number of (almost) cloud-free ASTER scenes for Marguerite Bay can presumably be attributed to an atmospheric circulation pattern where depression centers pass the northern part of the AP from west to east and produce a lee condition westward of the central plateau in this area. All these aspects supported the view that the area was the best available test site providing a suitable location against which DEMs produced from ASTER data using our single and multitemporal scenes approach can be compared. What is more, ASTER images provide a digital baseline for detection of future change in glacier extent in one of the most rapidly changing regions on Earth. As a result of analyzing these images we were able to compute as of 2008–2009 the retreat area behind the grounding lines of glaciers calving into Prince Gustav Channel, the Larsen A embayment, and the Larsen B embayment at about 358.5 km 2 , all of which contribute to global sea level rise. ASTER imagery acquired at the time of and before the February 2008 breakup of Wilkins Ice Shelf contributed considerably to documentation and understanding of the events. WIS is likely to experience more mass loss, although around 8,000 km 2 are currently (2013) in a stable condition. The first signs of the stress field adjusting to the new load situation after the failure of the ice bridge were already visible while this chapter was being written, 0 (dB) Altitude H (m) 14 > 0 > 20 H > 1,200 0 > 0 > 8 14 > 0 > 25 6 > 0 > 13 — H < 1,200 H < 500 suggesting that a future ice front will likely meet the worst case predicted by Braun et al. (2009). In contrast to breakups in the 1990s, the field of icebergs has dispersed considerably, making formation of an extensive ice melange area unlikely. Thus, albedo and ocean will presumably respond to the 2008/ 2009 series of retreats faster and stronger than they did to breakups in the 1990s. The dynamics of radar glacier zones in the northern AP are related to high interannual and seasonal climate variability in this region. The variability of surface air temperature and high frequency of days with positive temperature recorded at meteorological stations in the northern tip of the AP caused significant changes in the position and extension of radar glacier zones during the period of study. Therefore, the position and altitude of the boundaries of glacier zones can be used as proxies for variations in temperature for regions of the AP where no meteorological data are available. 30.6 SUMMARY AND CONCLUSIONS DEM evaluation suggests that stereo along-track data from Terra’s ASTER instrument can be used to generate reasonably accurate models for the AP, improving the spatial resolution of existing models. A successful generation of digital elevation models for specific sectors of the AP region will contribute to filling current gaps in topographic data. Based on these DEMs it should also be possible to perform geometric correction of satellite data and use them for subsequent semiautomatic derivation of ice drainage catchments and additional parameters required for GLIMS analysis. References 737 The glaciers calving into Prince Gustav Channel, the Larsen A embayment, and the Larsen B embayment showed a general pattern of retreat behind their grounding lines between 2001 and 2008– 2009, immediately after a period in which some glaciers actively surged in the early 2000s. A few of these glaciers started to surge again between 2007 and 2008, indicating that strong dynamic perturbations are still affecting the former tributary glaciers many years after the removal of ice shelves. Future studies should take advantage of available sequential ASTER images to derive ice velocities, another GLIMS objective, so that the dynamics of these highly active calving glaciers, affected as they are by the removal of ice shelves, can be better understood. Further analysis of glacier change in the northeastern AP using satellite data is necessary because of its potential impact on global sea level rise. The breakup events of Wilkins Ice Shelf in 2008 and 2009 are the most recent signs of its destabilization, which began in the 1990s. Development of failure zones in the vicinity of ice rises during the 15 years prior to the events and bending stresses induced by buoyancy forces made this ice shelf vulnerable to extensive mass loss. Suggested reasons for this development are increased basal melt as well as thermal and precipitation-induced changes in the material properties of ice. The recorded patterns of variations in the boundaries of radar glacier zones in low-altitude areas within the time period of the study (1993–2000), associated with high-altitude variations in the DSRZ detected by Arigony-Neto et al. (2009), show that, in contrast to the Antarctic Ice Sheet, variations in climatological and glaciological conditions on a relatively short timescale are typical for this region. These results validate the suitability of SAR data to derive superficial information about glaciers to be used as GLIMS parameters in areas where optical imagery is not available, or for providing complementary information for temporal analyses of glacier change. The case studies discussed in this chapter demonstrated some of the satellite-based approaches used nowadays to monitor the ice masses of one of the most dynamic ice-covered areas of the planet. The multitude of glacier types in the AP and the different scales of analyses needed to understand the glaciological processes happening in this region necessitate the use of diverse satellite datasets and ancillary data to address questions related to the interaction among glaciers, climate, and oceans. Furthermore, it calls attention to the need for and potential of synergic approaches between GLIMS activities and other satellite-based investigations of AP glaciers. 30.7 ACKNOWLEDGMENTS This work was partially supported under grants BR 2105/4-1/2/3 and BR 2105/8-1 from the German Research Foundation, and grants CNPq 480701/ 2008-3 and CNPq 573720/2008-8 (Brazilian National Institute for Cryospheric Sciences) from the Brazilian National Council for Scientific and Technological Development. 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