1. Introduction
Ice shelves are the floating extensions of ice sheets and play an important role in maintaining ice-sheet stability due to the back stresses they exert upon upstream grounded-ice flow (Dupont and Alley, Reference Dupont and Alley2005; Goldberg, Reference Goldberg, Richardson, Castree, Goodchild, Kobayashi, Liu and Marston2017). In Antarctica, approximately 74% of the coastline is fringed by ice shelves (Bindschadler and others, Reference Bindschadler2011), which lose approximately half of their mass through surface and basal melting, and half through calving and iceberg production (Depoorter and others, Reference Depoorter2013; Rignot and others, Reference Rignot, Jacobs, Mouginot and Scheuchl2013; Liu and others, Reference Liu2015). Where reductions in ice shelf area and thickness result in decreased amounts of back-stress, or ‘buttressing’, as has been observed across Antarctica over at least the duration of the satellite era (~1960 onwards; Cook and others, Reference Cook and Vaughan2010; Paolo and others, Reference Paolo, Fricker and Padman2015), ice velocities across the grounding line and over the remaining ice shelf may increase (Rignot and others, Reference Rignot2004; Scambos and others, Reference Scambos, Bohlander, Shuman and Skvarca2004; Fürst and others, Reference Fürst2016; Shepherd and others, Reference Shepherd, Fricker and Farrell2018). Thus, the loss of ice shelves can contribute to sea-level rise in an indirect way via lagged accelerations in grounded-ice discharge (Shepherd and Wingham, Reference Shepherd and Wingham2007; Gudmundsson and others, Reference Gudmundsson, Paolo, Adusumilli and Fricker2019).
On 12 July 2017, a 5834 km2 section of ice detached from the Antarctic Peninsula's Larsen C Ice Shelf (LCIS; Fig. 1) in response to a combination of long-term ice-shelf mechanical weakening processes and the loss of intra-rift mélange and fortifying coastal sea ice (Larour and others, Reference Larour, Rignot, Poinelli and Scheuchl2021; Christie and others, Reference Christie2022a; Wang and others, Reference Wang2022). The colossal size of this iceberg, named A-68, relative to LCIS’ total areal extent (12.3%) raises important questions about the impact of its calving on the dynamics of the remaining ice shelf (Hogg and Gudmundsson, Reference Hogg and Gudmundsson2017), since the loss of large sections of shelf ice can precondition collapse (Doake and others, Reference Doake, Corr, Rott, Skvarca and Young1998; Larour and others, Reference Larour, Rignot, Poinelli and Scheuchl2021). Indeed, since the late 20th century, several ice shelves in the Antarctic Peninsula have undergone catastrophic break up resulting from sustained calving beyond the compressive limits of stability, together with the effects of widespread surface melt-induced hydrofracture and oceanic forcing (Doake and others, Reference Doake, Corr, Rott, Skvarca and Young1998; Shepherd and others, Reference Shepherd, Wingham and Rignot2004; Scambos and others, Reference Scambos2009; Cook and Vaughan, Reference Cook and Vaughan2010; Banwell and others, Reference Banwell, MacAyeal and Sergienko2013; Massom and others, Reference Massom2018; Christie and others, Reference Christie2022a). Furthermore, several ice shelves have been projected to lose mass over the 21st century (Trusel and others, Reference Trusel2015; DeConto and Pollard, Reference DeConto and Pollard2016; Golledge and others, Reference Golledge2019; Sadai and others, Reference Sadai, Condron, DeConto and Pollard2020; Seroussi and others, Reference Seroussi2020; Sun and others, Reference Sun2020; DeConto and others, Reference DeConto2021), although there is low confidence in the magnitude of total loss due to considerable process uncertainty (Fox-Kemper and others, Reference Fox-Kemper2021). Assessing the dynamic impacts of recent changes in ice-shelf extent is therefore critical for diagnosing both present-day and future ice-shelf instability.
Map of Larsen C Ice Shelf (LCIS). Figure shows the pre-calving limits of iceberg A-68 and flowlines 1-7 along which the ice velocity profiles presented in Figures S4 and S5 were extracted. 10 km (red circles) and 50 km (blue circles) increments are marked along each flowline. Black lines indicate the position of the grounding line in 2019 (Christie and others, Reference Christie2022b); cyan and green lines, the position of the ice-shelf front in January 2017 and January 2018, respectively (Christie and others, Reference Christie2022c). The dashed black line between Kenyon Peninsula and the Gipps Ice Rise shows the boundary between the Larsen C and D ice shelves (Mouginot and others, Reference Mouginot, Scheuchl and Rignot2017a). Background shows median ice velocity magnitude observed between October 2014 and December 2016, superimposed over a Sentinel-1A extra wide swath sigma-nought image dated 10th July 2017 (two days before calving). Inset shows location of LCIS.
Existing studies of LCIS’ dynamic evolution have focused predominantly on the numerical modelling of potential ice mass loss scenarios (Borstad and others, Reference Borstad, Rignot, Mouginot and Schodlok2013, Reference Borstad, McGrath and Pope2017; Fürst and others, Reference Fürst2016; Reese and others, Reference Reese, Gudmundsson, Levermann and Winkelmann2018; Schannwell and others, Reference Schannwell, Cornford, Pollard and Barrand2018; Mitcham and others, Reference Mitcham, Gudmundsson and Bamber2022), and offer predictions of ice-velocity perturbation based on modelled ice-shelf ‘buttressing potential’ quotients derived using composite, multi-year ice velocity records (e.g. Rignot and others, Reference Rignot, Mouginot and Scheuchl2011). For example, Fürst and others (Reference Fürst2016) conducted ice-flow and calving experiments to chart areas of ‘passive ice’ (low buttressing potential) on LCIS; the loss of this ice was predicted to have little impact on ice-shelf dynamics and flux past the grounding line. Based on these experiments, they predicted that a tabular calving event of similar dimensions to that of A-68 would remove mostly passive ice, yielding limited change in both ice-shelf and grounded-ice velocities as a result (Fürst and others, Reference Fürst2016). Consistent with this prediction, Borstad and others (Reference Borstad, McGrath and Pope2017) and Mitcham and others (Reference Mitcham, Gudmundsson and Bamber2022) later simulated similar responses to A-68's breakaway, with minor shelf-averaged velocity accelerations in the months following calving totalling ⩽~10% relative to long-term baseline rates of flow. In the case of the findings presented by Mitcham and others (Reference Mitcham, Gudmundsson and Bamber2022), this response was accompanied by a commensurate grounding line flux increase of only 0.28%.
In the context of the studies discussed above, it is important to consider that the multi-annual composite velocity records underpinning their models may act to smooth out true, short-term variability in flow at or during the run up to calving, resulting in potentially biased projections of instantaneous ice-shelf response. Here, we utilise newly available, high spatial and temporal resolution Sentinel-1A/B synthetic aperture radar (SAR)-derived observations to examine the instantaneous impact of A-68's calving upon LCIS’ flow, and contextualise our findings with longer-term velocity records spanning 2014 to 2021.
2. Study area
LCIS is located on the eastern coast of the Antarctic Peninsula and prior to July 2017 covered an area of 47 455 km2 (Mouginot and others, Reference Mouginot, Scheuchl and Rignot2017a; Christie and others, Reference Christie2022c) (Fig. 1). LCIS is confined by Jason Peninsula and Bawden Ice Rise to the north, Kenyon Peninsula and Gipps Ice Rise to the south, and is nourished by an area of ~27 000 km2 of inland glacial ice which drains towards the Weddell Sea (Khazendar and others, Reference Khazendar, Rignot and Larour2011). Most glaciers feeding LCIS descend along steep gradients from high elevation plateaus situated along the Antarctic Peninsula, entering the ice shelf through several deep-bedded inlets (Khazendar and others, Reference Khazendar, Rignot and Larour2011; Fretwell and others, Reference Fretwell2013). The seaward locations of these thickest glaciers represent the starting points of the flowlines presented in Figure 1.
Following the abrupt collapse of several of its ice shelves since the late 20th century (cf. Section 1), the Antarctic Peninsula has contributed ~2.5 ± 0.4 mm to global sea-level, largely due to subsequent increases in outlet glacier discharge (Rignot and others, Reference Rignot2004; Reference Rignot2019; Scambos and others, Reference Scambos, Bohlander, Shuman and Skvarca2004; The IMBIE Team, 2018). LCIS is now the most northerly remaining ice shelf on the Antarctic Peninsula (Jansen and others, Reference Jansen2015) although, to date, it has exhibited no evidence of glaciological instability akin to that which presaged, for example, the collapse of its neighbouring Larsen A and B ice shelves (Massom and others, Reference Massom2018; Wang and others, Reference Wang2022). Relative to the rapid-melting ice shelves fringing the Bellingshausen Sea (Paolo and others, Reference Paolo, Fricker and Padman2015; Adusumilli and others, Reference Adusumilli2018), LCIS's primary source of ablation is iceberg calving (Rignot and others, Reference Rignot, Jacobs, Mouginot and Scheuchl2013). Major calving events from LCIS are, however, infrequent, and prior to the detachment of iceberg A-68, have occurred on only three occasions over the satellite era with iceberg areal extents ranging between 1260 and 6520 km2 (Skvarca, Reference Skvarca1994; Cook and Vaughan, Reference Cook and Vaughan2010; Christie and others, Reference Christie2022a). In this context, the calving of iceberg A-68 is not unprecedented within the observational era, and likely represents the decadal-scale tabular calving lifecycle common to all large ice shelves.
3. Methods
3.1 SAR-based velocities
We use high spatial and temporal resolution SAR-derived ice velocity records in our analyses. These products were generated from a combination of high precision, coherent and incoherent offset tracking techniques applied to all successive (6-/12-day) repeat-pass Sentinel-1A/B image pairs acquired in interferometric wide swath mode over the period November 2014 to December 2020, from which time complete observational coverage over LCIS exists. At time of writing, no processed velocity records exist for 2021. Importantly for our work, the products are corrected for tidal- and atmospheric-induced motion using a tide model (CATS2008; Erofeeva and others, Reference Erofeeva, Howard and Padman2019) and atmospheric reanalysis data (ERA5; Hersbach and others, Reference Hersbach2020), and are presented as monthly averaged observations of ice velocity to negate any residual tidal and atmospheric components not corrected for by CATS2008 and ERA5. Such phenomena represent the largest drivers of diurnal-to-bi-monthly ice-shelf velocity variability, which without correction may act to mask longer wavelength, calving-related dynamic signals. These monthly records were acquired from the ENVEO GmbH ‘Cryoportal’ data archive (https://cryoportal.enveo.at/) at a grid resolution of 200 m, alongside associated grids of variability (1 SD) and valid pixel count (i.e. the number of non-NaN velocity observations used in the production of each monthly per-pixel estimate) which we use for error assessment purposes (see below and Section 3.4). Further information about these products and the offset tracking techniques associated with their generation can be found in Nagler and others (Reference Nagler, Rott, Hetzenecker, Wuite and Potin2015, Reference Nagler2021), Wuite and others (Reference Wuite2015) and Shepherd and Engdahl (Reference Shepherd and Engdahl2021).
Standard errors associated with our monthly velocity records were calculated following previously reported techniques (Greene and others, Reference Greene, Blankenship, Gwyther, Silvano and van Wijk2017; Boxall and others, Reference Boxall, Christie, Willis, Wuite and Nagler2022) using Eqn 1:
where σ is the variation (1 SD) associated with the velocity record for month t, scaled by the number of valid pixels, N. Mean monthly variability over LCIS during the observational period is calculated to be 18 m yr−1 (Figure S1a and b), a value which corresponds well with previous Sentinel-1A/B-based ice-sheet velocity mapping exercises that have revealed typical 6- and 12-day image pair variabilities of ~10–30 m yr−1 and ~4–17 m yr−1, respectively (Nagler and others, Reference Nagler, Rott, Hetzenecker, Wuite and Potin2015; Mouginot and others, Reference Mouginot, Rignot, Scheuchl and Millain2017b; Friedl and others, Reference Friedl, Seehaus and Braun2021; Solgaard and others, Reference Solgaard2021; Rignot and others, Reference Rignot, Mouginot, Scheuchl and Jeong2022). For an average of 7 valid observations per pixel over the ice shelf per month, this variability value of 18 m yr−1 yields a mean monthly standard error of 6.8 m yr−1 (Figure S1c and d).
3.2 Short-term velocity change
To investigate short-term changes in ice-shelf velocity following A-68's calving, we first calculated the departure in LCIS’ flow across each of the six months post-calving (July–December 2017, inclusive) relative to the median velocity exhibited during the six months prior (January to June 2017, inclusive). Median velocity was calculated to minimise the influence of possible outliers contained in the individual monthly records, and January-June 2017 was chosen as a baseline to capture the post-calving velocity response of LCIS relative to that observed in the immediate run-up to A-68's calving. Since we utilise monthly averaged velocity records, ice shelf velocities for July 2017 include data from the eleven days before, and twenty days during and after, calving. Thus, the resulting velocity difference between July and the six months preceding calving will be dominated by, and offer unique insight into, LCIS’ instantaneous (~3-week) response to A-68's breakaway.
For added context, we also generated shelf-averaged velocity timeseries at monthly intervals spanning the entire processed Sentinel-1 velocity record (November 2014 to December 2020). During the production of this timeseries, we initially filtered the data to remove additional sources of potential error in three steps. First, we discarded all monthly records associated with poor spatial coverage across the ice shelf (defined here as <75%). Such records are typically associated with föhn-like conditions near the grounding line in 2014 and 2015 (Figure S1; cf. Luckman and others, Reference Luckman2014; Bevan and others, Reference Bevan2018), during which time SAR coherence (and, hence, accurate velocity retrieval) was compromised owing to the surface meltwater-induced attenuation of microwave radiation (Li and others, Reference Li, Lhermitte and López-Dekker2021). For the remaining records, spatial coverage is typically >90–95%. Second, we removed all monthly records produced using less than three image pairs (i.e. ‘valid pixel count’ <3). This applies only to June 2016 where the ‘valid pixel count’ was 1. Finally we culled all remaining pixels where velocity fell within standard error bounds (cf. Eq. 1).
3.3 Longer-term velocity change
In addition to examining short-term changes in post-calving velocity, we also calculated longer-term (annual) summaries of change relative to the pre-2017 Sentinel-1 record. These summaries were examined to shed light upon LCIS’ longer-term response to the calving of A-68 up to and including 2020. To do this, we generated annual velocity stacks for the years 2018, 2019 and 2020 by calculating the median of all monthly velocity records associated with each year, and then differenced each of these from the median velocity observed over all months spanning November 2014 to December 2016 (inclusive). The year 2017 was omitted from these calculations to avoid any potential contamination in velocity response from the months falling either side of A-68's calving.
3.4 Velocity change uncertainties
Using the standard error values associated with each monthly velocity record (cf. Section 3.1), propagated errors associated with our velocity change observations (cf. Sections 3.2 and 3.3) were quantified as the median standard error for each time period (i.e. ${v_{err_{\widetilde{pre-calving}}}}$
and ${v_{err_{\widetilde{post-calving}}}}$
) summed in quadrature. As with the calculation of average velocities, we use the median here to minimise the influence of possible standard error outliers associated with the individual monthly records. The tilde signs represent the medians of the monthly errors for the relevant time period. Thus, to formally quantify the error associated with, for example, the short-term (month-scale) change in LCIS’ velocity during August 2017 relative to the period January 2017‒June 2017 (cf. Section 3.2), $v_{err_{\delta t}}$
, Eqn 2 was used. For the error associated with our longer-term summaries (for example, the year 2018 relative to all months spanning October 2014‒December 2016; cf. Section 3.3), Eqn 3 was used.
For our analyses of short-term (monthly) changes in velocity, the second term within Eqn 2 represents the standard error associated with the sole post-calving month analysed only, since the observational sample size equals one. Maps of resulting error associated with our velocity change observations are shown in Figures S2 and S3, respectively, and were used to mask all regions exhibiting negligible ice-shelf velocity change defined as falling within error limits (i.e. ± $v_{err_{\delta t}}$
).
4. Results
In the following sections, all reported values are calculated for LCIS pixels falling outside error bounds only and, unless explicitly specified, do not include Larsen D Ice Shelf (LDIS) to the south (see Fig. 1 for location).
4.1 Short-term SAR-derived velocity change
Figure 2 shows the change in ice-shelf velocity for the six individual months following A-68's calving relative to the six months prior (cf. Section 3.2). While these changes are small relative to overall rates of ice-shelf advection (~10% of overall flow speed; Figs 1 and S4), we detect a marked oscillatory pattern in shelf-averaged flow in the months following A-68's calving, whereby the sign and month-to-month magnitude of anomalous flow appears to have alternated and gradually diminished through time, respectively, towards December 2017. The initiation of this oscillatory behaviour in the days and weeks immediately following A-68's calving (Fig. 2a) was associated with a pervasive slowdown in ice-shelf flow totalling 5–20 m yr−1 (mean = 11.3 m yr−1) across 79.3% of the ice shelf.
Change in ice-shelf velocity for each of the six months following the breakaway of iceberg A-68 relative to January–June 2017. Observations are masked where values fall within error (cf. Section 3.4 Eqn 2, and Figure S2). Black lines indicate the position of the grounding line in 2019 (Christie and others, Reference Christie2022b); cyan and green lines, the position of the ice-shelf front in January 2017 and January 2018, respectively (Christie and others, Reference Christie2022c). Data are superimposed over a hillshaded version of REMA DEM (Howat and others, Reference Howat, Porter, Smith, Noh and Morin2019).
In contrast to July 2017, August 2017 was characterised by significant increases in ice shelf velocities (>30 m yr−1) over a large part of the central ice shelf and the Cabinet and Adie inlets (Figs 1 and 2b). In total, velocity increases occurred across 46.0% of LCIS, constituting a mean change of 12.4 m yr−1. Reductions in velocity were also present during this time (across 19.4% of the ice shelf area), although – like most of the post-calving months shown in Figure 2 – these were largely confined to regions proximal to the grounding line of LCIS’ deepest-bedded glaciers (i.e. those upstream of Flowlines 4–7 in Fig. 1). Consistent with the oscillatory pattern discussed above, velocity signals during September and October 2017 showed, respectively, similar patterns and magnitudes of velocity change (Figs 2c and 2d) to those that occurred in July and August (Figs 2a and 2b). The magnitudes of velocity change in November and December 2017 were slightly smaller than those during the previous four months, and exhibited a change from predominantly faster ice shelf velocities in November (Fig. 2e) to more widespread velocity decreases, of up to ~30 m yr−1, in December (Fig. 2f).
4.2 Longer-term SAR-derived velocity change
Over annual timescales (Fig. 3), velocity differences were much more subdued (~⩽5% of overall flow speed; Figure S5) than those exhibited in the months immediately following A-68's calving (Fig. 2). Although parts of LCIS underwent velocity increases of ~10–20 m yr−1 in 2018 relative to the long-term, pre-A-68 Sentinel-1 record (Fig. 3a; especially near LCIS’ grounding line and central section), overall velocity changes exceeding error bounds were small. Indeed, only 9.5% of LCIS underwent velocity increases exceeding error between 2014–16 and 2018, and the mean overall speedup was only 2.9 m yr−1.
Change in ice-shelf velocity in the years following iceberg A-68's calving relative to all months spanning October 2014‒December 2016. Observations are masked where values fall within error (cf. Section 3.4, Eqn 3 and Figure S3). Black lines indicate the position of the grounding line in 2019 (Christie and others, Reference Christie2022b); cyan and green lines, the position of the ice-shelf front in January 2017 and January 2018, respectively (Christie and others, Reference Christie2022c). Data are superimposed over a hillshaded version of REMA DEM (Howat and others, Reference Howat, Porter, Smith, Noh and Morin2019).
In contrast to 2018, velocities in the centre of LCIS during 2019 had either returned to or decelerated from baseline rates of flow as observed between 2014–2016, in the latter case by ~10 m yr−1 (Fig. 3b). Elsewhere, velocities remained greater than in 2014–16 by up to 15 m yr−1, including a narrow band of acceleration at and immediately seaward of the grounding line along most of the ice shelf's margin south of Jason Peninsula, and a small section of the newly exposed ice front at ~67.5°S (Figs 1 and 3b). Velocity changes exceeding error occurred over 7.1% (velocity speedup) and 9.6% (velocity slowdown) of the ice shelf, respectively, with an overall, mean velocity slowdown of 0.7 m yr−1.
In 2020, velocities continued to slow relative to previous years, with the spatial signature of observations suggestive of a coherent deceleration across most of LCIS (Fig. 3c, see also Figure S3). During this time, velocity decreases below baseline (2014–16) rates of flow occurred across 12.4% of the ice shelf (Fig. 3c), with a mean velocity slowdown of 5.9 m yr−1.
Though not included in our calculations above, we note that much of the area residing immediately south of Gipps Ice Rise and Kenyon Peninsula, comprising the northernmost section of LDIS (cf. Fig. 1), exhibited no change in ice velocities in 2018 compared to those in 2014–16, suggesting no major, medium-term impact of the A-68 calving event (Fig. 3a). Ice at this location then accelerated in 2019 compared to both 2018 and 2014–16, exceeding pre-calving velocities by >30–141 m yr−1 (Fig. 3b). A similar pattern of acceleration continued into 2020 (Fig. 3c), with a particularly marked speedup immediately south of Gipps Ice Rise where rifts parallel to ice flow and orthogonal to the ice front were clearly visible (Fig. 3c). There, a section of ice extending approximately 25 km inland from the ice front accelerated to flow up to 500 m yr−1 faster in 2020 than in 2014–16. Conversely, a section of ice residing immediately south of this block, extending up to a prominent rift parallel to the ice front to Hearst Island, decelerated (Figs 1 and 3c). These patterns are consistent with variations in strain rates which ultimately led to the calving of the ~460 km2 iceberg ‘A-69’ from LDIS in June 2020 (Christie and others, Reference Christie2022a). The iceberg detached along a fracture parallel to the ice front, which is depicted by the marked boundary between fast- and slow-moving ice south of Gipps Ice Rise (Fig. 3c). Ultimately, the time-variable presence of this signal within our velocity change observations and its association with a confirmed calving event lends credence to the reliability of the more subtle velocity signals we observe at LCIS (Fig. 3).
5. Discussion
5.1 Short-term post-calving response of LCIS
Our observations present evidence for a previously undocumented response of LCIS to the calving of iceberg A-68 in July 2017. While falling close to the limits of detectability, in the weeks and months immediately following this event, the ice shelf appeared to undergo distinct, widespread and alternating patterns of anomalous deceleration and acceleration relative to baseline rates of ice flow measured during the earlier half of 2017 (Fig. 2). Critically, the amplitude of this anomalous month-to-month variability decayed in the months following calving, suggesting that LCIS underwent a damped harmonic oscillatory response to the breakaway of A-68. In other words, our findings point to new, observationally constrained evidence for the vibratory response of one of Antarctica's largest ice shelves to a calving-induced, major internal stress perturbation event. Given the corrections applied to our monthly averaged velocity records (Section 3.1), this behaviour suggests that tidal and atmospheric forcing cannot have been responsible for LCIS’ post-calving response. The periodicity of the observed oscillations further precludes the possible influence of oceanic forcing in the form of standing waves (also known as ‘seiches’) underneath the ice shelf (cf. Munk, Reference Munk1950), whose relatively short-lived presence would be smoothed out over the monthly timescales we consider.
The immediate impact of A-68's calving was to cause the ice shelf to slowdown (Fig. 2a; Section 4.1). This implies that the nascent iceberg A-68 exerted enhanced tensile stresses on LCIS’ upstream ice prior to its break off (that is, A-68 ‘pulled’ LCIS seaward through maximised longitudinal strain) which, upon calving, induced a recoil-like reactionary stress which opposed seaward flow and caused the ice shelf to decelerate rapidly over the course of the month. Like those exhibited prior to the breakaway of iceberg A-69 from LDIS in 2020 (cf. Section 4.2 and Fig. 3c), ice velocities seaward of LCIS’ eventual calving front were substantially greater than those behind it during January to June 2017 (Figure S4), supporting this interpretation. In this way, comparable stress-related response processes can also explain LCIS’ consequent speed-up in August 2017 (Fig. 2b), which acted to (over-)compensate for the instantaneous decrease in tensile stress felt immediately after A-68's calving in July 2017. Further (over-)compensations in longitudinal stress can similarly explain LCIS’ later oscillatory-like behaviour (Figs 2c-f), after which time the ice shelf eventually returned to near-baseline rates of flow.
To contextualise our short-term post-calving observations, shelf-averaged monthly variations in ice flow spanning November 2014 to December 2020 are shown in Figure 4 (cf. Section 3.2). There, the dampened harmonic oscillatory behaviour of LCIS discussed above following A-68's breakaway is apparent (second period of pink shading from July 2017 to March 2018 in Fig. 4), as is its restoration towards baseline rates of ice flow (associated with more muted month-to-month variability) from early 2018 onwards. Figure 4 also indicates the presence of several significant velocity perturbations between January 2015 and July 2016 (first period of pink shading in Fig. 4). Notably, these events exhibit velocities which generally exceed those observed following A-68's calving, and their month-to-month variability appears to fluctuate in an oscillatory-like manner similar to that detailed above (cf. Fig. 2). For the most part, the amplitude of month-to-month velocity variability during this time is also broadly analogous to the amplitudes of change witnessed in the immediate aftermath of A-68's calving and select months beyond (e.g. mid-2019), when the number of valid pixels used in the production of each monthly velocity estimate was greater owing to the availability of Sentinel-1B imagery. This gives confidence that the velocity perturbations we observe between January 2015 and July 2016 are real, and not simply related to the absence of Sentinel-1B data. Poor data coverage in 2014 and for several months in 2015 (timeseries gaps in Fig. 4) precludes any further, detailed historical analysis of this oscillatory behaviour.
Monthly velocity fluctuations across Larsen C Ice Shelf (LCIS) and links to rifting and calving. Time series shows mean monthly velocities averaged across LCIS spanning the processed Sentinel-1 record. Data gaps exist where ice-shelf coverage totals <75%, and where ice-shelf mean monthly ‘valid pixel count’ (numbers enclosed by white circles) totals <3 (cf. Section 3.2). Dashed vertical lines show the timings of major rifting events (cf. Hogg and Gudmundsson, Reference Hogg and Gudmundsson2017), colour coded according to the length of the rift as a percentage of the total length of iceberg A-68 at time of calving. Pink shading denotes times characterised by high amplitude, oscillatory month-to-month variability in ice flow as discussed in the text (see also Fig. 2); blue shading signifies times associated with more muted month-to-month velocity change. Blue lines denote pre-calving baseline flow used in the production of Figure 2 (median velocity magnitude spanning January–June 2017; cf. Section 3.2), extended back and forth in time for reference; cyan line, linear trend in velocity spanning all months with (near-)complete ice shelf coverage (February 2015 to November 2020). Grey and black bars denote Sentinel-1A and Sentinel-1A/B constellation coverage over LCIS, respectively.
Notwithstanding the limited 2014/2015 data coverage detailed above, we note that the earlier, high amplitude velocity variability exhibited between January 2015 and July 2016 correlates closely with the timing of rift propagation associated with iceberg A-68's formation (cf. Hogg and Gudmundsson, Reference Hogg and Gudmundsson2017). This provides compelling evidence that, upon rifting beyond some critical threshold(s) of A-68's total length (c.45–60%), substantial internal stress changes associated with the tearaway of most of the iceberg induced an analogous – albeit more significant – oscillatory-like response to that observed at the time of calving in July 2017 (Figs 2 and 4). Further rift propagation events (⩾70% of A-68's total length; Fig. 4) also likely contributed to LCIS’ oscillatory ice-flow behaviour between these times, although the ensuing, more frequent rifting events observed between December 2016 and June 2017 do not appear to have induced any major variations in ice shelf velocities exceeding those observed in the earlier Sentinel-1 record. We expect that these later rift propagation events were simply too small to elicit any major change in internal stress detectable by Sentinel-1 at monthly resolution.
5.2 Long-term post-calving response of LCIS
Compared to the short-term velocity fluctuations discussed above (Section 5.1), post-calving changes in ice flow integrated across annual timescales were small (Figs 3 and S5), and are suggestive of a minor but temporally progressive deceleration in velocity relative to baseline (2014–16) rates of flow (cf. Section 4.2). This minor deceleration trend is also evident in Figure 4, revealing that the calving of iceberg A-68 had no significant impact upon longer-term, LCIS-wide ice dynamics up to and including 2020. This finding lies in good agreement with the temporally averaged, SAR-derived observations (to 2019) presented by Mitcham and others (Reference Mitcham, Gudmundsson and Bamber2022) (cf. Section 1), and with recent velocity trends observed across LCIS using optical-based satellite imaging techniques (Christie and others, Reference Christie2022a). Proximal to LCIS’ grounding zone, especially (where velocity changes are an accurate proxy for variability in grounded ice discharge to the ocean), this finding is also consistent with relatively unchanged rates of grounded ice mass-loss over the past ~20 years (Rignot and others, Reference Rignot2019; Velicogna and others, Reference Velicogna2020; Chuter and others, Reference Chuter, Zammit-Mangion, Rougier, Dawson and Bamber2022).
Overall, our observations of no significant long-term dynamical change at LCIS mirror the response associated with most historical calving events in Antarctica (Cook and Vaughan, Reference Cook and Vaughan2010; Christie and others, Reference Christie2022a; Greene and others, Reference Greene, Gardner, Schegel and Fraser2022). This lack of response does, however, contrast with other notable calving events in neighbouring regions of the Antarctic Peninsula and West Antarctica in recent decades, which have since resulted in significant ice-shelf velocity accelerations. Much greater velocities have, for example, been observed across SCAR Inlet Ice Shelf in the years following Larsen B Ice Shelf's 2002 disintegration (Wuite and others, Reference Wuite2015; Rignot and others, Reference Rignot2019), as well as more recently at Pine Island Glacier Ice Shelf, West Antarctica, in response to a 19-km long retreat of its ice front since 2017 (Joughin and others, Reference Joughin, Shapero, Smith, Dutrieux and Barham2021). Similarly, the partial collapse of an ice bridge on Wilkins Ice Shelf between February and July 2008 resulted in widespread ice-shelf velocity increases to up to three times their pre-collapse values (Rankl and others, Reference Rankl, Fürst, Humber and Braun2017). In each of the above cases, the velocity changes have been attributed directly to significant losses in ice-shelf buttressing (Wuite and others, Reference Wuite2015; Rankl and others, Reference Rankl, Fürst, Humber and Braun2017; Joughin and others, Reference Joughin, Shapero, Smith, Dutrieux and Barham2021).
5.3 Ice-shelf damage and the importance of passive ice
The contrasting nature of our annual-scale observations relative to post-calving velocity increases elsewhere in Antarctica (Section 5.2) emphasises the importance of passive ice in regulating LCIS’ longer-term stability (cf. Section 1). That is, our findings provide important observation-based verification of several previous modelling studies that have suggested that the buttressing potential afforded by A-68 prior to its breakaway was small. Indeed, Fürst and others (Reference Fürst2016) concluded from ice-flow modelling experiments that the area of ice which formed A-68 was primarily passive, meaning that its calving would have had little effect on longer-term ice velocities across the remaining LCIS and its feeder glaciers. Later finite element modelling experiments by Reese and others (Reference Reese, Gudmundsson, Levermann and Winkelmann2018) revealed similar, low ‘buttressing flux response’ numbers (a measure of the change in ice flux across the grounding line for a given amount of localised ice-shelf thinning) at and proximal to the nascent A-68, providing additional evidence that its presence exerted little resistance upon upstream ice flow.
Following Section 1, the clear but limited changes in velocity magnitude above error we observe in the months following A-68's calving (Figs 2 and 4) are also somewhat consistent with the studies of Borstad and others (Reference Borstad, McGrath and Pope2017) and Mitcham and others (Reference Mitcham, Gudmundsson and Bamber2022), who modelled the velocity response of A-68's calving and reported only limited increases in flow (⩽~10%) relative to long-term, observationally constrained rates. We note, however, that the near-shelf-wide acceleration trends reported in these studies appear inconsistent with the longer-term trend of ice-flow deceleration we observe between 2015 and 2020 (Fig. 4), a discrepancy likely attributable to model and/or boundary input biases. In terms of ice-shelf stability more generally, we further note that our observations do not appear to support the modelling-derived conclusions of Jansen and others (Reference Jansen2015) who, contrary to the findings of the studies discussed above, predicted that A-68's breakaway may render LCIS instantaneously susceptible to runaway calving and collapse.
Notwithstanding the importance of passive ice for regulating longer-term ice-shelf stability, over much shorter timescales, the hitherto undocumented, monthly-scale oscillations in ice flow we observe either side of iceberg A-68's calving (Figs 2 and 4) suggest the presence of far-reaching changes in ice shelf strain. By implication, such pervasive rifting- and calving-related phenomena likely represent an important, short-term mechanism of ice-shelf damage extending far beyond the regions of passive ice identified by models (e.g. Fürst and others, Reference Fürst2016; Reese and others, Reference Reese, Gudmundsson, Levermann and Winkelmann2018). Ultimately, we expect that such damage may have played a key role in preconditioning LCIS towards future rifting and/or calving, enabled through a process of enhanced ice-fabric weakening focused especially along the margins of slow-flowing promontories where shear-induced deformation and crevassing are maximal (Jansen and others, Reference Jansen2010; Reference Jansen2015; Borstad and others, Reference Borstad, McGrath and Pope2017; Alley and others, Reference Alley2018; Lhermitte and others, Reference Lhermitte2020). In this regard, continued, high-resolution surveillance of LCIS will be desirable for elucidating the significance, and future implications of, this previously unseen damage mechanism.
6. Summary and implications
Using comprehensive ice velocity records derived from Sentinel-1A/B SAR, we present evidence suggesting that Larsen C Ice Shelf (LCIS) underwent pervasive, oscillatory-like patterns of ice-flow deceleration and acceleration in the months following the calving of iceberg A-68 in July 2017. While relatively short-lived, close to the limits of detectability and superimposed upon a longer-term trend of ice-flow deceleration between at least 2014 and 2021, our observations further suggest that similar oscillatory behaviour occurred in response to major rifting events associated with A-68's formation. Acting as a reliable proxy for changes in ice shelf strain, these phenomena reflect previously undocumented, short-term drivers of ice-shelf damage which extend far inland of the regions of ‘passive ice’ predicted by models. Ultimately, this damage may have important implications for preconditioning future rifting and calving at LCIS, and suggests that similar transient processes may be important at other climatically vulnerable ice shelves around Antarctica.
Supplementary material
The supplementary material for this article can be found at https://doi.org/10.1017/jog.2023.102.
Data availability
The Sentinel-1A/B SAR-derived velocity grids utilised in this study are available courtesy of ENVEO IT GmbH at: https://cryoportal.enveo.at/data/. The processed velocity observations presented in this manuscript are available at doi:10.17863/CAM.101851 (Deakin and others, Reference Deakin, Christie, Boxall and Willis2023). Links to all other datasets mentioned in the text are included in the reference list.
Acknowledgements
The authors thank Thomas Nagler and Jan Wuite of ENVEO IT GmbH for their initial discussions and access to the processed SAR velocity grids before they were made publicly available, and the European Space Agency and EU Copernicus programme for making the Sentinel-1 data used in this study freely available. KAD also thanks Gabriel Amable for initial discussions in support of this work.
Author's contributions
KAD conceived of the project and carried out the analysis under the supervision of FDWC and ICW. FDWC and KB provided technical assistance to KAD and calculated the velocity errors. KAD, FDWC and ICW wrote the paper with input from KB.
Financial support
We acknowledge the following sources of funding received during the completion of this work: St Catharine's College, Cambridge academic bursary (to KAD); UK Natural Environment Research Council Grant NE/T006234/1 (to ICW); and UK NERC PhD Studentship awarded through the University of Cambridge C-CLEAR Doctoral Training Partnership Grant NE/S007164/1 (to KB). This work was also produced with the financial assistance of the Prince Albert II of Monaco Foundation (to FDWC).
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