Antarctic Bottom Water (AABW) is considered as the great ventilator of the world deep ocean and is a critical component of the global climate system1,2. AABW is sourced by dense saline shelf waters, locally produced in several polynyas, where low sea ice concentrations (SICs) and open water conditions are maintained during winter and favour local sea ice and brine production3,4. Coastal polynyas are usually associated with the presence of local topographic or glacial features and synoptic-scale gravity winds4. Although they only represent a small fraction of the area covered by sea ice, polynyas are considered of key importance for the Earth climate system3,5. Indeed, while the 13 major Antarctic coastal polynyas only represent ~1% of the maximum ice area, they are responsible for the production of 10% of the Southern Ocean sea ice3. Recently, it has been shown that ~25% of the AABW is sourced from the export of Adélie Land Bottom Water (ALBW) produced in the George V Land polynyas2,6. ALBW mainly originates from the Adélie Depression off the coast of George V Land3,6,7, where the Mertz Glacier (MG) Polynya (MGP) develops in winter along the western flank of the MG Tongue (MGT) and further extends to the West in the adjacent coastal bays (Commonwealth, Watt and Buchanan Bays; Fig. 1b; refs 8, 9). The MGP constitutes the third most productive polynya in Antarctica, with a winter area of up to 6,000 km2 and an annual sea ice production of 120 km3 over the 1992–2001 period3,4.

Figure 1: Pre- and post-calving sea ice conditions in the George V Land.
figure 1

Aqua MODIS satellite images showing sea ice conditions in the study area during summer (a) and winter (b) before the 2010 calving event, and during summer (c) and winter (d) after the 2010 calving event. The white star in a red circle indicates the core location; the Dumont D’Urville station is indicated by a red square; blue shadings indicate glacial features, the MGT and the B09B iceberg; the MGP area in winter before and after the calving is designated by the yellow grid on b,d; and the blue arrow indicates the general direction of the East Wind Drift; coastline is marked by the black dotted line. (e) Three-month averaged SSM/I time series of daily SIC anomalies in CB (dark blue) and in the Mertz area (MGP—light blue), for the period 1978–2012 C.E. (Common Era) using 1978–2009 as the reference period (for the exact grid points locations, see Fig. 7). The red shading indicates the 2010 calving event.

Early in 2010, the MG underwent massive calving and lost half its tongue after collision with the B09B iceberg. The generation of an 80-km-long iceberg and subsequent retreat of the MG front had a profound impact on both regional icescape and ocean conditions9,10,11. Satellite passive microwave data show that SIC increased by 50% (relative to the 1979–2009 period) in the MGP area after the calving (Fig. 1e). Advection of thick consolidated sea ice and presence of fast ice downstream the MG in the MGP (Fig. 1c,d) led to a large reduction in sea ice production in the MGP, which in turn affected dense water formation9,10,11. Within 2 years following the calving, bottom water salinity decreased by over 0.30 psu in Commonwealth Bay (CB)9.

Located in the southern part of the polynya, CB is ideal for studying past dynamics of the MGP and dense water formation9. Indeed, mooring observations and satellite data showed that oceanic and sea ice conditions (Fig. 1e) over the CB and MGP areas have experienced similar and synchronous pre- and post-calving changes over the recent years9. In addition, recent observations highlighting the presence of the saltiest waters of the Adélie depression in CB suggest that large production rates of dense shelf water occur in the bay9,12. Based on past expeditions, it has been suggested that the MG previously underwent similar calving events in the early part of the twentieth century13. However, these sporadic observations are insufficient to reconstruct past MGT dynamics with a high level of confidence.

In the present study, we provide a detailed reconstruction of surface and bottom oceanic conditions in the MGP over the last 250 years. This reconstruction is based on high-resolution analyses of diatom assemblages, diatom-specific biomarkers and major element abundances along a well-dated interface sediment core retrieved in January 2010 at CB (Fig. 1a; 66°54,38′ S—142°26,18′ E; 775 m depth). This study represents the first detailed assessment of the MG-MGP system dynamics over the last few centuries, and therefore provides essential information on how the system recovers after major perturbations such as calving events. We also evaluate the impact of the recent positive shift in the Southern Annular Mode (SAM) on MGP surface conditions through a century-long atmospheric reanalysis.


Multidecadal trends of sea surface conditions

Variations of Fragilariopsis cylindrus populations and di-unsaturated highly branched isoprenoid (HBI) lipid [HBI:2] abundances characterize spring sea ice occurrence14,15, while summer open ocean conditions are inferred from high abundances of open water diatoms16 (see Methods section). Titanium (Ti) content is used here to infer changes in terrigenous supply to the ocean17, thus reflecting the variability of the terrigenous delivery by glacial melting, the dominant process in Antarctic coastal areas at such timescale18,19. High (low) relative abundances of open water diatoms are concomitant with high (low) contents of Ti and, conversely, with low (high) relative abundances of F. cylindrus and low (high) concentrations of [HBI:2] (Fig. 2). Minimum abundances of [HBI:2] and F. cylindrus associated with maxima of open water diatoms and Ti during 1740–1760, 1800–1845 and 1880–1915 periods (Fig. 2), therefore indicate the presence of a well-developed polynya characterized by low SIC during the winter, early spring sea ice retreat and long summer season. The presence of a well-developed MGP promoted intense sea ice formation during winter and enhanced brine-induced convection. Variations in bottom current velocities were estimated from changes in sediment grain size inferred from Zirconium versus Rubidium (Zr/Rb) relative abundances20. Assuming that greater deep-reaching convection is associated with intensified bottom currents, the high Zr/Rb ratios (Fig. 2) recorded during periods of well-developed MGP suggest enhanced bottom currents favouring a coarse sedimentation at the core location. In contrast, the 1760–1800, 1845–1880 and 1915–1960 periods are characterized by maxima in [HBI:2] and F. cylindrus relative abundances and minima in open water diatoms, Ti and Zr/Rb records (Fig. 2). This reflects the presence of heavier sea ice conditions in spring, leading to shorter growing seasons and cooler summers, associated with reduced inputs from glacial runoffs and melting. During these intervals, a reduction of the MGP area and sea ice production coincided with a weaker bottom circulation, as revealed by the presence of finer (low Zr/Rb) sediments. Our records therefore suggest that since the mid-eighteenth century, surface ocean conditions and MGP activity alternated between periods of high sea ice presence and periods of prolonged open ocean conditions.

Figure 2: Sea ice and ocean conditions in CB over the last 250 years.
figure 2

Sea ice proxies: standardized concentrations of HBI:2 (light blue) and relative abundances of F. cylindrus (dark blue). Open water proxies: standardized relative abundances of open water diatom group (red) and titanium content (orange). Bottom current variability: standardized Zr/Rb ratio (green). Black curves represent the low-pass-filtered data, with a cutoff frequency at 1/32 (in year). The blue shadings indicate decades following each calving event with marked increase in SIC in the CB area.

Cyclic pattern

These multidecadal trends of the MG-MGP system are further characterized by a strong asymmetric evolution with sharp increases in SIC at ~1760, ~1845 and ~1915, followed by a slow decrease over the subsequent decades (Fig. 2). A similar sharp increase observed after the 2010 calving event (Fig. 1e) suggests that, at least for the past 250 years, these asymmetric oscillations (~70 years periodicity) are related to a series of large calving events. Each of these events probably induced a rapid closing of the MGP as the loss of the ice tongue allowed for sea ice transported within the East Wind Drift to enter the area.

This scenario is further supported by the wavelet analysis of our data set, which shows that all variables exhibit a common high power in the 60–80 year band, throughout the entire record (Fig. 3). Although such periods (60–80 years) are close to the limit of detection (the bottom of the cone influence), they are characterized by a high statistical significance level of the period (95%, according to ref. 21). In addition, in the 60–80 year band, a positive correlation, characterized by rightward pointed arrows, is shown by cross-wavelet analyses (see Methods section) between sea ice proxies (Fig. 3a) and between open water proxies (Fig. 3b). In contrast, as indicated by leftward pointed arrows, negative correlations occur in the 60–80 year band when comparing sea ice versus open water proxies (Fig. 3c–f). Interestingly, continuous wavelet transforms indicate that open water and sea ice diatom signals (Supplementary Fig. 1) exhibit an additional ~20–25 year cyclicity, which is absent from the geochemical proxies. Although the causes remain unclear, differences in the spectral pattern of diatom and geochemical records may be attributed to the origin of the proxies themselves. The [HBI:2] is synthesized by diatoms living within or attached to sea ice. As such, we expect a direct response of [HBI:2] to SIC and the timing of ice waning14. Sea ice-related diatoms such as F. cylindrus thrive at the sea ice margin while open water diatoms thrive in the water column. Therefore, we believe that diatoms respond to both the timing of sea ice waning and oceanic biotic and abiotic factors such as stratification, upwelling and the injection of warmer waters15,16,17, which are expressed at shorter timescales22,23.

Figure 3: Relationship between proxies and cyclicity of sea surface conditions in the MGP area.
figure 3

Cross-wavelet transform (XWT) on the sedimentary proxies (using Morlet wavelet and Monte Carlo methods21) between (a) [HBI:2] versus F. cylindrus; (b) Ti versus open water diatoms; (c) Ti versus F. cylindrus; (d) [HBI:2] versus open water diatoms; (e) open water diatoms versus F. cylindrus; and (f) [HBI:2] versus Ti. Statistically significant periods are identified by the black circled red zones. Rightward pointed arrows indicate positively correlated signals while leftward pointed arrows indicate negatively correlated signals. Yrs, years.

Barrier effect of the MG

Each calving event is characterized by relatively elevated abundances of the sea ice proxies for a couple of decades, followed by a slow decrease of the sea ice proxies and a concomitant increase of the open water proxies. These results suggest that each event was followed by a slow and constant re-advance of the glacier, but that a few decades are necessary for the tongue to reach a sufficient length to prevent sea ice advection in the area. As such, during few decades after 1800, 1880 and 1960 (Fig. 2), the tongue probably acted as a barrier and deflected the East Wind Drift pack ice northward, thus restoring favourable conditions for the establishment of the polynya. Although only limited observations exist to reconstruct the recent history of the MGP, it is clear that at least one major calving event occurred between 1912, when the Australasian Antarctic Expedition led by Mawson (1911–1914) measured a 150-km-long tongue from the grounding line, and 1958, when the Soviet Antarctic Expedition reported a 113-km-long tongue13. The sharp increase in sea ice proxies in 1915 strongly suggests that this event occurred only a few years after Mawson’s expedition. Given the mean growth rate of the tongue of ~1 km per year24, the glacier had presumably reached ~150–160 km at that time when it calved. This length is similar to the one reached by the glacier before the 2010 calving25,26 and is in line with Mawson’s observations in 1912. If the MGT lost half (80 km) of its length, similar to the 2010 calving event, it would have taken ~40 years for the tongue to grow back from ~80 km in 1915 to 113 km, based on the Soviet Antarctic Expedition in 1958. These results suggest that from the 1960, s, the ice tongue was then long enough to effectively act as a barrier for drifting ice. In the 1990s, signs of imminent calving were already detected with the formation of two major rifts near the glacier grounding line and the front of the glacier grounding on the Mertz Bank to the north13,25. The shallow bathymetry of the bank (Supplementary Fig. 2) enhances local tidal currents exerting lateral stress on the tip of the glacier, likely impacting the tongue along-flow velocity26. In addition, the presence of several icebergs released by upstream glaciers and grounded onto the Mertz bank13,26 probably further increases the lateral distortion of the tongue. As such, it appears that beyond a threshold of ~150–160 km, lateral stresses exerted on the sides and at the lie of the tongue lead to its rupture.

Recent changes in seasonality

Interestingly, the analysis of the upper sediment section show that while the MGT was sufficiently long to promote open water conditions in the lie of the glacier during the last 50 years, both [HBI:2] and F. cylindrus remained relatively abundant in the sediments (Fig. 2). In addition, Zr/Rb values did not show a marked increase as expected during this phase (Fig. 2). This suggests that, in contrast to previous cycles, pre-calving conditions over recent decades were characterized by a more persistent sea ice cover during spring and were associated with weaker bottom water circulation than observed during previous cycles. We also note higher Ti contents (terrigenous inputs) along with greater abundances of open water diatom species (and in particular large centric diatoms; Fig. 4), suggesting strong glacial melting and more persistent open water conditions led by warmer surface waters during summer over the recent decades. Warmer open water conditions during the summer are further confirmed by the large peak of a specific HBI isomer [HBI:3] during the past 40 years (Supplementary Fig. 3). High abundances of [HBI:3] in sediments reflect the contribution of phytoplanktonic-derived organic matter14, and thus indicate a higher phytoplankton productivity during the summer (Supplementary Note 1). Overall, these results therefore provide strong evidence for changes occurring over the growing season in recent decades. From our records, this apparent shift in seasonality is characterized by cooler and icier springs, warmer and more open summers in line with recent atmospheric and oceanic observations from other areas in the Southern Hemisphere22,27.

Figure 4: Atmospheric forcing and impacts on the sea ice free season during the instrumental period in the MGP area.
figure 4

Evolution of the SAM according to the reconstructed Marshall index (blue, annual values and black, 11 years moving average) over the last 250 years31. Open water proxies: standardized relative abundances of T. antarctica sp (pink), large centric diatom group (yellow; see Methods section for species composition) and F. kerguelensis (orange). The blue shadings indicate decades following each calving event with marked increase in SIC in the CB area.


Our results strongly suggest that surface oceanic conditions and dense shelf water production are closely related to the MGP presence and activity. Reasons for the ~70 years cyclicity of the MGP are still not fully understood but, given the major constraints of the local topography, it is likely that these cycles are set by the rate of advance and along-flow velocity of the MG. However, according to several studies13,25, icebergs released from upstream outlet glaciers (for example, Ninnis Glacier) could have impacted the stability of the MGT when they grounded and/or passed through the area. In addition, when the tongue is too short to constitute a barrier, these icebergs can impact the regional oceanography for several years, leading to a temporary increase in sea ice conditions, as observed since 2010 with the presence of the B09B iceberg in front of CB (Fig. 1c,d). The resolution of our records, however, does not allow us to capture such phenomena, if they ever occurred in or around CB in the past. Our data also indicate a close relationship between the MG history and MGP dynamics between 1740 and 1960. However, since the 1960s, our records suggest unexpectedly cool and icy springs at a time where the MGT should have reached a sufficient length to promote the presence of a well-established MGP.

We propose that, superimposed on the large multidecadal oscillations generated by the MG dynamics, additional factors contributed to modulating sea surface conditions in the area. The SAM, principal mode of atmospheric variability over the Southern Ocean28, has shown a steadily increasing index over the last 50 years (refs 27, 29; and Figs 4 and 5a), with a more positive trend in summer27,30. Reconstructions indicate that this increase is unprecedented over the last few centuries31 possibly due to ozone depletion and a rise in greenhouse gases29,32, and recent investigations have argued that such trend had a direct influence on sea surface conditions in several regions around Antarctica through modulation of the wind pattern22,23,29,33,34,35. The recent positive trend in the SAM index is indeed associated with an intensification of the polar vortex32 leading to a southward shift of enhanced circumpolar westerlies28. This, in turn, led to a more intense Antarctic Circumpolar Current (ACC)35 and associated ocean eddy activity36. We postulate that such large-scale changes impacted the sea ice distribution in spring, modified the summer off-shelf ocean circulation due to changes in the large-scale wind stress pattern and are the dominant cause for the contrasted response of the Adélie Land continental shelf over the last 50 years.

Figure 5: Evolution of the SAM and of the wind pattern over the Adélie-George V Land since the nineteenth century.
figure 5

(a) Standardized values of SAM index (5 years running mean; blue), computed in the 20CR reanalysis following ref. 70 and the total wind direction angle at 2 m (green; °) computed in the red box of the lower panel using the same reanalysis. The North direction indicates the 0° modulo 360° and the angle is counted positively clockwise. (b) Annual mean wind speed from 20CR reanalysis averaged over the period 1871–2010. The red box indicates the study area where the wind have been computed in a.

Indeed, several studies have evidenced a close link between the planetary circulation in the southern polar atmosphere and the katabatic wind regime, the latter being part of the large-scale meridional tropospheric circulation over Antarctica37,38,39,40. Observations in East Antarctica revealed that an intensified tropospheric vortex was associated with weakened katabatic winds over the Antarctic margin40, and analysis of the atmospheric wind fields during the last 140 years from the twentieth century reanalysis (20CR) reanalysis41 confirms a significant westward shift of the wind pattern in the George V Land over recent decades (Fig. 5a, green curve; and Supplementary Note 2). A weakening of the meridional wind circulation and thus increasing zonal circulation over the last decades as suggested by refs 40, 42 have also been observed in the region34,43. Indeed, at seasonal to inter-annual timescales, sea ice conditions in the MGP area have been shown to be sensitive to the latitudinal location of the Antarctic Circumpolar Trough and associated to more along shore wind transport34,43. In the present scenario, reduction of katabatic winds intensity over the MGP area would weaken the northward transport of sea ice, resulting in the retention of more ice within the area. The latter would delay the onset of sea ice melt in spring in agreement with higher sea ice proxies in our record since 1960. Although based on a restricted number of data points, a reduction of sea ice proxies in the uppermost sediment sections suggests a recent tendency towards a more reduced sea ice cover in spring, which is in line with the recent analysis of the sea ice seasonality in the area using the satellite records44.

Our data also indicate warmer sea surface conditions during summer over recent decades. As recently observed in several Antarctic regions, it is argued here that intrusions of warm Circumpolar Deep Water (CDW) onto the continental shelf promoted open water conditions and higher sea surface temperatures7,23,33,45. Increasing CDW contribution onto the Antarctic Peninsula shelf was linked to the recent changes in the strength of the SAM46. Indeed, modelling studies have shown that advection of CDW onto the Antarctic continental shelf is linked to enhanced upwelling southward of the ACC, promoted by a southward shift and strengthening of the Southern Ocean Westerlies35,47. Surface wind stress curl calculated from the 20CR reanalysis indeed suggests long periods of strong positive trend in upwelling-favourable vertical velocities with positive values starting roughly after 1950, concomitant with the SAM trend (Supplementary Fig. 4 and Supplementary Note 2). In the Mertz region, in contrast with West Antarctica, flooding of the shelf by the CDW occurs as synoptic weather timescale intrusions rather than as a continuous flow7. However, the proximity of George V Land continental shelf to the southern ACC boundary facilitates transport of CDW into the Mertz region48, as suggested in other Antarctic areas23, providing that adequate dynamical forcing exists to drive this water mass on the shelf. According to ref. 49, a number of mechanisms involving interaction of the zonal flow with the topographic troughs disseminated along the Antarctic shelf break are likely to favour such transport. While some of these may be linked to the internal variability of the flow50, some would be the result of enhanced wind-driven zonal flow. We note that, off the Adélie Land shelf, a more zonal wind pattern in the 20CR reanalysis (Fig. 5) over recent decades was concomitant to the southward shift (Supplementary Fig. 5) and the strengthening35,47 of the Westerlies at mid latitudes. Increasing zonal wind circulation poleward may have contributed to accelerate the westward flowing Antarctic Slope Current, the southern branch of the Australian Antarctic Basin cyclonic circulation51,52, thus favouring the inflow of CDW through nonlinear momentum advection onto the shelf trough. Recent observations suggest that a weaker and more zonal circulation promote uplift and enhanced onshore intrusion of CDW45, and studies attributed an increased abundance of terrigenous particles in the sediments to enhanced melting of both continental and sea ice during periods of increased advection of warm CDW onto the shelf17,18,19,53. The high terrigenous content recorded in CB2010 since 1960 (Fig. 2) can therefore be interpreted as a result of enhanced melting of regional glaciers in response to increased advection of warm CDW onto the shelf. This enhanced melting of glacial ice could also be contributing to further freshening the ALBW as reported by Lacarra et al.9

Our results demonstrate that, in response to glacial dynamics and local physiography, recurrent massive calving events of the MG occurred over the last 250 years. These events had profound impacts on ocean surface conditions and dense water production of the downstream polynya. Taking into consideration that many of these glacier-polynya systems are disseminated around Antarctica4 and that dense shelf water is ultimately a precursor of AABW, whose impact on large-scale ocean circulation is well known1,2, our study provides evidence that local processes may contribute to alter global ocean and climate systems. In contrast to previous cycles, our data indicate that during the last 50 years, the region was experiencing a more compact sea ice cover, a larger supply of glacial meltwater and a slowdown of bottom currents. These results suggest a reduction of dense water production and are consistent with the long-term freshening of the ALBW observed in the Australian Antarctic Basin since the late 1960s (refs 54, 55). This contrasted response of the MGP region during the last Mertz cycle may just be a transitory phenomenon as the SAM increase over that period is thought to be partly due to ozone depletion in the polar vortex. Since studies are predicting that the ozone hole will replenish in the future decades56, natural multidecadal glacier cycles such as those identified in our records are likely to take over.


Sediment material and chronology

A 30.5-cm-long interface core was retrieved aboard the R/V Astrolabe (66°54.38′ S; 142°26.18′ E; 775 m water depth) during the 2010 COCA cruise. Positive X-ray images performed on the SCOPIX image-processing tool57 gave detailed information on sediment density and structure. SCOPIX images revealed that, in contrast to high accumulation sites from Dumont d’Urville Trough, sediments from CB were massive with no signs of laminations. The core was sampled continuously at 0.5 cm resolution and its chronological framework was determined based on 210Pb excess (210Pbxs; T1/2=22.3 years), which is rapidly incorporated into the sediment from atmospheric fallout and water column scavenging. The activities of 210Pb and 226Ra were measured on dried sediments by non-destructive gamma spectrometry using a well-type, high-efficiency low-background detector equipped with a Cryo-cycle (CANBERRA). Activities are expressed in mBq g−1 and errors are based on 1 s.d. counting statistics (Fig. 6). 210Pbxs was determined by subtracting the activity supported by its parent isotope, 226Ra, from the total 210Pb activity in the sediment. Mass accumulation rate (0.025 g cm−2 y−1) was calculated from the sedimentary profiles of 210Pbxs, plotted against cumulative mass. The deposition time (in years) was obtained by dividing the cumulative dry mass per unit area by mass accumulation rate. The deposition year for each sediment layer was subsequently estimated based on the 2010 sampling date for the sediment–water interface.

Figure 6: CB2010 chronology.
figure 6

CB2010 age model (dark line) based on 210Pb excess (210Pbxs) and associated age-model errors (grey area). The inset corresponds to the down-core profile of 210Pbxs (error bars correspond to 1 s.d.).


Micropaleontological analyses were performed according to the methodology described in ref. 58. For each sample, 300–350 diatom valves were counted and data are presented as species relative abundances. Briefly, diatom identification was performed to the species or species group level at a ~5-year resolution. Sixty-eight diatom species were identified in down-core assemblages, from which only a dozen species presented abundances higher than 2% of the total diatom population. Only these species were considered relevant for reconstructing environmental changes. Diatom species or species groups we confront here experience similar ranges of variability in CB2010, ~2.5–13% for F. cylindrus, ~1–9% for F. kerguelensis and ~0–7% for the large centric group and Thalassiosira antarctica abundances, respectively (Supplementary Fig. 6).

F. cylindrus is one of the most common diatoms found along the Adélie Land margins59 as it thrives within stratified sea ice-covered waters15. Large abundances of F. cylindrus in sediments indicate the presence of a sea ice cover persisting over 7.5 months per year15. In contrast, the open water diatom assemblage, composed by F. kerguelensis and large centric diatoms, characterizes open water conditions during summer16.

F. kerguelensis dominates assemblages of the open ocean zone south of the Polar Front where sea ice is absent during summer60. Similarly, high abundances of large centric diatom species, such as T. lentiginosa or T. oliverana, commonly occur in the Southern Ocean south of the Polar Front in areas characterized by permanent open ocean conditions16,61. Relative abundances of T. lentiginosa show an inverse relationship with sea ice cover with high occurrences between 0 and 4 months of sea ice presence per year and a decline towards prolonged sea ice duration16. T. oliverana is clearly dominant in locations where open ocean conditions to sea ice edge during summer occur16. T. antarctica has been described as a dominant species within diatom assemblages in non-stratified or weakly stratified Antarctic surface waters62. T. antarctica blooms in open waters during summer–autumn, and produces resting spores at the end of the growing season when sea ice returns63. T. antarctica resting spores, the main form encountered in sediments, is most abundant in regions where sea ice is present for at least 6 months per year, and is believed to be induced under nutrient-stressed conditions or low light intensities15.

Geochemical data

Few marine and freshwater diatoms belonging to Haslea, Navicula, Pleurosigma and Rhizosolenia genera were recently found to be synthesizing HBIs14,64. A di-unsaturated isomer [HBI:2] has been identified in Antarctic sea ice and isotopic analyses provide evidence for that this isomer to be synthesized by sea ice dwelling diatoms. In contrast, tri-unsaturated HBI isomers [HBI:3] have been identified in water column phytoplankton14. Recent studies have proposed the use of [HBI:2] and [HBI:3] to reconstruct variations of Holocene Antarctic sea ice duration as complementary sea ice proxy to diatom counts65. Biomarker analysis followed the technique described by ref. 14 and were performed every 0.5 cm through the core. Briefly, an internal standard was added to the freeze-dried sediments, lipids were extracted using a dichloromethane/methanol mixture to yield a total organic extract, which was then purified using open column chromatography (silica). Hydrocarbons were analysed using a gas chromatograph coupled to a mass spectrometry detector.

Ti and Zr are considered to be direct indicators of terrigenous inputs as these elements are not involved in biological cycles17. In the literature, variations in Ti content are largely used to infer past changes in terrigenous supply to the ocean17. Microfabric analysis of sediment in the Mertz-Ninnis and Adélie troughs show that both terrigenous content and Ti content are low in spring laminae and increase over the growing season (when open water diatoms dominate the siliceous assemblage) and during which the summer glacial melting is high17,53,66. Indeed, in Antarctic coastal areas, delivery of terrigenous particles is possible via several dominant modes as meltwater discharge, ice rafting, runoff from outlet glaciers and aeolian transport, although this latter source is considered negligible in coastal East Antarctic regions17,18,19. Variations in Zr to Rb content ratio track changes in sediment grain size, where Zr represents the coarsest sediment fraction and Rb represents the finest20. Ti, Zr and Rb contents were measured on slab sections at a 2 mm resolution along the entire core using an AAVATECH XRF core-scanner67.

Satellite data

Daily SICs for the time period 1978–2012 were obtained from the National Snow and Ice Data Center data repository. The data set is based on passive microwave observations from the Nimbus-7 SSMR (1978–1987), DMSP SSM/I (1987–2007) and SSMIS (2007–2012) radiometers processed with the NASA Team algorithm68 at a spatial resolution of 25 × 25 km. Averaged concentrations were calculated over two specific domains, CB and the entire MGP domain (Fig. 7). Daily anomalies were calculated using the average of the pre-calving 1978–2009 period and then low-pass filtered using a 3-month moving average (Fig. 1e). SIC data were standardized. Anomalies represent differences between the daily value and the mean daily value calculated over the reference period.

Figure 7: Pixels locations for extraction of SICs.
figure 7

MODIS satellite image (2008/12/26) of the George V Land indicating the grid points used for the extraction of the daily SIC values: white star in a red circle indicates the core location; red spots correspond to the CB area and green spots represent the MGP area.

Spectral analysis

Unlike many traditional mathematical methods (for example, Fourier analysis), the wavelet approach can be used to analyse time series that contain non-stationary spectral power at many different frequencies21. For geological time series, although visual comparison of plots is commonly used, cross-wavelet analysis permits detection, extraction and reconstruction of relationships between two non-stationary signals simultaneously in frequency (or scale) and time (or location)69. The continuous wavelet transform (CWT; Supplementary Fig. 1) of time series is its convolution with the local basis functions, or wavelets, which can be stretched and translated with flexible resolution in both frequency and time. The principle of cross-wavelet analysis and the complete method we used are described in ref. 21. We used the MATLAB package for cross-wavelet analysis written by Grinsted et al.21 and applied the Morlet wavelet as the mother function on our data set. This method provides a good balance between time and frequency localization, and we used Monte Carlo simulations to provide frequency-specific probability distribution (global wavelet spectrum) that can be tested against wavelet coefficients. Statistical significance was estimated against a red noise model21. In this study, to test the relevance of our proxies, their statistical relationships and to examine periodicities in a frequency domain, we compared the two time series by their CWTs, which we hypothesized are linked in some way. The resulting cross wavelet transform (XWT, Fig. 3) exposed their common power and relative phase in time–frequency space of the two signals. Data were previously standardized, which did not introduce any change in the shape of the records but normalized the amplitude of the variations (Supplementary Fig. 6).

Atmospheric reanalysis

To analyse the Southern Hemisphere atmospheric circulation during the last 140 years, we used the recent 20CR Project version 2 (ref. 41), consisting of an ensemble of 56 realizations with 2° × 2° gridded 6-hourly weather data from 1871 to 2010. Each ensemble member was performed using the NCEP/GFS (National Center for Environmental Prediction/Global Forecast System) atmospheric model, prescribing the monthly sea surface temperature and sea ice changes from HadISST as boundary conditions, and assimilating sea level pressure data from the International Surface Pressure Databank version 2 ( We used the ensemble mean to perform our analysis. An important caveat concerns the fact that few data were assimilated at the beginning of the reanalysis in the Southern Hemisphere, owing to the lack of available observations. Nevertheless, this product is one of the best data sets available for the evaluation of atmospheric circulation changes at a large scale in the Southern Hemisphere. Wind speed products were plotted over the Terre Adélie-George V Land (Fig. 5) and the offshore region ~55–60°S (Supplementary Fig. 5).

Additional information

How to cite this article: Campagne, P. et al. Glacial ice and atmospheric forcing on the Mertz Glacier Polynya over the past 250 years. Nat. Commun. 6:6642 doi: 10.1038/ncomms7642 (2015).