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        High-resolution ice cores from US ITASE (West Antarctica): development and validation of chronologies and determination of precision and accuracy
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        High-resolution ice cores from US ITASE (West Antarctica): development and validation of chronologies and determination of precision and accuracy
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Abstract

Shallow ice cores were obtained from widely distributed sites across the West Antarctic ice sheet, as part of the United States portion of the International Trans-Antarctic Scientific Expedition (US ITASE) program. The US ITASE cores have been dated by annual-layer counting, primarily through the identification of summer peaks in non-sea-salt sulfate (nssSO4 2–) concentration. Absolute dating accuracy of better than 2 years and relative dating accuracy better than 1 year is demonstrated by the identification of multiple volcanic marker horizons in each of the cores, Tambora, Indonesia (1815), being the most prominent. Independent validation is provided by the tracing of isochronal layers from site to site using high-frequency ice-penetrating radar observations, and by the timing of mid-winter warming events in stable-isotope ratios, which demonstrate significantly better than 1 year accuracy in the last 20 years. Dating precision to ±1 month is demonstrated by the occurrence of summer nitrate peaks and stable-isotope ratios in phase with nssSO4 2–, and winter-time sea-salt peaks out of phase, with phase variation of <1 month. Dating precision and accuracy are uniform with depth, for at least the last 100 years.

1. Introduction

The International Trans-Antarctic Scientific Expedition (ITASE) program is an international effort to improve our spatial picture of the Antarctic ice sheet. ITASE places emphasis on the surface and near-surface characteristics of the ice sheet, complemented by deep ice radar profiling and atmospheric sampling at altitudes upwards of 20 km. The first phase of the United States’ effort has focused on the West Antarctic ice sheet (WAIS), and has completed four field seasons comprising oversnow traverses that included ice coring, atmospheric sampling, surface horizontal and vertical velocity measurements, and radar observations of near-surface stratigraphy, ice-sheet internal layering and bed topography. The traverses covered a total distance of >5000km and comprise an unprecedented sampling of the Antarctic ice sheet that, when combined with data from other ITASE projects, will result in a comprehensive spatial and temporal map of Antarctic climate, atmospheric chemistry and ice-sheet surface mass balance.

As part of US ITASE, ice cores were obtained from 23 sites across the WAIS, between the Antarctic Peninsula, South Pole and the Ross Sea and Amundsen Sea ice drainages. At 21 of these sites, cores reaching to depths between ~50 and ~300m were obtained, providing continuous records of snow chemistry covering at most sites at least 200 years, a benchmark time frame in the original ITASE implementation plan (Mayewski and Goodwin, 1996). These cores greatly expand the inventory, and widen the spatial coverage, of ice-core records available from earlier projects in West Antarctica, which include the long ice cores at Byrd (Johnsen and others, 1972) and Siple Dome (Taylor and others, 2004a), and shorter records from Siple Station and Dyer Plateau (Mosley-Thompson and others, 1990; Thompson and others, 1994) and in the Ross Ice drainage area (Kreutz and others, 2000a).

Ice-core records of past snow properties and near-surface atmospheric chemistry are widely used as proxy records of past climate conditions and as constraints for ice-sheet surface mass balance and ice deformation studies. The importance of obtaining multiple ice cores is that a single ice core, like a single weather station, will be representative only at some local or regional spatial scale, depending on the timescale of interest. This is particularly true in West Antarctica, because the spatial coherence of interannual climate variability is relatively small, and ice-sheet topography is sufficiently complex that there may also be significant microclimatic effects. Results from recent deep coring projects suggest that on longer timescales as well, significant climate changes appearing in one location in WestAntarctica may not necessarily be felt at another (e.g. Siple Dome vs Byrd; see Taylor and others, 2004a). In contrast, the East Antarctic ice sheet appears to be quite uniform on both short (Schneider and Steig, 2002; Schneider and others, 2004) and long timescales (Jouzel and others, 2001; Watanabe and others, 2003).

The use of multiple ice cores and the measurement of multiple parameters can provide complementary information about the atmospheric and surface conditions that are being sampled. Consistently accurate and precise dating of ice cores is critical to the success of this approach. Placing Antarctica in the context of global climate variability requires ice cores that can be rigorously calibrated against direct meteorological observations on the same timescales. In this paper, we discuss the methods used for developing depth vs age relationships for the US ITASE cores, and we quantify the accuracy and precision of the resulting chronologies through several independent methods. Application of the resulting, highly resolved records to climatological and ice-sheet surface studies, based on these results, is the subject of several other papers (e.g. Dixon and others, 2004; Kaspari and others, 2004, 2005; Rick and Albert, 2004; Spikes and others, 2004; Schneider and others, 2005).

2. Site Selection, Ice Coring and Analysis

West Antarctica has the specific advantage over East Antarctica as an ice-core drilling location that snow accumulation rates are generally high (>8 cm ice equivalent; e.g. Vaughan and others, 1999). However, West Antarctic temperatures are high enough at lower elevations that problems associated with surface melting or diffusive changes of chemical properties may be a concern. Selection of coring sites took this into account and traverse routes were therefore restricted largely to the high-plateau portion of the WAIS. Some areas were avoided for purely logistical reasons, most importantly the presence of crevasses. Target coring depths were chosen with the goal of obtaining at least 200 years of climate history from each core, combined with efficiency of field operations. In practice, this meant that we obtained deeper cores (>60 m) only where it was deemed necessary due to the high accumulation rates, though at selected sites longer records were obtained. Core locations are shown in Figure 1. Elevations, latitudes and longitudes of the US ITASE cores specifically discussed in this paper are given in the figure captions. Additional details on core depths and locations for all the US ITASE cores are archived at the US National Snow and Ice Data Center (www.nsidc.org).

Fig. 1. Map of West Antarctica showing the location of US ITASE cores collected between 1999 and 2003. Locations specifically discussed in the text are named and shown by white circles with crosses.

Cores were retrieved using two different mechanical drilling systems. For the main ice core at each site, we used an Icefield Instruments EclipseTM drill that obtains 1m sections of 82mm diameter cores. The drill was mounted on a sled and transported by snowmobile as a field-ready unit, saving drill set-up time. The Eclipse has the disadvantage of requiring that firn be excavated to allow space for the vertically swinging drill arm; thus the upper 1m of snow cannot be sampled with the drill. In the first two field seasons we sampled the upper 1–2m separately, after excavation for drill access, to obtain a continuous record up to the surface. In the third and fourth seasons we replaced firn-pit sampling with shallow coring, using a new system from Glacier DataTM. The Glacier Data design is similar to that of the Eclipse but is considerably lighter and can drill directly from the surface; 50mm diameter cores are obtained. We tested this drill to 40m depth at Byrd Station and are confident that it can achieve much greater depths. Details on the drill designs are available from Icefield Instruments (www.icefield.yk.ca) and Glacier Data (www.glacierdata.com) respectively.

Core loss

In general, the 82mm cores were packaged in the field and sampled later at the US National Ice Core Laboratory in Colorado; the 50mm cores were either analyzed on-site or subsampled in the field and placed in cleaned sample containers, kept frozen until ready for analysis in the laboratory. All sampling was done by a team wearing Tyvek clean suits, masks and polypropylene gloves to prevent contamination. In the laboratory, established procedures were followed for clean chemical sampling using melter headsdesigned to separately sample the outside and inside of the core. Concentrations of hydrogen peroxide, formaldehyde and selected major ions were measured by continuous flow analysis using the fluorescence or photometric detection methods (Röthlisberger and others, 2000) at the University of Arizona; stable-isotope concentrations (δ18O and δD) were analyzed by mass spectrometry using CO2 equilibration and Cr reduction at the University of Washington; all other geochemical measurements were conducted at the University of Maine using ion chromatography. Details of the sampling and measurement procedures used are given in Buck and others (1992) and Frey and others (in press).

3. Establishment Of Depth–age Relationships From Seasonal Variations

Figures 2 - 6 show selected geochemical profiles from three sites (US ITASE 2000-1, 2000-4, and 2001-5) to illustrate the most important findings with respect to ice-core dating at US ITASE sites in West Antarctica. Other core profiles are similar and support the conclusions derived from these examples. We refer to these figures in this and in subsequent sections of the paper.

Fig. 2. Profiles of non-sea-salt sulfate (nssSO4 2–), nitrate (NO3 ) and oxygen isotope ratios (δ18O) in US ITASE core 2000-1, from 1981 to 2001. Note the distinct rise in sulfate levels beginning in 1991/92, due to the Pinatubo eruption. Dashed lines are for reference and show 1 January of selected years.

Fig. 3. Same as Figure 2, but for US ITASE core 2000-4, and also showing surface temperature from the Advanced Very High Resolution Radiometer (AVHRR) satellite. Arrows show suggested correlations between mid-winter warming events and mid-winter isotope (deuterium/hydrogen = δD) anomalies.

Fig. 4. Same as Figure 3, but for US ITASE core 2001-5, and showing sodium concentrations (Na+) in place of nitrate. Arrows show suggested correlations between mid-winter warming events and mid-winter oxygen isotope anomalies.

Fig. 5. Same as Figure 4, but showing the years 1808–30 in US ITASE core 2001-5, and showing NO3 in place of Na+, and showing magnesium concentrations (Mg2+) in the bottom panel. Cross on right side of upper panel shows mean and standard deviation of SO4 2– concentrations measured in fresh snow during summer at core site 2001-6. Note significantly elevated sulfate levels in ~1816–17, due to the Tambora eruption, and in 1810–11.

Fig. 6. Oxygen isotope (δ18O) record from US ITASE core 2000-2. Dashed line is measured data; bold line shows 19-point smoothed data. Arrows show inferred annual summer peaks between the surface (2001) and the depth of the radar reflector, independently attributed to the year 1991 from correlation with US ITASE core 2000-4.

For the relatively high-accumulation sites we selected, geochemical and physical properties of the US ITASE cores show that there is excellent preservation of seasonal cycles in virtually all geochemical parameters and in grain-size variations that mark the transitions from summer to fall and winter to spring. This is a prerequisite for obtaining high-quality timescales. We also found that agreement between results from the 82mm ice cores, which generally start ~1m below the surface, and from the overlapping shallower snow pits and 50mm cores, is excellent. Exceptions to the general rule of unambiguous seasonal indicators in the US ITASE cores are:

  • 1. at the lowest-elevation/warmest sites (1999-1 and 1999-2), diffusion of the more mobile species, notably hydrogen peroxide (H2O2), water stable-isotope ratios (δ18O, δD) and nitrate (NO3 ), preclude the detection of seasonal cycles in these species beyond the upper ~10m of firn;

  • 2. at most sites, we found that wind crusts in the physical stratigraphy were not reliably correlated with other indicators of annual snow accumulation; in general, we found more than one such layer in most years.

We established initial age vs depth relationships for the US ITASE cores through the identification of seasonal peaks from all the major geochemical time series considered together (SO4 2–, Na+, Ca2+, Cl, Mg2+, K+ and NO3 ), coupled with visual stratigraphy, but not including stable-isotope ratios and hydrogen peroxide. In practice, we find that the least ambiguous seasonal variations are in the sulfate concentrations, and in particular the derived parameter nssSO4 2– (non-sea-salt sulfate, also referred to as ‘excess sulfate’, determined by applying a standard sea-water ratio of 30.61 (Na+), 1.1 (K+), 3.69 (Mg2+), 1.16 (Ca2+), 55.04 (Cl) and 7.68 (SO4 2–) to the ion concentrations in each sample; see O’Brien and others (1995) and Dixon and others (2004) for details). Sulfate deposition in West Antarctica reflects both sea-salt and non-sea-salt sources, with a strong altitude dependence on their relative importance. At lower elevations, the biogenic-source SO4 2– fractions may overwhelm volcanic signals. This appears to be important at Siple Dome (elevation 600 m), which when combined with the rapid diffusion of stable isotopes (Cuffey and Steig, 1998) and somewhat ambiguous visual stratigraphy, has made dating to the interannual level problematic at this site (Taylor and others, 2004b). In the case of the US ITASE cores, there is a fairly small difference between the SO4 2– and nssSO4 2– data; however, using the latter has the advantage of narrowing the width of the seasonal maxima, and of accentuating anomalously large peaks that are identified with large, globally significant explosive volcanic events.

On the basis of two independent influences on seasonal sulfate concentrations, we assigned the nssSO4 2– peaks to earlysummer (nominally 1 January) of each year (Figs 25). The primary source of nssSO4 2– is the oxidation of various sulfur compounds beginning with dimethyl sulfide (DMS) which is produced by phytoplankton, with blooms generally beginning in December as sea-ice melt-induced surface water stratification becomes established, and peaking in early January (Arrigo and others, 1999; Kettle and others, 1999). The secondary source for nssSO4 2– is input from the upper troposphere and lower stratosphere, representing both volcanic inputs, and anthropogenic and additional biogenic sulfur from extrapolar regions (Delmas, 1982; Legrand and Mayewski, 1997). The peak input of this secondary source is also expected to occur in early austral summer, due to the spring-time break-up of the polar vortex. In addition to this a priori reasoning, numerous ice-core studies support the assignment of the nssSO4 2– peak to early summer (Whitlow and others, 1992; Wagenbach and others, 1998; Kreutz and Mayewski, 1999). Also, measurements of optical depth from the atmosphere at South Pole place the maxima precisely in early January (Bergin and others, 1998). Finally, we note that nssSO4 concentrations in fresh snow from a late December snowstorm in 2001, near site US ITASE 2001-6, are indistinguishable from the typical ice-core nssSO4 maxima (Fig. 5).

4. Accuracy Of Timescales

Having established timescales for the cores that are based on seasonal variations alone, with nssSO4 2– providing the nominal assignment of calendar dates, i.e. time of year, we used several independent measures to validate the timescales. The validation procedures provide a means to estimate both the precision and accuracy of the timescales.

The identification of volcanic marker horizons provides a particularly important validation tool. In each of the US ITASE cores that have been analyzed for sulfate concentrations (US ITASE 1999-1, 2000-1, 2000-4, 2000-5, 2001-2, 2001-3, 2001-5) and in several additional West Antarctic cores, Dixon and others (2004) identified elevated nssSO4 2– levels at times consistent with the known dates of eruption of the following volcanoes (dates given in parentheses): Tambora, Indonesia (1815); Cosiguina, Nicaragua (1835); Krakatau, Indonesia (1883); Agung, Indonesia (1963); Pinatubo, Philippines, and Cerro Hudson, Chile (1991). An ‘unknown’ event, which has an established age of 1808/09 from Greenland ice cores and other evidence (Zielinski and others, 1994; Chenoweth, 2001), was also identified. Specifically, elevated levels of nssSO4 2– begin in 1810, 1816, 1837, 1885, 1964 and 1992. These ages, from the independent layer counting, are consistently 1–2 years after the eruption date of the volcanoes assigned to them, consistent with the typical stratospheric transport time across the circumpolar vortex. For the most recent volcanoes, we know from satellite observations that the stratospheric SO4 2– clouds from Cerro Hudson and Pinatubo were centered over the South Pole in September and November 1991 (Cacciani and others, 1993; Saxena and others, 1995). Because the seasonal cycle in SO4 2– begins to rise in September, it is difficult to demonstrate that the volcanic signal is registered precisely at the expected time. However, the background levels clearly begin to rise no earlier than 1991 and no later than 1992 in all cores (Figs 24), and the most prominent summer peak in all of the cores, after the 1964 peak attributed to Agung, occurs in January 1992.

On the basis of the seasonal ion-chemistry data and the volcanic marker horizons, a conservative estimate for the absolute dating accuracy for the US ITASE cores is < ± 2 years. Strictly, this applies only at the times of the identified horizons. A concern that arises in assigning this value to the entire length of the cores is the possibility that, while the length of time between different volcanic horizons may be correct, there may be some timescale variation within these intervals that is greater than 1 year, particularly for the longer interval 1886–1963 when no volcanic horizons were identified. Indeed, in examining the δ18O record from site 2001-5, we noted one year (1893) in which there appeared to be a ‘missing’ δ18O annual cycle. Subsequent review of the nssSO4 2– profile also showed a weak nssSO4 2– peak at this time, suggesting that this year may have been misidentified as a summer peak. No such differences were observed in the other cores analyzed. Based on this comparison, we consider the overall, absolute dating accuracy to be conservatively ± 2 years overall, and much better than ± 1 year in the most recent (last ~20 years) parts of the US ITASE cores.

We can further demonstrate that the relative dating accuracy is in general no worse than 1 year. In particular, this higher level of accuracy applies for all the cores at those depths at which volcanic horizons (or total beta measurements that reveal known atomic bomb test events) have been identified, since all of these horizons occur in the same year in all of the cores analyzed (Dixon and others, 2004). For two of the cores, we can further demonstrate a relative dating accuracy of ± 1 year throughout the entire length of the records. Spikes and others (2004) showed, using shallow radar stratigraphy, that it was possible to unambiguously trace lines from the 2000-4 site to the 2000-5 site and to obtain identical ages ± 1 year at each. Arcone and others (2005) have also traced layers between sites 2000-4 and 2000-2, and place the 1991 summer layer at 10.1m depth at 2000-2. While core 2000-2 remains to be processed for mostgeochemical measurements, from the stable-isotope profile (Fig. 6) we obtain 10.2m for summer 1991, amounting to a difference of ~1 month at this high-accumulation site (estimated 46 g cm–2 a–1 mean for the past decade). The hydrogen peroxide record also indicates a depth of 10.2m for late spring 1990 (Frey and others, in press).

Additional information from the stable-isotope and hydrogen peroxide concentrations further supports the estimated ± 1 year accuracy. Seasonal δ18O, δD and H2O2 cycles in these cores, which were not used in the original layer counting, provide an independent check on the assumption that the nssSO4 2– variations are seasonal. For most cores, the δ18O cycles are unambiguously seasonal through at least AD 1900, except for cores 1999-1 and 1999-2 where rapid isotope diffusion eliminates the seasonal variations at much shallower depths. In some cores the seasonal variations are detectable through the entire length (e.g. sites 2001-5 (Fig. 5) and 2002-4 (Jacobel and others, 2005). For the most recent 20 years, the stable-isotope ratios provide an especially robust indicator of accuracy, because of the strong link between stable-isotope ratios and temperature. Schneider and others (2005) show that the correlation between climatological monthly mean stable-isotope values in these cores and local monthly temperature anomalies from AVHRR satellite observations is r = 0.98. (The ‘climatological monthly mean’ is the mean of all Januarys, all Februarys, etc. for 1982–99.) There is a distinctive mid-winter warming period that appears at some sites in some years in the temperature records. We find that there are elevated isotope values at the corresponding sites in the correct years (Figs 3 and 4). Shuman and others (1995) found a similar correspondence in Greenland ice cores. We cannot demonstrate this for all the cores; in US ITASE core 2000-1, for example, diffusion has eliminated sub-seasonal variations. Importantly, though, while there are some years in which the isotope anomalies do not appear, there are no years in which the mid-winter isotope values are elevated without a corresponding mid-winter warming seen in the temperature records. This is particularly clear at the highest-accumulation site, in core 2001-5 (Fig. 4). These results indicate that the correct years have been identified with no uncertainty for at least the last 20 years, i.e. the length of the satellite records.

5. Precision Of Timescales

We now consider the dating precision of the US ITASE cores. By precision, in this context, we mean the uncertainty in correct assignment of calendar months for individual years in the records. The annual-layer counts are defined in terms of peak-to-peak intervals between nominally ‘summer’ values of geochemical measurements. In all cases, we used simple linear interpolation to define the timescale between these nominal 1 January values. The precision of the timescales thus depends on the precision of the assumptions (1) that the nssSO4 2– peaks actually coincide with 1 January and (2) that net snow accumulation is uniform throughout the year.

While there is no direct way to test these assumptions in the past, we noted above that there is independent evidence that the nssSO4 2– peaks in early January (Bergin and others, 1998), and that this timing reflects a combination of sea-ice melt and the break-up of the polar vortex. Analyses of sea surface DMS concentrations (Kettle and others, 1999), sea-ice variations (personal communication from C. Bitz, 2004), and stratospheric temperatures from US National Centers for Environmental Prediction (NCEP)/US National Center for Atmospheric Research (NCAR) re-analysis data (Waugh and others, 1999) indicate that all vary by <1 month, which would suggest that the maximum in nssSO4 2– peak also varies by about this amount except during volcanic events. We also have some direct evidence that it is reasonable to attribute the midpoint in seasonal nssSO4 2– to ‘winter’ (nominally 1 July by linear interpolation). As shown in Figures 4 and 7, maxima in sodium (Na+) and minima in hydrogen peroxide (H2O2) and stable isotopes all occur within 1–2 months of the nominal midpoint of the year, consistent with previous observations suggesting these are all winter signatures. As noted above, the occurrence of some mid-winter warming events in the stable-isotope records further indicates correct identification of winter layers to within ~1 month (Figs 3 and 4). The H2O2 data provide perhaps the most robust evidence for the timing of mid-winter, since the predominant source of atmospheric H2O2 is of photochemical origin, limiting production to the sunlit season. The only existing set of all-year-round measurements of H2O2 in the Antarctic troposphere stems from a coastal site and shows a distinct seasonal cycle, with a minimum around the winter solstice (Riedel and others, 2000). Year-round snow sample studies at the South Pole provide evidence that the same annual cycle is recorded in the surface snow and preserved at depth as a function of accumulationrate and temperature (McConnell and others, 1998). Hydrogen peroxide shows preservation of the seasonal signature at all core sites with more than approximately 30 g cm–2 a–1 of annual accumulation down to depths >60m (Frey and others, in press). Unfortunately, strong diffusional loss to the atmosphere and redistribution within the firn preclude a precise attribution of mid-winter at low-accumulation sites (<15 g cm–2 a–1) beyond the upper ~10m of the firn (Frey and others, in press).

Fig. 7. Comparison of nssSO4 2– and H2O2 concentrations in US ITASE core 2001-5, between 1998 and 2002.

On the basis of the above discussion, we suggest that a precision of ± 1 month is a conservative estimate for the US ITASE cores, at least for the most recent years where we have independent calibration from the satellite-based temperature data. To verify that this stated precision is applicable to the full length of the records, we quantitatively examined the timing of nssSO4 2– relative to other seasonal markers. To do this, we determined the variability in the coherence and phase of nssSO4 2– vs NO3 , Na+ and stable isotopes in each of the cores. We calculated the Thompson multi-taper (Thomson, 1982; Percival and Walden, 1993) phase and coherence spectra using three tapers over successive 10 year intervals from AD 1900 to 2000 to determine the mean and standard deviation of the phase. In all cases, greatest coherence is (as expected) at the annual cycle (i.e. frequency = 1 a–1), and the phase at this frequency varies by <1 month. There is no temporal trend in either phase or coherence (though we restricted our analysis to the interval 1900–2000 because of diffusion of the seasonal δ18O variations). As illustrated in Figure 8a, NO3 is in phase (0.0 ± 0.4 months) with nssSO4 2–, consistent with the evidence that, like nssSO4 2–, its variability is influenced by input from the upper troposphere/lower stratosphere (Mayewski and Legrand, 1990; Mulvaney and Wolff, 1993). Stable isotopes (Fig. 8b) are closely in phase with nssSO4 2– as well, with a slight lead of 0.1 months ( ± 0.9 month), consistent with the timing of warmest temperatures and the high seasonal isotope/temperature correlation (Schneider and others, 2005). Finally, Na+ (Fig. 8c) leads nssSO4 2– by ~5 ± 0.7 months, consistent with other evidence that Na+ peaks in late winter (Bergin and others, 1998; Kreutz and others 2000b). Given that advection to the ice sheet of sea-salt aerosols by both summer and winter storms can lead to enhanced Na+ concentrations, as expressed in relatively noisy Na+ records with multiple peaks in a given year (Fig. 4), the consistency of phase is remarkable, and further attests to the consistency in the seasonal timing of the nssSO4 2– peaks. This suggests that the identification of ‘winter’ in our records (nominally 1 July) is also precise to ± 1 month. This in turn implies that snowfall throughout the year in West Antarctica is reasonably uniform: there is apparently insufficient variability in the seasonal timing of snowfall to influence the phase relationships by more than 1 month. Preservation of all annual layers further indicates that wind erosion or sublimation is insufficient in magnitude to remove annual snow accumulation. Both of these inferences are consistent with the precipitation modeling analyses of Bromwich and others (2004), which indicate a seasonal variation in snowfall amounts in West Antarctica of <25% and sublimation over precipitation ratios of <15%.

Fig. 8. Coherence and phase for non-sea-salt sulfate (SO4 2–) compared with (a) NO3 in US ITASE core 2001-5; (b) δ18O in core 2000–5; and (c) Na+ in core 2000-4. The bandwidth is ~0.1 months. Bold lines show mean value; dashed lines are one standard deviation based on 10 year increments. Horizontal solid line in each upper panel is the 95% confidence limit for coherence.

6. Discussion

Recent work using paleoclimate proxy data has highlighted the importance of obtaining multiple, well-dated records at annual or better resolution, that can be used in calibration against the spatially comprehensive, but temporally very short, instrumental record of climate. Many analyses have emphasized tree ring records, primarily because the dating accuracy is excellent, and also because such records are available from nearly all continents and can therefore provide a representative sampling of climate variability (e.g. Mann and others, 1998; Jones and Widmann, 2003). As a general rule, available ice-core records have been too spatially sparse, and insufficiently resolved to contribute significantly to quantitative paleoclimate syntheses (Mann andJones, 2003), except where the longest timescales are concerned. Yet the polar regions, and Antarctica in particular, represent a large area that is inaccessible to such methods unless ice cores are used. An additional hindrance is that the instrumental record in Antarctica is particularly sparse and short, essentially limited to the last ~40 years.

One of the major goals of the overall ITASE program is to document Antarctic climate variability in the recent past (the last 200–2000 years) by obtaining highly resolved ice-core records distributed across the Antarctic ice sheet. Obtaining both high resolution and a high level of accuracy and precision is critical if we are to use multiple ice cores together as stacked records to reduce noise, or in multivariate regression models that are calibrated directly against the instrumental climate record (e.g. Schneider and others, 2005). The accuracy and precision obtained for the US ITASE cores recovered and analyzed from West Antarctica represent a significant contribution toward these efforts.

Importantly, for the period of overlap with the instrumental data (~40 years, and only ~20 years for satellite data), the absolute accuracy is demonstrably better than 1 year, and precision is well below the length of a season, allowing for calibration against both annually averaged and seasonal indicators of climate variability from the instrumental record. For longer-term records, the estimated relative accuracy of ± 1 year is very promising, as any systematic errors would affect all the cores together and therefore be negligible for these cores taken as a group. We further emphasize that we consider our estimates of absolute accuracy (< ± 2 years) to be quite conservative, given the relative accuracy of < ± 1 year from the radar analyses. In section 3, we raised the point that we cannot rule out systematic biases in the cores between the stratigraphic tie points provided by the volcanic horizons. However, we suggest that it is in fact quite unlikely that the same number of years have been misidentified in multiple ice cores. That the ice-core-based age of the Tambora eruption is identical in all of the records is suggestive of an absolute accuracy of < ± 1 year. It is further notable that, in general, dating accuracy in layer-counted ice cores is expected to decrease with depth (age), since errors in layer counting will be cumulative. In the case of the US ITASE cores, however, the accuracy should be approximately uniform in distribution, because there is a roughly even distribution of well-dated volcanic layers throughout the cores.

Accurate and precise dating of paleoclimate proxy records is a critical step in using such records to extend our knowledge of climate and environmental change prior to the time period covered by the instrumental record. Our analyses suggest that the use of multiple Antarctic ice cores for quantitative investigation of climate variability on timescales significantly shorter than decadal is feasible with existing data. Complete spatial coverage of the Antarctic continent will be important. The spatial coverage of well-dated ice cores from West Antarctica, plus published data from East Antarctica, appears to be sufficient to reconstruct Antarctic mean temperature over the last ~100–200 years (Schneider and others, 2005), and may be adequate for reconstruction of interannual variations in the ‘Southern Annular Mode’ (Thompson and Wallace, 2000), but may be insufficient to reconstruct higher-order patterns of variability, such as the Pacific South America (Schneider and others, 2005) or ‘Antarctic Dipole’ (Yuan and Martinson, 2001) patterns in temperature, sea-ice and geopotential height anomalies. It will therefore be important to combine records from the US ITASE cores with those from other ITASE projects, and with existing highly resolved cores such as Law Dome in East Antarctica (Masson-Delmotte and others, 2003) and the Dyer Plateau on the Peninsula (Thompson and others, 1994). Care must be taken to ensure that consistent standards of accuracy and precision are used in all datasets.

Acknowledgements

We gratefully acknowledge the support of the US Antarctic Research Program, the New York Air National Guard 109th Airborne Division, the staff of Raytheon Polar Services and A. Zielinski at the University of Maine for help in, and getting to, the field. The first author was supported by grant OPP 0196105 from the US National Science Foundation. Suggestions by R. Mulvaney and two anonymous reviewers led to improvements to the manuscript.

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