New MIS 19 EPICA Dome C high resolution deuterium data: Hints for a problematic preservation of climate variability at sub-millennial scale in the “oldest ice”

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Abstract

Marine Isotope Stage 19 (MIS 19) is the oldest interglacial period archived in the EPICA Dome C ice core (~ 780 ky BP) and the closest “orbital analogue” to the Holocene — albeit with a different obliquity amplitude and phase with precession. New detailed deuterium measurements have been conducted with a depth resolution of 11 cm (corresponding time resolution of ~ 130 years). They confirm our earlier low resolution profile (55 cm), showing a relatively smooth shape over the MIS 20 to MIS 18 time period with a lack of sub-millennial climate variability, first thought to be due to this low resolution. The MIS 19 high resolution profile actually reveals a strong isotopic diffusion process leading to a diffusion length of at least ~ 40 cm erasing sub-millennial climate variability. We suggest that this diffusion is caused by water-veins associated with large ice crystals at temperatures above −10 °C, temperature conditions in which the MIS 19 ice has spent more than 200 ky. This result has implications for the selection of the future “oldest ice” drilling site.

Introduction

The EPICA Dome C ice core providing more than 800 thousands of years (ky) of climate variability is the longest available climatic record obtained from ice cores. Thanks to different proxies such as stable water isotopes (Jouzel et al., 2007), aerosols (Lambert et al., 2008, Wolff et al., 2010a), CH4 (Loulergue et al., 2008, Spahni et al., 2005) or CO2 (Lüthi et al., 2008, Siengenthaler et al., 2005), local, regional and global variations of climate and environment have been characterized over eight glacial–interglacial cycles (Fig. 1). If long term climate variability is considered to be driven by variations of incoming insolation due to slow changes of orbital parameters (Berger and Loutre, 1991, Laskar et al., 1993), the precise role of seasonal and latitudinal insolation distribution remains disputed. The climate system response involves threshold effects and internal feedbacks, making the understanding of the Earth climate complex (Paillard, 1998).

Interglacial periods offer the possibility to compare the climate system response under different orbital configurations and without the major influence of northern hemisphere glacial ice sheets. Thanks to EPICA Dome C ice core strong differences have been revealed between the nine past and current interglacial periods regarding their duration, trend or intensity (Fig. 1, Fig. 2) (EPICA-community-members, 2004, Jouzel et al., 2007, Masson et al., 2000). The current interglacial period has been compared to past interglacials with a specific focus on Marine Isotope Stage (MIS) 5 and 11 (Loutre and Berger, 2003, Loutre, 2003, Masson-Delmotte et al., 2006, Ruddimann, 2005), with implications for the future long term influence of Earth's orbit and the timing of the next Ice Age.

In this context, the following study focuses on the oldest interglacial archived in the EPICA Dome C (EDC) ice core: MIS 19, occurring around 780 thousands of years (ky) before present (B.P.). The full sequence of events, from the end of the previous glacial period (MIS 20) to the beginning of the following one (MIS 18), is detected between depths of 3147 and 3190 m. Corresponding ages range between ~ 749 and ~ 801 ky with an absolute uncertainty of 6 ky (2σ) (Fig. 3) as given by the current EDC3 chronology (Parrenin et al., 2007a). This dating is relatively well constrained for MIS 19, thanks to the Matuyama–Bruhnes geomagnetic reversal identification from Beryllium 10 measurements (Dreyfus et al., 2008, Raisbeck et al., 2006). The integrity of the climate records in EDC ice is confirmed down to ~ 801 ky (Jouzel et al., 2007), despite indications of ice flow perturbation in the bottom part of the core (Dreyfus et al., 2007).

MIS 19 is interesting for two reasons: (i) it occurred during an orbital configuration quite similar to the present one; and (ii) the EPICA Dome C low resolution proxy records exhibit comparable magnitudes for MIS 19 and the Holocene (Fig. 1, Fig. 2). Section 2 is thus dedicated to a detailed comparison of orbital contexts and EPICA records for these two periods.

During the glacial inception from MIS 19 to MIS 18, the low resolution EPICA Dome C water stable isotope record (Jouzel et al., 2007) has revealed millennial variability principally marked by the occurrence of three consecutive warm events (hereafter called Antarctic Isotope Maxima — AIM, following EPICA-community-members, 2006, and noted A, B, C on Fig. 2). These AIM events were also identified in the CH4 and CO2 signals (Loulergue et al., 2008, Lüthi et al., 2008). To improve the temporal resolution and to document the sub-millennial climate variability during MIS 19, we have conducted new high resolution measurements of water stable isotope ratios (δD of HDO molecules, hereafter called deuterium) on the EDC ice core fine cuts (Section 3). This new sampling, allowing to increase the temporal resolution from ~ 650 years (low resolution published data) to ~ 130 years, confirms the robustness of the previous low resolution isotopic signal (Section 4.1) but reveals at the same time a strong smoothing of the deuterium signal (Section 4.2), which erases potential new information on climate variability. This result leads to an analysis of the isotopic diffusion in ice, a process commonly studied for its implication in the impairment of climatic signals (Section 4.3). Section 4.4 is then dedicated to the comparison between modelled and data-derived diffusion calculation. This comparison suggests that the deepest EDC ice is affected by physical processes that alter the preservation of the full stable isotope variability. We finally investigate the possible mechanisms at play.

Section snippets

Comparison of MIS 19 and Holocene orbital contexts and EPICA proxy records

We compare the orbital configurations around MIS 19 and of the current interglacial, both characterized by a low eccentricity and therefore small variations of the precession parameter (Fig. 1). By aligning the respective early interglacial maxima of MIS 1 (~ 11 ky BP) and MIS 19 (~ 787 ky BP, according to the EDC3 chronology, Parrenin et al., 2007a), Fig. 2 enables a more detailed comparison of orbital contexts over a 50 ky interval (panels e and f). The EDC3 dating method (Parrenin et al., 2007b)

Data

The insert in Fig. 3 shows the cutting scheme for the EPICA Dome C ice core. The ~ 3260 m of the core is continuously cut in two different ways for the water isotopes measurements: the first type of samples called “bag” samples (hereafter low resolution LR) is cut every 55 cm along the core with 9 mm square sides; the second type of samples called “fine” samples (hereafter high resolution HR) corresponds to 11 cm long paved pieces. The analysis of these HR samples therefore improves both the depth

Results description

The high resolution data (Fig. 2b, blue) show a good agreement with the low resolution data (grey). They confirm the regular deuterium increase along the transition MIS 20 to MIS 19, the shape of MIS 19 optimum, and the occurrence of three consecutive Antarctic Isotopic Maxima (noted A, B and C) during the transition to MIS 18. The “calculated” signal (black) compared to low resolution data (grey) confirms the quality of measurements along MIS 19 and 18, with a satisfying correspondence between

Conclusion and perspectives

MIS 19 occurring around 780 ky BP appears as a close “orbital analogue” for the Holocene, with orbital context more similar than during MIS 5 or MIS 11 (a point also evoked by Tzedakis, 2009). In order to improve the available temporal resolution of water stable isotope data, we have conducted new deuterium measurements on 395 high resolution samples for the period between MIS 20 and MIS 18. Despite the improved resolution from ~ 650 y to ~ 130 y confirming earlier results, no new information on MIS

Acknowledgements

The authors wish to thank in particular R. Röthlisberger and E. Wolff for the data communication and help and G. Raisbeck for the helpful discussion. They are very grateful to the two anonymous reviewers who have contributed to improve the manuscript. This work is a contribution to the European Project for Ice coring in Antarctica (EPICA), a joint European Science Foundation/European Commission (EU) scientific program, funded by the EU and by national contributions from Belgium, Denmark,

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