Isotope calibrated Greenland temperature record over Marine Isotope Stage 3 and its relation to CH4
Introduction
The climate over the last glacial period was characterised by numerous abrupt climate changes known as Dansgaard–Oeschger (DO) events [1]. They can be traced in paleorecords from the Arctic ice sheets, as well as from tropical and subtropical regions [2], [3], [4], [5]. DO events are most prominently represented in δ18Oice, the oxygen isotope ratio in Greenland ice cores. They have been related to shifts of the ocean thermohaline circulation (THC) [6], [7], [8]. DO events in Greenland typically start with a rapid warming of about 8 up to 16 °C within a few decades [9], [10], [11], [12] followed by a more gradual cooling phase over several centuries and a rapid drop back towards cold stadial conditions. The long lasting DO events were preceded by massive ice surges from the northern ice sheets, documented by debris deposits at the ocean floor known as Heinrich (H) events [13].
Water isotopes in ice cores (δ18Oice or δD) are useful temperature proxies because changes in isotopic composition of precipitation in polar regions are mainly related to variations of temperatures at the site of precipitation. The present day spatial relationship between δ18Oice and temperature, αspatial, is estimated at 0.67‰/K for Greenland [14]. α depends on variations of the seasonal precipitation distribution [17] and/or changes occurring at the source region [18], [19] of precipitation. Therefore, the present day αspatial cannot be used to quantitatively interpret past climate shifts [15], [16].
Measurements of the isotopic composition of nitrogen δ15N and/or argon δ40Ar on air trapped in ice cores can be used to calibrate the δ18Oice to temperature relation, during an event of rapid temperature change [9], [10], [11], [12], [20], [21], [22]. Because atmospheric δ15N is constant [23], changes of this air parameter trapped in ice indicate fractionations due to gravitation and thermal diffusion [24]. Rapid warming or cooling at the surface produces a temperature gradient in the firn that forces the heavier isotopes to migrate towards the cold end. This results in an alteration of the isotope signal trapped in the ice core. The surface temperature change can be reconstructed by comparing the measured isotope fractionation with firn gas diffusion model calculations. This approach has been used to deduce rapid temperature changes for several DO events [9], [10], [11], [12], [20], [24], [25] during the last glacial epoch.
Here we present a reconstruction of the temperature evolution over 9 consecutive DO events (events 9 to 17) during Marine Isotope Stage (MIS) 3, based on high resolution δ15N measurements on the ice core from the North Greenland Ice Core Project (NorthGRIP) [26], using a new on-line technique [27], [28]. This record is compared with existing high resolution CH4 measurements from the NorthGRIP [29] (DO 9–12), and the GISP2 [31], [30] (DO 9–17) ice cores. Additionally, we present new highly resolved CH4 measurements from the NorthGRIP ice core for the time period of DO 15–17. This allows us to compare in detail methane and reconstructed temperature evolutions over a longer time period including rapid temperature variations (DO 9–17).
Section snippets
Method
Firn, the porous upper 50–100 m of an ice sheet, can be divided into three zones from top to bottom: (i) The convective zone, where the air is well mixed with the atmosphere; (ii) The diffusive column, where the isotopic and elemental composition of the air is altered by diffusion, such as gravitational settling [32], [33] and thermal diffusion [9], [20], [24]; (iii) The non-diffusive zone, where no vertical mixing of the air occurs.
Isotopic enrichment due to gravitational fractionation, e.g.
Greenland temperature evolution during MIS 3
In Fig. 2 the calculated surface temperature evolution is shown over the time period from 64 and 38 kyr BP corresponding to nearly the complete MIS 3. MIS 3 is characterized by various abrupt temperature changes with amplitudes of up to 15 °C (in about 200 yr). A typical mean rate of the temperature change at the beginning of DO events was 0.5 ± 0.1 °C/decade (Table1, Fig. 3). However, maximum temperature rates are about 1 °C/decade. The amplitude of the temperature changes attributed to the
Conclusions
The abrupt temperature changes associated with the 9 consecutive DO events 9–17 are in the range of 8 to 15 °C. The 12.5 °C temperature change of DO 12 is consistent with an earlier reconstruction of 12 °C on ice from a different site and using a different method [11]. This finding also supports earlier results from DO 19 that showed a 16 °C temperature change in GRIP as well as in NorthGRIP [9], [12].
Furthermore, a detailed comparison of the temperature evolution with measurements of the
Acknowledgements
We would like to thank two anonymous reviewers for their extensive comments and suggestions that improved this manuscript considerably. We thank Gregor Hausammann for his support during the CH4 measurements. This work, as part of the NorthGRIP Project, was supported by the University of Bern and the Swiss National Science Foundation. The NorthGRIP Project is coordinated by the Department of Geophysics at the Niels Bohr Institute for Astronomy, Physics and Geophysics, University of Copenhagen.
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