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18O [P. M. Grootes, E. J. Steig, M. Stuiver, E. D. Waddington, D. L. Morse, Eos 75, 225 (1994)] and Vostok δD [J. Jouzel et al., Nature 364, 407 (1993)].
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Mayewski, P.A.1
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18O [P. M. Grootes, E. J. Steig, M. Stuiver, E. D. Waddington, D. L. Morse, Eos 75, 225 (1994)] and Vostok δD [J. Jouzel et al., Nature 364, 407 (1993)].
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Stager, J.C.1
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18O [P. M. Grootes, E. J. Steig, M. Stuiver, E. D. Waddington, D. L. Morse, Eos 75, 225 (1994)] and Vostok δD [J. Jouzel et al., Nature 364, 407 (1993)].
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Ann. Glaciol.
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Steig, E.J.1
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12
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0030431163
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18O [P. M. Grootes, E. J. Steig, M. Stuiver, E. D. Waddington, D. L. Morse, Eos 75, 225 (1994)] and Vostok δD [J. Jouzel et al., Nature 364, 407 (1993)].
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0027879561
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18O [P. M. Grootes, E. J. Steig, M. Stuiver, E. D. Waddington, D. L. Morse, Eos 75, 225 (1994)] and Vostok δD [J. Jouzel et al., Nature 364, 407 (1993)].
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Jouzel, J.1
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thesis, University of Washington, Seattle
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E. J. Steig, thesis, University of Washington, Seattle (1996).
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15N, as described [T. Sowers, M. Bender, D. Raynaud, J. Geophys. Res. 94, 5137 (1989)].
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-3 [C. M. Sucher, thesis, University of Rhode Island, Narragansett (1997)]. This value is about 2% lower than that obtained at GISP2 or the South Pole [M. Battle et al., Nature 383, 231 (1996)].
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Craig, H.1
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thesis, University of Rhode Island, Narragansett
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Sucher, C.M.1
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The original firn thickness is assumed to be 50 m (ice equivalent depth). Thinning due to glacier flow was calculated as described [E. D. Waddington, D. L. Morse, P. M. Grootes, E. J. Steig, NATO ASI Ser. 112, 499 (1993); D. L. Morse, thesis, University of Washington, Seattle (1997)].
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thesis, University of Washington, Seattle
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The original firn thickness is assumed to be 50 m (ice equivalent depth). Thinning due to glacier flow was calculated as described [E. D. Waddington, D. L. Morse, P. M. Grootes, E. J. Steig, NATO ASI Ser. 112, 499 (1993); D. L. Morse, thesis, University of Washington, Seattle (1997)].
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Morse, D.L.1
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wet) is the dry-deposition flux.
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E. J. Steig, P. J. Polissar, M. Stuiver, R. C. Finkel, P. M. Grootes. Geophys. Res. Lett. 23, 523 (1996); E. Bard, G. M. Raisbeck, F. Yiou, J. Jouzel, Earth Planet. Sci. Lett. 150, 453 (1997); R. C. Finkel and K. Nishiizumi, J. Geophys. Res. 102, 26699 (1997).
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The uncertainty in GISP2 Δage is taken from comparison of results from two independent calculations, which are in agreement within ± 100 years [(8) and J. Schwander et al., J. Geophys. Res. 102, 19483 (1997)]. Uncertainty in the curve match is taken as one-half the sampling interval, generally 1000 years for the period from 20 to 15 kyr B.P. and 150 years for the period from 15 to 10 kyr B.P.
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13C response during this period [C. D. Charles and R. G. Fairbanks, Nature 355, 416 (1992); C. D. Charles, J. Lynch-Stieglitz, U. S. Ninnemann, R. G. Fairbanks, Earth Planet. Sci. Lett. 142, 19 (1996)].
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13C response during this period [C. D. Charles and R. G. Fairbanks, Nature 355, 416 (1992); C. D. Charles, J. Lynch-Stieglitz, U. S. Ninnemann, R. G. Fairbanks, Earth Planet. Sci. Lett. 142, 19 (1996)].
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13C response during this period [C. D. Charles and R. G. Fairbanks, Nature 355, 416 (1992); C. D. Charles, J. Lynch-Stieglitz, U. S. Ninnemann, R. G. Fairbanks, Earth Planet. Sci. Lett. 142, 19 (1996)].
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13C response during this period [C. D. Charles and R. G. Fairbanks, Nature 355, 416 (1992); C. D. Charles, J. Lynch-Stieglitz, U. S. Ninnemann, R. G. Fairbanks, Earth Planet. Sci. Lett. 142, 19 (1996)].
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0001292197
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2 along the Antarctic coastal margin. Local heat fluxes from leads and polynyas in the western Ross Sea, kept open by the strong westerly katabatic wind flow [D. D. Kurtz and D. Bromwich, ibid., p. 177; H. J. Zwally and J. C. Comiso, ibid., p. 203], may be two orders of magnitude higher [D. J. Cavalieri and S. Martin, ibid., p. 227].
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3543068837
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2 along the Antarctic coastal margin. Local heat fluxes from leads and polynyas in the western Ross Sea, kept open by the strong westerly katabatic wind flow [D. D. Kurtz and D. Bromwich, ibid., p. 177; H. J. Zwally and J. C. Comiso, ibid., p. 203], may be two orders of magnitude higher [D. J. Cavalieri and S. Martin, ibid., p. 227].
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Kurtz, D.D.1
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3543099266
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2 along the Antarctic coastal margin. Local heat fluxes from leads and polynyas in the western Ross Sea, kept open by the strong westerly katabatic wind flow [D. D. Kurtz and D. Bromwich, ibid., p. 177; H. J. Zwally and J. C. Comiso, ibid., p. 203], may be two orders of magnitude higher [D. J. Cavalieri and S. Martin, ibid., p. 227].
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Antarct. Res. Ser.
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Zwally, H.J.1
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2 along the Antarctic coastal margin. Local heat fluxes from leads and polynyas in the western Ross Sea, kept open by the strong westerly katabatic wind flow [D. D. Kurtz and D. Bromwich, ibid., p. 177; H. J. Zwally and J. C. Comiso, ibid., p. 203], may be two orders of magnitude higher [D. J. Cavalieri and S. Martin, ibid., p. 227].
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The sensitivity of Taylor Dome to local oceanographic conditions may depend on ice sheet configuration, especially the position of the Ross Ice Sheet/Ice Shelf margin. Although the Ross Ice Sheet may not have reached all the way to the continental shelf break during the last glacial maximum [K. J. Licht, A. E. Jennings, J. T. Andrews, K. M. Williams, Geology 24, 223 (1996)], the distance between Taylor Dome and seasonally open water would have been greater, and local atmospheric circulation patterns may have been altered [D. L. Morse, E. D. Waddington, E. J. Steig, Geophys. Res. Lett. 25, 3383 (1998)]. We do not therefore expect a simple linear relation between proxies of ocean circulation and Taylor Dome δD even if, as we suggest, changes in ocean circulation are the primary forcing mechanism.
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The sensitivity of Taylor Dome to local oceanographic conditions may depend on ice sheet configuration, especially the position of the Ross Ice Sheet/Ice Shelf margin. Although the Ross Ice Sheet may not have reached all the way to the continental shelf break during the last glacial maximum [K. J. Licht, A. E. Jennings, J. T. Andrews, K. M. Williams, Geology 24, 223 (1996)], the distance between Taylor Dome and seasonally open water would have been greater, and local atmospheric circulation patterns may have been altered [D. L. Morse, E. D. Waddington, E. J. Steig, Geophys. Res. Lett. 25, 3383 (1998)]. We do not therefore expect a simple linear relation between proxies of ocean circulation and Taylor Dome δD even if, as we suggest, changes in ocean circulation are the primary forcing mechanism.
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Morse, D.L.1
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Steig, E.J.3
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61
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3543053524
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-
note
-
We thank G. Denton and M. Stuiver for suggesting an ice core at Taylor Dome, P. Grootes for directing the field program, the Polar Ice Coring Office and Antarctic Program of NSF for logistical and financial support, and R. Alley and M. Kaplan for helpful comments on the manuscript.
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