4.7 Article

A phase-space model for Pleistocene ice volume

Journal

EARTH AND PLANETARY SCIENCE LETTERS
Volume 307, Issue 1-2, Pages 94-102

Publisher

ELSEVIER SCIENCE BV
DOI: 10.1016/j.epsl.2011.04.018

Keywords

glacial cycles; climate model; orbital forcing; mid-Pleistocene transition; eccentricity

Funding

  1. NSF-MGG [0926735]
  2. Directorate For Geosciences [926735] Funding Source: National Science Foundation
  3. Division Of Ocean Sciences [926735] Funding Source: National Science Foundation

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We present a phase-space model that simulates Pleistocene ice volume changes based on Earth's orbital parameters. Terminations in the model are triggered by a combination of ice volume and orbital forcing and agree well with age estimates for Late Pleistocene terminations. The average phase at which model terminations begin is approximately 90 +/- 90 degrees before the maxima in all three orbital cycles. The large variability in phase is likely caused by interactions between the three cycles and ice volume. Unlike previous ice volume models, this model produces an orbitally driven increase in 100-kyr power during the mid-Pleistocene transition without any change in model parameters. This supports the hypothesis that Pleistocene variations in the 100-kyr power of glacial cycles could be caused, at least in part, by changes in Earth's orbital parameters, such as amplitude modulation of the 100-kyr eccentricity cycle, rather than changes within the climate system. (c) 2011 Elsevier B.V. All rights reserved.

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