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Mechanisms of Holocene palaeoenvironmental change in the Antarctic Peninsula regionDepartment of Geography, University of Durham, South Road, Durham DH1 3LE, UK, m.j.bentley{at}durham.ac.uk, British Antarctic Survey, Natural Environment Research Council, High Cross, Madingley Road, Cambridge CB3 0ET, UK
British Antarctic Survey, Natural Environment Research Council, High Cross, Madingley Road, Cambridge CB3 0ET, UK
British Antarctic Survey, Natural Environment Research Council, High Cross, Madingley Road, Cambridge CB3 0ET, UK
Department of Geography, University of Durham, South Road, Durham DH1 3LE, UK
Department of Geosciences, Hamilton College, Clinton NY 13323, USA
British Antarctic Survey, Natural Environment Research Council, High Cross, Madingley Road, Cambridge CB3 0ET, UK
British Antarctic Survey, Natural Environment Research Council, High Cross, Madingley Road, Cambridge CB3 0ET, UK
Department of Earth & Environmental Studies, Montclair State University, Upper Montclair NJ 07043, USA
Department of Geology, Colgate University, 13 Oak Drive, Hamilton NY 13346, USA
GeoBiosphere Science Centre, Quaternary Sciences, Sölvegatan 12, S-223 62 Lund, Sweden
British Antarctic Survey, Natural Environment Research Council, High Cross, Madingley Road, Cambridge CB3 0ET, UK
Department of Geography, Loughborough University, Loughborough LE11 3TU, UK The Antarctic Peninsula is one of the three fastest warming regions on Earth. Here we review Holocene proxy records of marine and terrestrial palaeoclimate in the region, and discuss possible forcing mechanisms underlying past change, with a specific focus on past warm periods. Our aim is to critically evaluate the mechanisms by which palaeoclimate changes might have occurred, in order to provide a longer-term context for assessing the drivers of recent warming. Two warm events are well recorded in the Holocene palaeoclimate record, namely the early Holocene warm period, and the `Mid Holocene Hypsithermal' (MHH), whereas there are fewer proxy data for the `Mediaeval Warm Period' (MWP) and the `Recent Rapid Regional' (RRR) warming. We show that the early Holocene warm period and MHH might be explained by relatively abrupt shifts in position of the Southern Westerlies, superimposed on slower solar insolation changes. A key finding of our synthesis is that the marine and terrestrial records in the AP appear to show markedly different behaviour during the MHH. This might be partly explained by contrasts in the seasonal insolation forcing between these records. Circumpolar Deep Water (CDW) has been implicated in several of the prominent changes through the Holocene but there are still differences in interpretation of the proxy record that make its influence difficult to assess. Further work is required to investigate contrasts between marine and terrestrial proxy records, east—west contrasts in palaeoclimate, the history of CDW, to retrieve a long onshore high resolution record of the Holocene, and determine the role of sea ice in driving or modulating palaeoclimate change, along with further efforts to study the proxy record of the RRR and the MWP.
Key Words: Antarctic Peninsula Southern Ocean palaeoclimate Southern Westerlies ENSO climate models Circumpolar Deep Water Holocene.
The Holocene, Vol. 19, No. 1,
51-69 (2009) |
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