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GSA Bulletin; December 1996; v. 108; no. 12; p. 1626-1644; DOI: 10.1130/0016-7606(1996)108<1626:PCOYIT>2.3.CO;2
© 1996 Geological Society of America
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Productivity cycles of 200–300 years in the Antarctic Peninsula region: Understanding linkages among the sun, atmosphere, oceans, sea ice, and biota

Amy Leventer1, Eugene W. Domack2, Scott E. Ishman3, Stefanie Brachfeld4, Charles E. McClennen5 and Patricia Manley6

1 Limnological Research Center, University of Minnesota, Minneapolis, Minnesota 55455
2 Department of Geology, Hamilton College, Clinton, New York 13323
3 U.S. Geological Survey, Reston, Virginia 22092
4 Institute for Rock Magnetism, University of Minnesota, Minneapolis, Minnesota 55455
5 Department of Geology, Colgate University, Hamilton, New York 13346
6 Department of Geology, Middlebury College, Middlebury, Vermont 05753

Compared to the rest of the world's oceans, high-resolution late Holocene paleoclimatic data from the Southern Ocean are still rare. We present a multiproxy record from a sediment core retrieved from a deep basin on the western side of the Antarctic Peninsula that reveals a dramatic perspective on paleoclimatic changes over the past 3700 yr. Analyses completed include measurement of magnetic susceptibility and granulometry, bed thickness, particle size, percent organic carbon, bulk density, and microscopic evaluation of diatom and benthic foraminiferal assemblages and abundances. Downcore variability of these parameters demonstrates the significance of both short-term cycles, which recur approximately every 200 yr, and longer term events ({approx}2500 yr cycles) that are most likely related to global climatic fluctuations.

In the upper 600 cm of the core, lower values of magnetic susceptibility (MS) are correlated with lower bulk density, the presence of thinly laminated units, specific diatom assemblages, and generally higher total organic carbon content. Below 600 cm, magnetic susceptibility is uniformly low, though variability in other parameters continues. The magnetic susceptibility signal is controlled primarily by dilution of ferromagnetic phases with biosiliceous material. This signal may be enhanced further by dissolution of magnetite in the magnetic susceptibility lows (high total organic carbon). The role of variable primary productivity and its relationship to paleoclimate is assessed through the diatom data. In particular, magnetic susceptibility lows are characterized by higher than normal abundances of Chaetoceros resting spores. Corethron criophilum and/or Rhizosolenia spp. also are found, as is a higher ratio of the most common species of Fragilariopsis versus species of Thalassiosira. These assemblages are indicative of periods of high primary productivity driven by the presence of a meltwater stabilized water column. The 200 yr cyclicity noted in other paleoclimatic records around the world suggests a global forcing mechanism, possibly solar variability. In addition to the cyclic changes in productivity, overall elevated productivity is noted below 600 cm, or prior to ca. 2500 yr B.P. This increased productivity may represent the tail end of a Holocene climatic optimum, which is widely recognized in other parts of the world, but as yet is poorly documented in Antarctica.




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