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Late Quaternary fire regimes of Australasia
Authors:S.D. Mooney  S.P. Harrison  P.J. Bartlein  A.-L. Daniau  J. Stevenson  K.C. Brownlie  S. Buckman  M. Cupper  J. Luly  M. Black  E. Colhoun  D. D’Costa  J. Dodson  S. Haberle  G.S. Hope  P. Kershaw  C. Kenyon  M. McKenzie  N. Williams
Affiliation:1. Earth Observatory of Singapore, Nanyang Technological University, 639798, Singapore;2. Research School of Earth Sciences, The Australian National University, Canberra ACT 0200, Australia;3. Division of Earth Sciences, Nanyang Technological University, 639798, Singapore;4. Australian Antarctic Division, Department of Sustainability, Environment, Water, Population and Communities, Kingston 7150, Australia
Abstract:We have compiled 223 sedimentary charcoal records from Australasia in order to examine the temporal and spatial variability of fire regimes during the Late Quaternary. While some of these records cover more than a full glacial cycle, here we focus on the last 70,000 years when the number of individual records in the compilation allows more robust conclusions. On orbital time scales, fire in Australasia predominantly reflects climate, with colder periods characterized by less and warmer intervals by more biomass burning. The composite record for the region also shows considerable millennial-scale variability during the last glacial interval (73.5–14.7 ka). Within the limits of the dating uncertainties of individual records, the variability shown by the composite charcoal record is more similar to the form, number and timing of Dansgaard–Oeschger cycles as observed in Greenland ice cores than to the variability expressed in the Antarctic ice-core record. The composite charcoal record suggests increased biomass burning in the Australasian region during Greenland Interstadials and reduced burning during Greenland Stadials. Millennial-scale variability is characteristic of the composite record of the sub-tropical high pressure belt during the past 21 ka, but the tropics show a somewhat simpler pattern of variability with major peaks in biomass burning around 15 ka and 8 ka. There is no distinct change in fire regime corresponding to the arrival of humans in Australia at 50 ± 10 ka and no correlation between archaeological evidence of increased human activity during the past 40 ka and the history of biomass burning. However, changes in biomass burning in the last 200 years may have been exacerbated or influenced by humans.
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