Study of the eolian fraction of late Quaternary sediments from the tropical Atlantic reveals that two modes of long-term climate variability have existed in tropical Africa during the last 150,000 yr. Tropical northwest Africa (i.e., the southwestern Sahara and Sahel) was driest during glaciations and stades, but wetter than at present during interglaciations and interstades. This may be a response to ice sheets at higher latitudes, via equatorward displacement of the westerlies and the subtropical high. In contrast, central equatorial Africa (southeast of the Sahara) was most arid during interstades and times of ice growth, and most humid during deglaciation. Wet periods in this area correspond to insolation maxima in northern hemisphere summer. A 23,000-yr precessional rhythm is suggested, supporting a direct link between African Monsoon intensity and orbitally modulated insolation. The late Holocene is the only time observed when both areas are arid during an interglacial episode. This may reflect, in part, anthropogenic disturbance of late Holocene climates.
High‐ and low‐latitude forcing of terrestrial African paleoclimate variability is demonstrated using 900 ka eolian and biogenic component records from Ocean Drilling Program site 663 in the eastern equatorial Atlantic. Terrigenous (eolian dust) and phytolith (savannah grass cuticle) accumulation rate records vary predominantly at 100 and 41 kyr periodicities and spectral phase estimates implicate high‐latitude forcing. The abundance of freshwater diatoms (Melosira) transported from dry African lake beds varies coherently at 23–19 kyr orbital periodicities and at a phasing which implicates low‐latitude precessional monsoon forcing. Modeling studies demonstrate that African climate is sensitive to both high‐ and low‐latitude boundary conditions. African monsoon intensity is modulated by direct insolation variations due to orbital precession, whereas remote high‐latitude forcing can be related to cool North Atlantic sea surface temperatures (SSTs) which promote African aridity and enhance dust‐transporting wind speeds. The site 663 terrigenous and phytolith records covary with North Atlantic SST variability at 41 °N (site 607). We suggest that Pleistocene African climate has responded to both high‐latitude North Atlantic SST variability as well as low‐latitude precessional monsoon forcing; the high‐latitude influence dominates the sedimentary record. Prior to circa 2.4 Ma, terrigenous variations occurred primarily at precessional periodicities (23–19 kyr), indicating that African climate was largely controlled by low‐latitude insolation variations prior to the onset of high‐amplitude glacial‐interglacial climate change.
Two major goals of Leg 108 were to investigate late Cenozoic changes in (1) North African aridity and (2) atmospheric circulation over the equatorial Atlantic and Sahelian/Saharan Africa. Several high-resolution records from Ocean Drilling Program Leg 108 are pertinent to these problems. Dust fluxes from Africa to the Atlantic were low during the final 3 m.y. of the Miocene and then increased markedly during the Pliocene and Pleistocene. The increasing Pliocene-Pleistocene dust fluxes suggest major aridification of North Africa, possibly accompanied by an increase in the amplitude of aridity/humidity cycles. Other evidence from the northwest African margin (influxes of fluvial clay, terrestrial carbon, freshwater diatoms, and pollen) also suggests increasing aridity and larger oscillations during the Pliocene and Pleistocene, along with increased intensity of coastal trade winds. Because prominent changes in long-term dust fluxes preceded Northern Hemisphere glaciation by 1.5 Ma, Northern Hemisphere ice sheets were not the major factor in the evolution of African climate, in agreement with late Pleistocene evidence at orbital time scales. The apparent synchroneity of several major long-term changes in climate over Africa and the equatorial Atlantic with changes in the Southern Ocean and South Atlantic suggests long-term linkage in the responses of these two regions, again similar to late Pleistocene linkages at orbital time scales. The ultimate source of forcing of these changes at tectonic time scales is not fully resolved. The Messinian closing and abrupt reopening of the Mediterranean left no obvious imprint on signals of African dust flux. One plausible source of forcing is large-scale tectonic uplift, which occurred at unusually rapid rates during the latest Cenozoic in Southeast Asia (Tibet and the Himalayas), East Africa, and South America (the Andes and Altiplano). Modeling experiments show that uplift causes large-scale rearrangements of atmospheric circulation, including the strength and position of the upper tropospheric jet streams and the lower tropospheric high-and low-pressure cells that control surface winds and moisture balances.
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