All inorganic geochemical data discussed in this publication are listed in Table T1. The most important aspects of the data set are presented and discussed below.
The investigated sediments may be regarded as clay or calcareous nannofossil-rich clay with carbonate contents between 5 and 30 wt%. According to our own data (Table T1) as well as shipboard measurements (Shipboard Scientific Party, 2000), the organic carbon contents vary between 0.2 and 0.5 wt%, suggesting permanently oxygenated conditions at the seafloor and a moderate organic carbon flux.
In a ternary plot (Fig. F3), which shows the relative proportions of SiO2 (representing quartz or opaline silica), Al2O3 (representing clay minerals), and CaO (representing carbonate), the sediments can be described as mixtures of biogenous carbonate with an aluminosilicate component that has a slightly higher Al content than average shale. Sediments and soils consisting of highly weathered material—predominantly found in tropical regions—are known for their high Al contents (Mason and Moore, 1985). Because there are no samples plotting toward higher SiO2 contents in the ternary plot, quartz and biogenic silica fractions are rather low or negligible (Fig. F3).
In contrast to sediments from ODP Site 1145, which show a certain eolian (loess) influence (Wehausen and Brumsack, 2002), sediments from Site 1143 presented here are characterized by relatively low TiO2/Al2O3 ratios (Fig. F4). Whereas Site 1145 samples plot closer to the dilution line for loess (Schnetger, 1992), Site 1143 samples plot toward higher Al2O3 values, relatively close to the data point for Mekong suspended matter (SPM) (Martin and Meybeck, 1979). However, in addition to material from the Mekong River, there seems to have been at least one other source with slightly higher Ti and lower Al contents delivering material to this part of the South China Sea because all samples plot above the ratio for Mekong SPM (Fig. F4).
Depth profiles of CaCO3, SiO2, and Al2O3 contents demonstrate that the bulk composition of the sediments show a high variability with time (Fig. F5). SiO2 and Al2O3 display the same pattern (correlation coefficient: r2 = 0.92), which again shows that there is no significant contribution of biogenic opal to the total SiO2 content. Only very few diatoms and radiolarians were found in the late Pliocene sediments of Site 1143 (Shipboard Scientific Party, 2000).
With regard to the carbonate contents, two different types of carbonate cycles have been reported for South China Sea sediments (Thunell et al., 1992). Carbonate cycles with higher carbonate contents during glacials ("Pacific type"), reflecting the varying carbonate compensation depth (CCD) or lysocline, are only observed in sediments deposited in water depths below 3500 m. Classical carbonate cycles, showing lower carbonate content during glacials due to dilution by terrigenous detrital material and higher carbonate contents during interglacials ("Atlantic type") (Thunell et al., 1992), are found in water depths above 3000 m. At present, the water depth of Site 1143 is 2772 m. Assuming a similar depth during the Pliocene (permanent sedimentation above the CCD), "Atlantic-type" carbonate cyclicity should be expected at this location. Our data show that carbonate contents are generally lower and terrigenous detrital matter (SiO2 and Al2O3) contents are higher during glacial stages (Fig. F5). This supports "Atlantic-type" carbonate cycles mode (i.e., dilution cycles). Minimum carbonate and maximum terrigenous detrital matter contents are observed for oxygen isotope Stages 100, 104, 106, and 110. Beyond some small peaks in sediment composition (i.e., changes of short duration), the carbonate terrigenous detrital matter relationship displays low variability before 2.85 Ma (Fig. F5).
In order to define changes in the composition of the terrigenous detrital matter, we either use elemental contents that were calculated on a carbonate-free basis (see "Materials and Methods") or ratios of terrigenous detrital elements.
In general, slight changes in the composition of terrigenous detrital matter are discernible. A few distinct thin layers show significantly lower contents of most major components of the noncarbonate fraction (Fig. F6). TiO2 (cfb) displays a relatively strong variation throughout the investigated interval. A shift toward lower TiO2 (cfb) values occurs at ~2.9 Ma. SiO2 (cfb) and K2O (cfb) covary more or less with TiO2 (cfb) but show relatively little variability. The Al2O3 (cfb) content displays only small variations in sediments older than 2.6 Ma. In the upper part of the core, variations are stronger with an opposite pattern compared to SiO2 (cfb), TiO2 (cfb), and K2O (cfb) (Fig. F6A).
The Si/Al ratio shows low variations in sediments >2.6 Ma and higher variation in sediments <2.6 Ma (Fig. F6A). In contrast, Ti/Al displays strong variations throughout the whole section (Fig. F6B), mainly driven by the TiO2 (cfb) content with relatively high amplitude variations (Fig. F6A). K/Al, Cr/Al, Rb/Al, and Zr/Al ratios covary more or less with the Ti/Al ratio, and all five parameters display long-term changes. They decrease between 2.9 and 2.5 Ma and slightly increase again thereafter.
To observe and interpret those changes in terrigenous detrital matter composition with respect to global ice volume and sea level changes, we compared the Al2O3 (cfb) and TiO2 (cfb) records with the benthic 18O curve (Fig. F7). Higher contents of Al2O3 (cfb) are present during glacial stages owing to an enhanced contribution of strongly weathered material from the Asian continent or adjacent islands. TiO2 (cfb) contents, which are lower during glacials, are due to stronger fluvial input of material with low Ti content (e.g., suspended matter from Mekong River) (Martin and Meybeck, 1979). Until 2.8 Ma, a significant increase in Al2O3 (cfb) content is not seen. A weak enrichment in Al is visible at oxygen isotope Stage 110 (2.73 Ma), which marks the onset of major glaciation cycles of the Northern Hemisphere (Tiedemann et al., 1994). Amplitudes of Al2O3 (cfb) content increase after 2.55 Ma, and the strongest Al enrichments are present during isotope Stages 100, 96, and 82. The highest amplitudes and, thus, the strongest minima are present in the TiO2 (cfb) record between 2.45 and 2.8 Ma.
What are the climatic and/or oceanographic mechanisms causing changes in terrigenous detrital matter composition? There are four possible scenarios, as known from earlier publications and described in the following paragraphs.
The Ba content calculated on a carbonate-free basis or the Ba/Al ratio are parameters that may serve as indicators for paleoproductivity (Dymond et al., 1992; Francois et al., 1995). Both show exactly the same cyclic profile, but we prefer to use Ba/Al ratios for the sake of a better comparability with other studies where this proxy has been applied (Wehausen and Brumsack, 1999; Shimmield and Mowbray, 1991). Before using such Al-normalized total Ba contents as a proxy for marine productivity conditions, it has to be evaluated whether the fluctuations are solely related to changes in terrigenous input, are only caused by variations in barite preservation (Schenau et al., 2001), or are indicative of real changes in barium flux rates and oceanic productivity. From other marine geochemical studies (Wehausen and Brumsack, 1999; Shimmield and Mowbray, 1991), as well as from the composition of the Earth's upper crust (Taylor and MacLennan, 1985) or average shale (Wedepohl, 1971, 1991), we know that the background Ba/Al value, at maximum, should be 70 x 10-4. Because of the relatively high Al contents typical of a region with intense tropical weathering (see "Changes in Terrigenous Detrital Matter Composition"), the background value for the South China Sea is lower than it is for average shale or sediments from higher latitudes. The Ba/Al variability of the investigated sediments is higher than any reasonable lithogenic background value. Therefore, the peaklike Ba enrichments in the data set (Fig. F8) are likely caused by an enhanced bio-barite flux (Dehairs et al., 1980; Bishop, 1988; Gingele and Dahmke, 1994) and thus could be used as a proxy for paleoproductivity. Certainly, the preservation of barite as determined by the degree of saturation in bottom and pore waters is an important factor influencing the Ba contents of marine sediments (McManus et al., 1998; Schenau et al., 2001). However, when pore water sulfate concentrations are more or less constant (i.e., under permanently oxic conditions), the degree of saturation itself is only controlled by the flux of barite (which acts as a positive feedback). Therefore, we do not believe that productivity and the associated barium flux were only constant or even lower when Ba enrichments are present in the sediment. Instead, a positive relationship between productivity and barium content of the sediments is most likely.
The Ba/Al ratio corresponds very well to the 18O curve. This indicates that productivity was lower during glacial stages and higher during interglacials. Exceptions are seen in the lower part of the core (during stages 110 and 120, productivity was slightly higher). The covariation between the Ba/Al ratio and carbonate content suggests that increases in carbonate contents during interglacial stages are not only due to less dilution but are also caused by enhanced biological production. Shimmield and Mowbray (1991) found a very good correlation between 18O of planktonic foraminifers, Ba/Al, and carbonate records for late Quaternary sediments from the northwest Arabian Sea. They proposed that the nutrient supply through upwelling of intermediate waters was the triggering factor for higher productivity during interglacials. A similar explanation may be valid for Site 1143 sediments, although we cannot solve the paleoclimatic and paleoceanographic mechanism causing a higher nutrient supply during interglacials in the southern South China Sea. One possibility may be the stronger inflow of nutrient-rich waters from the Sunda shelf. Another possibility is enhanced upwelling caused by stronger monsoonal winds.
The P/Al ratio displays a cyclic record that correlates with Ba/Al and carbonate contents (Fig. F8). The primary flux of phosphorus into marine sediments mainly appears in three different forms: organic material, fish remnants, and iron oxides that have a high adsorption capacity for phosphorus (Froehlich et al., 1988; Van Cappellen and Berner, 1988; Van Cappellen and Ingall, 1994). Lithogenic phosphorus is generally of minor importance. In deeper buried sediment layers phosphorus may still be present in these forms, but here, diagenetically formed carbonate-fluoroapatite (CFA) is responsible for the major fraction of phosphorus (Ruttenberg and Berner, 1993). About 80% of the total P in Pliocene sediments from various settings were found to be present as CFA (Delaney, 1998).
Despite the dominance of authigenic phosphorus phases in deeper buried sediments, the covariation of P/Al ratio, carbonate content, and Ba/Al ratio suggests that the primary availability (i.e., changes in bioproductivity and phosphorus flux) had a significant influence on the phosphorus content of Site 1143 sediments. Another important factor for phosphorus burial is the carbonate content because the high surface area and adsorption capacity of calcite might trigger the formation of iron oxyhydroxide coatings, adsorbing agents for phosphorus (Delaney, 1998).
In general, Fe2O3 (cfb) contents display variations that covary with those of SiO2 (cfb) (Figs. F9A, F6A). Besides these minor fluctuations caused by changes in terrigenous detrital matter composition, there are some small spikes and three very prominent peaks. These layers are characterized by lower terrigenous detrital matter contents (Fig. F6A) and enrichments in iron, sulfur, and the trace elements As, Co, and Ni (Fig. F9B). These trace elements are known to form stable sulfides or to coprecipitate with iron sulfides under sulfidic conditions (Jacobs and Emerson, 1985; Huerta-Diaz and Morse, 1992; Calvert and Pedersen, 1993). Vanadium, mainly present in the form of vanadyl cations in organic complexes under reducing conditions (Szalay and Szilagyi, 1967; Emerson and Huested, 1991), does not show a significant enrichment. All of this suggests the presence of pyrite and other metal sulfides of diagenetic origin in the form of small concretions that seem to have formed very locally. Evidence for microbial sulfate reduction was given by the pore water data (Shipboard Scientific Party, 2000).
High Mn/Al ratios well above the ratio for average shale and a partial covariation between Mn and carbonate contents (Fig. F9A) suggests the presence of manganese coatings on carbonate tests (Boyle, 1983; Franklin and Morse, 1983) or the presence of authigenic manganese carbonates (Thomson et al., 1986). Whereas Sr clearly correlates with CaCO3 (r2 = 0.96), Mn/Al displays a more specific behavior, probably caused by changes in terrigenous detrital matter flux. Furthermore, some enrichments in manganese are seen that cannot be explained by carbonate contents or terrigenous input. The Mn/Al peaks at 2180, 2210, 2260, and 2430 ka may, for example, represent periods of a strong import of Mn from the shelf. Such an Mn accumulation mechanism has been reported for the Cretaceous Indian Ocean (Thurow et al., 1992). Oxygen-deficient conditions led to the mobilization of Mn(II) from shelf sediments and transport via the oxygen minimum zone into deeper regions of the basin. Since the Mn enrichments occurred during interglacials and corresponding times of high bioproductivity, the existence of an enhanced oxygen minimum zone is very likely.