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1.
A reevaluation of the oceanic uranium budget for the Holocene 总被引：4，自引：0，他引：4
We present a new assessment of the pre-anthropogenic U budget for the Holocene ocean. We find that the gross input of U to the ocean lies in the range 53±17 Mmol/year, where the dominant source is river runoff (42.0±14.5 Mmol/year) and the direct discharge of groundwater could represent a significant additional input (9.3±8.7 Mmol/year). The soluble U flux associated with the aeolian input of crustal dust is minor (1.8±1.1 Mmol/year), falling well within the errors associated with the riverine flux. Removal of U to the organic rich sediments of salt marshes and mangrove swamps during river–sea mixing may significantly modify the riverine flux, such that the net U input is reduced to 42±18 Mmol/year. Evaluation of the U isotope budget demonstrates that the limits we have established on the U input flux are reasonable and suggests that direct groundwater discharge may play a significant role in maintaining the oceanic excess of 234U. The total sink of U from the ocean lies in the range 48±14 Mmol/year. We find that three major processes control the magnitude of this flux: (1) removal to oxygen-depleted sediments (26.9±12.2 Mmol/year); (2) incorporation into biogenic carbonate (13.3±5.6 Mmol/year); and (3) crustal sequestration during hydrothermal alteration and seafloor weathering (5.7±3.3 Mmol/year). The removal of U to opaline silica (0.6±0.3 Mmol/year) and hydrogenous phases (1.4±0.8 Mmol/year) is minimal, falling well within the errors associated with the other sinks. That the input and output fluxes balance within the calculated errors implies that U may be in steady state in the Holocene ocean. In this case, the input and output fluxes lie in the range 34–60 Mmol/year, giving an oceanic U residence time of 3.2–5.6×105 years. However, given the large uncertainties, a significant imbalance between the Holocene input and output fluxes cannot be ruled out. The constancy of the ancient seawater U concentration implies that the U budget is in steady state over the time period of a glacial–interglacial climate cycle (105 year). A Holocene flux imbalance must, therefore, be offset by an opposing flux imbalance during glacial periods or at the interglacial–glacial transition. We suggest that the storage of U in the coastal zone and shallow water carbonates during interglacial periods and the release of that U at or following the interglacial–glacial transition could be sufficient to affect the short-term stability of the U budget. Providing tighter constraints on U fluxes in the Holocene ocean is a prerequisite to understanding the U budget on the time scale of a glacial–interglacial climate cycle and using this element as a valuable palaeoceanographic proxy. 相似文献
2.
Boron isotope systematics in large rivers: implications for the marine boron budget and paleo-pH reconstruction over the Cenozoic 总被引：5，自引：0，他引：5
The chemical composition of the oceans and long-term climate changes are believed to be linked. Reconstruction of seawater pH evolution is desirable as pH may be related to atmospheric pCO2, and hence to climate evolution. Boron isotopes in oceanic carbonates have been suggested to be a proxy for oceanic paleo-pH reconstruction. Nevertheless, the calculation of paleo-pH values over geological periods requires a precise knowledge of the boron isotopic composition of the oceans when calcite precipitated. We present the systematics of boron isotopic composition of the world's main rivers. We deduce a continental boron flux to the oceans of 38×1010 gB/year with a mean isotopic composition of +10‰. These results lead to a balanced boron budget in the oceans and allow the development of a model for the marine boron secular evolution over the past 100 Myr. It is shown that the oceanic boron cycle is mainly controlled by the boron continental discharge and the boron uptake from the oceans during low temperature alteration of oceanic crust. However, the recent important increase of the clastic sediment supply, linked to the Himalayan erosion, impacts the oceanic boron budget by enhancing significantly the boron uptake by adsorption on sediments. We predict a boron isotopic composition in the oceans lower during the Cenozoic and slightly higher during the Cretaceous than today. The modelled values for the marine boron isotopes follow the variations of boron isotopes in carbonates over the Cenozoic era provided by previous studies, suggesting that the variations of the seawater pH may not have been important on this time scale. If this is the case, it involves that buffering mechanisms occur in the oceans to maintain seawater pH at a roughly constant value against past atmospheric pCO2 variations. 相似文献
3.
Knowledge of the subduction input flux of nitrogen (N) in altered oceanic crust (AOC) is critical in any attempt to mass-balance N across arc-trench systems on a global or individual-margin basis. We have employed sealed-tube, carrier-gas-based methods to examine the N concentrations and isotopic compositions of AOC. Analyses of 53 AOC samples recovered on DSDP/ODP legs from the North and South Pacific, the North Atlantic, and the Antarctic oceans (with larger numbers of samples from Site 801 outboard of the Mariana trench and Site 1149 outboard of the Izu trench), and 14 composites for the AOC sections at Site 801, give N concentrations of 1.3 to 18.2 ppm and δ15NAir of −11.6‰ to +8.3‰, indicating significant N enrichment probably during the early stages of hydrothermal alteration of the oceanic basalts. The N-δ15N modeling for samples from Sites 801 and 1149 (n = 39) shows that the secondary N may come from (1) the sedimentary N in the intercalated sediments and possibly overlying sediments via fluid-sediment/rock interaction, and (2) degassed mantle N2 in seawater via alteration-related abiotic reduction processes. For all Site 801 samples, weak correlation of N and K2O contents indicates that the siting of N in potassic alteration phases strongly depends on N availability and is possibly influenced by highly heterogeneous temperature and redox conditions during hydrothermal alteration.The upper 470-m AOC recovered by ODP Legs 129 and 185 delivers approximately 8 × 105 g/km N annually into the Mariana margin. If the remaining less-altered oceanic crust (assuming 6.5 km, mostly dikes and gabbros) has MORB-like N of 1.5 ppm, the entire oceanic crust transfers 5.1 × 106 g/km N annually into that trench. This N input flux is twice as large as the annual N input of 2.5 × 106 g/km in seafloor sediments subducting into the same margin, demonstrating that the N input in oceanic crust, and its isotopic consequences, must be considered in any assessment of convergent margin N flux. 相似文献
4.
JOÃO TRABUCHO ALEXANDRE JUAN PEDRO RODRÍGUEZ‐LÓPEZ POPPE L. DE BOER 《Sedimentology》2011,58(5):1217-1246
The Aptian/Albian oceanic anoxic event 1b contains the record of several perturbations in the global carbon cycle and multiple black shale levels, particularly in the Western Tethys. The local lithological expression of an oceanic anoxic event depends on palaeogeographical and depositional setting as well as on regional palaeoclimate. Marine sediments at a particular location may therefore be more or less organic‐rich (or not at all) and they may consist of different lithologies. In most studies, however, much of the lithological variability associated with oceanic anoxic events is left unaccounted for and, thus, the exact processes leading to the enrichment of organic matter in these marine sediments and their subsequent preservation in the geological record are unknown. This study focuses on the local sedimentary processes behind the deposition of organic‐rich sediments at Deep Sea Drilling Project Site 545 and Ocean Drilling Program Sites 1049 and 1276 in the North Atlantic during oceanic anoxic event 1b. Although specifically dealing with the sediments deposited during this particular event at these localities, it is expected that the same processes were responsible for determining the exact sedimentary products at localities in similar settings, as well as during other similar events in the Mesozoic. Here, it is shown that the deposition of organic‐rich sediments during oceanic anoxic event 1b was a consequence of the enhanced productivity favoured by upwelling and by riverine nutrient input, or aeolian fertilization of the euphotic zone depending on geographical location. Slope instability processes resulted in the transfer of part of these organic‐rich sediments from the shelf to deep sea depocentres as mud‐laden organic‐rich turbidites, especially in the northern North Atlantic. The so‐called ‘black shales’ are much more varied than their name implies. The end product of sedimentation during an oceanic anoxic event at a particular location is commonly the result of several equifinal processes acting on a local scale rather than the direct result of basinal or even global mechanisms. 相似文献
5.
古海洋、古气候研究的新工具 总被引：1，自引：1，他引：1
“分子温度计”是通过有机地球化学方法获得的沉积物中烯酮化合物的相对丰度来估算古海水表面温度的。烯酮化合物的不饱和度（Ｕｋ３７）与其生物母源Ｅｍｉｌｉａｎｉａｈｕｘｌｅｙｉ的生长温度密切相关，同时这种信息不受有机质溶解与成岩作用影响，而能较完整地保存于海洋沉积物中，因而通过它能很好地反映古海洋与古气候的演变。这种方法不受盐度、上升流与极地冰盖变化等因素影响，尤其适用于碳酸盐贫乏海区的古海洋与古气候研究 相似文献
6.
Abstract: The occurrences of the Early Archean carbonate minerals are compiled and their precipitation processes are investigated for the Warrawoona Group, Pilbara Craton. Sedimentary carbonate rocks such as limestone and dolostone are very rare, and only a small amount of sedimentary carbonate minerals are sometimes contained in the hydrothermal bedded chert, implying that a sink of CO2 was minor in the Early Archean sediments. Moreover, it is very likely that the activity of cyanobacteria forming stromatolites was considerably low in the Early Archean. Microfossils and carbonaceous matter in the hydrothermal cherts are probably derived from a non-photosynthetic microorganisms related to the seafloor hydrothermal activity. Their preservation in sediments may play a very minor role in carbon sink of the Earth's surface.
On the other hand, carbonatized volcanic rocks subjected to seafloor hydrothermal alteration occur ubiquitously in the Early Archean greenstone belts such as the Warrawoona Group, suggesting that the hydrothermally altered oceanic crust had large amounts of CO2 as carbonate minerals. Global carbon cycle in the Early Archean is considered to have been controlled by the intense seafloor hydrothermal alteration. Large amounts of CO2 were sunk into the oceanic crust by the alteration. The carbonatized oceanic crust was partly accreted to the continents and/or island–arcs, and partly subducted into the mantle without decomposition. Significant amounts of carbonate minerals in the carbonatized oceanic crust were very likely to store in the accretionary prisms and mantle, consequently giving rise to a decrease of atmospheric and oceanic CO2 . 相似文献
On the other hand, carbonatized volcanic rocks subjected to seafloor hydrothermal alteration occur ubiquitously in the Early Archean greenstone belts such as the Warrawoona Group, suggesting that the hydrothermally altered oceanic crust had large amounts of CO
7.
南海东部次海盆的沉积记录蕴含着区域内中中新世以来沉积物的风化过程和演化历史信息.本文分析了国际大洋发现计划IODP 349航次南海东部次海盆U1431站位沉积物的主、微量元素和Sr-Nd同位素特征.研究显示,样品中化学风化蚀变指数为49~74,表明源区的化学风化强度为低到中等强度.沉积物在风化过程中以斜长石风化为主.含有火山碎屑的岩性单元Ⅵ和Ⅶ及55X-2层位受到含Fe、Mg矿物组分的物质来源输入影响,其余沉积物主要来自长英质源区.Sr和Nd同位素特征显示不同风化程度的沉积物源区具有明显差异.通过与周围潜在源区进行对比,推断12.8 Ma至今,U1431站位的物源主要来自珠江流域,印支半岛、吕宋和巴拉望提供了少量物质.其中12.5~7.4 Ma,沉积物源区受到周围岩浆活动形成的基性物质输入的影响,但仍以珠江源区为主.6.5 Ma以后,台湾岛隆升剥蚀的陆源物质进入中央海盆.因此,台湾岛成为源区之一. 相似文献
8.
Jodie K. Fisher Gregory D. Price Malcolm B. Hart Melanie J. Leng 《Cretaceous Research》2005,26(6):853-863
Carbon and oxygen isotope data from Cenomanian–Turonian sediments from the southwest of the Crimea are presented. The sediments consist of limestones, marls and organic-rich claystones, the latter with total organic carbon values up to 2.6 wt. %, representing Oceanic Anoxic Event 2. A shift to more negative δ18O values through the uppermost Cenomanian into the lowermost Turonian may be the result of warming; however, petrographic analysis shows that the samples have undergone a degree of diagenetic alteration. The carbon isotope data reveal a positive excursion from 2.7‰ to a peak of 4.3‰ at the Cenomanian/Turonian boundary; values then decrease in the early Turonian. This excursion is comparable to those of other Cenomanian–Turonian sections, such as those seen in the Anglo-Paris Basin, and is thought to be due to global changes in the oceanic carbon reservoir. On this curve are a number of negative δ13C excursions, just below the Cenomanian/Turonian boundary. It is suggested that these negative excursions are associated with the uptake of light carbon derived from the oxidation and deterioration of organic material during localised exposure of the sediments to oxic or meteoric diagenetic conditions, possibly during sea-level fluctuations. 相似文献
9.
10.
G. N. Baturin 《Geochemistry International》2017,55(5):418-427
Published and original data on the contents of 50 elements in carbonaceous sediments from seas (Black, Baltic, and Caspian) and fertile oceanic shelves (shelves of Namibia, Peru, Chile, and California) are generalized. The comparison of these results with the average composition of ancient carbonaceous shales reveals both similarities and differences in the distribution of indicator trace elements (Re, Hg, Se, Ag, Cd, Tl, U, Mo, As, Ni, and Zn). Correlation coefficients were analyzed to determine the characteristic element associations. It is established that oceanic carbonaceous sediments are closer in composition to carbonaceous shales than their marine analogues, which is related to the differences in sedimentation conditions, including hydrological, hydrochemical, and biogeochemical factors. The role of anoxic environment in the accumulation of chalcophile elements in sediments is estimated. The comparison of the contents of some mobile trace elements in oceanic water and carbonaceous sediments of modern oceans demonstrates that the water composition affects the composition of carbonaceous sediments and can be used for deciphering the composition of ancient ocean water. 相似文献
11.
S. E. Church 《Contributions to Mineralogy and Petrology》1973,39(1):17-32
The isotopic composition of Pb and Sr and the abundance of trace elements in oceanic sediments provide several independent mechanisms for determining the limits of oceanic sediment involvement in andesite genesis. These data, particularly the Th/U values and the Sr87/Sr86 values, indicate that oceanic sediment involvement is probably limited to 2% or less for andesitic magmas in the Cascade Mtns. The isotopic and chemical data on continental sedimentary rocks limit their involvement to 10% or less. The isotopic composition of Pb in all calcic and calc-alkaline or orogenic volcanic rocks however does not depend on crustal materials, and cannot be accounted for by mixing oceanic sediment and oceanic ridge basalt leads in all cases. One is not justified in using the lead growth curve for oceanic sediment as a convenient and arbitrary end member in these mixing model calculations, and therefore the model of Armstrong (1971) does not appear to offer a universal solution. It appears that alkali basalt-like leads may play an important role in the genesis of andesitic rocks. 相似文献
12.
Surface sediment, speleothems, and bat guano from two adjacent, topographically different cave sites in eastern Spain have been studied palynologically to elucidate the potential of cave sediments for palaeoenvironmental reconstruction. A cave opening with a large entrance and constant width presented far fewer problems of alteration in the pollen assemblages than a sac‐like cave opening with a constricted entrance. Pollen concentration is linked primarily to the amount of pollen input rather than to the result of post‐depositional alteration. Sampling should be undertaken away from parietal and rear areas and avoiding moisture zones. Lateral differences in the pollen spectra indicate that sampling should be on the basis of a multiple‐profile approach and selection of dry rather than wet sediments. If these procedures are followed, within‐cave sediments can realistically reflect not only local but also regional vegetation of the site. Copyright © 2000 John Wiley & Sons, Ltd. 相似文献
13.
海洋Nd同位素演化已经成为示踪陆源风化输入和洋流循环改变的最重要的手段之一,得到了越来越多的应用,并取得了许多重要的成果。海水的Nd同位素组成主要受陆源输入物质控制,热液输入几乎可以忽略。由于Nd在海洋中的停留时间(约500～1000a)略小于海水的平均混合时间(约1500a),且各洋盆有不同的Nd同位素风化输入,因此现代各大洋海水具有不同的Nd同位素组成。在陆源输入稳定的情况下,可以利用海水的Nd同位素组成和演化来示踪水体的混合或洋流循环的改变。目前主要依靠对海洋中水成铁锰结壳、海洋钙质有孔虫壳体、磷酸质鱼骨头或鱼牙齿化石以及沉积物中铁锰氧化物组分等的研究来恢复和反演古海水的Nd同位素组成和演化。4种分析材料各有其优缺点。其中,通过对水成铁锰结壳的Nd同位素分析,基本建立了各大洋新生代以来的主要洋流的Nd同位素组成的长尺度演化。通过有孔虫壳体、鱼化石碎片和沉积物中Fe-Mn氧化物组分可以进行高时间分辨率的古海水Nd同位素演化示踪。利用海水Nd同位素演化可以示踪古洋流通道的开启或闭合,以及获得水体交换的直接信息,为研究构造运动与气候变化之间的关系提供指示。同时,将海水Nd同位素演化与气候变化的指标结合起来,可以用于示踪各种气候条件下洋流循环的改变,将洋流循环的改变与气候变化联系起来,研究两者之间的成因关系。对表层水体的Nd同位素组成的研究则可以示踪不同气候条件下大陆陆源风化输入的改变。 相似文献
14.
We have analyzed 25 trace elements (e.g., Sb, Tl, Sn, rare earth elements (REE), Th, U, Nb, Pb, Zr, Hf, and Y) in altered mid-ocean ridge basalts (MORB) from locations near the mouth of the Gulf of California. Our results imply that the heavy REE and Y are not seriously affected by seawater alteration, in agreement with previous studies. The elements Zr, Hf, Nb, light REE and Sr are enriched up to a factor of 2 in some extremely altered samples. However, element ratios between Zr, Hf, and Nb (e.g., Zr/Hf, and Zr/Nb) are not greatly affected, presumably due to the chemical similarity of these elements during any exchange process. The enrichment of Th and Sn is even higher. Antimony, Tl, Cs, Rb, Rb, and Ba are most easily altered by water-rock interaction and are therefore the best indicators for seawater alteration. The enrichment factor of the most mobile element Sb is up to 2000.
There is a weak correlation between the concentration in seawater and the enrichment factors. On the other hand, the worldwide pelagic clay pattern matches the enrichment pattern much more closely, and the limited data available for local oceanic sediments give an even better correlation. A plausible model to explain the enrichment pattern may be an elemental exchange between basalt and seawater that had interacted earlier with overlying sediments. 相似文献
15.
The distribution of Mn was examined in the bottom sediments and water column (suspended paniculate matter) of the Laurentian Trough. Gulf of St. Lawrence. A characteristic profile of Mn with depth in the sediment consisted of a Mn-enriched surface oxidized zone, less than 20 mm thick, and a Mn-depleted subsurface reducing zone. A subsurface Mn maximum occurred within the oxidized zone. Below this maximum the concentration dropped sharply to nearly constant residual levels in the reducing zone. The accumulating estuarine sediments are deficient in Mn compared to the river input of suspended matter and are definitely not the ultimate sink for manganese. Manganese escapes from the sediment by diffusion and resuspension, forming Mn-enriched, fine-grained particles which are flushed out in the estuarine circulation. 5.0 × 109gyr?1 of Mn, or 50% more than the river input of dissolved Mn. are exported to the open ocean. In spite of the efficient mobilization and export of Mn, the quantity exported is a small fraction (0.2%) of the total flux to the deep-sea sediments. This is related to the low levels of paniculate matter transported by the St. Lawrence River. The export phénomenon, however, is probably true of many coastal regions of muddy sediments and thus has interesting implications for the oceanic budget of Mn. 相似文献
16.
Shark Bay is an 8000 sq. km shallow marine embayment on the western coast of Western Australia. The waters exhibit a well established salinity gradient from oceanic to hypersaline. The chemical assemblage of sediment hydrocarbons along the salinity gradient may be classified into two distinct chemogeographic types. Firstly, oceanic sediments contain n-alkanes and a suite of highly branched and branched/cyclic C25 alkenes. Hypersaline sediments are characterised by a high relative abundance of a C25H50 alkene together with an analogous C20H40 alkene and its parent C20H42 alkene (2,6,10-trimethyl-7-(3-methylbutyl)-dodecane). A pair of alkanes C21H42 and C22H44 increase in concentration and relative abundance with depth. The hydrocarbons of the hypersaline basins are found in only trace amounts in oceanic sediments. These chemical signals are overlain by further input indicative of the immediate biotic community. 相似文献
17.
Upper Miocene to Holocene sediments from the Cascadia accretionary prism and its oceanic surroundings drilled during ODP Leg 146 are studied in order to reveal their alteration during the accretion. The conclusion is made that methane-bearing solutions play a leading role in the transportation of material and the formation of mineralogical-geochemical zonality within the prism. A considerable intensity and high rates of epigenetic alteration are noted. It is shown that low heat flow, absence of progressive subsidence of the accretionary prism, open character of the system relative to water circulation, and heterogeneity of the sedimentary sequence hindered the successive development of epigenesis. 相似文献
18.
Studies of hydrothermal circulation within partly buried basement on the eastern flank of the Juan de Fuca Ridge (JFR) have shown that ridge-flank geochemical fluxes are potentially important for the global budgets of some elements. There are major uncertainties in these flux calculations, however, because the composition of these basement fluids is strongly dependent on temperature and because they may be modified by interaction with the overlying terrigenous sediments, either by diffusive exchange with basement or during upwelling to the seafloor. To better understand the nature and temperature control of basalt-fluid and sediment-fluid reactions at the JFR flank, we have conducted laboratory experiments between 51 and 350°C and at 400 bars pressure. K, Rb, and Si are leached from basalt between 150 and 351°C, and Sr and U are taken up. The direction of exchange of Li and Ca with basalt varies with temperature. Li and Sr are removed from fluid at 150°C, but isotope studies show that there is simultaneous release of both elements from basalt, indicating that uptake is controlled by the formation of secondary minerals. Moreover, our experiments confirm that Sr isotope exchange with oceanic crust occurs at moderate temperature and is not confined to high-temperature axial hydrothermal systems. Our data and field data from the JDR flank indicate that uptake of U into basalt at moderate temperature could remove between 9.9 and 15 × 106 mol U yr−1 from the oceans. This is higher than a recent estimate based on measurements of U in altered ocean crust (5.7 ± 3.3 × 106 mol yr−1), which concords with arguments that the Δelement/heat ratios of JDR flank fluids are too large to be representative of average global flank fluids. K, Ca, Sr, Ba, Li, Si, and B are leached from terrigenous sediments between 51 and 350°C, and U is taken up. Cs and Rb are removed from the fluid below 100°C and leached from the sediment at higher temperature. Sr isotope data show that Sr is preferentially mobilised from volcanic components within terrigenous sediments, which may lead to an overestimation of the ridge-flank Sr isotope flux at the JDR if there is exchange of sediment pore fluids with basement. 相似文献
19.
The North Penninic basin was a subbasin in the northern part of the Mesozoic Tethys ocean. Its significance within the framework of this ocean is controversial because it is not clear whether it was underlain by thinned continental or oceanic crust. Remnants of the eastern North Penninic basin are preserved in the Alps of eastern Switzerland (Grisons) as low metamorphic "Bündnerschiefer" sediments and associated basaltic rocks which formed approximately 140–170 Ma ago (Misox Bündnerschiefer zone, Middle Jurassic to Early Cretaceous). Nb/U, Zr/Nb, and Y/Nb ratios, as well as Nd–Sr isotopic and REE data of most of the metabasalts point to a depleted MORB-type mantle origin. They have been contaminated by magmatic assimilation of Bündnerschiefer sediments and by exchange with seawater, but do not prove the existence of a subcontinental lithospheric mantle or continental crust beneath the North Penninic basin. This suggests that the studied part of the North Penninic realm was underlain by oceanic crust. Only the metabasalts from two melange zones (Vals and Grava melanges) show a more important contamination by crustal material. Since this type of contamination cannot be observed in the other tectonic units, we suggest that its occurrence is related to melange formation during the subduction of the North Penninic basin in the Tertiary. The North Penninic basin was probably, despite the occurrence of oceanic crust, smaller than the South Penninic ocean where the presence of oceanic crust is well established. Modern analogues for the North Penninic basin could be the transitional zone of the Red Sea or the pull-apart basins of the southernmost Gulf of California where local patches of oceanic crust with effusive volcanism have been described. 相似文献
20.
寒武纪晚期到奥陶纪早期的海洋动物多样性整体水平较低,生物地球化学研究认为可能与海洋氧化还原状态波动有关,但仍证据较少。保存良好的海相碳酸盐岩沉积被认为能够记录古代海水的地球化学信息,其铀同位素组成 (δ238U) 可用来反映全球海洋的氧化还原状态。文章测定了华南瓦儿岗剖面寒武系第十阶底部海相碳酸盐岩的δ238U值,结果显示在寒武纪第十期早期U同位素组成可能存在三次负漂移,对应的δ238U值分别为-0.8‰、-0.55‰和-0.60‰,指示三个海洋缺氧时段。通过U同位素质量平衡模型计算得出,三个缺氧时段全球海洋底层水体分别约有22％、3.5%和5%的缺氧面积。初步推断第一次缺氧可能与风化输入营养元素增强致初级生物生产力提高有关,而其后的两次缺氧可能与原先的海底缺氧水体在海侵阶段上涌扩散有关。 相似文献