南海沉积物中U,Th分布特征及其古环境意义   总被引：1，自引：0，他引：1  

温孝胜  刘韶  张惠玲  秦佩玲  赵焕庭 《热带海洋学报》1997,(3)

对采自南海深海中的两个柱样进行了分析。沉积速率分别为6.2cm·ka－1（317－82－25柱）和4．2cm·ka-1（90－37柱），均明显大于其他深海沉积速率，说明了南海这个边缘海的“放大效应”。此外，还分析了采自珠江口至外陆架的表层样，总结出从几元素在平面上的分布规律：从河口一陆架边缘～半深海，U，几含量的变化趋势均为多～少一多，Th／U比为小→大→小；而碳酸盐含量则显示出少→多→少的分布规律，即U，Th的含量与碳酸盐含量成反比，这可能是碳酸盐的所谓“稀释效应”所致。铀含量随柱样深度的变化曲线基本上与氧同位素曲线相吻合，其相关系数达0．67,证明U含量变化可能具有气候意义。Th的高含量点亦落在冷期之内。文中还探讨了水中铀的来源去向，说明了它能反映气候变化的原因。  相似文献   

Spatial and Temporal Distribution of Oxidation Events Occurring Below the Sediment-Water Interface     

Stefan  Forster 《Marine Ecology》1996,17(1-3):309-319

Abstract. Irrigation and bioturbation lead to transport of dissolved oxygen into anoxic sediments. The depthdistribution of local oxygen input and the total time of oxygen presence was measured at randomly sampled locations within anoxic sediments, originating from the North Sea.
In the laboratory, continuous redox potential records, displaying a transient increase and decrease when in contact with oxygen for a limited time, were used to record oxidation events'. Oxygen microelectrodes were used to confm the presence of oxygen. Measurements were performed for 180 d at 230 locations in the top 6 cm of sediment cores containing the natural macrofauna community.
4783 oxidation events m^-2· d^-1 were recorded within the upper 6 cm of the sediment. The number and duration of oxidation events declined with sediment depth below the oxic zone. Oxygen was present in the anoxic sediment, as determined from redox potential measurements, ≥ 6 h per day at 10% of the randomly chosen locations within the upper 3 cm. The overall distribution of oxidation events and their duration suggest that local, pulsed additions of oxygen by irrigation may be sufficient to maintain an oxidised sediment layer ( sensu J orgensen amp; R evsbech , 1989). Oxic environments along burrow walls rapidly fluctuate between oxic and anoxic conditions. Using oxygen microelectrodes the presence of oxygen (oxic conditions) in these halos was found to range from 2 to 12 h per day. Continuous redox measurements show that oxidised conditions fluctuate with the oxygen pulses and display the same durations, although these may range up to 21 h per day. Oxic and oxidised sediment volumes are estimated to represent < 1% and 3.7%. respectively, of the anoxic sediment to 6 cm depth. Recognition of temporal variability and spatial heterogeneity of sedimentary conditions may prove valuable for future conclusions drawn in other research fields.  相似文献   

台湾地区湖泊水库悬浮颗粒有机质之碳、氢、氧、氮、硫元素计量分析   总被引：1，自引：0，他引：1  

黄炳达  陈镇东 《海洋与湖沼》1994,25(1):29-37

对台湾地区１８个湖泊水库水体中悬浮颗粒有机质之碳，氢，氧，氮，硫和叶绿素α的含量进行了分析，其中ＰＯＯ乃首度以元素分析仪直接测量。结果为，ＰＯＣ，ＰＯＨ，ＰＯＯ，ＰＯＮ，ＰＯＳ含量分别介于１３８－８３７０μｇ／Ｌ，１３．７－９２６．１μｇ／Ｌ，３１－２６２３μｍ／Ｌ，１４－１２６５μｇ／Ｌ，１．９－４９．７μｇ／Ｌ之间，Ｃｈ１．ａ含量则介于０．３１－９６．７５μｇ／Ｌ之间，ＰＯＭ元素间原子数关系为  相似文献   

The trophic ecology of key megafaunal species at the Pakistan Margin: Evidence from stable isotopes and lipid biomarkers     

Rachel M. Jeffreys  George A. Wolff  Sarah J. Murty 《Deep Sea Research Part I: Oceanographic Research Papers》2009,56(10):1816-1833

The Arabian Sea is subject to intense seasonality resulting from biannual monsoons, which lead to associated large particulate fluxes and an abundance of organic carbon, a potential food source at the seafloor for benthic detritivores. We used the stable isotopes of carbon and nitrogen alongside lipid analyses to examine potential food sources (particulate and sedimentary organic matter, POM and SOM respectively) in order to determine trophic linkages for the twelve most abundant megafaunal species (Pontocaris sp., Solenocera sp., Munidopsis aff. scobina, Actinoscyphia sp., Actinauge sp., Echinoptilum sp., Pennatula aff. grandis, Astropecten sp. Amphiura sp. Ophiura euryplax, Phormosoma placenta and Hyalinoecia sp.) at the Pakistan Margin between 140 and 1400 m water depth. This transect spans a steep gradient in oxygen concentrations and POM flux. Ranges of δ¹³C and δ¹⁵N values were narrow in POM and SOM (4‰ and 2‰ for δ¹³C and δ¹⁵N, respectively) with little evidence of temporal variability. Labile lipid compounds in SOM originating from phytoplankton did exhibit seasonal change in their concentrations at the shallowest sites, 140 and 300 m. Benthic megafauna had broad ranges in δ¹³C and δ¹⁵N (>10‰ and >8‰ for δ¹³C and δ¹⁵N, respectively) suggesting they occupy several trophic levels and utilize a variety of food sources. There is evidence for feeding niche separation between and within trophic groups. Lipid biomarkers in animal tissues indicate a mixture of food sources originating from both phytoplankton (C_20:5(n-3) and C_22:6(n-3)) and invertebrate prey (C_20:1 and C_22:1). Biomarkers originating from phytodetritus are conserved through trophic transfer to the predator/scavengers. Six species (Pontocaris sp., Solenocera sp., Actinoscyphia sp., Echinoptilum sp., Amphiura sp. and Hyalinoecia sp.) showed a significant biochemical response to the seasonal supply of food and probably adapt their trophic strategy to low food availability. Biotransformation of assimilated lipids by megafauna is evident from polyunsaturated fatty acid distributions, for example, Echinoptilum sp. converts C_20:5(n-3) to C_24:6(n-3).  相似文献   

Evaluating microbial chemical choices: The ocean chemistry basis for the competition between use of O2 or NO3− as an electron acceptor     

《Deep Sea Research Part I: Oceanographic Research Papers》2014

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Crystallization conditions of magma from Longmen potassic pluton of the Trans-North China Orogen,North China Craton: Constraints from mineral chemistry and zircon trace elementSCIEI北大核心CSCD     

唐宗源  李杰  邓昌州  郑涵  刘少泽 《岩石学报》2023,(5):1370-1386

华北克拉通中部造山带发育的早白垩世钾质岩是研究华北克拉通中部幔源岩浆成因的天然样品,然而其成岩物理化学条件仍不明确。本文选取了涞源县龙门岩体中闪长岩和二长岩开展了矿物原位地球化学和锆石微量元素分析,以探讨矿物形成的温压条件及氧逸度与矿化的关系。分析结果显示,二长岩和闪长岩的锆石Th/U比值较高(>0.1),轻稀土亏损、重稀土富集,具明显的Ce正异常和Eu负异常特征,并具有明显的震荡环带,为典型岩浆成因锆石。电子探针结果显示,龙门岩体中斜长石主要为中性斜长石,黑云母为原生镁质黑云母,角闪石主要为钙铁闪石。闪长岩中角闪石结晶温度为793~842℃,压力为0.50~0.75GPa,深度范围为19~28km,具有较低氧逸度(log f O 2为-12.21~-11.38)和高的含水量(8.5%~10.75%);二长岩中黑云母结晶温度为764~788℃,具有更低的氧逸度(log f O 2=-15.14~-14.54);闪长岩和二长岩中锆石结晶温度为770~978℃,具有较低的氧逸度(ΔFMQ=-0.37~+1.70)。矿物化学分析表明,角闪石和黑云母虽都在地壳开始结晶,但角闪石形成于比黑云母更深的岩浆房。龙门岩体中角闪石、黑云母和锆石的结晶主要受岩浆分异控制,其地球化学动力学机制主要为岩浆上侵时减压熔融,进而引起岩浆氧逸度随岩浆演化而变化。随着岩浆上涌,闪长岩中角闪石随着温度降低和压力减少逐渐结晶,地幔交代作用导致二长岩中的黑云母具有较高的X Mg值,进而形成镁质黑云母。结合区域地质背景,古太平洋板块(伊佐奈琦板块)俯冲-后撤释放的流体交代上覆岩石圈地幔对中部造山带钾质岩(~141Ma)的形成有一定贡献,该过程导致了岩浆具有较高的含水量,但龙门岩体低的氧逸度和区域上较厚的岩石圈制约了成矿金属物质(Fe-Au等)的迁移和富集,因而不利于亲硫、亲铁元素聚集以及铁、金矿化的形成。  相似文献   

兴蒙造山带北部岩石圈地幔橄榄岩氧逸度特征研究     

刘金霖  李怀滨  王建  张云峰 《岩石学报》2021,37(7):2073-2085

在大兴安岭北部的诺敏和科洛地区的新生代玄武岩中发现了尖晶石相的橄榄岩包体。地幔橄榄岩中橄榄石的Mg~#说明了研究区上地幔具有部分难熔的特点。在橄榄石含量与Fo图解中,有一部分橄榄岩包体落在太古代和元古代的地幔区域,揭示了研究区的岩石圈地幔存在古老岩石圈地幔的残余。研究区方辉橄榄岩与二辉橄榄岩有显示高氧逸度值FMQ+1.95～3.01,这与一般情况下相对还原的古老岩石圈地幔的低氧逸度值形成鲜明对比,可能为古生代的古亚洲洋以及中生代的古太平洋相继俯冲到了兴蒙造山带之下,导致当时岩石圈地幔的氧化所致。在地幔包体的反应边中发现了富钾熔体(K20 1%-6%),这被认为研究区地幔经历了多期富钾流体活动,富钾流体的来源可能与俯冲再循环的壳源物质有关。  相似文献   

大叶藻(Zostera marina)的热值和元素含量(碳、氮、磷)及其相关性     

杨贵福  邢坤  李耕  刘海映  潘玉洲  张力 《海洋与湖沼》2015,46(1):212-220

选取辽宁獐子岛近岸海域大叶藻样品,对其须根、根状茎和不同生长阶段叶片的灰分含量、热值和元素含量(碳、氮、磷)及其相关性进行研究,结果表明:在不同生长阶段,叶片长度随着生长顺序先增大后减小;灰分含量随着叶片生长逐渐升高,且极显著小于根状茎和须根(P0.01);不同部位干质量热值差异极显著(P0.01),以初生叶最高,为(14.89±0.040)k J/g,后逐渐减小,在须根中最小,为(8.15±0.079)k J/g;不同生长阶段叶片的去灰分热值差异不大,但极显著大于须根和根状茎(P0.01);碳、氮、磷含量均呈同一趋势:初生叶幼叶成熟叶1成熟叶2衰老叶根状茎须根;N/P比值为27.08,说明大叶藻存在P限制;N/P比值在根状茎中最大,须根中最小,这说明大叶藻存在能量的转移和存贮;大叶藻不同部位灰分含量与干质量热值、去灰分热值、碳含量、氮含量、磷含量之间呈极显著的负相关(P0.01),干质量热值与碳含量、氮含量、磷含量之间呈极显著的正相关(P0.01);大叶藻不同部位的热值与碳、氮、磷元素含量之间均呈显著的线性关系(P0.05)。  相似文献   

Heavy ion formation in Titan's ionosphere: Magnetospheric introduction of free oxygen and a source of Titan's aerosols?     

E.C. Sittler Jr.  A. Ali  J.F. Cooper  R.E. Johnson  D.T. Young 《Planetary and Space Science》2009,57(13):1547-17884

Discovery by Cassini's plasma instrument of heavy positive and negative ions within Titan's upper atmosphere and ionosphere has advanced our understanding of ion neutral chemistry within Titan's upper atmosphere, primarily composed of molecular nitrogen, with ~2.5% methane. The external energy flux transforms Titan's upper atmosphere and ionosphere into a medium rich in complex hydrocarbons, nitriles and haze particles extending from the surface to 1200 km altitudes. The energy sources are solar UV, solar X-rays, Saturn's magnetospheric ions and electrons, solar wind and shocked magnetosheath ions and electrons, galactic cosmic rays (GCR) and the ablation of incident meteoritic dust from Enceladus’ E-ring and interplanetary medium. Here it is proposed that the heavy atmospheric ions detected in situ by Cassini for heights >950 km, are the likely seed particles for aerosols detected by the Huygens probe for altitudes <100 km. These seed particles may be in the form of polycyclic aromatic hydrocarbons (PAH) containing both carbon and hydrogen atoms C_nH_x. There could also be hollow shells of carbon atoms, such as C₆₀, called fullerenes which contain no hydrogen. The fullerenes may compose a significant fraction of the seed particles with PAHs contributing the rest. As shown by Cassini, the upper atmosphere is bombarded by magnetospheric plasma composed of protons, H₂⁺ and water group ions. The latter provide keV oxygen, hydroxyl and water ions to Titan's upper atmosphere and can become trapped within the fullerene molecules and ions. Pickup keV N₂⁺, N⁺ and CH₄⁺ can also be implanted inside of fullerenes. Attachment of oxygen ions to PAH molecules is uncertain, but following thermalization O+ can interact with abundant CH₄ contributing to the CO and CO₂ observed in Titan's atmosphere. If an exogenic keV O+ ion is implanted into the haze particles, it could become free oxygen within those aerosols that eventually fall onto Titan's surface. The process of freeing oxygen within aerosols could be driven by cosmic ray interactions with aerosols at all heights. This process could drive pre-biotic chemistry within the descending aerosols. Cosmic ray interactions with grains at the surface, including water frost depositing on grains from cryovolcanism, would further add to abundance of trapped free oxygen. Pre-biotic chemistry could arise within surface microcosms of the composite organic-ice grains, in part driven by free oxygen in the presence of organics and any heat sources, thereby raising the astrobiological potential for microscopic equivalents of Darwin's “warm ponds” on Titan.  相似文献   

The East Asian monsoon during MIS 2 expressed in a speleothem δO record from Jintanwan Cave, Hunan, China     

Jason Cosford  Hairuo Qing  Yin Lin  Bruce Eglington  Dave Mattey  Yue Gau Chen  Meiliang Zhang  Hai Cheng 《Quaternary Research》2010,73(3):541-549

Stalagmite J1 from Jintanwan Cave, Hunan, China, provides a precisely dated, decadally resolved δ¹⁸O proxy record of paleoclimatic changes associated with the East Asian monsoon from ∼29.5 to 14.7 ka and from ∼12.9 to 11.0 ka. At the time of the last glacial maximum (LGM), the East Asian summer monsoon weakened and then strengthened in response to changes in Northern Hemisphere insolation. As the ice sheets retreated the East Asian summer monsoon weakened, especially during Heinrich event H1, when atmospheric and oceanic teleconnections transferred the climatic changes around the North Atlantic to the monsoonal regions of Eastern Asia. A depositional hiatus between ∼14.7 and 12.9 ka leaves the deglacial record incomplete, but an abrupt shift in δ¹⁸O values at ∼11.5 ka marks the end of the Younger Dryas and the transition into the Holocene. Comparisons of the J1 record to other Chinese speleothem records indicate synchronous climatic changes throughout monsoonal China. Further comparisons to a speleothem record from western Asia (Socotra Island) and to Greenland ice cores support hemispherical-scale paleoclimatic change. Spectral and wavelet analyses reveal centennial- and decadal-scale periodicities that correspond to solar frequencies and to oscillations in atmospheric and oceanic circulation.  相似文献