内蒙古阿巴嘎旗阿德拉嘎碱长花岗岩锆石LA- ICP- MS U- Pb年龄、地球化学特征及构造意义

阿巴嘎旗阿德拉嘎碱长花岗岩位于贺根山蛇绿岩带北侧。为了确定该碱长花岗岩体的岩石成因类型,探讨其构造环境,对该岩体进行了野外地质、岩石学、地球化学和LA-ICP-MS锆石U-Pb年代学研究。锆石LA-ICP-MS U-Pb测年表明,阿德拉嘎碱长花岗岩体的侵位年龄为310.7±2.6 Ma,形成时代为晚石炭世。岩石地球化学研究表明,阿德拉嘎碱长花岗岩具有较高的SiO₂、Na₂O+K₂O含量和较高的Ga/Al、(Na₂O+K₂O)/CaO值,相对贫CaO、MgO、Sr、Ba、Eu、Ti和P。稀土元素总量较低,轻重稀土分馏不明显,稀土配分曲线呈海鸥性,负铕异常明显(δEu=0.15～0.37)。岩石学和岩石地球化学特征表明,该碱长花岗岩为A型花岗岩,形成于弧后伸展构造环境,为晚石炭世古亚洲洋向西伯利亚俯冲作用的产物。     

内蒙古巴林右旗胡都格绍荣岩体的年代学、地球化学、Hf同位素特征及构造背景

大兴安岭地区晚中生代的大地构造背景一直存在争议,通过对内蒙古巴林右旗胡都格绍荣岩体进行锆石U-Pb测年、岩石地球化学以及锆石Lu-Hf同位素分析,探讨其形成时代及构造背景.胡都格绍荣岩体主体岩性为似斑状黑云母二长花岗岩,LA-ICP-MS锆石U-Pb测年确定其加权平均年龄为129.9±1.4 Ma(MSWD=0.91),指示其侵位于早白垩世.花岗岩具有高SiO₂、Na₂O、K₂O含量,低CaO、MgO含量,富集Cs、Rb、K、Th、U、Zr,亏损Ba、Sr、P、Ti,轻稀土富集,具明显Eu负异常(δEu=0.35~0.44),10 000×[w(Ga)/w(Al)]为2.08~3.05,表明其为典型的A型花岗岩.Hf同位素分析结果显示,锆石具有正的ε_Hf(t)值(2.24~9.41),Hf两阶段模式年龄为1 030~570 Ma,平均为809 Ma,结合其微量元素特征,认为岩浆来源于新元古代地壳的部分熔融.胡都格绍荣花岗岩指示研究区在早白垩世为伸展构造背景,可能与蒙古-鄂霍茨克洋闭合关系更为密切.      

内蒙古沙麦钨矿花岗岩岩石地球化学、锆石U-Pb年代学及其地质意义

沙麦钨矿床位于内蒙古东乌旗地区,是该区目前已探明的中型岩浆热液型钨矿床。矿体主要赋存在黑云母二长花岗岩和黑云母二长花岗斑岩中,对这两种花岗质岩石的岩相学、岩石地球化学和LA-ICP-MS锆石U-Pb年代学进行了研究。结果表明,黑云母二长花岗岩锆石U-Pb年龄为135.6±1.6 Ma和136.3±1.8 Ma,黑云母二长花岗斑岩锆石U-Pb年龄为138.6±1.1 Ma,二者侵位时间均为早白垩世。两种花岗质岩体具有富SiO₂(73.73%～78.23%)、高钾钠(Na₂O+K₂O)(7.56%～8.89%)、贫MgO(0.09%～0.20%)、贫CaO(0.51%～0.89%)、贫TiO₂(0.03%～0.12%)的特征,属于过铝质-高钾钙碱性系列;微量元素富集Rb、K、Th和U,相对亏损Sr、Ba、Nb、P和Ti元素,具有强烈的Eu负异常,具有较高的FeO^T含量,较高的FeO^T/MgO和FeO^T/(FeO^T+M...     

大别造山带汤池早白垩世富碱侵入岩成因及地质意义

本文对大别造山带北淮阳东段汤池地区早白垩世富碱侵入岩进行岩石学、锆石U-Pb年代学、岩石地球化学及锆石Lu-Hf同位素分析,揭示其成因及地质意义。该套岩石主要由正长花岗岩、石英正长岩和正长斑岩组成,伴有辉绿玢岩发育。锆石U-Pb定年结果显示,辉绿玢岩、正长花岗岩和正长斑岩分别形成于130.3±1.7 Ma、128.4±1.7 Ma和122.3±1.5 Ma,为早白垩世岩浆活动的产物。汤池辉绿玢岩相对贫硅(SiO₂=45.23～56.92 wt.%)和富碱(Na₂O+K₂O=5.24～8.04 wt.%),Mg^#值较高(平均值为48);而其他岩类具有高硅(SiO₂=62.44～77.25 wt.%)、高碱(Na₂O+K₂O=7.97～10.35 wt.%)、低CaO含量以及较高的Ga/Al和FeO^T/MgO比值,与典型的A型花岗岩化学特征相似。辉绿玢岩大多数锆石ε_Hf(t)值变化范围为-6.4...     

海南加茂地区红峰队岩体锆石U-Pb年代学、Hf同位素及其对构造环境的指示

本文在野外地质调查的基础上,对海南加茂地区红峰队细中粒黑云母正长花岗岩体进行锆石年代学、Hf同位素及地球化学等特征的深入研究,以揭示该岩体形成的构造环境。结果显示,红峰队花岗岩体锆石LA-ICP-MS U-Pb年龄为259.5±1.3 Ma,形成于晚二叠世;具有高硅(SiO₂=72.26%～75.69%)、富碱(K₂O+Na₂O=8.51%～9.18%),高钾(K₂O/Na₂O=1.13～1.7),贫CaO(0.38%～0.75%)和P₂O₅(0.01%～0.02%)等地球化学特征,A/CNK值为0.99～1.08,属于准铝质-弱过铝质花岗岩;富集Rb、Th、U、K、Pb、Nd、Zr、Hf、Sm和轻稀土,明显亏损Ba、Nb、Ta、Sr、P、Eu、Ti,具强烈的负Eu异常;锆石饱和温度也较低(767～796℃);显示该岩体属于高分异I型花岗岩;ε_Hf(t)值变化较小(+3.0～+7.3),反映了其岩浆来源较为均一。...     

川西九龙白台花岗岩地球化学特征、锆石U-Pb年龄和Hf同位素组成及其稀有金属成矿意义

为揭示川西九龙白台花岗岩成因及其与稀有金属成矿的关系,笔者等对白台花岗岩开展了岩相学、岩石地球化学、LA-ICP-MS锆石U-Pb年代学、锆石微量元素地球化学、Hf同位素地球化学测试。结果显示,白台黑云母二长花岗岩具高SiO₂(69.01%～70.55%)、高K₂O(3.86%～4.99%)、高碱(K₂O+Na₂O=7.41%～8.18%),低CaO(1.49%～2.2%)、低MgO(0.44%～0.57%)等特征,里特曼指数σ=2.03～2.43,A/CNK=1.07～1.14,为弱过铝质的高钾钙碱性系列岩石;微量元素特征显示相对富集Rb、K等大离子亲石元素,相对亏损Nb、P、Hf等高场强元素;球粒陨石标准化的稀土元素配分模式为明显的轻稀土富集和重稀土亏损的右倾型。白台黑云母二长花岗岩锆石U-Pb年龄为(213～212)Ma,ε_Hf(t)值为-7.4～-1.1,Hf同位素二阶模式年龄T_DM2为(1.6～1.2)Ga。研究结果表明,白台花岗岩形成于后碰撞伸...     

湘东光明萤石矿黑云母花岗岩地球化学特征及其对萤石成矿的启示

光明萤石矿产出于湘东锡田岩体北部,为探究矿区内黑云母花岗岩与萤石成矿的关联,对岩体和萤石矿体进行了系统的地球化学研究,并利用LA-(MC)-ICP-MS对黑云母花岗岩中锆石开展了U-Pb年代学、微量元素及Hf同位素地球化学研究。结果显示,黑云母花岗岩具有高硅(SiO₂=72.62%～77.34%)、高碱(Na₂O+K₂O=6.03%～8.66%)、富铝(Al₂O₃=12.02%～13.83%)特征,A/CNK值介于1.07～1.14之间,为过铝质花岗岩。3个样品低U锆石的²⁰⁶Pb/²³⁸U年龄加权平均值在215～218 Ma之间,指示花岗岩侵位于印支期。矿区黑云母花岗岩印支期—燕山期锆石年龄为237～133 Ma,在230～210 Ma、190～170 Ma、150～130 Ma存在3个较集中的年龄峰期,暗示岩浆侵位后受到热事件影响,推测矿区岩浆活动具有多阶段性。黑云母花岗岩岩体有较强的负Eu异常,且富集大离子亲石元素Rb、Th、U...     

南蒙古额尔德尼早白垩世A型花岗岩年代学、地球化学、Hf同位素特征及其地质意义

南蒙古额尔德尼(Erdene)花岗岩体位于整个东北亚巨量白垩纪花岗岩浆活动的西缘。本文对南蒙古额尔德尼地区花岗岩进行了锆石U-Pb年代学、岩石地球化学和锆石Hf同位素研究,以确定其形成时代、岩石成因及大地构造背景。研究结果表明：额尔德尼地区花岗岩岩石类型主要为黑云母花岗岩。LA-ICP-MS锆石U-Pb定年结果为(123.4±1.4)Ma,形成于早白垩世。岩石具有高硅(w(SiO₂)为71.01%～72.66%)、富碱(w(Na₂O+K₂O)为8.52%～8.90%)、贫磷(w(P₂O₅)为0.06%～0.11%)、贫镁钙(w(MgO)为0.27%～0.39%,w(CaO)为1.10%～1.27%)的特征,铝饱和指数A/CNK为1.05～1.07,属于弱过铝质岩石;富集Rb、U、Th等大离子亲石元素和Ta、Zr、Hf等高场强元素,亏损Nb、Sr、Ba等高场强元素,具有明显的Eu负异常(δEu=0.11～0.15),岩浆平均温度为816℃,属A₁型花岗岩,形...     

内蒙古海拉斯图乌拉A型花岗岩年代学、地球化学特征及其构造意义

内蒙古苏尼特左旗查干敖包镇南部紧邻中蒙边境线海拉斯图乌拉一带发育的一套钠铁闪石霓辉石碱性花岗岩,是二连—贺根山构造带的重要组成部分,通过对其进行年代学、地球化学研究,以探讨区域构造演化。锆石LA-ICP-MS U-Pb同位素年龄测试结果显示该岩体的侵位年龄为(285.4±1.1) Ma,属早二叠世。岩石地球化学研究表明该岩石具高硅、富碱、准铝、贫镁钙的特点,其化学成分SiO₂含量为76.12%~80.10%,Na₂O+K₂O含量为7.62%~9.19%,MgO含量为0.06%~0.10%,CaO含量为0.11%~0.20%,碱性指数(K₂O+Na₂O)/Al₂O₃=0.98~1.04,属于碱性岩系,岩石稀土总量偏低,轻、重稀土元素分馏明显,δEu 为0.37~0.51,Eu强烈亏损,属造山后伸展事件的产物。其成因可能和华北板块与西伯利亚板块对接后的伸展作用有关,指示二连—贺根山构造带在早二叠世可能已进入造山后演化阶段。     

东昆仑东段早泥盆世“A”型花岗岩的确定——来自乌兰东地区都南哑合黑云母花岗岩锆石U-Pb年代学、元素地球化学证据

都南哑合岩体位于东昆仑东段乌兰东呼德生地区,通过对岩体锆石U-Pb定年和岩石地球化学进行研究,分析该岩体成因及构造背景。结果表明：都南哑合岩体主要为黑云母花岗岩,锆石²⁰⁶Pb/²³⁸U加权平均年龄为(413.3±2.1) Ma,岩体结晶年龄为早泥盆世;岩石属准铝质-过铝质高钾钙碱性系列,具高硅,SiO₂=71.13%～74.67%、富碱,Na₂O+K₂O=8.3%～9.26%,低铝,Al₂O₃=12.28%～13.56%、贫钛,0.15%～0.31%、贫镁,0.22%～0.34%及富钾特征。K₂O/Na₂O=0.69～1.64,平均1.36;稀土元素分布曲线呈强负铕,δEu=0.18～0.42,平均0.26,异常轻稀土富集的右倾型;富集大离子亲石元素Rb,K和高场强元素Th,La,Ce,Nd。Ba相对亏损,Sr强亏损;明显亏损高场强元素P,Ti,弱富集Nb,Ta,Sm,Zr,Hf,Y,Yb...     

Research Progress of Long-term Ocean Temperature Changes in the Southern Ocean

In the recent decades， a large amount of anthropogenic heat has been absorbed and stored in the Southern Ocean. Results from observations and climate models' simulations both show that the Southern Ocean displays large warming in the upper and subsurface ocean that maximizes at 45°~40°S. However， the underlying mechanisms and evolution processes of the Southern Ocean temperature changes remain unclear， leaving the Southern Ocean to be a hotspot of climate change studies in the recent years. The present study summarized the current progress in the observations and numerical modeling of long-term temperature changes in the Southern Ocean. The effects of changes in wind， surface heat flux， sea-ice and other factors on the ocean temperature changes were presented， along with the introduction to the role of oceanic mean circulation and eddies. The present study further proposed that a deepening of the understanding in the Southern Ocean temperature change may be achieved by investigating the fast and slow responses of the Southern Ocean to external radiative forcing， which are respectively associated with the fast adjustments of the ocean mixed-layer and the slow evolution of the deep ocean. Specifically， the striking and fast mixed-layer ocean warming north of 50°S is tightly related to the surface heat absorption over upwelling regions and wind-driven meridional heat transport， resulting in enhanced warming around 45°S. While in the slow response of the Southern Ocean temperature， the enhanced ocean warming shifts southward and downward， mainly associating with the heat transfer from oceanic eddies. The Southern Ocean temperature has pronounced climatic effects on many aspects， such as global energy balance， sea-level rise， ocean stratification changes， regional surface warming and atmospheric circulation changes. However， large model biases/deficiencies in simulating the present-day climatology and essential ocean dynamic processes last in generations of climate models， which are the main challenge in advancing our understanding in the mechanisms for the Southern Ocean climate changes. Therefore， to achieve reliable future projections of the Southern Ocean climate， substantial efforts will be needed to improve the model performances and physical understanding in the relative role of various processes in ocean temperature changes at different time scales.     

Ocean sea-ice modelling in the Southern Ocean around Indian Antarctic stations

An eddy-resolving coupled ocean sea-ice modelling is carried out in the Southern Ocean region (9\(^{\circ }\)–78\(^{\circ }\)E; 51\(^{\circ }\)–71\(^{\circ }\)S) using the MITgcm. The model domain incorporates the Indian Antarctic stations, Maitri (11.7\({^{\circ }}\)E; 70.7\({^{\circ }}\)S) and Bharati (76.1\({^{\circ }}\)E; 69.4\({^{\circ }}\)S). The realistic simulation of the surface variables, namely, sea surface temperature (SST), sea surface salinity (SSS), surface currents, sea ice concentration (SIC) and sea ice thickness (SIT) is presented for the period of 1997–2012. The horizontal resolution of the model varies between 6 and 10 km. The highest vertical resolution of 5 m is taken near the surface, which gradually increases with increasing depths. The seasonal variability of the SST, SSS, SIC and currents is compared with the available observations in the region of study. It is found that the SIC of the model domain is increasing at a rate of 0.09% per month (nearly 1% per year), whereas, the SIC near Maitri and Bharati regions is increasing at a rate of 0.14 and 0.03% per month, respectively. The variability of the drift of the sea-ice is also estimated over the period of simulation. It is also found that the sea ice volume of the region increases at the rate of 0.0004 \(\hbox {km}^{3}\) per month (nearly 0.005 \(\hbox {km}^{3}\) per year). Further, it is revealed that the accumulation of sea ice around Bharati station is more as compared to Maitri station.     

太古宙的洋-陆与古地理问题*

大陆最古老的陆壳物质是沉积岩中4.4 Ga的碎屑锆石,最古老的陆壳岩石年龄为4.1-4.0 Ga,出露面积约20 km²。3.9-3.6 Ga的古老陆核出露在不同克拉通中,而大陆的生长峰期是在2.9-2.7 Ga,全球稳定的陆壳圈层形成是在~2.5 Ga,被称为克拉通化。陆壳以英云闪长岩-奥长花岗岩-花岗闪长岩(TTG)为代表,体积占古老陆壳的~70%以上。古陆表现为高级片麻岩区-花岗绿岩带格局(穹隆-龙骨格局),与显生宙的洋-陆格局不同,暗示构造体制的差异。火山沉积组合即是围绕高级片麻岩地体以层状向斜方式存在的绿岩带,后者相对变质很浅或未变质。早期地球演化中,先有陆还是先有洋、陆核形成和生长的机制、什么时候开始有露出海面的陆地、太古宙时期的洋-陆格局等等都还没有定论。古元古代时期,全球长期处于伸展阶段,巨厚的裂谷型沉积以及伴随的大氧化事件,可能是开启古地理研究的最早地质时期。本文还以华北克拉通为例,作了陆壳演化的简单介绍。     

太古宙的洋-陆与古地理问题*

大陆最古老的陆壳物质是沉积岩中4.4 Ga的碎屑锆石,最古老的陆壳岩石年龄为4.1-4.0 Ga,出露面积约20 km²。3.9-3.6 Ga的古老陆核出露在不同克拉通中,而大陆的生长峰期是在2.9-2.7 Ga,全球稳定的陆壳圈层形成是在~2.5 Ga,被称为克拉通化。陆壳以英云闪长岩-奥长花岗岩-花岗闪长岩(TTG)为代表,体积占古老陆壳的~70%以上。古陆表现为高级片麻岩区-花岗绿岩带格局(穹隆-龙骨格局),与显生宙的洋-陆格局不同,暗示构造体制的差异。火山沉积组合即是围绕高级片麻岩地体以层状向斜方式存在的绿岩带,后者相对变质很浅或未变质。早期地球演化中,先有陆还是先有洋、陆核形成和生长的机制、什么时候开始有露出海面的陆地、太古宙时期的洋-陆格局等等都还没有定论。古元古代时期,全球长期处于伸展阶段,巨厚的裂谷型沉积以及伴随的大氧化事件,可能是开启古地理研究的最早地质时期。本文还以华北克拉通为例,作了陆壳演化的简单介绍。     

An Overview of Ocean Predictability and Ocean Ensemble Forecast

Ocean is a highly complex and nonlinear dynamical system. The inevitable errors in both data and numerical models lead to uncertainties in ocean numerical prediction. By understanding features and properties in the ocean on multiple scales, it is important to quantify and estimate the predictability of the ocean, and analyze the reasons and mechanism of error growth. The efforts focus on investigating the method to reduce the uncertainties and errors in forecasting and increase the time limit of ocean predictability. The advances will result in improved marine forecasting models and forecasting skill. Understanding limitations and identifying the research needed to increase accuracy will lead to fundamental progress in ocean forecast, which is of great significance. The present study described and illustrated the mechanics and computations involved in modeling and predicting uncertainties for ocean prediction and its modern applications. Firstly, it discussed the fundamental concept and classification of the ocean predictability. The research status of ocean predictability is introduced including the dynamics methodologies and the ocean ensemble prediction. Three of the dynamical computational methodologies including the singular vector, Lyapunov exponent and bred vector method were introduced. Three ocean ensemble prediction methods including initial condition ensemble, multi-model ensemble and atmospheric forcing ensemble were described and illustrated. Finally, this paper gave a future prospective of ocean predictability and its application.     

Phosphorus Cycle in the Ocean

The behavior of phosphorus is considered at major stages of the sedimentary cycle beginning with supply sources for its delivery into the ocean to precipitation and its sedimentation, localization and subsequent diagenetic redistribution in bottom sediments. River runoff represents the main phosphorus source in the ocean. It delivers annually about 1.5 Mt of dissolved phosphorus and more than 20 Mt of suspended phosphorus into the ocean. Up to 80% of the suspended phosphorus incorporated in the lithogenic material precipitates within submarine continental margins. Phosphorus dissolved in seawater repeatedly participates in biogeochemical processes owing to its assimilation by phytoplankton that annually consumes from 1.5 to 2.5 Gt of phosphorus. Dissolved phosphorus is incorporated in organic remains and precipitates from seawater by a biogenic mechanism, too. Only a part of phosphorus settled onto the bottom is buried in sediments. Due to reducing diagenetic processes, up to 30–40% of the primarily precipitated phosphorus diffuses from the upper layer of sediments into bottom water. Diffusion flux into the ocean significantly exceeds the supply of dissolved phosphorus from river runoff. The absolute mass phosphorus dispersed in sediments is several orders of magnitude greater than the mass concentrated in phosphorite deposits. However, the majority of phosphorite formation epochs coincide with the intensification of total phosphorus accumulation in marine sediments in conditions of humid climate, intense chemical weathering of rocks on continents, and considerable expansion of the oceanic shelf area.     

Mercury in the Southern Ocean

We present here the first mercury speciation study in the water column of the Southern Ocean, using a high-resolution south-to-north section (27 stations from 65.50°S to 44.00°S) with up to 15 depths (0-4440 m) between Antarctica and Tasmania (Australia) along the 140°E meridian. In addition, in order to explore the role of sea ice in Hg cycling, a study of mercury speciation in the “snow-sea ice-seawater” continuum was conducted at a coastal site, near the Australian Casey station (66.40°S; 101.14°E). In the open ocean waters, total Hg (Hg_T) concentrations varied from 0.63 to 2.76 pmol L⁻¹ with “transient-type” vertical profiles and a latitudinal distribution suggesting an atmospheric mercury source south of the Southern Polar Front (SPF) and a surface removal north of the Subantartic Front (SAF). Slightly higher mean Hg_T concentrations (1.35 ± 0.39 pmol L⁻¹) were measured in Antarctic Bottom Water (AABW) compared to Antarctic Intermediate water (AAIW) (1.15 ± 0.22 pmol L⁻¹). Labile Hg (Hg_R) concentrations varied from 0.01 to 2.28 pmol L⁻¹, with a distribution showing that the Hg_T enrichment south of the SPF consisted mainly of Hg_R (67 ± 23%), whereas, in contrast, the percentage was half that in surface waters north of PFZ (33 ± 23%). Methylated mercury species (MeHg_T) concentrations ranged from 0.02 to 0.86 pmol L⁻¹. All vertical MeHg_T profiles exhibited roughly the same pattern, with low concentrations observed in the surface layer and increasing concentrations with depth up to an intermediate depth maximum. As for Hg_T, low mean MeHg_T concentrations were associated with AAIW, and higher ones with AABW. The maximum of MeHg_T concentration at each station was systematically observed within the oxygen minimum zone, with a statistically significant MeHg_Tvs Apparent Oxygen Utilization (AOU) relationship (p < 0.001). The proportion of Hg_T as methylated species was lower than 5% in the surface waters, around 50% in deep waters below 1000 m, reaching a maximum of 78% south of the SPF. At Casey coastal station Hg_T and Hg_R concentrations found in the “snow-sea ice-seawater” continuum were one order of magnitude higher than those measured in open ocean waters. The distribution of Hg_T there suggests an atmospheric Hg deposition with snow and a fractionation process during sea ice formation, which excludes Hg from the ice with a parallel Hg enrichment of brine, probably concurring with the Hg enrichment of AABW observed in the open ocean waters. Contrastingly, MeHg_T concentrations in the sea ice environment were in the same range as in the open ocean waters, remaining below 0.45 pmol L⁻¹. The MeHg_T vertical profile through the continuum suggests different sources, including atmosphere, seawater and methylation in basal ice. Whereas Hg_T concentrations in the water samples collected between the Antarctic continent and Tasmania are comparable to recent measurements made in the other parts of the World Ocean (e.g., Soerensen et al., 2010), the Hg species distribution suggests distinct features in the Southern Ocean Hg cycle: (i) a net atmospheric Hg deposition on surface water near the ice edge, (ii) the Hg enrichment in brine during sea ice formation, and (iii) a net methylation of Hg south of the SPF.     

链接热带东印度洋环流的海洋波动桥梁

热带印度洋环流动力研究对认识海盆尺度物质和水体交换、区域乃至全球气候变化具有重要意义,亦服务于人类的生产生活。回顾了近年来基于中国科学院南海海洋研究所热带印度洋观测取得的环流动力方面的研究进展,探讨提出海洋波动桥梁概念,即：赤道波通过水平传播、垂向传播和东边界反射,在赤道上混合层、次表层和中深层调制着赤道流系的生成与变化;随着波动能量在东边界以沿岸开尔文波和反射罗斯贝波的形式往外赤道传输,赤道动力过程亦调节着外赤道的环流结构变化。作为能量传输的十字路口,海洋东边界是环流变化的动力支点。在其支撑下,海洋波动成为环流间重要的能量纽带,贡献于环流的动力联系,是东印度洋环流多尺度变化的重要内因。基于观测,初步探讨了大尺度气候模态等外因对热带东印度洋环流的影响。凝练的海洋波动桥梁动力学框架,为进一步研究热带印度洋的环流的特征、变化及影响提供科学启示。