Phytoplankton chemotaxonomy in the Atlantic sector of the Southern Ocean during late summer 2009

A chemotaxonomic investigation of surface phytoplankton was undertaken on a research cruise to the Atlantic sector of the Southern Ocean during late austral summer 2009. Based on pigment signatures, several distinct regions emerged that were delineated by physical features. CHEMTAX analysis of high performance liquid chromatography (HPLC) pigment data indicated that diatoms generally dominated communities south of the Antarctic Polar Front (APF), particularly in regions of elevated biomass where chlorophyll-a (chl-a) was >1.5 µg l⁻¹ and diatoms comprised >80% of biomass. Pigment signatures representative of haptophytes-8, indicative of Phaeocystis antarctica, were dominant near the ice shelf. Chl-a concentrations were 0.2–0.6 µg l⁻¹ between the APF and the Subtropical Front (STF) and outputs suggested that chlorophytes, haptophytes-8 and haptophyte-6, in the form of coccolithophores, were the major constituents. Very low chl-a levels (<0.2 µg l⁻¹) were observed north of the STF and the prokaryotes Synechococcus spp. and Prochlorococcus spp. were the dominant groups in these oligotrophic waters.     

南印度洋偶极子及其影响研究进展

回顾了对南印度洋副热带海气相互作用的研究,总结了南印度洋偶极子事件背景下的气候变化。印度洋海表温度的方差表明南印度洋是整个印度洋海温变率最强的区域,年际海温变化最显著的特征就是海温呈现西南—东北向的偶极子型分布,被称为南印度洋偶极子(Southern Indian Ocean Dipole, SIOD)。南印度洋海温偶极子的形成主要是受大尺度大气环流调整的影响。南印度洋副热带反气旋环流异常引起了印度洋热带东风异常和副热带西风异常的变化,影响了潜热通量、上升流和Ekman热输送,进而引起了海温变化。SIOD对热带和热带外大气环流也有影响,尤其会影响亚洲夏季风降水异常,例如我国的降水异常和南印度洋偶极子海温异常具有显著相关关系。此外,SIOD模态所引起的经向环流异常与南海、菲律宾地区的反气旋环流异常也有紧密联系。     

热带印度洋偶极子事件和副热带印度洋偶极子事件的联系

分别对热带印度洋偶极子事件和副热带印度洋偶极子事件的时间序列进行了周期分析。结果表明,热带印度洋偶极子事件的主要振荡周期为2 a和4 a,而副热带偶极子事件的主要振荡周期为8 a;对整个印度洋海区的海表温度距平进行2~8 a的带通滤波,发现未滤波之前,2个事件的相关性很低,而在进行了滤波之后,2个事件的相关性有很大的提高,并且当副热带印度洋偶极子事件超前热带印度洋偶极子事件9个月时,二者具有很强的相关性。通过对温度场和风场的分析,从物理上解释了2个事件之间的相互联系。     

印度洋偶极子及其可预报性研究进展

主要介绍印度洋偶极子(IOD)的时空特征、演变机制和可预报性的研究进展。IOD是东西热带印度洋反相的海温异常,是热带印度洋的年际海温变率最主要的两种异常结构之一。关于IOD的演变机制,特别是ENSO在其中所起作用,一直是学界争论的热点。一些学者认为,IOD是ENSO通过遥相关作用对热带印度洋造成的影响;另一些学者则认为,IOD是热带印度洋内部海气振荡的产物。本研究重点讨论这两种观点的相关证据以及IOD与ENSO的关系。此外,现有多数模式对IOD的预报时效小于3~4个月,潜在的预报时效则大于5个月,但这些对IOD的可预报性研究尚处于起步阶段,还有很大发展空间。     

印度洋海表温度的变化及其对印度夏季季风降水影响的诊断研究

对印度洋海表温度(SST)的主要特征及变化趋势进行分析,并研究了其与印度夏季季风降水(ISMR)和季风环流的关系,揭示出:从北印度洋到南半球中高纬度印度洋,SST最显著的变化模态是全海盆一致的变化,近50 a来总体趋势是上升的,在1976,1986年以及1996年间分别有一次跳跃性增温,与太平洋SST变化趋势基本一致.除了长期变化趋势外,南印度洋中高纬度比热带地区有更显著的模态分布.在印度洋SST升温的背景下,ISMR具有逐渐减少的趋势,但两者相关较弱.印度洋SST发生跳跃后的不同阶段,许多海区SST与ISMR相关均发生变化,但在春季,热带外南印度洋具有一对相对稳定区,其分布与EOF分析的第2模态相似.根据它们的分布,文中定义了春季南半球偶极子(SIOD),在正SIOD(PSIOD)情况下印度降水偏多,而负SIOD(NSIOD)则反之.环流分析表明,PSIOD(NSIOD)通过与大气的相互作用,对夏季马斯克林高压具有增强(减弱)作用,进而使得索马里越赤道气流增强(减弱),在印度地区低空产生异常的辐合(辐散),高层辐散(辐合),从而影响印度季风环流,使得印度季风降水偏多(少).     

An evaluation of the application of CHEMTAX to Antarctic coastal pigment data

Presented is an evaluation of the application of CHEMTAX (CHEMical TAXonomy) to Antarctic coastal pigments collected along the western Antarctic Peninsula (wAP). Overall analytical error is <20% for all pigments involved in the analysis. CHEMTAX was stable within a range of input pigment ratios; data were analyzed in three bins based on light depths, with each year's data run independently. Results were validated by comparison to those from CHEMTAX methods that included randomized error, feedback loops and additional diagnostic pigments. Blooms during mid-summer (chlorophyll a concentrations >5 ??g L⁻¹) were dominated primarily by either diatoms or cryptomonads. Mixed flagellates can also be abundant and Pheaocystis spp. and prasinophytes are frequently present in low concentrations. Comparison with microscopy shows CHEMTAX to give superior results in identifying Pheaocystis spp. with favorable results for other groups. This analysis shows CHEMTAX to be a reliable and stable tool for providing estimations of the main phytoplankton taxa in wAP waters based on long-term data collected during a 12-year time series.     

热带印度洋和太平洋海气相互作用事件的协调发展

对次表层海温距平的分布和变化的分析表明,在热带印度洋和太平洋都存在海温距平的偶极子模态,即在赤道附近大洋东、西两个部分的海温距平在不少年份呈反符号分布。进一步分析表明,两大洋海温距平的偶极子模态间有密切的联系。在分析它们和850hPa纬向风距平后指出,正是Walker环流异常把两大洋的海温距平变化联系起来。     

Fronts and strong currents of the upper southeast Indian Ocean

1 IntroductionBaroclinic component is the dominant part ofAntarcticCircum polarCurrent (ACC) (FandryandPillsbury,1979),and a baroclinictransportation asso-ciatedwithfrontsmakesupthem ajoritypartoftheto-talbaroclinictransportation oftheACC (Nowlin andCliff…     

The Indian Ocean HydroBase: A high-quality climatological dataset for the Indian Ocean

The present study developed a high-quality climatological dataset for the Indian Ocean - the Indian Ocean HydroBase (IOHB) - from a combined dataset including the World Ocean Database 1998 version 2 (WOD98v2). Methods are similar to those used by previous studies for other oceans. Japanese data for the IOHB originated from the Japanese datasets MIRC (Marine Information Research Center) Ocean Dataset 2001 and Far Seas Collection; these datasets contain more Japanese observations than WOD98v2. Water mass properties in the IOHB climatology are consistent with previous studies. Seasonal patterns of properties near the sea surface are well reproduced, and deep-layer properties are consistent with the Reid-Mantyla climatology that is derived from high-quality observations. The isopycnal climatology of the IOHB differs from the World Ocean Atlas 2001 (WOA01) along the fronts associated with the Antarctic Circumpolar Current (ACC). The WOA01 shows a warm and saline intermediate water intrusion from South Africa to the east along the northern edge of the front. Such an intrusion is absent in IOHB where less saline intermediate water extends continuously northward from the southern ocean. The WOA01 shows a continuous belt of low potential vorticity along the ACC. This feature is less distinct in the IOHB climatology and in the Reid-Mantyla climatology. The IOHB consists of a 1° × 1° gridded climatology and the datasets of raw and quality-controlled hydrographic stations. The latter is valuable for quality control of the Argo float salinity data as climatological reference. These datasets are available freely via the Internet.     

印尼贯穿流对印度洋的热量贡献

本文基于海洋环流模式模拟的高分辨率欧拉场,利用拉格朗日追踪方法,评估了印尼贯穿流（ITF）对印度洋的热量贡献。通过计算ITF水体在印度洋的传输路径及伴随的温度变化来获取ITF水体在印度洋的热量传输过程。模拟结果表明ITF进入印度洋后主要向西流动并在到达马达加斯加后分叉,进入南、北印度洋。热收支分析表明ITF在北印度洋吸收0.41 PW热量,在南印度洋释放0.56 PW热量;这两个过程相互补偿,导致ITF对整个印度洋的净加热贡献并不显著,只有0.15 PW。进一步的检查ITF离开印度洋的出口（跨过34°S）,结果表明ITF主要随着位于西边界的奥古拉斯流和位于东边界的利文流离开印度洋。约89%的ITF水体沿着西边界离开印度洋,其余的11%主要沿着东边界离开印度洋;前者对整个印度洋的净加热贡献为0.10 PW,后者的净加热贡献为0.05 PW。     

南印度洋SST在20世纪60年代的年代际转变及其相关气候变化过程

The change of sea surface temperature(SST) in the southern Indian Ocean(SIO) during the recent six decades has been analyzed based on oceanic reanalysis and model, as well as atmospheric data. The results show that a thermal regime shift in SIO during the 1960 s, which is not caught enough attentions, has been of equal magnitude to the linear warming since 1970. Empirical Orthogonal Function(EOF) analyses reveal that a thermal shift is combined with atmospheric changes such as the weakening of westerly during the period of 1960–1967. Inner dynamic connections can be defined that when the westerly winds turn weak, the anticyclonic wind circulation between westerly winds and the trade winds decreases, which further reduces the SST to a negative peak in this period. It is noted that the shifts in the 1960 s are also evident for Southern Hemisphere. For example, subtropical high and the entire westerly winds belt at high latitudes both change dramatically in the 1960 s. This large-scaled process maybe link to the change of southern annular mode(SAM).     

赤道印度洋中部断面东西水交换的季节变化及其区域差异

采用海洋再分析资料和实测资料研究了热带印度洋中部东西水交换特征。结果表明存在两个相互独立的过程,即北印度洋过程(4°~6°N)和赤道过程(2°S-2°N)。北印度洋过程受季风影响显著,11月至翌年3月冬季风期间表现出很强的低盐水向西输送,5-9月夏季风期间则为高盐水向东输送;由于冬季风期间的输送较强,年平均表现为低盐水向西输送。赤道过程分为表层过程和次表层过程。表层赤道过程受局地风场驱动,有明显的半年周期;4-5月和10-11月的东向流将赤道西印度洋的高盐水向东输送,其余月份相反;向东的输送较强,年平均表现为净高盐水向东输送。在次表层赤道过程没有明显的季节变化,海流全年一致向东,将海盆西部的高盐水向东输送。     

A Record of Palaeo-Tsunami in the Indian Ocean

The history of catastrophic events on the Indian coast helps us to understand the frequency and magnitude of the tsunamis that occurred in the Indian Ocean. These catastrophic events have changed the coastal landscape and have left significant records for further studies. These rare events have occurred in the Indian Ocean. There have been megatsunamigenic events in the past due to volcanic eruptions and earthquakes. Those events due to earthquakes have proved more catastrophic than the volcanic activities. There has been limited official records of the causality and magnitude of palaeo-tsunamigenic events. These have been studied using the various proxies. The rate of sedimentation is a proportional tool to study the magnitude of a tsunami and this has proved to be a successful tool along with foraminiferal assemblages. Causes for a tsunami to occur are by and large, the subduction zone earthquakes of the Indian plate has been the most common source for tsunami in the Indian Ocean. More often the Andaman and Nicobar and the Indonesian islands have been vulnerable to tsunami than the mainland of India and Sri Lanka.

In summary, in the last 200 years at least three basin-wide tsunamis have occurred, with several smaller tsunami affecting one or more coastlines in the region. The December 2004 M-9 tsunami seems to have been the largest and most destructive in the last two centuries, suggesting most tsunami are likely to be smaller but still allowing the possibility that even larger tsunami could be generated in propitious circumstances.     

Phytoplankton, nutrients and hydrography in the frontal zone between the Southwest Indian Subtropical gyre and the Southern Ocean

A survey was made of the Southwest Indian Ocean frontal region between 30 and 50°E containing the Agulhas Return, Subtropical and Subantarctic Fronts. From CTD, SeaSoar and extracted samples the distribution of nitrate, silicate and chlorophyll a is shown to be strongly linked to the front and water mass structure, varying zonally and meridionally. Surface chlorophyll a concentrations were low to the north and south leaving a band of elevated chlorophyll between the Subtropical and Subantarctic Fronts. The low concentration of chlorophyll a to the north, in Subtropical Water, was clearly due to nitrate limitation. Between the Subtropical and Subantarctic Fronts, where the chlorophyll a concentrations were highest, the surface layer showed silicate depletion limiting diatom growth. South of the Subantarctic Front there were deep extending, low concentrations of chlorophyll a, but despite plentiful supplies of macro-nutrients and a well-stratified surface layer, high concentrations of chlorophyll a were absent. Changes from west to east were associated with the meandering of the Southern Ocean Fronts, especially the Subtropical Front, and their strength and proximity to each other. Concentrations of chlorophyll a peaked where the Agulhas Return, Subtropical and Subantarctic Fronts were in close proximity. Combined frontal structures appear to have particularly pronounced vertical stability and are associated with enhanced upwelling of nutrients and leakage of nutrients across the front. Light levels are high within the shallow stable layer. Such conditions are clearly favourable for biological growth and support the development of larger-celled phytoplankton communities.     

南印度洋海表温度距平冬季重现特征与机制的初步分析

本文主要利用1958–2016年GECCO2等资料通过超前/滞后相关分析方法,分析了南印度洋海表温度距平（SSTA）冬季−冬季重现的时空特征,并探讨了海洋和大气强迫对其形成的贡献。结果显示,SSTA冬季−冬季重现主要发生在南印度洋15ºS以南海域,特别是在马达加斯加岛至澳大利亚西南部之间的海域（15º～45ºS,70º～100ºE）重现信号最为显著。重现信号除了主要发生在次年冬季外,在部分海域重现信号发生较早,可在次年秋季发生并持续至随后的冬季。进一步分析表明,混合层深度冬深夏浅的变化（即海洋重现机制）是研究海域SSTA冬季重现的主因。另外,在马达加斯加岛南部海域和澳大利亚西南部海域海面净热通量对SSTA的重现也有直接的贡献。     

热带西南印度洋上升流区季节和年际变化研究及与印太系统海气相互作用

用59年Ishii再分析温度资料,讨论了热带西南印度洋(SWTIO)上升流区的季节和年际变化以及与上升流区有关的温度距平的变化,同时分析了其与热带印太海气系统的关系,结果显示SWTIO 上升流在南半球冬、夏季比较强,春季最弱。它的范围在5°~1°S,在东西向从50°E可以伸展到90°E。该上升流区的变化与温跃层的温度距平有密切的关系,并存在明显的5 a振荡周期。SWTIO上升流区温度距平的5 a周期振荡是由热带东印度洋温度距平在最大垂直温度距平曲面(MTAL)上向西沿着11.5°~6.5°S传播过来的,它与热带太平洋的温度距平传播方式不同。SWTIO上升流是热带印太海气系统的一个重要组成部分,印度洋偶极子 超前SWTIO上升流区温度变化5个月,最大相关系数达到0.57,NINO3区指数超前SWTIO上升流区指数2个月达到0.49。当热带印太区域的大气风场改变,影响热带太平洋和印度洋表层SSTA,出现ENSO和DIPOLE,进一步向西传播到SWTIO次表层,导致SWTIO上升流区出现改变。     

东南印度洋沿岸海温年代际振荡及经向传播探讨

用SODA资料分析了热带西南印度洋上升区温度距平与整个南印度洋温度距平的时滞相关, 发现热带西南印度洋上升区温度距平与65°S, 105°E附近200 m深度的温度距平存在滞后10 a的相关振荡, 同时探讨了其可能的机制为温跃层内的斜压内波驱动, 即65°S, 105°E附近200 m深度的温度距平沿着温跃层上层在东南印度洋沿岸从高纬度向低纬的传播, 传播时间大约为10 a左右, 这种信号在传播过程中表现得较弱, 而在起点和终点的两端振荡比较强。波动的传播相比振荡本身要显得弱。     

ENSO and Indian Ocean dipole mode in three coupled GCMs

The simulated ENSO and Indian Ocean dipole (IOD) mode events from three coupled GCMs with the same oceanic component model, CPMO, CPM1 and FGCMO, are compared. The only difference between the CPMO and the CPM 1 comes from the coupling scheme at the air-sea interface, e.g., flux anomaly coupling scheme for the former and direct coupling scheme for the latter. The FGCMO is also a directly coupled GCM, but its atmospheric component model is the NCAR CCM3 rather than the NCC T63AGCM as in the other two coupled GCMs CPMO and CPM1. All three coupled models show E1Nifio-like interannual variability in the tropic Pacific, but the FGCMO shows a bit stronger amplitude of E1 Nifio events and both the CPMO and the CPM1 show much weaker amplitude than the observed one. In the meanwhile, the quasi-biennial variability dominates in the FGCMO simulations, and 4 a and longer periods are significant in both the CPMO and CPM 1 models. As the E1 Nifio events simulated by the three coupled GCMs, the simulated Indian Ocean dipole mode events are stronger from the coupled model FGCMO and weaker from both the CPMO and CPM1 models than those from observation.     

热带东北印度洋海域管水母类的群落结构特征

管水母是海洋浮游动物中的重要类群,通常可作为海流或水团的指示种,其分布受温度、盐度和食物的影响。本文根据2011年4月在东印度洋海域(5°S~5°N,80°~98.5°E)26个站的调查资料,分析了管水母种类组成、丰度分布和群落结构特征。共鉴定管水母37种,以热带大洋广布种和赤道种为主,其中扭形爪室水母Chelophyes contorta、巴斯水母Bassia bassensis、双小水母Nanomia bijuga和短深杯水母Abylopsis eschscholtzi是调查海域的优势种。依据调查站位设置及环境特征,将调查海域分东部断面、赤道断面和西部断面3个区域。各个调查站种数变化范围为2~14种,东部和西部断面的种类较丰富,而赤道断面近岸区种数低,离岸区种数增多。管水母的平均丰度为(1.04±0.58)个/m3,分布不均匀,东部断面和西部断面的丰度比赤道断面高,特别是赤道断面近岸区丰度在1.0个/m3以下。调查海区的管水母属于比较典型的热带大洋性生态类群。群落结构分析表明,东部和西部断面的群落结构相似度较高,二者与赤道断面的相似度均较低。调查海域管水母种类和丰度的分布受水文和生物环境因子的综合影响。双小水母Nanomia bijuga可作为东部断面和赤道断面近岸区沿岸水团的指示种,锥体浅室水母Lensia conoides和褶玫瑰水母Rosacea plicata可作为西部断面100m以下涌升水团的指示种。     

Space-Time Characteristic Analysis of Wind Field over the South Indian Ocean

1 IntroductionThe South Indian Ocean is the only way which must be passed in marine traffic among Africa, Asia and Oceania. With the development of the international traffic, it becomes more and more frequent to navigate over the South Indian Ocean. More and more hydrometeorological safeguards especially the safeguards of important cruise lines are required. However, data for the region in China is absent except the Indian Ocean Climate Atlas (1973)[1] which has short fixed number of…