2017年绿潮浒苔(Ulva prolifera)生理特征及孢子囊形成情况分析

近几年来在我国青岛海域连续暴发的浒苔绿潮造成了巨大的经济损失并且破坏了近海海洋生态系统平衡。因此,浒苔绿潮受到了越来越多的关注。本研究重点关注了绿潮暴发期间不同海域浒苔藻体生理特征和孢子囊形成情况。研究发现,不同海域里浒苔藻体生理特征差异显著,孢子囊比例显著不同,并且观察到漂浮浒苔的原位萌发。2017年5月中旬,我们在苏北浅滩紫菜养殖区域(33.78°N,121.29°E)对筏架绠绳上生长的绿藻,退潮后滩涂散落的绿藻和涨潮时海面上漂浮的绿藻进行为期5天的野外采集。另外,在2017年6月随科考船对浒苔暴发海域的浒苔样本进行采集。采集范围在(33.5°—36.5°N, 120°—124°E)。结果表明,从低纬度到高纬度,浒苔F_v/F_m(光系统Ⅱ最大光化学量子产量)值从0.65逐渐降低至0.3左右;YⅡ(光系统Ⅱ实时光化学量子产量)值也从最高0.5左右降低至最低0.1。此外,定生浒苔F_v/F_m值为0.6—0.8左右,明显高于漂浮浒苔; YⅡ值也有类似趋势。在孢子囊形成比例方面,定生浒苔约有5%藻体形成了孢子囊,而漂浮浒苔中孢子囊形成比例达到20%。数据表明,低纬度区域为浒苔来源地,浒苔生理活性良好,孢子囊形成比例低。随着浒苔往北漂移,其生理活性降低。并且,漂浮浒苔孢子囊形成比例显著性高于定生浒苔。本文认为,浒苔脱离来源区后,孢子囊的快速形成、成熟和孢子释放以及孢子的原位萌发是浒苔生物量激增的重要原因。     

季风转换期东印度洋的赤道流系结构和水文特征

基于2013-04夏季风转换期间航次观测数据,对赤道东部印度洋3支东向强流及其水文特征进行分析。结果表明,沿赤道在表层存在Wyrtki急流,在温跃层深度存在赤道潜流,它们携带着阿拉伯海的高盐水向东输运,81°E断面上,核心流量分别为4.76Sv和12.18Sv;南赤道逆流核心在5°S附近,核心流量7.4Sv,并伴有高盐特性。     

2014年春季季风间期东印度洋赤道及其邻近海域硅藻群落

2014年4月10日至5月13日在东印度洋赤道区及其邻近海域(10.08°N-6.00°S,80.00°~96.10°E)进行硅藻物种组成和群落结构的调查。分析了45个网采样品,共鉴定出浮游硅藻34属113种(包括变种、变形及未定名种),大部分物种为热带外洋性种以及暖海外洋性种,与该海区的热带及亚热带的环境特征一致。优势种为佛氏梯形藻(Climacodium frauenfeldianum)、地中海细柱藻(Leptocylindrus mediterraneus)、密聚角毛藻(Chaetoceros coarctatus)、美丽漂流藻(Planktoniella foromsa)、大西洋角毛藻那不勒斯变种(Chaetoceros atlanticus var. neapolitanus)、距端假管藻(Pseudosolenia calcar-avis,即距端根管藻Rhizosolenia calcaravis)、圆柱几内亚藻(Guinardia cylindrus)、达蒂角毛藻(Chaetoceros dadayi)、伏氏海线藻(Thalassionema frauenfeldii)、离心列海链藻(Thalassiosira excentrica)、瘤面角毛藻(Chaetoceros bacteriastroides)以及笔尖根管藻粗径变种(Rhizosolenia styliformis var. latissima)等。硅藻的平均细胞丰度为1.855×103个/m3,其平面分布不均匀,赤道断面细胞丰度较低,高值区出现在海区北部。聚类分析发现有7种生态类群,这些硅藻的种类和丰度平面分布与上层水体(200 m以浅)温度、盐度及营养盐的水柱平均值有较好的对应关系。     

2013年赤道波动调制下的东印度洋春季Wyrtki急流季节内变化研究

A strong spring Wyrtki jet(WJ) presents in May 2013 in the eastern equatorial Indian Ocean. The entire buildup and retreat processes of the spring WJ were well captured by two adjacent Acoustic Doppler Current Profilers mounted on the mooring systems. The observed zonal jet behaved as one intraseasonal event with the significant features of abrupt emergence as well as slow disappearance. Further research illustrate that the pronounced surface westerly wind burst during late-April to mid-May, associated with the active phase of a robust eastwardpropagating Madden–Julian oscillation in the tropical Indian Ocean, was the dominant reason for the rapid acceleration of surface WJ. In contrasting, the governing mechanism for the jet termination was equatorial wave dynamics rather than wind forcing. The decomposition analysis of equatorial waves and the corresponding changes in the ocean thermocline demonstrated that strong WJ was produced rapidly by the wind-generated oceanic downwelling equatorial Kelvin wave and was terminated subsequently by the westward-propagating equatorial Rossby wave reflecting from eastern boundaries of the Indian Ocean.     

热带东印度洋春季浮游植物群落结构空间特征分析

基于2013年3月至5月采集的热带东印度洋海域(10.0°S～4.0°N, 83.0°～97.5°E)浮游植物水样样品,分析了其种类组成、优势类群、细胞丰度等群落特征参数,综合比较了水平和垂向上浮游植物种类及丰度的差异性,初步探讨了其成因。结果表明：2013年春季热带东印度洋微型浮游植物共鉴定出306种,主要由硅藻、甲藻、金藻、蓝藻、裸藻和隐藻六大门类组成,其优势类群主要以粒径较小的隐藻、微型甲藻、菱形藻、环沟藻等为主。水平分布上,各水层浮游植物细胞丰度分布趋势相似,但斑块特征明显,其高值区位于88°E断面赤道以南次表层水域(30 m、75 m),局部区域细胞丰度值可达10⁴ cells/L以上;与其毗邻的东南部、东部水域为低值区,并向赤道延伸。垂直剖面上,硅藻和甲藻广泛分布在各取样深度,但分布特征有明显的空间差异和规律,0 m、30 m大部分站位硅藻种类比例在0.2～0.3甚至更低,甲藻在0.7～0.8,随着水层加深(75 m、100 m、150 m、300 m),硅藻种类占比上升到0.5～0.6,甲藻降低到0.4～0.5,无论硅藻还是甲藻种类数75 m层最丰富。30 m和75 m水层细胞丰度明显高于其他水层。甲藻是热带东印度洋微型浮游植物种类和细胞丰度的重要贡献者,低生物量海域表现的更为明显,贡献率大于80%。该研究将极大丰富东印度洋浮游植物群落空间特征基础信息较匮乏的现状,为量化、评估该海域的生物资源提供数据支撑。     

赤道东印度洋和孟加拉湾障碍层厚度的年际变化及其影响机制

Interannual variability(IAV) in the barrier layer thickness(BLT) and forcing mechanisms in the eastern equatorial Indian Ocean(EEIO) and Bay of Bengal(BoB) are examined using monthly Argo data sets during 2002–2017. The BLT during November–January(NDJ) in the EEIO shows strong IAV, which is associated with the Indian Ocean dipole mode(IOD), with the IOD leading the BLT by two months. During the negative IOD phase, the westerly wind anomalies driving the downwelling Kelvin waves increase the isothermal layer depth(ILD). Moreover, the variability in the mixed layer depth(MLD) is complex. Affected by the Wyrtki jet, the MLD presents negative anomalies west of 85°E and strong positive anomalies between 85°E and 93°E. Therefore, the BLT shows positive anomalies except between 86°E and 92°E in the EEIO. Additionally, the IAV in the BLT during December–February(DJF) in the BoB is also investigated. In the eastern and northeastern BoB, the IAV in the BLT is remotely forced by equatorial zonal wind stress anomalies associated with the El Ni?o-Southern Oscillation(ENSO). In the western BoB, the regional surface wind forcing-related ENSO modulates the BLT variations.     

赤道东印度洋和孟加拉湾障碍层厚度的季节内和准半年变化

利用2002—2015年ARGO网格化的温度、盐度数据, 结合卫星资料揭示了赤道东印度洋和孟加拉湾障碍层厚度的季节内和准半年变化特征, 探讨了其变化机制。结果表明, 障碍层厚度变化的两个高值区域出现在赤道东印度洋和孟加拉湾北部。在赤道区域, 障碍层同时受到等温层和混合层变化的影响, 5—7月和11—1月受西风驱动, Wyrtki急流携带阿拉伯海的高盐水与表层的淡水形成盐度层结, 同时西风驱动的下沉Kelvin波加深了等温层, 混合层与等温层分离, 障碍层形成。在湾内, 充沛的降雨和径流带来的大量淡水产生很强的盐度层结, 混合层全年都非常浅, 障碍层季节内变化和准半年变化主要受等温层深度变化的影响。上述两个区域障碍层变化存在关联, 季节内和准半年周期的赤道纬向风驱动的波动过程是它们存在联系的根本原因。赤道东印度洋地区的西风(东风)强迫出向东传的下沉(上升)的Kelvin波, 在苏门答腊岛西岸转变为沿岸Kelvin波向北传到孟加拉湾的东边界和北边界, 并且在缅甸的伊洛瓦底江三角洲顶部(95°E, 16°N)激发出向西的Rossby波, 造成湾内等温层深度的正(负)异常, 波动传播的速度决定了湾内的变化过程滞后于赤道区域1~2个月。     

赤道印度洋偶极子对重庆夏季降水的影响分析

利用重庆34个气象台站1961—2017年夏季降水量、NCEP/NCAR的再分析月平均高度场资料和海面温度资料,分析发现,上年秋季尤其是11月的赤道(热带)印度洋偶极子(tropical Indian Ocean dipole,TIOD)模态与重庆夏季降水存在正相关关系。通过前期海面温度对大气环流的影响分析,结果表明:上年11月TIOD和夏季500 hPa高度场的相关与重庆夏季降水和高度场的相关一致,显示出从高纬度到低纬度"+、-、+"的相关分布,反映出当上年11月TIOD正位相(负位相)时,次年夏季环流场表现出乌拉尔山阻塞高压明显(不明显)、中纬度30°～37°N低值系统活跃(不活跃),西太平洋副热带高压偏强(弱)、位置偏南(北)的重庆夏季典型的降水偏多环流特征;前期赤道太平洋ENSO暖事件和前期TIOD事件同时发生时,两个事件的作用相互叠加,使得西太平洋副热带高压加强西伸并且位置偏南,造成重庆夏季降水的异常偏多。     

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。     

Spatiotemporal variation and mechanisms of temperature inversion in the Bay of Bengal and the eastern equatorial Indian Ocean

In the northern Bay of Bengal, the existence of intense temperature inversion during winter is a widely accepted phenomenon. However, occurrences of temperature inversion during other seasons and the spatial distribution within and adjacent to the Bay of Bengal are not well understood. In this study, a higher resolution spatiotemporal variation of temperature inversion and its mechanisms are examined with mixed layer heat and salt budget analysis utilizing long-term Argo（2004 to 2020） and RAMA（2...     

Contributions of shortwave radiation to the formation of temperature inversions in the Bay of Bengal and eastern equatorial Indian Ocean: A modeling approach

Variations in incoming shortwave radiation influence the net surface heat flux, contributing to the formation of a temperature inversion. The effects of shortwave radiation on the temperature inversions in the Bay of Bengal and eastern equatorial Indian Ocean have never been investigated. Thus, a high-resolution (horizontal resolution of 0.07°×0.07° with 50 vertical layers) Regional Ocean Modeling System (ROMS) model is utilized to quantify the contributions of shortwave radiation to the temperature inversions in the study domain. Analyses of the mixed layer heat and salt budgets are performed, and different model simulations are compared. The model results suggest that a 30% change in shortwave radiation can change approximately 3% of the temperature inversion area in the Bay of Bengal. Low shortwave radiation reduces the net surface heat flux and cools the mixed layer substantially; it also reduces the evaporation rate, causing less evaporative water vapor losses from the ocean than the typical situation, and ultimately enhances haline stratification. Thus, the rudimentary outcome of this research is that a decrease in shortwave radiation produces more temperature inversion in the study region, which is primarily driven by the net surface cooling and supported by the intensive haline stratification. Moreover, low shortwave radiation eventually intensifies the temperature inversion layer by thickening the barrier layer. This study could be an important reference for predicting how the Indian Ocean climate will respond to future changes in shortwave radiation.     

The distribution of chlorophyll a in the tropical eastern Indian Ocean in austral summer

To study the effect of hydrographic factors on the spatial distributions of chlorophyll a (Chl a), an investigation was carried out in the tropical eastern Indian Ocean (80 -100 E along 7 S, and 7 -18 S along 80 E) in December 2010. The fluorescent method was used to obtain total Chl a and size-fractioned Chl a at the 26 stations. The results show that surface Chl a concentration averaged at (0.168 ± 0.095) mg/m 3 s.d. (range: 0.034-0.475 mg/m 3 ), concentrations appeared to be higher in the west for longitudinal variations, and higher in the north for latitudinal variations. Furthermore, the surface Chl a concentration was lower (0.034-0.066 mg/m 3 ) in the region to the south of 16 S. There was a strong subsurface Chl a maximum layer at all stations and the depth of the Chl a maximum increased towards to the east and south along with the respective nitracline. The spatial variation of Chl a was significant: correlation and regression analysis suggests that it was primarily affected by PO 3 4 , N(NO 3 -N+NO 2 -N) and temperature. Size-fractionated Chl a concentration clearly showed that the study area was a typical oligotrophic open ocean, in which picophytoplankton dominated, accounting for approximately 67.8% of total Chl a, followed by nanophytoplankton (24.5%) and microphytoplankton (7.6%). The two larger fractions were sensitive to the limitation of P, while picophytoplankton was primarily affected by temperature.