2016年中国沿海海平面上升显著成因分析及影响

使用中国沿海及西北太平洋区域的水位、海温、气温、气压和风等水文气象资料,详细分析了2016年中国沿海海平面显著升高的成因及影响。分析结果表明:（1）2012-2016年,中国沿海海平面处于准2 a、4 a、准9 a和准19 a周期振荡的高位,几个周期振荡高位叠加,对该时段海平面上升起了一定的作用;（2）2016年,中国沿海气温和海温较1993-2011年的平均值分别高0.7℃与0.5℃,均处于1980年以来高位;气压较1993-2011年的平均值低0.2 hPa;（3）2016年4月、9月、10月和11月,中国沿海海平面均达到1980年以来同期高位,这4个月的风场距平值在东海以南均明显偏大,且以偏南向和向岸风为主,风生流使得海水向岸堆积,沿海长时间以增水为主,对当月局部海平面上升的贡献率达到40%~80%;（4）2016年,中国沿海降水总体偏多,局部区域降水量达到历史同期最高,加上沿海径流量的增加,对沿海局部海平面升高有一定贡献;（5）2016年9-10月,有5个台风相继影响我国南部沿海,持续的风暴潮增水导致台风影响期间的海平面高于当月平均海平面70~360 mm,风暴潮和洪涝灾害给当地造成直接经济损失超过30亿元。     

台湾以东黑潮路径识别与变化规律

为研究对中国台湾以东海域黑潮路径及其变化,本文基于法国空间局AVISO中心提供的1993—2015年的卫星遥感海表流场逐日资料,对121°—125°E,22.4°—25°N海域黑潮路径进行了逐日识别,得到了共计23年累计8400天的台湾以东黑潮流轴的逐日路径,并研究其在不同纬度的流轴位置及其对应的表面黑潮流量的时空变化规律。主要结论如下:(1)采用模糊C-均值聚类法对台湾以东黑潮流轴路径进行聚类分析,发现台湾以东黑潮流轴在24°N以南出现明显摆动,形成正常和偏东两种路径;黑潮流轴存在明显的时间变化,流轴偏东现象年平均大约出现25次,大致每隔3年出现一次偏东较少的现象,各月流轴偏东次数以4、5月最少,10月至次年3月较多;(2)台湾以东黑潮表面流量大小在6.2—8.3×104m2/s之间;总体上来说,纬度越高流量越大,在23.5°N左右范围内存在一个流量低值中心;在24.3°N以北流量总体较大,且增长趋势稳定,同时表面流量大小具有较强的季节和年际变化特征。     

Numerical assessment of tsunami attack on a rubble mound breakwater using OpenFOAM®

A numerical assessment study of tsunami attack on the rubble mound breakwater of Haydarpasa Port, located at the southern entrance of the Istanbul Bosphorus Strait in the Sea of Marmara, Turkey, is carried out in this study using a Volume-Averaged Reynolds-Averaged Navier-Stokes solver, IHFOAM, developed in OpenFOAM^® environment. The numerical model is calibrated with and validated against the data from solitary wave and tsunami overflow experiments representing tsunami attack. Furthermore, attack of a potential tsunami near Haydarpasa Port is simulated to investigate effects of a more realistic tsunami that cannot be generated in a wave flume with the present state of the art technology. Discussions on practical engineering applications of this type of numerical modeling studies are given focusing on pressure distributions around the crown-wall of the rubble mound breakwater, and the forces acting on the single stone located behind the crown-wall at the rear side of the breakwater. Numerical modeling of stability/failure mechanism of the overall cross-section is studied throughout the paper.The present study shows that hydrodynamics along the wave flume and over the breakwater can be simulated properly for both solitary wave and tsunami overflow experiments. Stability of the overall cross-section can only be simulated qualitatively for solitary wave cases; on the other hand, the effect of the time elapsed during tsunami overflow cannot be reflected in the simulations using the present numerical tool. However, the stability of the overall cross-section under tsunami overflow is assessed by evaluating forces acting on the rear side armor unit supporting the crown-wall of the rubble mound breakwater as a practical engineering application in the present paper. Furthermore, two non-dimensional parameters are derived to discuss the stability of this armor unit; and thus, the stability condition of the overall cross-section. Approximate threshold values for these non-dimensional parameters are presented comparing experimental and numerical results as a starting point for engineers in practice. Finally, investigations on the solitary wave and tsunami overflow experiments/simulations are extended to the potential tsunami simulation in the scope of both representation of a realistic tsunami in a wave flume and stability of the rubble mound breakwater.     

不同气候模态下西北太平洋秋刀鱼资源丰度预测模型建立

秋刀鱼（Cololabis saira）资源对海洋环境因素极为敏感,不同气候模态可能对秋刀鱼资源丰度产生不同的影响。根据1990-2014年西北太平洋日本的秋刀鱼渔业中单位捕捞努力量渔获量（CPUE,以此作为资源丰度）,以及相应产卵场、索饵场的海表温（SST）遥感数据,探讨太平洋年际震荡（PDO）指数冷、暖年下,秋刀鱼资源丰度CPUE变化与产卵场、索饵场SST的关系,并分别建立资源丰度的预测模型。研究表明,PDO冷年索饵场4月SST与年CPUE显著相关（P<0.05）,PDO暖年索饵场11月的SST与年标准化CPUE显著相关（P<0.05）。PDO冷、暖年的秋刀鱼资源丰度的预测模型中,CPUE均与索饵场11月的SST、索饵场4月SST呈现正相关的关系,统计学上为显著相关（P<0.05）。PDO冷年（2012年）和PDO暖年（2014年）的CPUE预测值与实际值相对误差分别为14.03%、-16.26%,具有较好的拟合效果。研究认为,不同气候模态下,可用于秋刀鱼资源丰度预测的环境因子不同,上述建立资源丰度模型可用于业务化运行。     

超慢速扩张环境下超镁铁质岩系统的热液硫化物成矿机理以及启示

西南印度洋63.5°E热液区是在超慢速扩张洋脊发现的首个超镁铁质岩热液系统。对取自该区的热液硫化物样品进行了系统的矿物学和地球化学分析,矿物学分析结果表明:该热液区硫化物为富Fe型高温硫化物,且经历了较深程度的氧化蚀变,大量中间态的Fe氧化物充填在硫化物矿物间的孔隙及内部解理中;这些硫化物相以白铁矿为主,其次是等轴古巴矿和少量铜蓝,缺乏黄铁矿、闪锌矿。据推断,该区的热液成矿作用分为4个阶段:低温白铁矿阶段→高温等轴古巴矿阶段→自形白铁矿阶段→后期海底风化阶段（少量铜蓝以及大量的Fe的羟氧化物）。与之相对应,地球化学分析结果表明这些硫化物的Fe含量较高（31.57%~44.59%）,Cu含量次之（0.16%~7.24%）,而Zn含量普遍较低（0.01%~0.11%）;微量元素较为富集Co（328×10-6~2 400×10-6）和Mn（48.5×10-6~1 730×10-6）。该区硫化物中较高含量的Fe、Co与超镁铁质岩热液系统相似,明显高于镁铁质岩热液系统。独特的热液硫化物矿物学特征和元素组成可能与该区普遍出露的地幔岩、橄榄岩蛇纹石化作用以及拆离断层的广泛发育的环境有关。     

基于星载红外辐射计的北极海表温度数据对比分析

本文基于2016年MODIS(ModerateResolutionImagingSpectroradiometer)-Aqua、MODIS-Terra和VIIRS(Visible Infrared Imager Radiometer Suite)三种红外辐射计的海表面温度(Sea Surface Temperature,SST)数据,统计了北极地区红外SST1月和7月的覆盖率及有效覆盖天数,并与Argo(Arrayfor Real-timeGeostrophicOceanography)浮标数据进行了匹配验证,直观获取北极SST误差分布情况并研究SST遥感观测能力,为更好地了解北极地区从而应对气候变化提供一定的资料基础。结果表明,北极地区红外辐射计SST数据7月的覆盖率和有效观测天数均高于1月,1月三种数据相差不大,7月VIIRS的覆盖率和有效观测天数均优于MODIS-Aqua和MODIS-Terra,联合三种红外辐射计的覆盖率和有效观测天数相较于单星有所增加, 1月覆盖率最高为8%, 7月最高接近70%,表明多星联合探测是提高北极地区SST数据覆盖率和观测天数的有效方法;北极地区SST数据的误差普遍高于全球总体水平, VIIRS白天、夜间的均方根误差(E_(rms))均低于MODIS-Aqua和MODIS-Terra, MODIS-Aqua白天SST的E_(rms)高于MODIS-Terra,夜间则低于MODIS-Terra。综合来看, VIIRS在北极的覆盖率、有效观测天数及与浮标的匹配结果在三种红外辐射计中为最优。     

基于ROMS和4DVAR的沿轨与网格化SSH数据同化效果评价

Remote sensing products are significant in the data assimilation of an ocean model. Considering the resolution and space coverage of different remote sensing data, two types of sea surface height(SSH) product are employed in the assimilation, including the gridded products from AVISO and the original along-track observations used in the generation. To explore their impact on the assimilation results, an experiment focus on the South China Sea(SCS) is conducted based on the Regional Ocean Modeling System(ROMS) and the four-dimensional variational data assimilation(4 DVAR) technology. The comparison with EN4 data set and Argo profile indicates that, the along-track SSH assimilation result presents to be more accurate than the gridded SSH assimilation, because some noises may have been introduced in the merging process. Moreover, the mesoscale eddy detection capability of the assimilation results is analyzed by a vector geometry–based algorithm. It is verified that, the assimilation of the gridded SSH shows superiority in describing the eddy's characteristics, since the complete structure of the ocean surface has been reconstructed by the original data merging.     

Newly discovered hydrothermal fields along the ultraslow-spreading Southwest Indian Ridge around 63°E

The ultraslow-spreading Southwest Indian Ridge(SWIR) to the east of the Melville fracture zone is characterized by very low melt supply and intensive tectonic activity. Due to its weak thermal budget and extremely slow spreading rate, the easternmost SWIR was considered to be devoid of hydrothermal activity until the discovery of the inactive Mt. Jourdanne hydrothermal field(27°51′S, 63°56′E) in 1998. During the COMRA DY115-20 cruise in2009, two additional hydrothermal fields(i.e., the Tiancheng(27°51′S, 63°55′E) and Tianzuo(27°57′S, 63°32′E)fields) were discovered. Further detailed investigations of these two hydrothermal sites were conducted by Chinese manned submersible Jiaolong in 2014–2015. The Tiancheng filed can be characterized as a lowtemperature(up to 13.2°C) diffuse flow hydrothermal field, and is hosted by fractured basalts with hydrothermal fauna widespread on the seafloor. The Tianzuo hydrothermal field is an inactive sulfide field, which is hosted by ultramafic rocks and controlled by detachment fault. The discovery of the three hydrothermal fields around Segment #11 which receives more melt than the regional average, provided evidence for local enhanced magmatism providing heat source to drive hydrothermal circulation. We further imply that hydrothermal activity and sulfide deposits may be rather promising along the easternmost SWIR.     

构造-岩浆作用对热液活动的控制机理: 马努斯海盆为例

综述了马努斯海盆热液区构造特征、基底差异, 结合马努斯海盆热液区热液活动与构造-岩浆特征, 探讨了二者的耦合关系, 以及构造-岩浆作用对热液活动的影响和控制。马努斯海盆位于西南太平洋俾斯麦海的东北部, 是世界上扩张速度最快的海盆之一。马努斯海盆西部(马努斯扩张中心, Manus Spreading Center, MSC)主要由海盆扩张成熟期产生的大洋中脊玄武岩组成, 属于成熟弧后扩张中心,发育Vienna Woods热液区; 海盆东部(东南裂谷, Southeast Rift, SER)则是一个拉张裂谷, 处于扩张的早期阶段, 属于不成熟弧后扩张中心, 发育PACMANUS、DESMOS、SuSu Knolls三大热液区。MSC与大洋中脊的热液活动相似, 而SER因受到火山、俯冲作用影响更为显著, 其热液流体具有岩浆流体和俯冲流体的特征。与Vienna Woods热液压相比, PACMANUS、DESMOS以及SuSu Knolls三个热液区的水深相对较浅(1 150～1 740 m), 是地球内部热物质由内向外迁移的结果, 其下部岩浆作用强烈。此外,岩浆脱气作用和数值模拟结果表明, PACMANUS热液系统中具有岩浆流体的输入。与Vienna Woods热液区相比, PACMANUS、DESMOS、SuSu Knolls热液区的热液活动强度及流体组成主要受控于岩浆作用。     

基于MISR多角度光学遥感影像的海面风速估算实验

太阳耀光是来自粗糙海面的直接太阳反射光,其强度与海面粗糙度密切相关,而海面粗糙度主要受海面风场影响。因此,包含太阳耀光信息的光学遥感影像在海洋动力过程和海面风速探测中具有积极意义。本文利用2016年2月到2017年3月期间成像的25幅Terra卫星MISR(Multi-angle Imaging Spectro Radiometer)传感器的多角度遥感影像,分别提取了太阳的高度角和方位角、正视和后视影像的卫星观测角、方位角等信息,校正获得正视和后视影像的太阳耀光辐射强度,进一步反演海表面粗糙度信息,进而计算海面风速。最后利用ECMWF(European Centre for Medium-Range Weather Forecasts)的模式风速数据与反演获得的风速结果进行对比验证。结果表明,两者的相关系数较高(R=0.745),均方根误差和平均绝对偏差值分别为1.514 m·s^-1和1.319 m·s^-1。初步实验结果表明,利用MISR多角度光学遥感影像估算海表面风速是可行性的。