冬、夏季渤黄海表层沉积物粒度特征差异及其成因分析

对渤海、黄海海域冬、夏两季表层沉积物取样,通过激光粒度仪得出粒度参数,进而分析讨论冬季强的沿岸流的作用、黄海暖流、夏季冷水团的影响以及地形、海底地貌特征、物源特征等对表层沉积物分布造成的影响。结果表明,冬、夏两季渤黄海表层沉积物粒度特征总体上相差不大,但部分海域如渤海中北部、渤海中南部、北黄海西北部近渤海海峡北部海域、山东半岛东北部海域、南黄海中部沉积物粒度特征存在明显季节性差异。表层沉积物粒度特征季节性差异与地形地貌、沿岸流、黄海暖流、黄海冷水团及物源密切相关。本研究对于探讨渤黄海不同季节表层沉积物沉积特征的影响机制、了解渤黄海区海洋动力过程的季节差异有积极意义。     

南黄海中部全新世磁性铁质球粒富集层的发现和意义

国际上对于微玻璃陨石、磁性铁质球粒方面的研究取得了不少进展,包括研究其年代学、分布特征、矿物学特征、地球化学特征等[1~5].人们认为,形成这些微玻璃陨石、磁性铁质球粒的地质事件对生物灭绝、古气候、古环境演变有明显影响[3,6,7].     

黄海冷水团演变过程及其与邻近水团关系的分析

黄海冷水团是出现在黄海的一种独特的水文现象.文中利用覆盖整个黄海的GDEM三维水温资料,结合近期一些大型调查所获得的有关观测研究结果,首先较系统地分析了黄海冷水团的形成和演变过程,并对冷水团3个冷中心的季节演变提出了一些与前不同的认识.同时,通过对黄海冷水团形成、发展和消亡与该海域温跃层演变关系的分析,进一步揭示了黄海冷水团演变的机理.然后,探讨了黄海冷水团演变过程中与青岛和仁川东南海域冷水团以及东海北部底层冷水的关系.分析表明,在黄海冷水团发展的鼎盛时期,青岛冷水团和仁川东南海域冷水团以及东海北部底层冷水皆包络其中.     

温度骤降对大黄鱼Larimichthys crocea鱼卵与仔鱼的影响

滨海电厂温排水停止排放以及季节更替、寒潮来袭等现象会引起海水温度降低,从而对鱼类等变温生物产生冷冲击效应。本研究通过模拟水温骤降情形,以孵化率、死亡率、畸形率等为指标,探讨了温度骤降对大黄鱼早期发育阶段(鱼卵和仔鱼)的冷冲击作用。研究发现,大黄鱼仔鱼(3日龄)对温度骤降的敏感性略高于鱼卵。在大黄鱼鱼卵和仔鱼的适温范围内,当水温由22 ℃骤降至19 ℃或16 ℃时,鱼卵的孵化率和死亡率无明显变化,而胚胎发育和仔鱼的生长发育均减缓,仔鱼的死亡率提高;水温超出适温范围,由22 ℃骤降至13 ℃或10 ℃时,对鱼卵和仔鱼造成致命的冷冲击伤害,48 h累积死亡率分别为84.6%~100%和72.1%~98.2%。由此推测:当水温骤降超出适温范围后,大黄鱼的早期发育阶段遭受致命的冷冲击伤害,从而影响种群补充和年龄结构。     

冷泉系统甲烷气体渗漏的声学特征及潜在环境效应

The amount of methane leaked from deep sea cold seeps is enormous and potentially affects the global warming,ocean acidification and global carbon cycle. It is of great significance to study the methane bubble movement and dissolution process in the water column and its output to the atmosphere. Methane bubbles produce strong acoustic impedance in water bodies, and bubble strings released from deep sea cold seeps are called "gas flares"which expressed as flame-like strong backscatter in the water column. We characterized the morphology and movement of methane bubbles released into the water using multibeam water column data at two cold seeps. The result shows that methane at site I reached 920 m water depth without passing through the top of the gas hydrate stability zone(GHSZ, 850 m), while methane bubbles at site II passed through the top of the GHSZ(597 m) and entered the non-GHSZ(above 550 m). By applying two methods on the multibeam data, the bubble rising velocity in the water column at sites I and II were estimated to be 9.6 cm/s and 24 cm/s, respectively. Bubble velocity is positively associated with water depth which is inferred to be resulted from decrease of bubble size during methane ascending in the water. Combined with numerical simulation, we concluded that formation of gas hydrate shells plays an important role in helping methane bubbles entering the upper water bodies, while other factors, including water depth, bubble velocity, initial kinetic energy and bubble size, also influence the bubble residence time in the water and the possibility of methane entering the atmosphere. We estimate that methane gas flux at these two sites is 0.4×10~6–87.6×10~6 mol/a which is extremely small compared to the total amount of methane in the ocean body, however, methane leakage might exert significant impact on the ocean acidification considering the widespread distributed cold seeps. In addition, although methane entering the atmosphere is not observed, further research is still needed to understand its potential impact on increasing methane concentration in the surface seawater and gas-water interface methane exchange rate, which consequently increase the greenhouse effect.     

Macrobenthic infaunal communities associated with deep‐sea hydrocarbon seeps in the northern Gulf of Mexico

There are thousands of seeps in the deep ocean worldwide; however, many questions remain about their contributions to global biodiversity and the surrounding deep‐sea environment. In addition to being globally distributed, seeps provide several benefits to humans such as unique habitats, organisms with novel genes, and carbon regulation. The purpose of this study is to determine whether there are unique seep macrobenthic assemblages, by comparing seep and nonseep environments, different seep habitats, and seeps at different depths and locations. Infaunal community composition, diversity, and abundance were examined between seep and nonseep background environments and among three seep habitats (i.e., microbial mats, tubeworms, and soft‐bottom seeps). Abundances were higher at seep sites compared to background areas. Abundance and diversity also differed among microbial mat, tubeworm, and soft‐bottom seep habitats. Although seeps contained different macrobenthic assemblages than nonseep areas, infaunal communities were also generally unique for each seep. Variability was 75% greater within communities near seeps compared to communities in background areas. Thus, high variability in community structure characterized seep communities rather than specific taxa. The lack of similarity among seep sites supports the idea that there are no specific infauna that can be used as indicators of seepage throughout the northern Gulf of Mexico, at least at higher taxonomic levels.     

碱性玄武岩形成的时限及其地质意义

中国华北克拉通及邻区的早前寒武纪不存在碱性玄武岩。全球范围内碱性玄武岩的形成也存在时限性，它们在中新生代以来相对大量的出现。碱性玄武岩可划分为钾质碱性玄武岩和钠质碱性玄武岩两大类，后者还可作进一步划分。它们在同位素组成和元素组成上存在相互过渡的变化，这与地幔源区外来加入物质的种类和比例不同有关。高压和低程度熔融是所有碱性玄武岩形成的必要条件。研究表明，碱性玄武岩形成具时限性主要与地球热状态从热向冷的历史演化有关。碱性玄武岩的形成需要地幔俯冲作用，可达到相当深度的地幔俯冲作用只是到了太古宙以后才发生，并在中新生代以来达到高潮。     

Community structure of infaunal macrobenthos around vestimentiferan thickets at the San Clemente cold seep,NE Pacific

The San Clemente cold seep lies within 100–200 km of other reducing habitats in the NE Pacific, offering an opportunity to compare diversity and species overlap among reducing habitats (i.e. whale‐, kelp‐, and wood‐falls) at similar depths within a single region. Video observations from the research submersible Alvin at the San Clemente seep (1800 m depth) indicated clumps (‘thickets’) of vestimentiferans distributed as meter‐scale patches interspersed with vesicomyid clam beds and black sediments. Sediment‐core samples were collected at distances of 0 to 80–200 m along randomly oriented transects radiating outward from vestimentiferan thickets to evaluate changes in macrofaunal community structure from thickets into the background community. Macrofaunal abundance was elevated at distances of 0–1 m compared to 80–200 m (i.e. the ‘background’ community). The tube‐building frenulate worms Siboglinum spp., along with peracarid crustaceans, dominated sediments within 1 m of vestimentiferan thickets. Species diversity was depressed within 1 m of thickets but with high rates of species accumulation, suggesting that seep sites greatly increase sediment heterogeneity and facilitate colonization by non‐background macrofaunal species. Stable isotope data indicate chemosynthetic nutrition for some dominant macrofaunal species within 1 m of tubeworm thickets. The macrofaunal community near vestimentiferan thickets in San Clemente seep contains intermediate levels of species richness and diversity compared to other deep‐sea seep areas in the northeast Pacific. There was low species overlap between the San Clemente seep macrofauna and communities in reducing habitats near wood‐, whale‐, and kelp‐falls at similar depths within the region, suggesting that seeps harbor a distinct infaunal community.     

A comparison of the main methods for estimating probabilities of extreme still water levels

Sea-level return periods are estimated at 18 sites around the English Channel using: (i) the annual maxima method; (ii) the r-largest method; (iii) the joint probability method; and (iv) the revised joint probability method. Tests are undertaken to determine how sensitive these four methods are to three factors which may significantly influence the results; (a) the treatment of the long-term trends in extreme sea level; (b) the relative magnitudes of the tidal and non-tidal components of sea level; and (c) the frequency, length and completeness of the available data. Results show that unless sea-level records with lengths of at least 50 years are used, the way in which the long-term trends is handled in the different methods can lead to significant differences in the estimated return levels. The direct methods (i.e. methods i and ii) underestimate the long (> 20 years) period return levels when the astronomical tidal variations of sea level (relative to a mean of zero) are about twice that of the non-tidal variations. The performance of each of the four methods is assessed using prediction errors (the difference between the return periods of the observed maximum level at each site and the corresponding data range). Finally, return periods, estimated using the four methods, are compared with estimates from the spatial revised joint probability method along the UK south coast and are found to be significantly larger at most sites along this coast, due to the comparatively short records originally used to calibrate the model in this area. The revised joint probability method is found to have the lowest prediction errors at most sites analysed and this method is recommended for application wherever possible. However, no method can compensate for poor data.     

样品保藏方式与时间对海洋底栖细菌及原生生物荧光计数效能的影响

DAPI荧光染色技术已广泛应用于浮游细菌及原生生物的定量研究,但对底栖生物的定量效能尚缺必要的研究。比较了冷冻和冷藏两种保藏方式以及保存时间对DAPI荧光计数底栖细菌、蓝细菌、硅藻、不同粒级自养小鞭毛虫(PNF)和异养小鞭毛虫(HNF)的影响。对黄海冷水团三个站位表层2cm底栖样品进行的4℃冷藏与?20℃冷冻避光保存的比较研究表明,两种保藏方式下两个站位的所有研究对象均无显著差异,但另一站位的PNF(2~5μm和5~10μm)的冷藏保存显著优于冷冻保存。对选取的另外两个站位(0~2cm和2~5cm分层)的样品经1个月和4个月冷藏保存后的分析表明,对于底栖细菌、蓝细菌、PNF(5~10 μm)、PNF(10 μm)、HNF(10 μm)和硅藻在保存1个月和4个月后的计数没有显著差异,而对于PNF(2～5 μm)、HNF(2～5 μm)、HNF(5～10 μm)保存4个月的数量明显低于保存1个月的样品,如其中一个站位的0～2cm分层的PNF(2～5 μm)丰度减少了47.4%,2～5cm分层的丰度减少了59.6%,HNF(2～5 μm)和HNF(5～10 μm)经4个月后丰度降为0。本研究表明,对底栖细菌、蓝细菌以及原生生物的定量计数可因样品、保藏方式及保存时间的不同而产生差异,因此对于底栖样品短期内宜采用避光、冷藏保存,并在带回实验室后尽快分析。