渤海生态动力过程的模型研究 Ⅱ.营养盐以及叶绿素a的季节变化

利用在本系列研究第一部分中所建立的耦合的生物物理模型,模拟了渤海浮游植物生物量和营养盐含量的年度循环特征.模拟结果显示:藻类的春季水华是由经过一冬积累在水体中的营养盐导致,而水华开始的时间在浅水区明显早于深水区,对此深水区水体层化结构的形成可能起着重要作用;另一方面,河载营养盐与悬起的沉积物所释放的营养盐是诱发夏季水华的共同原因.基于模型结果,我们还发现:渤海的浮游植物动力特性就整体而言依然受无机氮限制,但是在莱州湾,磷限制特性表现得非常明显,这主要是由于每年黄河都要携带大量的无机氮进入海水,从而导致莱州湾营养盐的氮磷比已远远超过16.     

阿拉伯海的扩张历史：某些新的控制条件

根据海台、无震海岭．活动洋中脊以及几条破碎带，可把阿拉伯海划分成几个深海盆地．这些盆地的进化历史已从地球物理的研究中推演出来．东阿拉伯海盆(EAB)位于Laxmi-Laceadive海岭及印度的西部大陆坡之间，被认为其下伏是由裂谷和相关过程形成的过渡地壳，     

An Experi mental Study on Wave-Induced Dynamic Stresses in Seabed

1 .IntroductionEvery year ,Taiwanis subjectedtotwo or three typhoonintrusions in average which always causedisasters . Most of the disasters which occur around the coastal zone are due to seabed instability andcoastal structure destruction caused bytyphoo…     

60Co－γ辐照对坛紫菜原生质体诱变的研究

利用^60Co-γ射线对坛紫菜（Porphyra haitanensis）原生质体进行辐照诱变，发现原生质体对^60Co-γ射线有极强的耐受性。前期的培养结果表明，原生质体是一种理想的诱变材料。诱变结果表明，^60Co-γ射线对坛紫菜可诱变剂量范围很大，从200-1300 Gy均有突变株生成。诱变后细胞的存活率不宜作为坛紫菜诱变最佳剂量的指标。     

海浪波群的谱特征分析

海浪的波谱特征分析对认识海浪有重要的意义，因为海浪谱反映了海浪的结构成分。这对海工建筑、海洋运输、船舶制造、海浪预报和海浪模拟等均有重要的实用意义。 波群是伴随海浪经常出现的一种自然现象，且经常伴随大浪的出现而出现。实践证明，波群具有极大的破坏力，其破坏性远比单个波大得多，它是海浪破坏海工建筑物的重要因子，许多防波堤的破坏并非是由单个波的作用，而是由相继出现的几个大波(波群)作用的结果。早先，人们对波群这种习见的现象研究甚少。自1974年葡萄牙锡尼斯港深水防波堤的破坏之后，对波群的研究才日益受到重视。 对波群的研究目前多采用包络方法、马尔科夫链方法和波能过程线法。波群研究的主要内容是波群的统计特征(如波群链长统计)；另外，波群的模拟也是重要的研究内容之一。目前用包络方法研究波群比较普遍，且有不少研究成果。徐德伦等(2001)综述了这方面的研究进展及结果，文圣常等(1984)也进行了详尽的讨论。 以往的研究大都是研究波群的统计特征，如合田良实(1976)、 Ewing(1973)、Rye(1974)。而针对地域性的波浪，我国学者也只是以包络方法为基础讨论了不同地域海浪波群的统计特征(常德馥，1987；葛明达，1986；范顺庭，1998)。就波群本身的结构特征而言，即波群的波谱分析特征以往的研究涉及尚少。作者拟借助于谱分析方法，对带有典型波群的实测的海浪记录来分析海浪波群的波谱结构，进而借此对海浪波群的结构特征进行深入探讨。     

东海沿岸海区垂直环流及其温盐结构动力过程研究Ⅱ．温盐结构

对于本研究采用的动力学模型及其垂直环流的模拟结果已在第Ⅰ部分论述。作者将对与垂直环流对应的温、盐结构进行分析。温度和盐度模拟结果表明：冬季东海沿岸海区的温、盐分布均为近岸低、外海高;近岸温、盐呈垂直均匀分布,在外海出现分层,其温度为表层高、底层低,而盐度却为表层和底层高,中层偏低,长江口以南的近表层以下形成自近岸伸向外海的弱低盐水舌;长江冲淡水区及长江口以北和其以南外海的近表层有温、盐跃层生成,深底层温、盐呈均匀分布,且保持低温高盐特征;随着海区自北往南纬度的降低,岸坡和水深的增大及沿岸下降流的增强,温度和盐度自近岸至外海的垂直均匀分布跨度逐渐变窄;外海近表层的温、盐跃层强度自北至长江口逐渐增强,而自长江口至南逐渐减弱,其位置自北往南逐渐上移;冬季沿岸下降流使长江冲淡水区的盐跃层变厚。夏季海区的温度分布为近岸和外海高,近岸稍远出现冷水涌升,垂向上呈现显著分层,盐度分布为近岸低、外海高;长江冲淡水区及杭州湾以南外海的次表层存在温、盐跃层,其跃层以上出现混合层,且保持高温低盐特征,跃层以下温、盐大致呈均匀分布,并保持低温高盐特征;随着海区自南往北纬度的增高、岸坡和水深的减小及沿岸上升流自南至长江口和自长江口至北的增强和继而减弱,长江冲淡水区的温、盐跃层强度自南至长江口逐渐增强,而自长江口至北逐渐减弱,外海次表层的温、盐跃层强度却自南至长江口逐渐减弱,自长江口至北又逐渐增强,其温、盐跃层的位置自南往北逐渐上移;夏季沿岸上升流使长江冲淡水区的盐跃层变薄。     

Marine mammals from northeast Atlantic: relationship between their trophic status as determined by delta13C and delta15N measurements and their trace metal concentrations

The relationship between trophic position through delta13C and delta15N and trace metal concentrations (Zn, Cd, Cu and Hg) was investigated in the tissues of six marine mammal species from the Northeast Atlantic: striped dolphin Stenella coeruleoalba, common dolphin, Delphinus delphis, Atlantic white-sided dolphin Lagenorhynchus acutus, harbour porpoise Phocoena phocoena, white beaked-dolphin Lagenorhynchus albirostris, grey seal Halichoerus grypus stranded on French Channel and Irish coasts. White-beaked dolphins, harbour porpoises, white-sided dolphins, common and striped dolphins display the same relative and decreasing trophic position, as measured by delta15N values, along both the Irish and French channel coasts, reflecting conservative trophic habits between these two places. Hepatic and renal Cd concentrations were significantly correlated to muscle delta13C and delta15N values while Hg, Zn and Cu did not. These results suggest that Cd accumulation is partly linked to the diet while other factors such as age or body condition might explain Hg, Zn or Cu variability in marine mammals. Combined stable isotope and trace metal analyses appear to be useful tools for the study of marine mammal ecology.     

东太平洋海隆上的现代成矿作用

研究了活动的“黑色吸烟者”区大洋底层水中，悬浮和溶解诉Ｈｇ、Ｃｅ，Ｚｎ的空间分布，当液体从喷泉的管道中流出时，在周围的海水敢特殊的蘑菇状异常区，可达海底以上１０００ｍ处。该区富含溶解的锌和铈但贫溶解的汞。悬浮状态的金属异常区到达较低的层位，在该处水的上升速度接近或小于悬浮颗粒的下沉速度。随着向较高层位过渡 ，明显地观察到悬浮状态向溶解状态的转移过程。     

Impact-generated atmospheres over Titan, Ganymede, and Callisto

The competition between impact erosion and impact supply of volatiles to planetary atmospheres can determine whether a planet or satellite accumulates an atmosphere. In the absence of other processes (e.g., outgassing), we find either that a planetary atmosphere should be thick, or that there should be no atmosphere at all. The boundary between the two extreme cases is set by the mass and velocity distributions and intrinsic volatile content of the impactors. We apply our model specifically to Titan, Callisto, and Ganymede. The impacting population is identified with comets, either in the form of stray Uranus-Neptune planetesimals or as dislodged Kuiper belt comets. Systematically lower impact velocities on Titan allow it to retain a thick atmosphere, while Callisto and Ganymede get nothing. Titan's atmosphere may therefore be an expression of a late-accreting, volatile-rich veneer. An impact origin for Titan's atmosphere naturally accounts for the high D/H ratio it shares with Earth, the carbonaceous meteorites, and Halley. It also accounts for the general similarity of Titan's atmosphere to those of Triton and Pluto, which is otherwise puzzling in view of the radically different histories and bulk compositions of these objects.