伊豆—小笠原海沟之西迁和菲律宾海板块之北...     

Otsuki  K 赵国先 《海洋地质译丛》1991,(6):9-17

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Impacts of stormwater discharges on the nearshore benthic environment of Santa Monica Bay     

Schiff K  Bay S 《Marine environmental research》2003,56(1-2):225-243

Although large loads of potentially toxic constituents are discharged from coastal urban watersheds, very little is known about the fates and eventual impacts of these stormwater inputs once they enter the ocean. The goal of this study was to examine the effects of stormwater discharges on the benthic marine environment of Santa Monica Bay. Sediment samples were collected across a gradient of stormwater impact following significantly sized storm events offshore Ballona Creek (a predominantly developed watershed) and Malibu Creek (a predominantly undeveloped watershed). Sediments offshore Malibu Creek had a greater proportion of fine-grained sediments, organic carbon, and naturally occurring metals (i.e., aluminum and iron), whereas sediments offshore Ballona Creek had higher concentrations of anthropogenic metals (i.e., lead) and organic pollutants (i.e., total DDT, total PCB, total PAH). The accumulation of anthropogenic sediment contaminants offshore Ballona Creek was evident up to 2 km downcoast and 4 km upcoast from the creek mouth and sediment concentrations covaried with distance from the discharge. Although changes in sediment texture, organic content, and an increase in sediment contamination were observed, there was little or no alteration to the benthic communities offshore either Ballona or Malibu Creek. Both sites were characterized as having an abundance, species richness, biodiversity and benthic response index similar to shallow water areas distant from creek mouths throughout the Southern California Bight. There was not a preponderance of pollution tolerant, nor a lack or pollution sensitive, species offshore either creek mouth.  相似文献   

盐渍土壤的介电特性     

Sree.  K 《海岸工程》1996,15(4):81-85

采用Ｌ波段介电探针，对沙壤，砂质粘土和粘土三种不同性质的土壤作了详尽的实验室实验，结果显示，土壤的盐度同介电常数的实无关，而同虚部相关，并随盐度的增加而增加。还表明，实数部分更多的依赖于土壤的湿度，虚数部分取决地土壤的盐度，土壤的含钠性对介电常数的实部和虚部都无影响。本研究展示了Ｌ波段对土壤盐度的微波响应。同时说明，在湿壤的条件下，采用Ｌ波段，将盐壤从钠壤中分离出来的可能性。  相似文献   

Molecular identification of bloom-forming species Phaeocystis globosa(Prymnesiophyta)and its dispersal based on rDNA ITS sequence analysis   总被引：3，自引：1，他引：3  

Chen Yueqin  Shao Peng  Wang Ning  Zhou Hui  Qu Lianghu  Linda K. Medlin 《海洋学报(英文版)》2003,22(2)

Abstract-The colony-forming Phaeocystis species are causative agents of dense bloom occurrences incoastal waters worldwide. It is difficult to separate them because of the different morphologies associatedwith their colonial stages. In this study we applied molecular approaches to analyze the genetic variationof Phaeocystis globosa and Phaeocystis pouchetii from several geogrtaphic regions, and to assist in tracingthe dispersal of bloom-forming Phaeocystis species in coastal waters of China. The Sequences of the inter-nal transcribed sacers (ITS1 and ITS2) of rDNA and the 5.8S ribosomal RNA gene of Phaeocystisstrains were determined. Sequence comparison shows that P.globosa was the most divergent toP. pouchetii, exhibiting sequence divergence higher than 0.08. However, lower genetic divergences ex-isted between strains of P.globosa. The sequence comparison of the Phaeocystis rDNA ITS clearlyshows that the species isolated from the southeast coast of China is identified as P. globosa rather thanP. cf. po  相似文献   

阿拉伯海的扩张历史：某些新的控制条件     

A.K.Chaubey尹延鸿  李延成 《海洋地质前沿》1994,(1):12-13

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，  相似文献   

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

S.C.Chang  L.K.Chien  J .G.Lin  Y.F.Chiu 《中国海洋工程》2006,20(1)

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…  相似文献   

西南日本俯冲带的热状态“俯冲板块年龄史的影响     

Wang.  K 戴佩君 《海洋地质译丛》1996,(2):47-58

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

Das K  Beans C  Holsbeek L  Mauger G  Berrow SD  Rogan E  Bouquegneau JM 《Marine environmental research》2003,56(3):349-365

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.  相似文献   

东太平洋海隆上的现代成矿作用     

K.  AH 朱佛宏 《海洋地质》1995,(2):57-64

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。  相似文献   

Impact-generated atmospheres over Titan, Ganymede, and Callisto     

Zahnle K  Pollack JB  Grinspoon D  Dones L 《Icarus》1992,95(1):1-23

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.  相似文献