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41.
The aim of this work is to review studies to evaluate how emissions from fish cage farms cause eutrophication effects in marine environments. The focus is on four different scales: (i) the conditions at the site of the farm, (ii) the local scale related to the coastal area where the farm is situated, (iii) the regional scale encompassing many coastal areas and (iv) the international scale including several regional coastal areas. The aim is to evaluate the role of nutrient emissions from fish farms in a general way, but all selected examples come from the Baltic Sea. An important part of this evaluation concerns the method to define the boundaries of a given coastal area. If this is done arbitrarily, one would obtain arbitrary results in the environmental consequence analysis. In this work, the boundary lines between the coast and the sea are drawn using GIS methods (geographical information systems) according to the topographical bottleneck method, which opens a way to determine many fundamental characteristics in the context of mass balance calculations. In mass balance modelling, the fluxes from the fish farm should be compared to other fluxes to, within and from coastal areas. Results collected in this study show that: (1) at the smallest scale (<1 ha), the "footprint" expressing the impact areas of fish cage farm often corresponds to the size of a "football field" (50-100 m) if the annual fish production is about 50 ton, (2) at the local scale (1 ha to 100 km2), there exists a simple load diagram (effect-load-sensitivity) to relate the environmental response and effects from a specific load from a fish cage farm. This makes it possible to obtain a first estimate of the maximum allowable fish production in a specific coastal area, (3) at the regional scale (100-10,000 km2), it is possible to create negative nutrient fluxes, i.e., use fish farming as a method to reduce the nutrient loading to the sea. The breaking point is to use more than about 1.1 g wet weight regionally caught wild fish per gram feed for the cultivated fish, and (4) at the international scale (>10,000 km2) related to the Baltic Proper, the contribution from fish farms to the overall nutrient fluxes are very small. We have also given two case-studies at the local scale where the impact of the fish farm emissions are greatest and the idea is to identify coastal areas unsuitable and suitable for fish cage farms and the reasons why. It should also be stressed that the results presented here are exemplified using emissions from fish farms, but that the underlying principles to evaluate the ecosystem effects of nutrient discharges from point source emissions are valid in a wider and more general perspective.  相似文献   
42.
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   
43.
天然气水合物广泛分布在海洋和极地沉积物中。在这种沉积物中具备足够低的温度和足够高的压力使得甲烷气结晶变成水合物。由于水合物的广泛分布和其潜在的能源潜力—据估计其约为地球上所有化石燃料能源的两倍.引起了全世界科学界的关注。然而。至今为止对水合物的性质和分布还了解不够,还没有合适的技术能对水合物进行定量的评价。根据地形、海底温度、沉积条件以及有机碳等资料指出在印度近海具备天然气水合物形成的条件。因此有必要在印度大陆边缘系统开展地质、地球化学和地球物理分析,以识别和估算天然气水合物的储量,评价其资源潜力。类似“气烟囱”或气体溢出持征、地震剖面上的BSR、氯化物或硫化物异常都是识别水合物的有用标志。层析成像、AVO、波形反演是定量分析水合物和游离气含量的重要手段。此外,在地震方法无法识别的地方,电阻率异常也有助干天然气水合物的识别。本文给出一些划出水合物赋存区边界和定量分析水合物及其下伏游离气含量的重要研究成果和技术。  相似文献   
44.
巴巴多斯和新几内亚的海平面变化表明:在过去的15000a中曾有过两次大规模的冰川融水流.同其它环境变化(如北大西洋深水环流)相比,这两次融水流形成的时间显然有助于我们进一步了解从未次冰期到问冰期的气候变迁及新仙女木事件.  相似文献   
45.
激光烧蚀微探针等离子体质谱的地质应用。自1989年以来,我们实验室就积极开展了激光烧蚀微探针(LAM)试样引入系统的研究工作,这种技术适合于ICP—MS分析地质样品中小体积矿物(激光烧蚀孔穴直径低于10—100μm).对某些样品.采用Nd:YAG激光的基本IR波长(1064nm),作为多数用途,4倍频率(uv)的波长(266nm)能产生较小的直径,并较好地形成孔穴.  相似文献   
46.
陆坡上水合物矿床中甲烷(CH4)的灾难性释放已显著干扰了古新世/始新世温度最高(PETM)期(约55.5Ma)的全球气候和碳循环。我们调查了所有PETM期古温度和古二氧化碳替代矿物是否与假设考虑大量增加的甲烷散发到大气圈的影响相一致。  相似文献   
47.
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   
48.
不同厚度冰层下的冰下火山喷发产物:两个来自南极的实例J.L.Smellie等本文着重介绍南极半岛两个保存最好的冰下层序(亚历山大岛的芒特皮纳佛和格雷厄姆地北部的布朗布拉夫).通过对岩相和岩相组合的分析确定喷发时和喷发后作用过程,以及原始冰层的最小厚度...  相似文献   
49.
50.
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   
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