杭州湾北岸高能潮滩的基本特征

根据纵向泥沙输移中的能量变化,潮滩可分为侵蚀、堆积和稳定三种类型,杭州湾由于北岸潮滩冲淤变化较小,属于基本稳定岸滩。     

第23章 DNS模式:一种为大洋波浪预报而改进的谱模式

23.1 介绍 模拟与频率和方向相关的大洋波谱F（f,θ）的工作是极其困难的。唯一有点统一的理论（Hasselmann,1967）也还没有简化成一种实用形式。这篇研究中所探讨的是结合零散的,现有的理论,以达到这样一种目的:即发展一种与我们目前对风浪成长谱的了解相一致 ·95.的波谱模式。本章中我们将讨论一种离散的谱模式,这种模式采用了一种改进的能量传播的特征方法。数值方法最早是由Barnett等（1969）提出的。     

由偏顶蛤贝壳中稳定同位素剖面追溯海水温度记录

本文用在加拿大诺瓦·斯科舍省芬克湾采集到的两只活体偏顶蛤(Modiolus)贝壳上的氧同位素组成重建了过去十年间的底层海水温度记录,它也可作为一种独立的方法来确定贝壳上外生长线的沉积时间。由于对贝壳进行了密集采样(可多至每个贝壳沉积年份取15个样品),贝壳上的δ~(16)O变化反映了芬克湾底层海水的季节性变化。两只贝壳所得的温度剖面符合得很好,说明它们基本上是与真实的环境温度相对应的。本研究证明在海胆疾病爆发时底层海水的温度并没有异常升高,这说明疾病传播的关键因素是带病的生物体,而不是温度。同位素技术也说明了在贝壳外表面上可见的外生长线是年轮性的,它们是在每年冬季最低水温时沉积出来的。     

重金属对海洋围隔生态系中初级生产力的影响

1985年4月,中国和加拿大科学家首次在厦门合作进行添加重金属(Cu,Hg,Zn,Pb,Cd)的围隔生态系实验,实验是在海边大水池内的塑料袋中进行,实验结果说明低水平(ppb)混合重金属对浮游植物的影响首先表现在对光合作用速率的抑制作用,以及在浓度较低的情况下可能引起的种群演替现象,本文还阐述了颗粒有机碳(POC)和颗粒有机氮(PON)与初级生产力的相关性.     

Environmental consequence analyses of fish farm emissions related to different scales and exemplified by data from the Baltic--a review

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.     

贝尔凹陷构造演化及其对沉积和油气的控制作用

贝尔凹陷是海拉尔盆地南部的一个次级凹陷,凹陷内蕴藏着丰富的油气资源,是海拉尔盆地重要的油气探区之一。贝尔凹陷经历了三期构造演化,形成了三期不同类型的原型盆地,自下而上分别为下部伸展断陷盆地、中部裂后热沉降盆地和上部构造反转盆地。复杂的构造演化形成了复杂的断裂系统,贝尔凹陷纵向上主要发育了两套断裂系统,分别是发育于下部断陷盆地的下部断裂系统和发育于中部热沉降盆地的上部走滑断裂系统,上部构造反转盆地内断裂不发育。复杂的构造样式对凹陷内沉积体系的配置也起着很重要的控制作用。本文从贝尔凹陷构造演化和构造特征研究出发,分析了沉积作用对构造活动的响应,初步探讨了贝尔凹陷构造对油气藏形成的控制作用。     

下地壳基性麻粒岩流变强度实验研究

镁铁质基性麻粒岩被认为可能是大陆下地壳的主要组成岩石[1,2],涉及当前地球动力学研究中地壳变形和高原隆升,壳幔边界的力学耦合与拆离,底侵和拆沉作用等一系列地球动力学问题阳[3,4],具有重要的地球动力学意义.大陆下地壳的流变学性质是我们深入认识这些地球深部过程的关键点之一.     

Detection of a new interstellar molecular ion, H2COH+ (protonated formaldehyde)

A new interstellar molecular ion, H2COH+ (protonated formaldehyde), has been detected toward Sgr B2, Orion KL, W51, and possibly in NGC 7538 and DR21(OH). Six transitions were detected in Sgr B2(M). The 1(1,0)-1(0,1) transition was detected in all sources listed above. Searches were also made toward the cold, dark clouds TMC-1 and L134N, Orion (3N, 1E), and a red giant, IRC + 10216, without success. The excitation temperatures of H2COH+ are calculated to be 60-110 K, and the column densities are on the order of 10(12)-10(14) cm-2 in Sgr B2, Orion KL, and W51. The fractional abundance of H2COH+ is on the order of 10(-11) to 10-(9), and the ratio of H2COH+ to H2CO is in the range 0.001-0.5 in these objects. The values in Orion KL seem to be consistent with the "early time" values of recent model calculations by Lee, Bettens, & Herbst, but they appear to be higher than the model values in Sgr B2 and W51 even if we take the large uncertainties of column densities of H2CO into account. We suggest production routes starting from CH3OH may play an important role in the formation of H2COH+.     

A photochemical model of the martian atmosphere

The factors governing the amounts of CO, O2, and O3 in the martian atmosphere are investigated using a minimally constrained, one-dimensional photochemical model. We find that the incorporation of temperature-dependent CO2 absorption cross sections leads to an enhancement in the water photolysis rate, increasing the abundance of OH radicals to the point where the model CO abundance is smaller than observed. Good agreement between models and observations of CO, O2, O3, and the escape flux of atomic hydrogen can be achieved, using only gas-phase chemistry, by varying the recommended rate constants for the reactions CO + OH and OH + HO2 within their specified uncertainties. Similar revisions have been suggested to resolve discrepancies between models and observations of the terrestrial mesosphere. The oxygen escape flux plays a key role in the oxygen budget on Mars; as inferred from the observed atomic hydrogen escape, it is much larger than recent calculations of the exospheric escape rate for oxygen. Weathering of the surface may account for the imbalance. Quantification of the escape rates of oxygen and hydrogen from Mars is a worthwhile objective for an upcoming martian upper atmospheric mission. We also consider the possibility that HOx radicals may be catalytically destroyed on dust grains suspended in the atmosphere. Good agreement with the observed CO mixing ratio can be achieved via this mechanism, but the resulting ozone column is much higher than the observed quantity. We feel that there is no need at this time to invoke heterogeneous processes to reconcile models and observations.