海岛为何备受青睐     

恩波 《海洋世界》1996,(4)

在几百万分之一的地图上,蓝色的海洋中星星点点的分布着许许多多的岛屿。若在较大比例尺的地图上,大洋中和大陆边缘一带密密麻麻的岛屿,则更是数不清。对于这些四面环水,并在高潮时高于水面的自然形成的陆地区域,在过去并未能引起人们对它的特别关注。说起来,恐怕主要是两方面的原因:首先是由社会经济条件和科学技术水平决定的。设想,在社会生产水平低下,实践活动的范围非  相似文献   

软硬互层金刚石复合片钻头在地浸砂岩型铀矿中的研究及应用          下载免费PDF全文

要二仓  邢预恩  杨爱军 《探矿工程》2008,35(1):68-70

针对近年在巴音戈壁盆地及鄂尔多斯盆地钻探所遇到的复杂地质情况,研究试验了PDC钻头,在地浸砂岩铀矿钻探生产中取得了良好的效果,并制定总结了相应的钻进参数.  相似文献   

贻贝育苗中不同饵料的饲养效果比较     

张福绥  马江虎  何义朝  李淑英  刘祥生  于硕恩 《海洋科学集刊》1985,(25):91-102

培育双壳类软体动物幼苗所需的饵料，是指池内培育阶段适合于幼虫和幼苗(壳长一般在1mm以下)的饵料。育苗成功的关键问题之一为是否已经选择到这样的饵料。自40年代找到适宜的饵料生物以后，双壳类幼虫的培养才取得较明显的成效。以往利用过的一些饵料生物巳有文献系统记载。我国贻贝人工育苗是在分离与培养出扁藻以后才获得成功的。随着研究工作的深入以及适应各种不同情况的需要，采用的饵料种类越来越多样化。从生产性育苗特别是多茬育苗考虑，必须因地制宜地筛选出一定种数的饵料，以便在不同培养条件下有机动选择的余地。同一时还应找出适宜的投饵数量，以求取得较好的育苗效果。为此目的，我们于1975-1978年结合生产性育苗的需要进行了一些饵料饲养实验。本文根据实验结果以及多年来生产性育苗的实践，对贻贝育苗的饵料问题进行总结，侧重于不同饵料的饲养效果比较。  相似文献   

胶州湾贻贝苗源的发展     

张福绥  楼子康  马江虎  于硕恩  刘祥生  李淑英 《海洋科学集刊》1984,(22):115-126

贻贝(Mytilus edulis L.)是一种冷水性双壳类软体动物，它在我国沿岸分布的南限是胶州湾，但仅见于港内码头及船底上，且数量不多。 1958年青岛市水产局、原青岛市海水养殖场和中国科学院海洋研究所等单位曾一起自大连和烟台移贻贝苗至青岛试养，次年养殖架上也曾有少量幼苗附着，但未能大量繁殖起来。1971年后胶南县海水养殖试验场及青岛市第二海水养殖场等先后进行数十亩乃至数百亩移苗养殖，附苗量虽有所增长，但直至1974年仍缺乏生产意义。这种情况引起我们的思考:胶州湾贻贝苗源能否大量发展？它的限制因素是什么？ 1972年至1973年，我们与烟台地区海水养殖试验场等单位曾对烟台沿岸贻贝苗源进行调查研究，确认当时烟台苗种产量不高的主要原因是附着基不足，其次是亲贝不足，据此试验成功了“废旧草绠采苗法”。之后，随着采苗器材的增加及养殖面积的不断扩大，烟台芝罘湾已发展成为一个较好的苗场，通常可供万亩以上生产用苗。这个经验对我们开发胶州湾的苗源很有启发。 1975年胶南县在胶州湾大力推广“废旧草绠采苗法”，收割海带后保留废旧海带架两万台采贻贝苗， 1976年进一步扩大贻贝养殖面积，继续留绠采苗。我们在青岛市水产局及胶南县水产局等单位的协助下，于1975年9月及1976年8-9月，对胶州湾内及湾口(青岛前海)留绠采苗的情况进行了调查，这些调查资料即为本文的主要依据。  相似文献   

北黄试验海区的声速垂直结构模式与声线图     

孙琪田  张恩夫 《海洋通报》1996,15(1):21-26

从数理统计方法出发，对北黄试验海区收集来的从１９４９－１８７年的水文观测资料，按月按层地进行统计，并换算成声速，且绘制出逐月的声速垂直结构模式图，再依据射线理论，绘制分析了逐月的声线传播模式图，在为试验海区从事海上噪声和各类水声测试研究工作提供最蓁的海洋环境参数。  相似文献   

Imposex still evident in eastern Australia 10 years after tributyltin restrictions     

Gibson CP  Wilson SP 《Marine environmental research》2003,55(2):101-112

A survey of imposex in Thais orbita (Neogastropoda) along the New South Wales (NSW) coast, Australia, found imposex was still widespread 10 years after a partial ban on tributyltin (TBT) based antifouling paints. Transplant experiments also revealed that imposex was induced in T. orbita over a period of 9 weeks in Sydney Harbour, NSW. A comparison of the imposex data with that collected shortly after the introduction of restrictions on TBT revealed a general decline in imposex frequency occurring at open coast sites, an exception being the site at South West Rocks. Sites located within harbour/bay areas did not display a decline in imposex frequency but a decline in the severity of imposex was apparent. The observed decrease in imposex values in T. orbita may reflect a general decrease of butyltin contamination within the coastal environment. However, the persistence of contamination "hotspots" within harbours and bays remains a concern.  相似文献   

Underwater Acoustic Image Transmission System Based on DSP     

程恩  许茹 《海洋通报(英文版)》2002,4(1):27-33

The underwater acoustic image transmission system based on the high-speed DSP device TMS320C549 has been studied.We use Goertzel algorithm for source decoding and MFSK for modulation.Turbo code is used for channel coding and decoding.The purpose is to implement underwater video image data transmission.  相似文献   

Sediment oxygen profiles in a super-oxygenated antarctic lake     

Wharton RA  Meyer MA  McKay CP  Mancinelli RL  Simmons GM 《Limnology and oceanography》1994,39(4):839-853

Perennially ice-covered lakes are found in the McMurdo Dry Valleys of southern Victoria Land, Antarctica. In contrast to temperate lakes that have diurnal photic periods, antarctic (and arctic) lakes have a yearly photic period. An unusual feature of the antarctic lakes is the occurrence of O2 at supersaturated levels in certain portions of the water column. Here we report the first sediment O2 profiles obtained using a microelectrode from a perennially ice-covered antarctic lake. Sediment cores collected in January and October 1987 from Lake Hoare in Taylor Valley show oxygenation down to 15, and in some cases, 25 cm. The oxygenation of sediments several centimeters below the sediment-water interface is atypical for lake sediments and may be characteristic of perennially ice-covered lakes. There is a significant difference between the observed January and October sediment O2 profiles. Several explanations may account for the difference, including seasonality. A time-dependent model is presented which tests the feasibility of a seasonal cycle resulting from the long photoperiod and benthic primary production in sediments overlain by a highly oxygenated water column.  相似文献   

Coupled atmosphere-ocean models of Titan's past     

McKay CP  Pollack JB  Lunine JI  Courtin R 《Icarus》1993,102(1):88-98

We have developed a coupled atmosphere and ocean model of Titan's surface. The atmospheric model is a 1-D spectrally-resolved radiative-convective model. The ocean thermodynamics are based upon solution theory. The ocean, initially composed of CH4, becomes progressively enriched in ethane over time. The partial pressures of N2 and CH4 in the atmosphere are dependent on the ocean temperature and composition. We find that the resulting system is stable against a runaway greenhouse. Accounting for the decreased solar luminosity, we find that Titan's surface temperature was about 20 K colder 4 Gyr ago. Without an ocean, but only small CH4 lakes, the temperature change is 12 K. In both cases we find that the surface of Titan may have been ice covered about 3 Gyr ago. In the lakes case condensation of N2 provides the ice, whereas in the ocean case the ocean freezes. The dominant factor influencing the evolution of Titan's surface temperature is the change in the solar constant--amplified, if an ocean is present, by the temperature dependence of the solubility of N2. Accretional heating can dramatically alter the surface temperature; a surface thermal flux of 500 erg cm-2 sec-1, representative of small levels of accretional heating, results in a approximately 20 K change in surface temperatures.  相似文献   

Numerical simulation of the general circulation of the atmosphere of Titan     

Hourdin F  Talagrand O  Sadourny R  Courtin R  Gautier D  McKay CP 《Icarus》1995,117(2):358-374

The atmospheric circulation of Titan is investigated with a general circulation model. The representation of the large-scale dynamics is based on a grid point model developed and used at Laboratoire de Météorologie Dynamique for climate studies. The code also includes an accurate representation of radiative heating and cooling by molecular gases and haze as well as a parametrization of the vertical turbulent mixing of momentum and potential temperature. Long-term simulations of the atmospheric circulation are presented. Starting from a state of rest, the model spontaneously produces a strong superrotation with prograde equatorial winds (i.e., in the same sense as the assumed rotation of the solid body) increasing from the surface to reach 100 m sec-1 near the 1-mbar pressure level. Those equatorial winds are in very good agreement with some indirect observations, especially those of the 1989 occultation of Star 28-Sgr by Titan. On the other hand, the model simulates latitudinal temperature contrasts in the stratosphere that are significantly weaker than those observed by Voyager 1 which, we suggest, may be partly due to the nonrepresentation of the spatial and temporal variations of the abundances of molecular species and haze. We present diagnostics of the simulated atmospheric circulation underlying the importance of the seasonal cycle and a tentative explanation for the creation and maintenance of the atmospheric superrotation based on a careful angular momentum budget.  相似文献