台湾海峡海流结构及海水通量     

傅子琅  胡建宇 《热带海洋学报》1995,(3)

主要根据台湾海峡的实测海流资料，以夏、冬为代表季节，分析了台湾海峡２—３个纬向断面的海流结构，计算出各断面的海水通量。结果表明：夏季，台湾海峡中、北部海域各层的海流一般偏Ｎ向流动，Ｎ向的海水净通量为３．３２×１０６ｍ３·ｓ－１；冬季，高温高盐的黑潮水和南海水由南向北经南部断面进入台湾海峡，其海水通量分别为１．６９×１０６ｍ３·ｓ－１和０．５９×１０６ｍ３·ｓ－１；而东海水由北向南通过北部断面进入台湾海峡，其海水通量为１．０２×１０６ｍ３·ｓ－１，其中，有０．４０×１０６ｍ３·ｓ－１的海水沿着福建和广东近岸流进南海，其余０．６２×１０６ｍ３·ｓ－１的海水在台湾海峡北部混合后随同黑潮水和南海水流入东海。总之，流经台湾海峡的Ｎ向海水净通量为１．７４×１０６ｍ３·ｓ－１。  相似文献   

Miocene extensional detachments in the outcropping basement of the northern Alboran Basin (Betics) and their tectonic implications     

V. García-Dueñas  J. C. Balanyá  J. M. Martínez-Martínez 《Geo-Marine Letters》1992,12(2-3):88-95

Whether or not there are extensional detachment faults in the Alboran basement can be tested directly because a part of the Alboran Basin is now emerged. These detachments, related to crustal thinning beneath the Alboran Basin, occurred from the Aquitanian to Tortonian. The resulting extensional geometries can be described in general terms. During the Serravalian a considerable southwest extension of the basin took place, accompanied by south-southeast extension in the northern Gibraltar Arc. Other detachments affected by Serravalian extension can be found. The spreading of the Alboran was nearly coeval with roughly westward migration of the Gibraltar mountain front.  相似文献   

北黄海长山群岛海域沉积环境初步研究   总被引：3，自引：0，他引：3  

苗丰民  李光天 《海洋地质与第四纪地质》1995,15(1):131-141

本文在获取１９８９－１９９３年黄海北部长山群岛海域沉积物大量数据基础上，借助沉积物粒度分析（Ｑ型），揭示出该海域具有在“岛屿效应”影响下的４种环境能量类型，分析了与其适应的环岛沉积环境及其分布特征。  相似文献   

Influence of Kuroshio water on the distribution of dissolved oxygen in the northern East China Sea     

Fu Yongfa 《海洋学报(英文版)》1992,11(2):305-316

On the basis of the four-cruise investigation data of the Kuroshio by the R/V "Xiangyanghong 09", this paper lays stress on the discussion of the relationship between the Kuroshio current systems, the distribution of dissolved oxygen in the northern East China Sea (ECS) and seasonal variations.  相似文献   

细基江蓠脂肪酸组成研究     

徐世平  盛国英  傅家谟  王永川  潘国瑛 《热带海洋学报》1993,(3)

研究表明,南海细基江蓠Gracilaria tenuistipitata中主要含有C_9—C_(30)一元饱和脂肪酸,其中n-十六酸含量占脂肪酸组分的40％以上。单烯和二烯酸的含量较低,缺乏多烯酸及前列腺素类化合物。此外,还含有少量二元酸类、4-及5-羰基羧酸,其中后两者是首次在红藻中发现。南海细基江蓠的脂肪酸组成特征与南海海域水质较清、光照充足及水温较高等环境因素有关。  相似文献   

Stratigraphic framework of gas accumulations in the Ría de Pontevedra (NW Spain)     

Ruth Durán  Soledad García-Gil  Raquel Diez  Federico Vilas 《Geo-Marine Letters》2007,27(2-4):77-88

Knowledge of marine geological environments in which shallow gas is accumulating is becoming increasingly important in global studies of climate change because a measurable proportion of the total methane source comes from continental margins. Previous studies have revealed that coastal environments represent important geological environments where microbial methane is being generated, is accumulating, and is being released. In the Ría de Pontevedra, at least 4.5 km² of seafloor in the innermost part of the ría is underlain by sediments containing natural gas. Seismic interpretation contributes new findings for the definition of periods and geological environments in which the gas could have been generated, and is accumulating and released in the Ría de Pontevedra. Groundtruthing the seismic data (facies, environments) makes it possible to identify favourable geological environments for gas generation in the sedimentary infill of the Ría de Pontevedra. Sequence stratigraphy based on high-resolution seismic profiles and post-Last Glacial Maximum sea-level records makes it possible to establish the stratigraphic architecture of the ría and to define the periods in which gas could have been generated. The results of this study show that the sedimentary infill is composed of a fifth-order sequence developed since the Last Glacial Maximum. Within this sequence, gas appears to have accumulated in the Holocene deposits associated with the latest transgressive and highstand system tracts. Seismic analysis shows that gas could have been generated in different geological environments in the Ría de Pontevedra. If coastal environments at times of lower sea level were similar to those of the present, organic-rich mud deposits (deposited mainly in lakes, estuaries and floodplains) could have survived transgression and remained buried as potential gas sources in the inner part of the ría.  相似文献   

中国大洋生物基因研究开发基地成立     

岳夫 《海洋信息》2002,(4):32-32,27

2002年6月28日,“中国大洋生物基因研究开发基地”在厦门国家海洋局第三海洋研究所(下称海洋三所)成立,并正式挂牌。“基地”在中国大洋矿产资源研究开发协会(下称中国大洋协会)和海洋三所的相关研究方向基础上建立,目的是把中国大洋生物基因研究开发方面的工作推向深入和提高到一个新水平。国家海洋  相似文献   

Hydrogen and Helium under high pressure: A case for a classical theory of dense matter     

Vladan čelebonović 《Earth, Moon, and Planets》1989,45(3):291-298

When subject to high pressure, H₂ and ³He are expected to undergo phase transitions, and to become metallic at a sufficiently high pressure. Using a semiclassical theory of dense matter proposed by Savi and Kaanin, calculations of phase transition and metallisation pressure have been performed for these two materials. In hydrogen, metallisation occurs at p _M= (3.0 ± 0.2) Mbar, while for helium the corresponding value is p _M= (106 ± 1) Mbar. A phase transition occurs in helium at p _tr= (10.0 ± 0.4) Mbar. These values are close to the results obtainable by more rigorous methods. Possibilities of experimental verification of the calculations are briefly discussed.  相似文献   

Fluctuations of CaFz(Eu) scintillator background     

Z. Dvořák  K. Štukheil 《Solar physics》1989,123(1):189-192

Background signal of the scintillation detector routinely used for atmospheric Kr-85 counting follows fluctuations, and their connection with cosmic ray variations is searched for. A strong correlation between the 27-day moving average of sunspot numbers and the background is obtained from the 1988 data.  相似文献   

Further notes on the associated alpha-functions and related integrals in the theory of the light changes of eclipsing variables     

H. M. Srivastava  Zdeněk Kopal 《Astrophysics and Space Science》1989,162(2):181-204

With a view to furthering the theory of the light changes of eclipsing variables, developed before systematically by Z. Kopal, this paper presents a number of new (and computable) expressions for the associated alpha-function _n ⁰ ,(r₁,r₂,) (and also for its partial derivatives), where _n ⁰ ,(r₁,r₂,) represents the fractional loss of light suffered by an eclipse of a circular disc of fractional radiusr ₁ (and darkened at the limb to thenth degree) by an opaque disc of radiusr ₂, with their centres separated by a fractional (projected) distance , provided that the transparency of the occulting disc increases with the angle of foreshortening in the same manner as the limb-darkening of the eclipsed star (that is, when the transparency functiong(, ) of the second aperture is given by Equation (4) below). Many of the explicit expressions derived here are valid for any type of eclipse, occultation or transit, regardless of whetherr ₁>r ₂ orr ₁<r ₂. and for any degreen of the adopted law of limb-darkening. It is also pointed out how some of the results obtained in this paper are related to the various representations given earlier in the literature for the case =0.  相似文献