海洋生产总值核算方法研究   总被引：3，自引：0，他引：3  

何广顺  王晓惠  周洪军  郭越  徐丛春 《海洋通报》2006,25(3):64-71

在分析借鉴国内外海洋经济核算相关方法的基础上,研究探索了我国海洋经济核算的模式,以海洋生产总值核算为突破口,系统提出了我国海洋生产总值(GOP)核算的三种基本方法,即剥离法、扩展法、外推法。同时,对几种核算方法进行了综合分析和评估。为我国开展海洋经济核算工作打下了良好的基础。  相似文献   

山东荣成湾月湖口门落潮干道的推移质输运   总被引：6，自引：2，他引：6  

薛允传  高抒  贾建军 《海洋与湖沼》2002,33(4):356-363

改进了Gao等 ( 1 994)方法 ,并用以计算潮汐汊道口门落潮干道的垂线平均流速。利用月湖潮汐汊道系统冬、夏季各一个月的潮位资料 ,计算落潮干道的潮流流速和推移质输运率。结果表明 ,流速的计算值和实测值呈良好的相关性 ,落潮干道内落潮流的输沙能力高于涨潮流输沙能力  相似文献   

潮流沙脊的水力学问题探讨     

刘振夏  夏东兴 《海洋科学进展》1995,(4)

借用河流水力学顺直河道中有两个次生横向环流的假说来解释潮流沙脊的成因，水槽实验和实际观察也支持了这一观点．正是这一次生的纵轴横向环流（即螺旋流）将泥沙从沟槽带向脊顶，建造了大致与潮流方向平行的潮流沙脊．根据底质粒度成份和分布特点．可分为粗底质沙脊和细底质沙脊两类．前者组成物质偏粗，底质分布为脊细槽粗，后者组成物质偏细，底质分布为脊粗槽细．这是因为影响颗粒起动流速的主导因素不同，前者以重力为主，后者以颗粒间粘结力为主．它们都反映沟槽中流速大于脊顶处流速．  相似文献   

南极国际GPS跟踪站的海潮位移改正 (英文)     

Youwen Liu  Weiping Jiang  Xiaohui Zhou 《地球空间信息科学学报》2008,11(2):148-151

This paper describes the ocean loading tides corrections of GPS stations in Antarctica, such as the Great Wall station and Zhongshan station. Based on the theory of ocean loading tides, the displacement corrections of ocean loading tides on GPS stations in Antarctica are calculated by using the CRS4.0 ocean loading tides model. These corrections are also applied to GPS data processing. The GPS data are analyzed by the GAMIT software with and without these corrections. We compared and analyzed the GPS baseline components to get the differences. The results show that the ocean tidal displacement corrections have obvious effects upon GPS baseline components. Therefore, we should not ignore the ocean loading tides corrections of GPS stations in Antarctica to obtain precise and reliable results.  相似文献   

末次盛冰期以来印度尼西亚穿越流对东印度洋上部水体结构的影响          下载免费PDF全文

叶黎明  翦知湣  金海燕  成鑫荣 《第四纪研究》2008,28(3):458-464

海洋上部水体垂向结构变化对于理解热带海区在全球气候变化中的作用有着重要意义。通过分析印度尼西亚穿越流(ITF)出口处东印度洋帝汶海区SO18480-3孔中的浮游有孔虫表层种Globigerinoides ruber和温跃层种Pulleniatina obliquiloculata壳体氧碳同位素,并借助12个AMS¹⁴C测年数据重建了末次盛冰期(LGM)以来该区温跃层深度和营养盐水平的演化序列。壳体氧同位素(δ¹⁸O)记录表明温跃层古海洋学特征的变化幅度要大于表层海水,其差值(Δδ¹⁸O_(P-G))有效地反映了温跃层深度的变化,即冰消期和晚全新世温跃层较浅,LGM和早中全新世温跃层较深;并揭示出与全新世相比,LGM期间ITF总流量未显著减小,ITF对该区上部水体结构的影响受到了东西太平洋之间不对称性的调节。碳同位素(δ¹³C)记录则表明该区的古海洋学变化在不同程度上受到了南大洋的影响,并受本区上部水体垂向结构的控制,其差值(Δδ¹³_(G-P))在一定程度上反映了该区上部水体营养盐水平的变化。  相似文献   

渤海GNSS-R机载测风试验及其反演结果     

周兆明  符养 《武汉大学学报(信息科学版)》2008,33(3):241-244

对渤海GNSS-R机载试验进行了海面风场反演.结果表明,风速精度优于1 m/s,风向精度优于20°.  相似文献   

“全新特提斯洋”概念与广义特提斯构造域     

余星  许绪成  韩喜球  丁巍伟  胡航  何虎  余娅娜 《地质学报》2022,96(12):4131-4139

特提斯最初是指欧亚大陆南缘的古海洋，后逐渐引申出从元古宙、古生代到中生代的一系列位于劳亚大陆与冈瓦纳大陆之间的古大洋，如原特提斯洋、古特提斯洋和新特提斯洋，不同大洋在时间上前后交叠。如今横亘在冈瓦纳大陆(南极洲)和欧亚大陆之间的是印度洋，是新特提斯洋的继承者，可以另称为“全新特提斯洋”。这一概念的引申直接体现了印度洋与特提斯构造域一脉相承的关系，有助于将今论古、由此及彼，更直观地了解特提斯构造域的演化过程。本文按时间序列梳理了印度洋的大地构造演化和岩浆作用过程，识别了印度洋在155 Ma、120 Ma、90~84 Ma、76 Ma、65 Ma、52 Ma、45 Ma、38 Ma等关键时期的异常海底扩张记录，这些扩张事件将为标定新特提斯构造域的演化提供参照。其中155 Ma可能指示了新特提斯洋的鼎盛期，90 Ma指示了新特提斯洋的洋中脊俯冲，76~52 Ma是非洲- 阿拉伯大陆与欧亚大陆初始碰撞- 主碰撞(即新特提斯洋西部关闭)的时期，65~45 Ma是印度次大陆与欧亚大陆初始碰撞- 主碰撞(即新特提斯洋中部关闭)的时期，38 Ma是澳大利亚北部大洋开始净俯冲(即新提斯洋东部开始消减)的时间。印度洋扩张历史的研究为理解新特提斯洋消亡提供参考标尺。站在“后方”印度洋的角度，可以更清晰地透视“前线”特提斯构造域的演化过程，为理解板块构造活动规律提供支撑。  相似文献   

Sector collapse,sedimentation and clast population evolution at an active island-arc volcano: Stromboli,Italy   总被引：1，自引：0，他引：1  

P. Kokelaar  C. Romagnoli 《Bulletin of Volcanology》1995,57(4):240-262

Sciara del Fuoco is the subaerial part of a partially filled sector-collapse scar that extends to 700 m below sea level on Stromboli volcano. The collapse occurred <5000 years ago, involved 1.81 km³ of rock and is the latest of a series of major collapses on the north-west flank of Stromboli. A north-east trending arc-axial fault system channels magmas into the volcano and has caused tilting and/or downthrow to the north-west. The slope of the partial cone constructed between the lateral walls of the collapse scar acts as a channelway to the sea for most eruptive products. From 700 m below sea level and extending to >2200 m and >10 km from the shore to the NNW, a fan-shaped mounded feature comprises debris avalanche deposits (>4 km³) from two or more sector collapses. Volcaniclastic density currents originating from Sciara del Fuoco follow the topographic margin of the debris avalanche deposits, although overbank currents and other unconfined currents widely cover the mounded feature with turbidites. Historical (recorded) eruptive activity in Sciara del Fuoco is considerably less than that which occurred earlier, and much of the partial fill may have formed from eruptions soon after the sector collapse. It is possible that a mass of eruptive products similar to that in the collapse scar is dispersed as volcanogenic sediment in deep water of the Tyrhennian basin. Evidence that the early post-collapse eruptive discharge was greater than the apparent recent flux (2kg/s) counters suggestions that a substantial part of Stromboli's growth has been endogenous. The partial fill of Sciaria del Fuoco is dominated by lava and spatter layers, rather than by the scoria and ash layers classically regarded as main constituents of Strombolian (cinder) cones. Much of the volcanic slope beneath the vents is steeper than the angle of repose of loose tephra, which is therefore rapidly transported to the sea. Delicate pyroclasts that record the magmatic explosivity are selectively destroyed and diluted during sedimentary transport, mainly in avalanches and by shoreline wave reworking, and thus the submarine deposits do not record well the extent and diversity of explosive activity and associated clast-forming processes. Considerable amounts of dense (non-vesicular) fine sand and silt grains are produced by breakage and rounding of fragments of lava and agglutinate. The submarine extension of the collapse scar, and the continuing topographic depression to >2200 m below sea level, are zones of considerable by-passing of fine sand and silt, which are transported in turbidity currents. Evidently, volcanogenic sediments dispersed around island volcanoes by density currents are unlikely to record well the true spectrum and relative importance of clast-forming processes that occurred during an eruption. Marine sedimentary evidence of magmatic explosivity is particularly susceptible to partial or complete obliteration, unless there is a high rate of discharge of pyroclastic material into the sea.  相似文献   

A new tectonic scenario for the Sanandaj–Sirjan Zone (Iran)   总被引：3，自引：0，他引：3  

A. Ghasemi  C.J. Talbot 《Journal of Asian Earth Sciences》2006,26(6):683-693

Recent geochemical studies of volcanic rocks forming part of the ophiolites within the Zagros and Naien-Baft orogen indicate that most of them were developed as supra-subduction ophiolites in intra-oceanic island arc environments. Intra-oceanic island arcs and ophiolites now forming the Naien-Baft zone were emplaced southwestward onto the northeastern margin of the South Sanandaj–Sirjan Zone, while those now in the High Zagros were emplaced southwestward onto the northern margin of Arabia. Thereafter, subduction continued on opposite sides of the remnant oceans. The floor of Neo-Tethys Ocean was subducted at a low angle beneath the entire Sanandaj–Sirjan Zone, and the floor of the Naien-Baft Ocean was subducted beneath the Central Iranian Micro-continent. The Naien-Baft Ocean extended into North-West Iran only temporarily. This failed ocean arm (between the Urumieh-Dokhtar Magmatic Assemblage and the main Zagros Thrust) was filled by thick Upper Triassic–Upper Jurassic sediments. The Naien-Baft Ocean finally closed in the Paleocene and Neo-Tethys closed in the Early to Middle Eocene. After Arabia was sutured to Iran, the Urumieh-Dokhtar Magmatic Assemblage recorded slab break-off in the Middle Eocene.  相似文献   

中国近海初级生产力的遥感研究及其时空演化     

檀赛春  石广玉 《地理学报(英文版)》2006,16(4):447-457

1 Introduction Ocean primary productivity controls the exchange of carbon dioxide at the air-sea interface and plays an important role in the global carbon cycle and climate change. Most oceanographic research on primary productivity has focused on the ma…  相似文献