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61.
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Density, biomass and community structure of macrofauna were estimated together with several sediment characteristics at seven stations ranging from 208 m to 4460 m water depth along the OMEX transect in the Goban Spur area (NE Atlantic) during three seasons (October 1993, May 1994, and August 1995). Median grain size decreased with increasing water depth and showed no differences between the seasons. The percentages of organic carbon and total nitrogen were highest at mid-slope depths (1000 to 1500 m), and were significantly higher in August at the upper part of the slope to a depth of 1500 m. The C:N ratio in the surface layer amounted to 7 to 8 in May, 10 to 12 in August and 14 to 17 in October at all stations (except the deepest at 4460 m, where it was 11 in May and August), indicating arrival of fresh phytodetritus in May, and therefore seasonality in food input to the benthos. Densities of macrofauna decreased exponentially with increasing water depth. Significantly higher densities of macrofauna were found in May at the upper part of the slope to a depth of 1500 m. These differences were mainly due to high numbers of postlarvae of echinoids at the shallowest station and ophiuroids at the deeper stations. Biomass values also decreased with increasing water depth, but biomass was relatively high at the 1000 m station and low at 1500 m, due to relatively high and low mean weights of the individual macrofaunal specimens. No significant differences in biomass were found between the seasons. Respiration was high (15 to 20 mgC·m−2·d−1) in May at the upper part of the slope to a depth of 1000 m and low (1–3 mg C·m−2·d−1) at the deeper part. At the shallowest stations to a depth of 1000 m respiration was highest in May, at the mid-slope stations (1400–2200 m) it was highest in August, whereas the deepest stations (3600 to 4500 m) did not show any differences in respiration rates. In conclusion; seasonal variation in organic input is reflected in denstiy, community structure and activity of the macrofauna along the continental slope in the NE Atlantic. 相似文献
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The Sardinia Channel dataset was collected as part of the European Geotraverse (EGT)—a 4000 km seismic refraction line running from Northern Norway to the Sahara, designed to investigate the structure of the lithosphere beneath Europe. Wideangle seismic data recorded by ocean bottom seismometers deployed in the Sardinia Channel as part of the Southern Segment of the EGT, together with gravity data, were used to constrain the final crustal model. In the centre of the Channel the crust is identified as thinned continental in nature, with a crystalline thickness of 10 km overlain by 4 km of sediments and 2.5 km of water in the most extended region. High velocities in the lower crust in the central region are thought to represent an area of underplating or intrusion by igneous material caused by extension related to the opening of the Tyrrhenian Sea. The crust overlies an anomalously low velocity upper mantle. 相似文献
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本文根据胜利二号极浅海步行坐底钻井平台的作业和工作环境特点,进行了防腐措施研究,设计了切合实际的防腐措施。该平台在海上作业近四年进坞修理,经观测防腐情况良好。 相似文献
68.
东海海底地形分区特征和成因研究 总被引:20,自引:0,他引:20
东海一直以其特殊的大地构造地位受到国内外地学界的关注,但作为主要受构造控制的东海海底地形的研究,以往简单趋势性描述居多,专门深入系统的研究尚不多见。不久前完成的高精度、全覆盖多波束海底地形勘测覆盖了东海部分外陆架、大陆坡全部、冲绳海槽和东部岛坡的一部分,取得了海量的测深数据。据此编绘的勘测多波束水深图和结合测区外的传统资料编绘的海底地形图使我们有机会可以重新审视和系统研究东海的海底地形特征。在定量确定了陆架坡折线、陆坡坡脚线和东部槽坡坡脚线的基础上划分出了大陆架、大陆坡、冲绳海槽平原和东部岛坡4大地形区,继之对各区的海底地形特征进行了研究和描述,并在区内选取了有代表性的5条剖面进行了剖析。另外,从地球内营力和外营力两方面分析了影响东海海底地形发育的因素。调查分析表明:整个东海地形分带明显,地形类型多样:大陆架十分宽阔,总体北宽南窄,从大陆向海平缓倾斜,发育了广泛的NW-SE向沙脊群,自大陆向东南呈扇形发散;大陆坡呈NE-SW向条带展布,海底地形陡峻,呈阶梯状下掉,总体北缓南陡,其上峡谷密布,上穿切外陆架,下直达海槽,同时坡麓上海台沟谷伴生发育;冲绳海槽北浅南深,其内在平坦的背景上发育了众多的海山和海丘,其中心又有槽中槽地形;东槽坡地形复杂,发育了 相似文献
69.
应用ANSYS软件建立了平台和冰相互作用的有限元模型,构建了自升式平台的冰激振动模型,并计算基于2种冰力模型的自升式平台的动力响应。此动力分析方法具有建模方便和计算精度高的特点。以某自升式平台为例,计算了冰和平台结构相互作用的耦合效应,为自升式平台冰激振动安全评估提供了参考依据。 相似文献
70.
Yoshimi Kawai Hiroshi Kawamura Sumio Tanba Kentaro Ando Kunio Yoneyama Norio Nagahama 《Journal of Oceanography》2006,62(6):825-838
In order to investigate the validity of buoy-observed sea surface temperature (SST), we installed special instruments to measure
near-surface ocean temperature on the TRITON buoy moored at 2.07°N, 138.06°E from 2 to 13 March 2004, in addition to a standard
buoy sensor for the regular SST measurement at 1.5-m depth. Large diurnal SST variations were observed during this period,
and the variations of the temperatures at about 0.3-m depth could be approximately simulated by a one-dimensional numerical
model. However, there was a notable discrepancy between the buoy-observed 1.5-m-depth SST (SST1.5m) and the corresponding model-simulated temperature only during the daytime when the diurnal rise was large. The evaluation
of the heat balance in the sea surface layer showed that the diurnal rise of the SST1.5m in these cases could not be accounted for by solar heating alone. We examined the depth of the SST1.5m sensor and the near-surface temperature observed from a ship near the buoy, and came to the conclusion that the solar heating
of the buoy hull and/or a disturbance in the temperature field around the buoy hull would contribute to the excessive diurnal
rise of the SST1.5m observed with the TRITON buoy. However, the temperature around the hull was not sufficiently homogenized, as suggested in
a previous paper. For the diurnal rise of the SST1.5m exceeding 0.5 K, the daytime buoy data became doubtful, through dynamics that remain to be clarified. A simple formula is
proposed to correct the unexpected diurnal amplitude of the buoy SST1.5m. 相似文献