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41.
REEdistributioninwater-sedimentinterfacesystematdeepoceanfloor¥ZhangLijie;LiuJihuaandYaoDe(ReceivedFebruary1,1994;acceptedMay... 相似文献
42.
东太平洋沉积物U的地球化学 总被引:4,自引:0,他引:4
本文对地矿部“海洋四号”科学考察船1987-1989年在东赤道太平洋CC区所取得的27个深海表层沉积样品进行U的地球化学分析,探讨了U在深海沉积中的地球化学行为,结果表明,不同类型沉积的U含量不同,平均值由大至小的次序的含沸石粘土(2.16×10^-6),硅质粘土(1.95×10^-6),硅质软泥(1.65×10^-6),钙质硅质粘土(1.59×10^-6),在同类型沉积中U的分散性较大;U在区域 相似文献
43.
海山铁锰结壳基岩岩石学特征及其生长关系 总被引:2,自引:0,他引:2
为了研究海山铁锰结壳基岩类型与结壳壳层生长的关系。对麦哲伦海山及中太平洋海山区取得的铁锰结壳及其基岩样品在电子显微镜下进行了观察和研究。结果表明,上述2个区域基岩岩石类型主要有玄武岩,火山熔岩,火山碎屑岩,硅质岩和碳酸盐岩,其中麦哲伦海山玄武岩为块状构造,中太平洋海山玄武岩则主要为气孔-杏仁状构造,多发生蚀变或完全蚀变,硅质岩颗粒物质主要是硅藻,碳酸盐岩则以晶质灰岩为主,结壳壳层厚度在各类基岩类型上都有变化,以在玄武岩和碳酸盐岩上变化最大。 相似文献
44.
Paolo Boccotti 《Ocean Engineering》1997,24(3):281-300
The equation obtained in Part I predicts how an exceptionally high wave occurs at any fixed point
within a wind wave field. The equation may be applied with a theoretical spectrum or directly with the random time series obtained by an array of wave gauges in the field. From both approaches, it emerges that a very high wave at a breakwater occurs because a well-defined three-dimensional wave group at the apex of its development hits against the breakwater, and that a very high wave at some distance before the breakwater occurs because of the collision of two wave groups: the first one going back after having been reflected, and the second one approaching the breakwater. In order to test the theory, a special breakwater was assembled off the beach at Reggio-Calabria where the significant height of the wind waves typically ranges from 0.20 to 0.40 m. When an exceptionally high wave (H = 9.6 σ) occurred at a point before this breakwater, the records made by a gauge array confirmed all the essential features of the prediction. 相似文献
45.
The physical and chemical variability of the water column at subtidal station of an estuary in the Seto Inland Sea, Japan,
was studied over a 24-hour period during a spring tide (tidal range ca. 2 m) in May 1995. Surface water and several depths through the water column were monitored every one and two hours, respectively.
At each occasion, water temperature, salinity and dissolved oxygen concentration were measured and water samples were collected
for the determination of nutrients and suspended particulate matter (SPM). Disruptive changes in the physical and chemical
characteristics of the water was produced by the tidal cycle and the mixing of water masses of different origin. These changes
were highly significant both spatially and temporally, yet with varying effects on physical parameters, nutrients and the
different components of SPM. Significant differences in nutrient concentrations were also observed when the data-set was divided
into ebb and flood components, irrespective of the depth. Nitrate and nitrite rose to 1.8 times higher during the flood. Spatial
differences of SPM were less marked than those of nutrients, only particulate organic carbon (POC) being significantly higher
at the surface than in the intermediate and the lower layer. Both POC and pheopigment concentrations increased markedly through
the water column, being highest shortly before the lower low tide. In contrast, suspended solid (SS) content increased sharply
after the lower low tide (>40 mg l−1) and this coincided with a marked decrease of the C/SS content (<20 mg g−1). The lagtime between POC and SS tidal transport was caused by particle resuspension from the exposed intertidal sediments
as the tidal level rose, and particle transport selection in relation to the tidal state.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
46.
A. A. De Almeida 《Earth, Moon, and Planets》1992,56(1):61-74
Emission fluxes of CN, C2 and C3 carbon-bearing molecular species observed in the coma of comets Bennett (1969i 1970II), West (1975n 1976VI), P Halley (1982i), Hartley-Good (19851) and Bradfield (1987s) are analysed in the framework of Haser model. CN, C2 and C3 production rates are determined using recently derived fluorescence efficiencies. The dependence of CN, C2 and C3 production rates on the heliocentric distance and the possible correlations among these radicals is studied and briefly discussed. 相似文献
47.
Apatite fission-track (AFT) thermochronological modeling as a diagnostic tool for periods of stability (peneplanation) and tectonic activity (orogeny) has been broadly used in tectonic studies of Central Asia in recent years. We discuss more than 100 AFT ages of samples from the Kyrgyz Tien Shan and Altai and compare them with AFT data from northern Kazakhstan. Geological, geomorphological, and AFT data indicate intense activity in the Late Cenozoic Eurasian continental interior. The impact from the India-Eurasia collision on the northern Tien Shan, Altai, and northern Kazakhstan regions showed up at 11, 5, and 3 Ma, respectively, as a result of stress propagation into the continent, with the ensuing reactivation and mountain growth. We hypothesize that a distant effect of the Late Cenozoic India-Eurasia collision was to rejuvenate Paleozoic fault zones and to deform the Mesozoic sedimentary cover north of the collision front as far as the West Siberian Plate. The reactivation facilitated formation of tectonic oil and gas traps. The activity in northern Central Asia under the effect of the Indian indentation into Eurasia appears to continue and may evolve to include uplift of southern West Siberian plate with uplift. 相似文献
48.
Groundwater flow systems in turbidites of the Northern Apennines (Italy): natural discharge and high speed railway tunnel drainage 总被引:2,自引:0,他引:2
Alessandro Gargini Valentina Vincenzi Leonardo Piccinini Gian Maria Zuppi Paolo Canuti 《Hydrogeology Journal》2008,16(8):1577-1599
Turbidites crop out extensively in the Northern Apennine mountains (Italy). The huge amounts of groundwater drained by tunnels, built for the high speed railway connection between Bologna and Florence, demonstrate the aquifer-like behaviour of these units, up to now considered as aquitards. A conceptual model of groundwater flow systems (GFS) in fractured aquifers of turbidites is proposed, taking into account both system natural state and the perturbation induced by tunnel drainage. Analysis of hydrological data (springs, streams and tunnel discharge), collected over 10 years, was integrated with analysis of hydrochemical and isotopic data and a stream-tunnel tracer test. Hydrologic recession analysis of undisturbed conditions is a key tool in studying turbiditic aquifer hydrogeology, permitting the discrimination of GFS, the estimation of recharge relative to the upstream reach portion and the identification of springs most vulnerable to tunnel drainage impacts. The groundwater budgeting analysis provides evidence that the natural aquifer discharge was stream-focused through GFS, developed downslope or connected to main extensional tectonic lineaments intersecting stream beds; now tunnels drain mainly active recharge groundwater and so cause a relevant stream baseflow deplenishment (approximately two-thirds of the natural value), possibly resulting in adverse effects on local ecosystems. 相似文献
49.
B. R. De 《Astrophysics and Space Science》1996,239(1):25-33
Maxwell's displacement current equation is interpreted in the light of recent work to show that static magnetic field in free space should have a colocated and contemporaneous mass that is neither embodied in, nor can be anticipated from, the mass-energy relation. Thus magnetostatic field in the universe represents an invisible mass. Some consequences are discussed. 相似文献
50.
Paul A. Crowther Orsola De Marco M. J. Barlow P. J. Storey 《Astrophysics and Space Science》1996,238(1):119-123
We present a detailed, quantitative study of the standard [WC10] Wolf-Rayet central star CPD-56o 8032 based on new high resolution AAT UCLES observations and the Hillier (1990) WR standard model. Our analysis of CPD-56o 8032 gives the wind properties (T
*=34500K, lg (L/L
)=3.8, lg (M/M
a–1)=–5.4,v
=225 km s–1) and chemistry (C/He=0.5, O/He=0.1, by number), the latter suggesting an intimate relationship with the Ovi PN central stars and the PG 1159-035 objects. A comparison between the wind properties of CPD-56o 8032 and Sk-66o 40 (WN 10) indicates that low excitation, low wind velocity WR winds are common to both low mass PN central stars (WC sequence) and high mass post-LBV's (WN sequence). 相似文献