Mass-transport deposits on the Rosetta province (NW Nile deep-sea turbidite system, Egyptian margin): Characteristics, distribution, and potential causal processes   总被引：2，自引：0，他引：2  

Sbastien Garziglia  Sbastien Migeon  Emmanuelle Ducassou  Lies Loncke  Jean Mascle 《Marine Geology》2008,250(3-4):180-198

In the Nile deep-sea turbidite system (NDSTS), the province fed by the Rosetta branch of the Nile delta is characterised by the recurrent activity of gravity processes. Seven mass-transport deposits (MTDs) were recognised from the upper to the mid slope, downstream from imbricated scars (~ 30 km-long, ~ 200 m high) running along the shelf edge nearby the Rosetta canyon. Extending on surfaces between 200 and 5000 km², with estimated volumes from 3 to 500 km³, these MTDs represent about 40% (up to 90% locally) of the total Pleistocene–Holocene sedimentary thickness. Three types of MTDs can be distinguished on the basis of their scale. Each has also a distinctive internal configuration and distribution within the Rosetta depositional setting. Age estimates of two MTDs point towards relationships between climate and submarine mass failures through sea-level changes, sediment supply, or a combination of both. Additionally, the presence of gas in the sediment and earthquake shaking may have concurred to trigger large-scale failures on the low slope angles (1°–2°) of the Rosetta area.  相似文献   

往复潮流作用下推移质粒径趋势形成模拟初探   总被引：2，自引：0，他引：2  

于谦  高抒 《海洋与湖沼》2008,39(4)

粒径趋势分析是一种用于判断海洋环境中沉积物净输运方向的方法,但是至今粒径趋势形成的物理机制尚不够清楚,因而影响了粒径趋势分析适用条件的确定。针对这个问题,本文通过建立一维、推移质、往复流（近岸潮流）条件下的数值模型,采用正演方法模拟粒度参数在输运方向上的分布．以评价沉积动力过程的影响,初步探讨粒径趋势形成的物理机制。数值模型实验的初步结果显示,水动力条件的空间差异导致的沉积物粒度参数的空间分布符合粒径趋势分析的假设,粒径趋势分析中定义的两种粒径趋势可由沉积物输运强度的空间梯度而形成,并且在沉积物净输运方向上出现的频率最高。  相似文献   

俄罗斯阿尔丹地块西部穆龙斯克杂岩体中的碱性交代岩     

Ｖ．Ｍ．Ｂｉｒｙｕｋｏｖ 《国土资源》1999,(2)

含紫硅碱钙石、镁钠钙闪石（钠透闪石－石棉）及蓝色软透闪石的碱性交代岩的形成首先是由硅酸和碱（Ｎａ２Ｏ和Ｋ２Ｏ的不同作用）的隋性及ＦｅＯ,ＭｇＯ,ＣａＯ和Ａｌ２Ｏ３的强烈活性决定的。含蓝色软透闪石和镁钠钙闪石（钠透闪石－石棉）的交代岩是岩浆期后溶解演化的中期产物,而含紫硅碱钙石的交代岩却是其晚期的产物。  相似文献   

金属稳定同位素示踪关键金属的运移和超常富集     

胡霞  邓庚辛  陈栩琦  盛佳儒  黄方 《地质学报》2024,98(5):1550-1572

关键金属矿产对于国家经济和安全意义重大,然而其富集机制仍然存在争议,即受控于岩浆的结晶分异作用还是热液流体作用。传统的地球化学手段只能间接制约成矿物质的来源,难以区分分离结晶和岩浆热液作用对成矿的影响,而Rb、Ba、Sr、U等流体活动金属的同位素体系则对这两种机制具有不同的响应。笔者分别对喜马拉雅和华南地区的富关键金属花岗岩进行了Rb和Ba同位素研究,结果表明,当矿物结晶时,残留熔体中Ba同位素变重,Rb同位素不变;而当岩浆热液作用时,花岗岩中Ba同位素变轻,Rb同位素变重。此外,深部岩浆出溶的热液流体对亲流体易迁移的关键金属元素的富集具有重要贡献。上述研究表明,金属稳定同位素(尤其是流体活动金属的同位素)对于示踪岩浆- 热液作用和成矿流体来源具有非常好的效果。  相似文献   

微纳米金颗粒对卡林型金矿成矿的指示     

冯宏业  琚宜文  方维萱  朱洪建  余坤  陈博  乔鹏  肖蕾  陶丽茹 《地质论评》2024,70(S1):65-66

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帕米尔弧形构造带东北缘晚新生代构造活动的沉积与重矿物变化响应     

王子一  李康  李勇  安凯旋  陈才  林秀斌  程晓敢  陈汉林 《岩石学报》2021,37(5):1419-1430

帕米尔弧形构造带东北缘晚新生代沉积特征的研究对于理解帕米尔构造带弧形扩展机制具有重要意义.本文通过对帕米尔弧形构造带东北缘的晚新生代沉积地层的沉积特征对比研究和重矿物采样与组份分析,建立了帕米尔弧形构造带东北缘地区的晚新生代沉积联合柱状对比图和重矿物组份变化曲线.研究结果表明,晚新生代沉积与重矿物变化主要记录了帕米尔弧...  相似文献   

Time–space fractional governing equations of one‐dimensional unsteady open channel flow process: Numerical solution and exploration          下载免费PDF全文

Ali Ercan  M. Levent Kavvas 《水文研究》2017,31(16):2961-2971

Although fractional integration and differentiation have found many applications in various fields of science, such as physics, finance, bioengineering, continuum mechanics, and hydrology, their engineering applications, especially in the field of fluid flow processes, are rather limited. In this study, a finite difference numerical approach is proposed to solve the time–space fractional governing equations of 1‐dimensional unsteady/non‐uniform open channel flow process. By numerical simulations, results of the proposed fractional governing equations of the open channel flow process were compared with those of the standard Saint‐Venant equations. Numerical simulations showed that flow discharge and water depth can exhibit heavier tails in downstream locations as space and time fractional derivative powers decrease from 1. The fractional governing equations under consideration are generalizations of the well‐known Saint‐Venant equations, which are written in the integer differentiation framework. The new governing equations in the fractional‐order differentiation framework have the capability of modelling nonlocal flow processes both in time and in space by taking the global correlations into consideration. Furthermore, the generalized flow process may possibly shed light on understanding the theory of the anomalous transport processes and observed heavy‐tailed distributions of particle displacements in transport processes.  相似文献   

A search for electron cyclotron maser emission from compact binaries     

Gavin Ramsay  Catherine Brocksopp  Kinwah Wu  Bruce Slee  Curtis J. Saxton 《Monthly notices of the Royal Astronomical Society》2007,382(1):461-465

Unipolar induction (UI) is a fundamental physical process, which occurs when a conducting body transverses a magnetic field. It has been suggested that UI is operating in RX J0806+15 and RX J1914+24, which are believed to be ultracompact binaries with orbital periods of 5.4 and 9.6 min, respectively. The UI model predicts that those two sources may be electron cyclotron maser sources at radio wavelengths. Other systems in which UI has been predicted to occur are short period extrasolar terrestrial planets with conducting cores. If UI is present, circularly polarized radio emission is predicted to be emitted. We have searched for this predicted radio emission from short period binaries using the Very Large Array (VLA) and Australian Telescope Compact Array (ATCA). In one epoch, we find evidence for a radio source, coincident in position with the optical position of RX J0806+15. Although we cannot completely exclude that this is a chance alignment between the position of RX J0806+15 and an artefact in the data reduction process, the fact that it was detected at a significance level of 5.8σ and found to be transient suggests that it is more likely that RX J0806+15 is a transient radio source. We find an upper limit on the degree of circular polarization to be ∼50 per cent. The inferred brightness temperature exceeds 10¹⁸ K, which is too high for any known incoherent process, but is consistent with maser emission and UI being the driving mechanism. We did not detect radio emission from ES Cet, RX J1914+24 or Gliese 876.  相似文献   

Modification of dust-grain structure by sputtering     

M. D. Gray  M. G. Edmunds 《Monthly notices of the Royal Astronomical Society》2004,349(2):491-502

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Thermal desorption of water ice in the interstellar medium     

Helen J. Fraser †  Mark P. Collings  Martin R. S. McCoustra  David A. Williams 《Monthly notices of the Royal Astronomical Society》2001,327(4):1165-1172

Water (H₂O) ice is an important solid constituent of many astrophysical environments. To comprehend the role of such ices in the chemistry and evolution of dense molecular clouds and comets, it is necessary to understand the freeze-out, potential surface reactivity and desorption mechanisms of such molecular systems. Consequently, there is a real need from within the astronomical modelling community for accurate empirical molecular data pertaining to these processes. Here we give the first results of a laboratory programme to provide such data. Measurements of the thermal desorption of H₂O ice, under interstellar conditions, are presented. For ice deposited under conditions that realistically mimic those in a dense molecular cloud, the thermal desorption of thin films (≪50 molecular layers) is found to occur with zeroth-order kinetics characterized by a surface binding energy, E _des, of 5773 ± 60 K, and a pre-exponential factor, A , of 10^30 ± 2 molecules cm⁻² s⁻¹. These results imply that, in the dense interstellar medium, thermal desorption of H₂O ice will occur at significantly higher temperatures than has previously been assumed.  相似文献