不同顶管组合方式的管幕冻结温度场模型试验   总被引：1，自引：1，他引：0  

段寅  荣传新  程桦  蔡海兵  解德柱  丁杨龙 《冰川冻土》2020,42(2):479-490

拱北隧道作为港珠澳大桥珠海连接线的关键性工程， 在国内外首次成功运用了管幕冻结技术。以此为背景， 为更加全面地掌握饱和软土地层中管幕冻结温度场的分布特点， 开展了不同顶管组合方式下的管幕冻结温度场模型试验研究。试验结果表明： 各测点温度曲线在积极冻结期前4 h急剧下降， 随后逐渐减缓， 降至砂土冰点后趋于平稳， 三种布管方式均满足冻结设计要求； 冻结管中低温盐水提供的冷量首先传递给顶管管壁， 再以“面”的形式均匀地传递给周围土体； 积极冻结21 h后， 采用四根空顶管组合的C区冻结壁竖向范围最大， 空管管壁正上方冻结壁平均厚度约为105 mm， 在满足管幕刚度设计要求的前提下， 可采此布管方式以达到快速形成冻结帷幕的目的。限位管开启后的4 h内， 实顶管中线垂直距离100 mm范围内测点温度曲线虽有明显回升但仍维持在冻土冰点以下， 超出此范围后温度变化影响逐渐减弱， 且顶管间冻结壁稳定存在， 表明限位管在满足管间有效封水的条件下， 能在一定范围内起到定向限制地层冻胀的作用。优化后的双圆形冻结管在满足冻结设计要求的同时， 更加便于安装且经济环保。  相似文献   

探秘“能源新星”——干热岩          下载免费PDF全文

王文  吴纪修  施山山  李小洋 《探矿工程》2020,47(3):88-93

干热岩是近些年逐渐发展起来的清洁能源，指埋藏于地球表面3000 m以深，不含或含少量水或蒸汽等流体，温度在180 ℃以上且渗透率极低的岩体。对干热岩的应用主要是建立增强型地热系统进行发电。目前对干热岩的研究尚处于起步阶段,干热岩的热源、热储、形成机理、埋藏机制等都未形成完整的理论体系，干热岩的开发过程也面临诸如储层改造、高温钻探以及随钻监测等一系列的技术“瓶颈”。干热岩资源储量大，开发利用过程低碳环保、节能高效，是国际社会公认的优质清洁能源，但是干热岩研究程度低，开发难度大，需要不断的知识积累和技术积累。本文从科普的角度列举了干热岩的相关研究现状及存在的问题，以期能让更多的人对这一“能源新星”加深了解。  相似文献   

基于自然区块的城市热环境空间分异性研究     

杨智威  陈颖彪  吴志峰  千庆兰  黄清瑶 《地理科学进展》2019,38(12):1944-1956

通过有效解决建设用地子类划分,实现定量评价城市热环境的空间分异性,对改善城市生态环境、实现城市化的健康发展具有重要的意义和科学价值。论文以广州市为例,参考自然城市的概念,基于5类兴趣点(Point Of Interest,POI)开放数据,结合城市建设用地分类标准,构建5类自然区块;在Landsat 8遥感影像地表温度反演的基础上,计算分析自然区块下地表热场等级分布格局、热场平均值及热环境足迹范围,以对城市热环境空间分异性进行评价。研究表明：① 自然区块的构建,能准确地反映各类POI数据空间分布情况,能够实现对建设用地子类型的划分;② 5类自然区块内部地表热场等级均以高温像元为主,但等级分布具有显著差异。同时,自然区块的热场平均值由高到低的排序为：工业区块>商业服务业区块>交通与道路区块>居住区块>公共管理与服务区块;③ 自然区块形成的高温集聚区,存在热量扩散现象,实际影响范围大于其物理边界,5类自然区块的热环境足迹范围具有分异性。热环境足迹影响范围由大到小排序为：工业区块>商业服务业区块>居住区块>道路与交通区块>公共管理与服务区块。研究结果可为微观尺度上分析城市热环境、改善城市生态环境、实现城市化的健康发展提供科学依据。  相似文献   

Volatile element chemistry during accretion of the earth     

《Chemie der Erde / Geochemistry》2020,80(1):125594

We review some issues relevant to volatile element chemistry during accretion of the Earth with an emphasis on historical development of ideas during the past century and on issues we think are important. These ideas and issues include the following: (1) whether or not the Earth accreted hot and the geochemical evidence for high temperatures during its formation, (2) some chemical consequences of the Earth’s formation before dissipation of solar nebular gas, (3) the building blocks of the Earth, (4) the composition of the Earth and its lithophile volatility trend, (5) chemistry of silicate vapor and steam atmospheres during Earth’s formation, (6) vapor - melt partitioning and possible loss of volatile elements, (7) insights from hot rocky extrasolar planets. We include tabulated chemical kinetic data for high-temperature elementary reactions in silicate vapor and steam atmospheres. We finish with a summary of the known and unknown issues along with suggestions for future work.  相似文献   

An efficient and robust approach to predict ship self-propulsion coefficients     

《Applied Ocean Research》2019

Achieving a reliable and accurate numerical prediction of the self-propulsion performance of a ship is still an open problem that poses some relevant issues. Several CFD methods, ranging from boundary element methods (BEM) to higher-fidelity viscous Reynolds averaged Navier–Stokes (RANS) based solvers, can be used to accurately analyze the separate problems, i.e. the open water propeller and the hull calm water resistance. However, when the fully-coupled self-propulsion problem is considered, i.e. the hull advancing at uniform speed propelled by its own propulsion system, several complexities rise up. Typical flow simplifications adopted to speed-up the simulations of the single analysis (hull and propeller separately) lose their validity requiring a more complex solver to tackle the fully-coupled problem. The complexity rises up further when considering a maneuver condition. This aspect increases the computational burden and, consequently, the required time which becomes prohibitive in a preliminary ship design stage.The majority of the simplified methods proposed in literature to include propeller effects, without directly solve the propeller flow, in a high-fidelity viscous solver are not able to provide all the commonly required self-propulsion coefficients. In this work, a new method to enrich the results from a body force based approach is proposed and investigated, with the aim to reduce as much as possible the computational burden without losing any useful result. This procedure is tested for validation on the KCS hull form in self-propulsion and maneuver conditions.  相似文献   

鄂尔多斯地块—扬子地块深部电性结构特征及其动力学意义     

吕宏斌  叶高峰  金胜  魏文博  董浩  张乐天  谢成良  尹曜田 《地质论评》2020,66(4):813-828

位于青藏高原东北缘的秦岭造山带在大地构造上南接扬子地块、北接华北地块,是特提斯构造域和古亚洲洋构造域的转换带。本文基于对一条起始于扬子地块,穿过秦岭造山带和鄂尔多斯地块,到达河套地堑的南北向大地电磁测深剖面的研究,探讨秦岭造山带和其北侧的鄂尔多斯地块、南侧的扬子地块之间的接触关系,以及青藏高原物质东北向逃逸等地学问题。对实测数据进行了张量阻抗分解和维性分析等工作,并对剖面进行了二维反演,获得岩石圈电性结构模型。根据电阻率模型认为:在秦岭造山带北部发现大规模"瓶颈状"分布的低阻异常体(C2),可能为华北、华南地块双向俯冲前缘地幔物质的上涌通道,或者是青藏高原中、下地壳物质沿秦岭造山带中构造薄弱位置向东逃逸的通道;在秦岭造山带和大巴山弧形带边界处发现南倾的低阻异常(C1),解释为大巴山弧形带北缘的逆冲断裂在电性上的反映;电性结构模型中,扬子地块高阻异常体(R2、R3和R4)向北倾斜至秦岭造山带下方,而北部鄂尔多斯地块的高阻异常体(R5和R6)向南倾斜至秦岭造山带下方;高阻异常通常被认为是稳定岩石圈的反映,据此推断这两组相向俯冲至秦岭造山带下方的高阻异常是华北地块和扬子地块向秦岭造山带下方汇聚的电性结构探测依据;鄂尔多斯地块南、北电性差异较大,北部中、下地壳大规模分布电阻率值在3～100Ω·m之间的低阻异常体,可能为地幔上涌导致的局部熔融或含盐流体共同作用的结果。  相似文献   

扎格罗斯前陆盆地晚中新世快速剥露证据——来自磷灰石(U- Th)/He的约束     

李佳纬  孙继敏  吕丽星  张志亮  田晟辰  曹萌萌  李有生  苏柏 《地质学报》2020,94(12):3674-3688

伊朗扎格罗斯造山带是世界上最年轻的造山带之一，前人对其构造演化历史的研究尚存争议。前陆盆地蕴藏着丰富的造山带热史信息，为研究造山带的隆升和剥露历史提供了重要途径。本研究选取位于扎格罗斯前陆盆地前缘中部的Kuh- E Bedush向斜和Kuh- E Murdeh向斜翼部出露的第三纪陆相红层(Agha Jari组)为研究对象，共采集11个粗砂岩样品进行磷灰石(U- Th)/He测试分析。11个样品共得到38个单颗粒年龄，年龄区间为0. 8~79. 9Ma。大部分样品的单颗粒年龄比较分散，表明这些样品没有发生完全热重置。相反，位于Murdeh向斜剖面最底部的样品，(U- Th)/He年龄小于其对应的地层年龄，并且集中分布在8. 3~6. 8Ma，表明该样品发生了完全重置并记录了最后一次剥露事件的时间。因此，我们认为扎格罗斯前陆盆地于晚中新世~7. 5 Ma经历了一期快速剥露事件。此外，我们发现未重置的(U- Th)/He年龄大致分布在四个时间段：晚白垩纪—早古新世、早—中始新世、渐新世、早—中中新世。根据所得热年龄并结合前人研究设定了三种不同的热史，正演模拟结果与实际样品拟合较好，由此推断出前陆中部Agha Jari陆相红层沉积物可能来自于：①晚白垩世以来以蛇绿岩套为主的仰冲体持续剥露；②萨南达季- 锡尔詹变质带(SSZ)渐新世和中新世逐渐加速的剥露；③渐新世末堆积在仰冲体之上的同造山期砾岩，在中新世的大规模逆冲作用下重新剥露。  相似文献   

Strain analysis of a seismically imaged mass‐transport complex,offshore Uruguay     

Michael J. Steventon  Christopher A.‐L. Jackson  David M. Hodgson  Howard D. Johnson 《Basin Research》2019,31(3):600-620

Strain style, magnitude and distribution within mass‐transport complexes (MTCs) are important for understanding the process evolution of submarine mass flows and for estimating their runout distances. Structural restoration and quantification of strain in gravitationally driven passive margins have been shown to approximately balance between updip extensional and downdip contractional domains; such an exercise has not yet been attempted for MTCs. We here interpret and structurally restore a shallowly buried (c. 1,500 mbsf) and well‐imaged MTC, offshore Uruguay using a high‐resolution (12.5 m vertical and 15 × 12.5 m horizontal resolution) three‐dimensional seismic‐reflection survey. This allows us to characterise and quantify vertical and lateral strain distribution within the deposit. Detailed seismic mapping and attribute analysis shows that the MTC is characterised by a complicated array of kinematic indicators, which vary spatially in style and concentration. Seismic‐attribute extractions reveal several previously undocumented fabrics preserved in the MTC, including internal shearing in the form of sub‐orthogonal shear zones, and fold‐thrust systems within the basal shear zone beneath rafted‐blocks. These features suggest multiple transport directions and phases of flow during emplacement. The MTC is characterised by a broadly tripartite strain distribution, with extensional (e.g. normal faults), translational and contractional (e.g. folds and thrusts) domains, along with a radial frontally emergent zone. We also show how strain is preferentially concentrated around intra‐MTC rafted‐blocks due to their kinematic interactions with the underlying basal shear zone. Overall, and even when volume loss within the frontally emergent zone is included, a strain difference between extension (1.6–1.9 km) and contraction (6.7–7.3 km) is calculated. We attribute this to a combination of distributed, sub‐seismic, ‘cryptic’ strain, likely related to de‐watering, grain‐scale deformation and related changes in bulk sediment volume. This work has implications for assessing MTCs strain distribution and provides a practical approach for evaluating structural interpretations within such deposits.  相似文献   

一维综合孔径微波辐射计遥感海面温度的敏感性分析     

陈冠宇  艾未华  陆文  冯梦延 《海洋学报》2019,41(3):143-154

一维综合孔径微波辐射计能够有效提高观测的空间分辨率，其观测入射角通常在0°~55°范围内变化。为了开发适用于一维综合孔径微波辐射计的海面温度反演算法，需要评估其观测亮温对海洋大气环境要素的敏感性。利用海面发射率模型和大气辐射传输模型，构建了适用于一维综合孔径微波辐射计的微波海洋大气辐射传输模式，研究了C波段垂直和水平极化微波辐射亮温在不同入射角下对海洋大气环境要素的敏感性变化情况，并定量计算了相应的敏感系数。结果表明:垂直和水平极化亮温对海洋大气环境要素的敏感性表现出不同的特性。随着入射角的增大，垂直极化亮温对海面温度的敏感性增强，对海面风场的敏感性相对减弱；水平极化亮温则相反。由大气水汽含量和云液态水含量误差引入的垂直和水平极化亮温误差随入射角增大而增大，但是，即使在55°的大入射角下垂直和水平极化亮温误差仍小于0.12 K。对于海面温度反演精度优于1 K的要求，一维综合孔径微波辐射计的测温精度需优于0.6 K。研究结果对于一维综合孔径微波辐射计海面温度反演算法的研究和载荷设计具有一定的理论指导意义。  相似文献   

2015年台风“彩虹”过境后下山冷急流引起的南海北部海域异常海面降温   总被引：1，自引：0，他引：1  

石雨鑫  谢玲玲  郑全安  张书文  李明明  李君益 《海洋学报(英文版)》2019,38(5):62-75

This study deals with a unusual cooling event after Typhoon Mujigea passed over the northern South China Sea(SCS) in October 2015. We analyze the satellite sea surface temperature(SST) time series from October 3 to 18,2015 and find that the cooling process in the coastal ocean had two different stages. The first stage occurred immediately after typhoon passage on October 3, and reached a maximum SST drop of –2℃ on October 7 as the usual cold wake after typhoon. The second stage or the unusual extended cooling event occurred after 7d of the typhoon passage, and lasted for 5d from October 10 to 15. The maximum SST cooling was –4℃ and occurred after 12d of typhoon passage. The mechanism analysis results indicate that after landing and moving northwestward to the Yunnan-Guizhou Plateau(YGP), Typhoon Mujigea(2015) met the westerly wind front on October 5. The lowpressure and positive-vorticity disturbances to the front triggered meridional air flow and low-pressure trough,thus induced a katabatic cold jet downward from the Qinghai-Tibet Plateau(QTP) passing through the YGP to the northwestern SCS. The second cooling reached the maximum SST drop 4d later after the maximum air temperature drop of –9℃ on October 11. The simultaneous air temperature and SST observations at three coastal stations reveal that it is this katabatic cold jet intrusion to lead the unusual SST cooling event.  相似文献