东天山白山钼矿地球化学特征及地质意义     

涂其军  韩琼  王刚  马宏超 《新疆地质》2019,(1):7-16

白山钼矿赋矿岩体为花岗斑岩,其主量、微量及稀土元素地球化学特征研究表明,岩体属过铝质高钾钙碱性系列,并相对富集大离子亲石元素(Rb,Th,Sr等),亏损高场强元素(Nb,Ce,Zr等),以及具有LREE富集的右倾稀土元素分布模式。根据矿物稀土元素作为示踪剂提供的信息表明,含钼矿物的石英脉稀土元素组成和分布模式与壳幔同熔型花岗岩有众多相似之处,推测该成矿物质来源与花岗岩岩浆有关,来自同一源区,形成于碰撞后演化阶段向板内转化的构造环境,并具相同的成岩方式与成岩成矿同期。  相似文献   

Measurement of the deformation of sand in a plane strain compression experiment using incremental digital image correlation     

Wang  Pengpeng  Sang  Yong  Shao  Longtan  Guo  Xiaoxia 《Acta Geotechnica》2019,14(2):547-557

Acta Geotechnica - This work presents the results from a series of plane strain compression experiments on medium-density sands. In these experiments, a new type of plane strain experimental...  相似文献   

Centrifuge modelling of ground-borne vibrations induced by railway traffic in underground tunnels     

Yang Wenbo  Qian Zhihao  Tu Jiulin  Zhou Ziyang  Yan Qixiang  Fang Yong  He Chuan 《地震工程与工程振动(英文版)》2022,(2):517-528

Increased attention has been given to ground-borne vibrations induced by railway vehicles and to the effects of these vibrations as they propagate through the g...  相似文献   

An enhanced underwater camera apparatus for seabed observation of megabenthic epifauna in the northern Yellow Sea     

Yu  Nan  Sun  Song  Wang  Shiwei  Liu  Qun  Zhang  Guangtao  Zhang  Fang  Sun  Xiaoxia 《中国海洋湖沼学报》2020,38(6):1799-1810

Journal of Oceanology and Limnology - Seabed photographing has been applied with various underwater camera apparatuses (UCAs) for observations of megabenthic epifauna, which reveals more details...  相似文献   

对PCM编码式GPS站点布设模式的评价和改进     

邹镇宇  江在森  崔月菊  刘月  刘晓霞 《大地测量与地球动力学》2020,40(4):376-380

本文主要对PCM编码式的布设模式进行分析和改进,介绍PCM编码式和闭锁深度倍数式2种站点布设模式,然后在最小有效距离（MED）为6.31倍断层闭锁深度的情况下,通过精度评价方法对比2种布设模式的结果,发现二者相差不大。进一步研究MED的合理选择,结果表明,MED取20倍的闭锁深度比6.31倍的闭锁深度更为合理。在MED为20倍的情况下对比研究PCM编码式和常规闭锁深度倍数式布设模式的优劣,结果表明,PCM编码式的布设模式优于常规模式。将PCM编码式的布设模式应用于川滇地区的巧家-东川剖面进行检验,发现PCM编码式的结果优于目前站点分布得到的结果,说明合理的站点布设可得到精度更优的结果。本文研究对于断层形变监测中精确获取形变参数具有重要意义。  相似文献   

Characteristics and Origins of Suspended Pyrite in the Mixing Zone of the Yangtze Estuary     

Pang  Yue  Fan  Dejiang  Sun  Xiaoxia  Sun  Xueshi  Liu  Ming  Yang  Zuosheng 《中国海洋大学学报(英文版)》2020,19(4):801-810

For a long time, most studies about pyrite have focused on sediments while only a few have focused on pyrite in water. In this study, a method that combines the scanning electron microscopy(SEM) and the energy dispersive X-ray spectrometry(EDS) was used to compare pyrite particles suspended in water to those in associated bottom sediments, both obtained from the mixing zone of the Yangtze Estuary. It was found that the pyrite particles in the two media have similar morphologies and size distributions. The particle morphology mainly includes two types, single crystal and aggregate, and the particle size mainly ranges from 0.5 to 2 μm. The pyrite particles in water exhibit an increase in relative content towards the sea, and their transport and deposit processes are mainly affected by hydrodynamic conditions. It is concluded that the pyrite particles in the suspended matter mainly derived from the resuspension of sediments, which are products of the early diagenesis. Precursor minerals may appear during the formation of pyrite, but are generally restricted by the diagenetic environment and local microenvironment.  相似文献   

1979～2020年北极和青藏高原臭氧低值区的动力输送特征比较     

王启璐  徐雯雯  涂静怡  于淑洋  饶建  郭栋 《大气科学》2023,(3):866-880

基于ERA5月平均再分析资料,利用Lorenz环流分解方法从定常和瞬变以及基流和涡旋的角度对比了北极与青藏高原臭氧低值区的动力输送特征。结果表明：动力总输送在两地上平流层作用最强,均使其臭氧浓度降低,且定常输送均强于瞬变输送,纬向与经向输送的作用均大致相反。然而,动力输送在北极地区的作用强度远大于青藏高原地区。北极地区纬向输送使得平流层中上层臭氧浓度降低,平流层下层臭氧浓度升高,经向输送的作用与之相反且强度明显偏弱,二者均主要作用于上平流层。青藏高原地区纬向和经向输送除在上平流层均使得臭氧浓度降低外,二者作用大致相反且强度相当,输送大值区在垂直方向上存在双中心结构,分别位于上平流层与上对流层—下平流层（Upper Troposphere–Lower Stratosphere,简称UTLS）区。两地区纬向和经向输送的差异均主要由定常涡旋输送所造成。青藏高原地区定常与瞬变输送的强度差异没有北极地区大。此外,两地定常和瞬变输送中涡旋对臭氧纬向平均的输送均起到主要作用,体现出涡旋输送在两地臭氧浓度变化的动力输送过程中发挥着至关重要的作用。  相似文献   

地质环境信息系统上线安全检测工作实践     

殷铭  武建飞  屠陈子煜  杨宏斌  周萌  韩明伟 《国土资源信息化》2017,(2)

本文针对地质环境领域业务系统的特点,提出了一种信息系统上线安全检测的方法,深入探讨了上线安全检测实践中的基本流程、测评方法与测评成果,为提升地质环境信息系统安全运行和服务能力提供了技术支撑.  相似文献   

Solar Wind and Chromospheric Network     

Marsch  E.  Tu  C.-Y. 《Solar physics》1997,176(1):87-106

A physical model of the transition region, including upflow of the plasma in magnetic field funnels that are open to the overlying corona, is presented. A numerical study of the effects of Alfvén waves on the heating and acceleration of the nascent solar wind originating in the chromospheric network is carried out within the framework of a two-fluid model for the plasma. It is shown that waves with reasonable amplitudes can, through their pressure gradient together with the thermal pressure gradient, cause a substantial initial acceleration of the wind (on scales of a few Mm) to locally supersonic flows in the rapidly expanding magnetic field trunks of the transition region network. The concurrent proton heating is due to the energy supplied by cyclotron damping of the high-frequency Alfvén waves, which are assumed to be created through small-scale magnetic activity. The wave energy flux of the model is given as a condition at the upper chromosphere boundary, located above the thin layer where the first ionization of hydrogen takes place.Among the new numerical results are the following: Alfvén waves with an assumed f ^-1 power spectrum in the frequency range from 1 to ⁴ Hz, and with an integrated mean amplitude ranging between 25 and 75 km s⁴, can produce very fast acceleration and also heating through wave dissipation. This can heat the lower corona to a temperature of 5× 10⁵ K at a height of h=12,000 km, starting from 5× 10⁴ K at h=3000 km. The resulting thermal and wave pressure gradients can accelerate the wind to speeds of up to 150 km s^-1 at h=12,000 km, starting from 20 km s^-1 at h=3000 km in a rapidly diverging flux tube. Thus the nascent solar wind becomes supersonic at heights well below the classical Parker-Type sonic point. This is a consequence of the fact that any large wave-energy flux, if it is to be conducted through the expanding funnel to the corona, implies the building-up of an associated wave-pressure gradient. Because of the diverging field geometry, this might lead to a strong initial acceleration of the flow. There is a multiplicity of solutions, depending mainly on the coronal pressure. Here we discuss two new (as compared with a static transition region model) possibilities, namely that either the flow remains supersonic or slows down abruptly by shock formation, which then yields substantial coronal heating up to the canonical 10⁶ K for the proton temperature.  相似文献   

峨眉山之雨量     

涂长望  许鉴明 《气象学报》1936,12(10):560-573

地理位置欲充分了解峨眉多雨之原因必先明瞭其地理位置。峨眉位北纬二十九度二十八分,东经一○三度四十一分,居四川西南部,去省会成都一五0公里.其山自东高起拔海三0七0公尺,山巅高出峨眉县城二公里,在岷江流域  相似文献