低地球轨道（LEO）的大型航天器充电

本文根据ＬＥＯ中等离子体温度低，密度高，德拜长度小的特点，采用薄鞘层近似，计算了离子收集电流；根据电流平衡方程，考虑表面二次电子发射，计算了大型航天器表面在沉降电子流辐照下的充电特性。     

利用储层流体包裹体确定鄂尔多斯盆地塔巴庙区块上古生界油气充注期次和时期

流体包裹体是保存在储层中的微小流体样品,包含有丰富的地质信息。通过对鄂尔多斯盆地塔巴庙区块18口井的62块流体包裹体样品进行荧光观察和显微测温,认为该区上古生界地层共发生过6期流体活动,均与油气成藏有关,并以第二期—第六期的天然气充注为主。结合埋藏史分析可知,油气成藏分别发生在距今190～150Ma的早侏罗世中期—中侏罗世晚期,150～124Ma的中侏罗世晚期—早白垩世早期,124～101Ma的早白垩世早期—早白垩世中期,101～86Ma的早白垩世中期—早白垩世中末期和86～70Ma的早白垩世中末期—早白垩世末期。其中,早侏罗世中期—中侏罗世晚期为油气充注的初始阶段,中侏罗世晚期—早白垩世早期为轻质油的主要成藏时期,中侏罗世晚期至早白垩世末为研究区内目的层天然气的主要成藏时期。     

Critical conditions for natural gas charging and delineation of effective gas source rocks for tight sandstone reservoirs

Although it has been shown that the potential of tight‐sand gas resources is large, the research into the mechanisms of hydrocarbon charging of tight sandstone reservoirs has been relatively sparse. Researchers have found that there is a force balance during hydrocarbon charging, but discriminant models still have not been established. Based on the force balance conditions observed during gas migration from source rocks to tight sandstone reservoirs, a calculation formula was established. A formula for identifying effective source rocks was developed with the gas expulsion intensity as the discrimination parameter. The critical gas expulsion intensity under conditions of various burial depths, temperatures, and pressures can be obtained using the calculation formula. This method was applied in the Jurassic tight sandstone reservoirs of the eastern Kuqa Depression, Tarim Basin, and it was calculated that the critical expulsion intensity range from 6.05 × 10⁸ m³/km² to 10.07 × 10⁸ m³/km². The critical gas charging force first increases with depth and later decreases with greater depths. The distribution range of effective gas source rocks and total expelled gas volume can be determined based on this threshold. This method provides new insight into and method for predicting favourable tight‐sand gas‐bearing regions and estimating their resource potentials. Copyright © 2014 John Wiley & Sons, Ltd.     

Impact of the Vertical Velocity Field on Charging Processes and Charge Separation in a Simulated Thunderstorm

A three-dimensional(3D) charging-discharging cloud resolution model was used to investigate the impact of the vertical velocity field on the charging processes and the formation of charge structure in a strong thunderstorm. The distribution and evolution of ice particle content and charges on ice particles were analyzed in different vertical velocity fields. The results show that the ice particles in the vertical velocity range from 1 to 5 m s-1obtained the most charge through charging processes during the lifetime of the thunderstorm. The magnitude of the charges could reach 1014 n C. Before the beginning of lightning activity,the charges produced in updraft region 2(updraft speed 13 m s-1) and updraft region 1(updraft speed between 5 and 13 m s-1) were relatively significant. The magnitudes of charge reached 1013 n C, which clearly impacted upon the early lightning activity. The vertical velocity conditions in the quasi-steady region(updraft speed between –1 and 1 m s-1) were the most conducive for charge separation on ice particles on different scales. Accordingly, a net charge structure always appeared in the quasi-steady and adjacent regions. Based on the results, a conceptual model of ice particle charging, charge separation, and charge structure formation in the flow field was constructed. The model helps to explain observations of the"lightning hole" phenomenon.     

川中安平店-高石梯构造震旦系灯影组流体充注特征及油气成藏过程

川中地区震旦系灯影组储层时代老、埋藏深,经历了多期构造运动和成藏历史。岩芯观察和显微薄片观察结果表明,震旦系灯影组储层经历了六期流体充注,分别是第一世代沥青→第二世代白云石→第三世代粗晶-巨晶白云石→第四世代粗晶-巨晶白云石→第五世代沥青→第六世代方解石/石英,每期矿物中对应的流体包裹体特征记录了震旦系从早期形成的古油藏被破坏→古油气藏再形成→油裂解气和古气藏形成→水溶气形成→现今气藏形成的成藏事件和完整的成藏过程。第二世代-第四世代矿物形成于深埋过程中,是古油气藏形成期的产物,矿物的Sr、C、O稳定同位素表明向震旦系灯影组充注的流体主要是外源流体,具有从深部向浅部流动运移的特征;第六世代矿物所记录的水溶气的形成,也是震旦系最重要的成藏事件;现今的震旦系灯影组气藏主要是晚白垩世以来的构造隆升导致的水溶气脱溶聚集以及油气藏调整和改造的结果。     

X-Ray Line Transfer in Plasmas with Large Velocity Gradients

An astrophysically relevant experiment is compared to the output of a multidimensional radiation transfer code in which populations and radiation are self-consistently treated. Experimental Al Ly α spectra obtained with a very high-resolution spectrometer are presented as quantitative evidence of dot plasma non-planar expansion. Analysis of these spectra using the code is performed, in particular examining the effects of velocity gradients in directions other than that of the primary expansion. These calculations are found to be in good agreement with the experimental results. Usage of the Ly α doublet as a planarity diagnostic is discussed.     

铁路栈桥桥墩钢围堰的拆除爆破

钢围堰内混凝土拆除爆破工程较为鲜见 ,文章介绍了该工程所选取的爆破诸参数以及所采用的施工工艺 ,可供同行参考     

长春地区对流云起电过程的数值模拟

在三维强风暴动力和电耦合数值模式的基础上,考虑了粒子直径及降落末速差对转移电荷的影响,把非感应起电参数化方案作了进一步改进,对长春地区两次不同强度、不同环境风切变的对流云内电荷累积和电场发展过程进行了模拟分析。结果表明,对流云上升气流达到极大值时,较强和较弱两块云分别具有三极性和反偶极性电荷分布结构。垂直上升气流是表明电场发展强弱的重要参量。对发展强烈的对流云,较强的上升气流使霰和冰晶在云体的中上部维持较长的时间．存在感应和非感应起电的跃增。     

Lunar Prospector measurements of secondary electron emission from lunar regolith

We present the first in situ measurements of the secondary electron emission efficiency of lunar regolith, utilizing Lunar Prospector measurements of secondary electrons emitted from the negatively charged night side and accelerated upward by surface electric fields. By comparing measurements of secondary currents emitted from the surface and incident primary electron currents, we find that the secondary yield of lunar regolith is a factor of ∼3 lower than that measured for samples in the laboratory. This lower yield significantly affects current balance at the lunar surface and the resulting equilibrium surface potentials. This information must be folded into models of the near-surface plasma sheath, in order to predict the effects on dust and other components of the lunar environment, and ultimately determine the importance for surface exploration and scientific investigations on the Moon.     

基于贝叶斯方法的深层充电效应风险模型评估

高能电子穿透航天器并在其内部沉积电荷从而引发深层充电效应,是导致卫星故障的重要因素之一.为了评估深层充电效应诱发卫星异常的风险,本文基于贝叶斯方法,使用一颗地球同步轨道卫星的异常数据和GOES-8卫星的电子通量探测数据,计算了不同能量阈值及累积时间的电子注量、不同卫星配置下模拟仿真的沉积电荷,并分别与卫星异常建立一系列概率风险模型.本文从模型中随机抽样得到模拟异常,并与实测异常构造混淆矩阵以评估模型拟合优度,结果表明1.0MeV电子3日累积注量-卫星异常概率风险模型为该卫星最优模型.本文利用最优模型对该卫星深层充电效应风险进行了计算,在1.0MeV电子3日累积注量达到2.0×10~(10)cm~(-2)·sr~(-1)时,该卫星发生深层充电异常的平均后验概率为27%,且95%最小可信值为22%.根据最优模型,我们对该卫星最可能导致异常的部件的材料和结构等特征做出了推断.