岷江上游水系对龙门山断裂带右旋走滑作用的响应

汶川8.0级特大地震是岷江上游流域最新一次区域构造活动,在此次地震中,岷江河道因北川-映秀断裂北西盘的右旋走滑作用而被水平错动0.8±0.2 m,岷江河道南西方向的河流阶地也被同步位错0.6±0.1 m。切过龙门山主干断裂的岷江上游干、支流水系因若干次历史地震驱动的走滑作用而发生同步弯曲。根据水系水平扭错量和岷江干、支流初始形成时间计算可知,穿越岷江支流河道的汶川-茂县断裂右旋走滑速率为1～1.4 mm/a,切过岷江干流河道的北川-映秀断裂和彭县-灌县断裂右旋滑动速率分别为0.94 mm/a和0.71 mm/a。计算结果表明,龙门山各主干断裂右旋走滑作用有自北西向南东减弱的趋势。     

A Schumann-like resonance on Titan driven by Saturn's magnetosphere possibly revealed by the Huygens Probe

The low-frequency data collected with the antenna of the Permittivity, Wave and Altimetry experiment on board the Huygens Probe that landed on Titan on 14 January 2005 have been thoroughly analyzed considering different possible natural and artificial effects. Although a definite conclusion is still subject to the outcome of complementary inquiries, it results from our analysis that the observations can be explained, for the most part, in term of natural phenomena rather than being artifacts. Extremely-low frequency waves generated in the ionosphere of Titan, driven by the corotating Saturn's frozen plasma flow, are assumed to be the most likely source for the observation of the second eigenmode of a Schumann-like resonance at around 36 Hz in the moon-ionosphere cavity. This particular mode is thought to be enhanced with respect to other harmonics because of the particular location of the landing site with respect to that of the supposed sources. The power budget of the observed wave amplitude seems to be consistent with a rough model of the global current of the wake-ionosphere circuit. Broadband low-frequency noise events which are observed sporadically during the descent are probably due to shot noise on the antenna when the Probe is crossing aerosol clouds, an interpretation supported by post-flight ground tests. Contrary to the situation encountered on Earth, atmospheric lightning does not appear to be the source of a conventional Schumann resonance on Titan.     

Study of solar system planetary lightning with LOFAR

Radio signatures of lightning discharges have been detected by the Voyager spacecraft near Saturn and Uranus up to 40 MHz. Corresponding flux densities at the distance of the Earth are up to 1000 Jansky (Jy) for Saturn (1 event per minute above 50 Jy, with 30–300 ms duration) and up to a few tens of Jansky for Uranus. Low Frequency ARray LOFAR will allow us to detect and monitor the lightning activity at these two planets. Imaging will allow us to locate lightning sources on Saturn's disk (even if with moderate accuracy), which could then be correlated to optical imaging of clouds. Such observations could provide new information on electrification processes, atmospheric dynamics, composition, and geographical and seasonal variations, compared to the Earth. In addition, lightning may play a role in the atmospheric chemistry, through the production of non-equilibrium trace organic constituents potentially important for biological processes. LOFAR observations can also help us to assess the existence of lightning at Neptune (marginally detected by Voyager), at Venus (where their existence is very controversial), and at Mars (possibly resulting from dust cloud charging). At Jupiter, low-altitude ionospheric layers of meteoritic origin and/or intrinsically long discharge duration seem to prevent the emission and escape of high-frequency radio waves associated with lightning. LOFAR thus presents good possibilities for the detection and study of solar system planetary lightning; we also discuss its relevance to bring new information on Terrestrial lightning-related upper atmosphere transient phenomena (sprites, TIPPs…). Instrumental constraints are outlined.     

MapX与PowerBuilder集成技术在交通事故信息系统中的应用

针对复杂的道路交通事故信息,利用MapInfo公司的组件式控件MapX5.0,在PowerBuilder8.0开发环境下,使用SQLServer2005作为系统后台属性数据库,研究路段采用高分辨率的遥感数据为地图背景,设计开发了城市道路交通事故信息系统。该系统具有城市道路交通信息与道路交通事故信息的查询、分析和统计功能,使道路交通事故信息查询更迅速、直观。实际开发表明,PowerBuilder与地图控件MapX结合开发GIS应用系统,不仅开发过程简单、开发速度快,而且能充分发挥PowerBuilder快速高效管理、访问MapX空间数据库的优势。     

云分辨尺度下一种综合调整水物质含量的闪电资料同化方法

在直接调整水汽含量（称为F12）和直接调整冰相粒子浓度（称为Q14）两种闪电资料同化方法的基础上,提出了一种综合调整冰相粒子浓度和水汽含量（称为C17）的闪电资料同化方法,选取一次具有完整闪电观测资料（云闪加地闪）的飑线过程,利用WRF在云分辨尺度进行数值模拟,详细比较了3种闪电资料同化方法的模拟结果。与不进行闪电资料同化的控制试验相比,闪电资料同化试验明显改进了模式对流活动的模拟能力,但是不同同化方法有所差异。在同化时段内,F12方法中回波强度较小,形成大范围层云区,回波中心比实测偏向下游;Q14方法回波强度和落区同实测最为接近,但是对层云区的模拟无明显改进;C17方法综合了F12和Q14方法的优势,与F12方法相比,回波强度增大,落区更加接近实测,层云区面积扩大。同化结束后,F12方法冷池有所增强,雨区向东北方向延伸,但是强度较弱,形成大范围的弱降水区,同化正面效果保持最久;Q14方法低层大气偏干,地表冷池偏强,对流系统迅速移动并衰减,降水区域比实测偏南,同化正面效果消失较快;C17方法冷池范围和强度与实际观测最为接近,降水较F12方法增强,模拟出的飑线形态得到调整,模拟出了实测中的另一降水中心,同化正面效果保持时间延长。      

西藏扎西康铅锌银矿床含矿走滑断裂地球物理特征及找矿方向

扎西康铅锌银矿床位于北喜马拉雅大陆边缘褶冲带内,是西藏扎西康整装勘查区中大型铅锌锑银共生矿床之一。矿床赋存于下侏罗统日当组,容矿岩石为含碳钙质板岩、钙质板岩和构造角砾岩,矿体严格受近SN向和NE向断裂控制,呈脉状、透镜状产出。通过岩石物性分析,认为矿体具有中低电阻和中低极化的物性特征。在矿集区开展了音频大地电磁法(AMT)和激发极化法试验,结合地质地球物理初始模型,从地质背景、勘查模型角度分析,含矿走滑断裂的围岩具有中低极化率、断裂走向与极化率条带一致的特征;认为在中低极化率区域存在断裂,且断裂走向的垂直方向存在高极化、低电阻区,赋矿可能性较大。     

Mesozoic and Cenozoic structural deformation in the NW Tarim Basin,China: a case study of the Piqiang–Selibuya Fault

The Piqiang–Selibuya Fault is the most significant fault in the NW Tarim Basin, China. It has attracted increasing attention because of the discovery of a series of oil (gas) fields in and around the fault zone. The structural characteristics and evolution of the Piqiang–Selibuya Fault remain controversial. Field geological surveys and seismic data interpretation reveal that the fault has experienced three stages of activity. The thicknesses of the Permian and Miocene strata on opposing sides of the fault are clearly different, and these reveal that the fault has experienced two stages of significant thrusting. The first stage took place at the end of the Triassic and was associated with the Qiangtang Block amalgamated to the south margin of Eurasia. The second stage occurred at the end of the Miocene and might have been caused by the northwards overthrusting of the Pamir. These two stages of thrusting led to the lower–middle Cambrian detachment layer in the eastern part of the Keping thrust belt being 2 km shallower than in the western part. Since the Pliocene, the southern Tien Shan orogenic belt has been reactivated and thrust towards the interior of the Tarim Basin, and a series of ENE–WSW-trending thrust sheets have formed in the Keping thrust belt. Because of the different depth of the detachment layer on the opposing sides of the Piqiang–Selibuya Fault, the number and spacing of thrust sheets formed to the east of the fault differ from those to the west. This dissimilar deformation led to the strike–slip displacement on the Piqiang–Selibuya Fault. The three stages of fault activity record three important tectonic events in the NW Tarim Basin. Qualitative analysis of this activity helps us better understand the influence of the far-field effect of the collisions that occurred on the southern margin of the Eurasia plate on the structural deformation of the NW Tarim Basin.     

AD401-7井定向井卡钻复杂事故的处理及分析

AD4017井属于吐哈盆地鲁克沁油田ADI块构造。该区块在勘探开发初期极少出现因井下坍塌而发生的卡钻事故,AD4017井在井身结构设计时,参考的是前期地质勘探资料和邻井数据资料,未考虑到钻井过程中出现薄煤层夹层的情况,原有设计在该井段易导致井壁不稳,所以实际钻井过程中发生了卡钻事故。本文通过对AD4017井卡钻事故的研究,从地质因素、物理化学因素、工艺因素等几方面,深入分析了该井发生坍塌卡钻可能存在的原因及机理,并对这些原因导致的卡钻事故提出了针对性的预防措施和处理方法。     

岩心钻探烧钻事故浅析及实践

烧钻事故在岩心钻探施工过程中是最频发的事故之一,分析总结烧钻事故发生的原因和发生的必要条件,烧钻事故发生前出现的异常征兆,烧钻事故的预防措施、处理原则和方法;总结了几起烧钻事故的处理经验及教训,提出了如何做好预防和处理烧钻事故的措施建议。