河东煤田三交区块水文地质条件控气的正负耦合效应

煤层气的开采受多种地质因素的影响,不同区块的主控因素各不相同.山西河东煤田三交区块构造简单,煤岩渗透率和临储比相对其他区块较优,含气性良好,是煤层气开采的优势区块,但是区内不同气井产气量却相差很大.结合现场排采井采出水的水质分析实验与stiff图解法,综合分析各种地质因素,认为水文条件是该区块控气的主要因素,且水文地质控气存在着正负效应耦合的特殊性,合理分析水文地质特征是成功开采煤层气的关键所在.     

陕北地区奥陶纪马家沟组五段沉积时期岩相古地理演化*

陕北地区马家沟组五段沉积时期(简称马五期)沉积的碳酸盐岩地层是重要的天然气储集层。为明确各沉积期岩相古地理演化特征,在对周缘野外地质剖面考察、研究区内98口井的岩心观察、测井曲线形态分析的基础上,对陕北地区马家沟组马五₁₀—马五₁各亚段的岩相古地理演化特征进行了恢复。结果表明,马五₁₀—马五₁各亚段以海相碳酸盐岩台地沉积为主,包括局限台地、开阔台地和蒸发台地3种亚相,并进一步细分为: 云坪、膏云坪、含膏云坪、泥云坪、灰云坪、灰坪、颗粒滩、云灰坪、泥灰坪、膏盐湖等10种沉积微相;从马五₁₀到马五₁岩相古地理单元整体表现为自东向西的环带状分布特征,环带中心主要位于延长、延川和清涧一带,值得注意的是,马五₂沉积时期由于受南部较强构造抬升作用影响,古地理单元环带中心呈现出向西北挪移的特征,环带中心位于靖边、子长一带;马家沟组各沉积时期的旋回性环带沉积为储集层叠合发育奠定了物质基础,云坪、膏云坪、含膏云坪、颗粒滩微相易于形成有利储集空间,纵向上的马五₁₊₂、马五₄、马五₅、马五₇、马五₉亚段为该类相带较发育的层位,是区域勘探开发的重点领域。     

Infrared Observations from the New Solar Telescope at Big Bear

The 1.6 m clear aperture solar telescope in Big Bear is operational and with its adaptive optics (AO) system it provides diffraction limited solar imaging and polarimetry in the near-infrared (NIR). While the AO system is being upgraded to provide diffraction limited imaging at bluer wavelengths, the instrumentation and observations are concentrated in the NIR. The New Solar Telescope (NST) operates in campaigns, making it the ideal ground-based telescope to provide complementary/supplementary data to SDO and Hinode. The NST makes photometric observations in Hα (656.3 nm) and TiO (705.6 nm) among other lines. As well, the NST collects vector magnetograms in the 1565 nm lines and is beginning such observations in 1083.0 nm. Here we discuss the relevant NST instruments, including AO, and present some results that are germane to NASA solar missions.     

Connection Between Chromospheric Events and Photospheric Dynamics

We analyzed chromospheric events and their connection to oscillation phenomena and photospheric dynamics. The observations were done with the New Solar Telescope of Big Bear Solar Observatory using a broad-band imager at the wavelength of a TiO band and FISS spectrograph scanning Ca?ii and Hα spectral lines. The event in Ca?ii showed strong plasma flows and propagating waves in the chromosphere. The movement of the footpoints of flux tubes in the photosphere indicated flux tube entanglement and magnetic reconnection as a possible cause of the observed brightening and waves propagating in the chromosphere. An upward propagating train of waves was observed at the site of the downflow event in Hα. There was no clear relationship between photospheric waves and the Ca?ii and Hα events. Our observations indicate that chromospheric waves that were previously thought to originate from the photosphere may be generated by some events in the chromosphere as well.     

不同出游时间视角下游客流动网络结构及其分异特征——以西安市为例

以热门旅游城市西安市为研究区域,采集网络游记数据,综合运用社会网络分析和GIS空间分析方法,探讨不同出游时间下的游客流动网络结构及其分异特征,研究发现：① 不同的出游时间约束下,游客旅游出行行为表现出显著的时间异质性。② 基于游客流动的西安市旅游吸引物的节点结构具有显著的等级规模分异特征,随着出游时间的增加,旅游节点等级结构体系呈现出以高等级景点为枢纽的“强强”关联特征,高等级景点的游客集聚功能提升显著。③ 随着出游时间增加,西安市区旅游节点核心?边缘结构越明显,核心区的节点联系强度越大,区位邻近、知名度接近与交通便利是形成景点组团的关键因子。     

Active phase of a substorm as a chain of two types of reconnection: In the closed plasma sheet and in the open tail lobes

The maps of the field-aligned current (FAC) density distribution in the ionosphere obtained by the TIM-2 magnetogram inversion technique are used to investigate the August 27, 2001 substorm. The open magnetic flux Ψ and intensity J of the substorm current wedge (SCW) have been determined with a step of 1–5 min. The substorm onsets are divided into two types, PSR (plasma sheet reconnection) and TLR (tail lobe reconnection). The fast expansion tailward of the PSR region is described as the transition from PSR to PSR+TLR. Assuming that the SCW FACs flow down into the ionosphere from the edges of the disruption region of the cross-tail dawn-dusk current, several parameters of the disruption region have been estimated. The disrupted magnetic field has been found to be ∼5% of the undisrupted one for PSR and ∼95% for PSR+TLR. The disturbance power Q for PSR is an order of magnitude lower than that for PSR+TLR. The abrupt growth of Q during the transition from PSR to PSR+TLR is observed over the entire SCW area from its near-Earth part to the midtail and distant tail.     

Small variation of annual temperature in deep tunnel can produce annual variation in tilt and strain

In this paper,finite element method (FEM) of axisymmetric linear elastic model has been used to calculate the tilt and strain induced by small annual temperature variations in a deep tunnel. The results show that even if the am-plitude of the annual variation meets the construction standard of seismic station issued by China Earthquake Ad-ministration (the annual temperature variation amplitude in the tunnel is no more than 0.5 °C),a small annual tem-perature variation of amplitude just 0.2 °C in the tunnel would produce 10?7 rad changes in tilt and 10?7 changes in strain. Especially,at the end and the corner of the tunnel,changes of tilt and strain can be even larger. Therefore,in the future,it is an important task to reduce the annual temperature variation in the tunnel as far as possible. Within the tunnel,for both baseline instrument and pendulum instrument,the modeling suggests ways of construction of the tunnel and installation of the instrument to decrease the influence of the annual temperature variation.     

An Efficient System for Creating Synthetic InSAR Images from Simulations

In this work we visualize tsunami and earthquake simulation results with graphics hardware acceleration. The rapid improvement in the computational power of graphics hardware and its programmability has made general computation on Graphics Processing Units (GPUs) very compelling. We generate Synthetic InSAR images using GPUs. Interference phenomena have formed the underlying theory for Interferometric Synthetic Aperture Radar (InSAR) in unveiling dynamical Earth movements. In our approach light path differences are defined by the surface values to be visualized. These path differences then modulate the lighting intensity to generate the interference patterns. We can interactively visualize surface deformation patterns by leveraging the computational power of GPUs. Our visualization method is applied to simulations of rupture fault displacements during the tsunamogenic earthquake events, which are vital to understanding the subsequent wave propagation. We also integrate the visualization results into Google Earth virtual globe to provide the geological context of the visualized regions.     

潮汐测量中异常“震颤”信号的综合观测试验与挖掘

潮汐测量包含倾斜、应变和重力固体潮等,与地震观测具有共同的物理本质,观测量都与地壳运动有直接力学关系.两者的观测信号在频率域相互重叠、自然衔接,覆盖了从地震波至固体潮频段的所有地动信息.