Repeating microlensing events in the OGLE data     

J. Skowron  &#;. Wyrzykowski  S. Mao  M. Jaroszy&#;ski 《Monthly notices of the Royal Astronomical Society》2009,393(3):999-1009

Microlensing events are usually selected among single-peaked non-repeating light curves in order to avoid confusion with variable stars. However, a microlensing event may exhibit a second microlensing brightening episode when the source or/and the lens is a binary system. A careful analysis of these repeating events provides an independent way to study the statistics of wide binary stars and to detect extrasolar planets. Previous theoretical studies predicted that 0.5–2 per cent of events should repeat due to wide binary lenses. We present a systematic search for such events in about 4000 light curves of microlensing candidates detected by the Optical Gravitational Lensing Experiment (OGLE) towards the Galactic bulge from 1992 to 2007. The search reveals a total of 19 repeating candidates, with six clearly due to a wide binary lens. As a by-product, we find that 64 events (∼2 per cent of the total OGLE-III sample) have been misclassified as microlensing; these misclassified events are mostly nova or other types of eruptive stars. The number and importance of repeating events will increase considerably when the next-generation wide-field microlensing experiments become fully operational in the future.  相似文献   

Structural Evolution of Chepaizi Uplift and its Control on Stratigraphic Deposition in the Western Junggar Basin,China     

NI Minjie  CHEN Shi  LIU Zichao  SHANG Fengkai  QI Jiafu  WANG Lishuang 《《地质学报》英文版》2019,93(4):1060-1075

Geological mapping, interpreted cross sections, structural analyses and residual thickness maps were used to characterize the evolution of stress setting, structure and stratigraphic distribution of the Chepaizi Uplift, which is a NW-SE trending structure located in the Western Junggar Basin. The NS-trending faults show an important transpressional phase during the Late Permian, as demonstrated by tectonic stress field and stratigraphic thickness variations. A major compressional thrusting and strike-slip phase during the Late Jurassic created a series of NW-SE faults that originated by the large-scale uplift event in the Northern Tianshan. Faults were reactivated as thrust and dextral strike-slip faults. In addition, the angular unconformity observed between Jurassic and Cretaceous provide evidence of this tectonic event. Lots of normal faults indicate that the area records southward tilting and regional derived extensional stress that took place during the Neogene. Before that, thick Early Cenozoic strata are widely deposited. The balanced cross-section highlights the evolution of stress setting and stratigraphic distribution of the Chepaizi Uplift.  相似文献   

Flexure of the Indian plate and intraplate earthquakes   总被引：2，自引：0，他引：2  

Roger Bilham  Rebecca Bendick  Kali Wallace 《Journal of Earth System Science》2003,112(3):315-329

The flexural bulge in central India resulting from India's collision with Tibet has a wavelength of approximately 670 km. It is manifest topographically and in the free-air gravity anomaly and the geoid. Calculations of the stress distribution within a flexed Indian plate reveal spatial variations throughout the depth of the plate and also a function of distance from the Himalaya. The wavelength (and therefore local gradient) of stress variation is a function of the effective elastic thickness of the plate, estimates of which have been proposed to lie in the range 40–120 km. The imposition of this stress field on the northward moving Indian plate appears fundamental to explaining the current distribution of intraplate earthquakes and their mechanisms. The current study highlights an outer trough south of the flexural bulge in central India where surface stresses are double the contiguous compressional stresses to the north and south. The Bhuj, Latur and Koyna earthquakes and numerous other recent reverse faulting events occurred in this compressional setting. The N/S spatial gradient of stress exceeds 2 bars/km near the flexural bulge. The overall flexural stress distribution provides a physical basis for earthquake hazard mapping and suggests that areas of central India where no historic earthquakes are recorded may yet be the locus of future damaging events.  相似文献   

国道219线新-藏公路改建工程地质灾害评价   总被引：1，自引：0，他引：1  

李铁锋  刘长兵  李欣 《中国地质灾害与防治学报》2003,14(4):26-29

国道219线新-藏区界至红土达坂路段全长109．55km。大部分路段穿越湖盆槽谷中央部位，部分线路沿湖盆边缘台地布设，海拔高度介于5000-5400m之间，地势平坦开阔，多年冻土发育，工程地质条件较差；现有公路路基高度低，几乎没有排水设施。冬季易产生路基冻胀和涎流冰危害，春、夏季因冻土融化，常引起路基沉陷和翻浆，严重危害公路运输安全甚至阻断交通。公路工程修建活动将极大地改变冻土环境，使天然状态下的水分循环发生改变，导致多年冻土退化，上限加深，进一步诱发冻胀、融沉、热融滑塌等冻土灾害，加剧风沙灾害、诱发公路边坡失稳破坏。在即将进行的公路改、扩建工程中，应采取保护冻土的设计原则，优选线路，加强侧向排水，合理设置取弃土场。  相似文献   

青海地区盐渍土分布规律及其独特工程特性探讨     

罗友弟 《岩土工程技术》2010,24(2):75-78,83

针对青海一些地区盐渍土当硫酸钠含量小于1%时也会产生盐胀,而超氯盐渍土却不会产生溶陷的事实,进行了较为深入细致的论证和研究。以数据、事实为依据,得出了与现行理论及规范有较大出入的论断。  相似文献   

The Eocene unconformity of the Briançonnais domain in the French—Italian Alps,revisited (Marguareis massif,Cuneo); a hint for a Late Cretaceous—Middle Eocene frontal bulge setting     

A. Michard  G. Martinotti 《Geodinamica Acta》2013,26(5-6):289-301

Abstract

The tectonic significance of the Eocene unconformity in the Briançonnais domain, classically regarded as recording a compressional event, is re-evaluated, based on field studies in the Marguareis massif, Maritime-Ligurian Alps. In this external, weakly metamorphic Briançonnais unit, we describe N-trending, folded paleo-normal faults. These paleofaults operated during the Late Cretaceous-Late Eocene, and control both the thickness of the Senonian-Paleocene calcschists and the distribution of the disconformable Middle Eocene-Early Priabonian formations, i.e. the channelised, resedimented Nummulitic limestones, associated with sandy turbidites, and the sandy- calcareous Lower Flysch Noir. The chaotic Upper Flysch Noir (Priabonian), which includes olistoliths from the Helminthoid Flysch nappes, disconformably overlies the Late Cretaceous-Middle/Late Eocene levels. At the scale of the whole Briançonnais domain of the French-Italian Alps, the superimposed Senonian-Eocene disconformities would indicate extensional faulting and block tilting, associated with a regional uplift which caused emersion of part of the domain (most internal Briançonnais, Corsica). Extension and coeval uplift would record the crossing of the frontal flexure (external bulge) of the European/Briançonnais lower plate situated west of the Alpine subduction zone between 80–70 Ma and ～40 Ma, i.e. before the subduction of the Briançonnais plateau around 38–35 Ma. © 2002 Éditions scientifiques et médicales Elsevier SAS. All rights reserved.  相似文献   

准噶尔盆地车排子凸起侏罗系齐古组沉积相分析及储层展布--以车60井区齐古组地层-岩性油气藏为例   总被引：1，自引：0，他引：1  

德勒恰提  王威  李宏  陈剑  帕尔哈提 《沉积学报》2013,31(3):545-552

侏罗系齐古组为准噶尔盆地重要的含油气层系,其层序发育较完整,沉积相类型丰富。综合利用岩芯、测井、录井及相关测试资料,在沉积特征分析的基础上,对车排子车60井区齐古组沉积微相进行了系统研究。确定研究区齐古组主要为砾岩、砂岩、细砂岩、粉砂岩和泥岩构成的一套碎屑岩多旋回沉积组合,为典型的辫状河三角洲相沉积,其物源主要来自于北西和正北方向。平原辫状分流河道微相砂体为储集层骨架砂体,储集性能较好,前缘分支河道微相砂体及河口砂坝次之,为油气运移聚集的有利相带。该研究成果为油田开发方案的调整和动态分析提供了可靠的地质依据。  相似文献   

新疆塔里木盆地温宿凸起石油地质条件新认识          下载免费PDF全文

杨有星  高永进  张君峰  周新桂  张金虎  苗苗青 《中国地质调查》2019,6(4):11-16

为了弄清塔里木盆地温宿凸起构造演化、油源条件及圈闭类型等关键地质问题,通过石油地质条件综合分析,结合样品测试分析,查清了温宿地区油气成藏的关键因素,提出了石油地质条件新认识。结果表明:温宿凸起为一个继承性发育的古隆起,构造演化主要经历了4个发展阶段;温宿凸起油气藏类型以构造-岩性型为主;温宿凸起不发育烃源岩,但发育沟通拜城富烃凹陷的高效输导体系;温宿凸起新近系吉迪克组油气藏类型以构造-岩性型为主;油气的生成、运移、聚集主要发生在新近纪-第四纪,具有明显的晚期复式成藏特点;优越的盖层条件是温宿吉迪克组油气藏形成的重要因素。  相似文献   

A systematic fitting scheme for caustic-crossing microlensing events     

《Monthly notices of the Royal Astronomical Society》2009,395(2):787-796

We outline a method for fitting binary-lens caustic-crossing microlensing events based on the alternative model parametrization proposed and detailed by Cassan. As an illustration of our methodology, we present an analysis of OGLE-2007-BLG-472, a double-peaked Galactic microlensing event with a source crossing the whole caustic structure in less than three days. In order to identify all possible models we conduct an extensive search of the parameter space, followed by a refinement of the parameters with a Markov Chain Monte Carlo algorithm. We find a number of low-  χ²  regions in the parameter space, which lead to several distinct competitive best models. We examine the parameters for each of them, and estimate their physical properties. We find that our fitting strategy locates several minima that are difficult to find with other modelling strategies and is therefore a more appropriate method to fit this type of event.  相似文献   

Synthetic microlensing maps of the Galactic bulge     

E. Kerins  A. C. Robin  D. J. Marshall 《Monthly notices of the Royal Astronomical Society》2009,396(2):1202-1210

  相似文献