φ175 mm电磁随钻测量系统的研制及试验研究     

卢春华  雷晓岚  于小龙  李红梅  刘涛 《探矿工程》2013,40(12):63-67

在深孔、定向孔钻进过程中,对钻孔轨迹的控制十分重要。电磁随钻测量系统能够监测钻孔状态参数并通过无线电磁波实时传输至地面,具有信号传输速率高、不受钻井液影响等优势。详细阐述了一种自主研发的电磁随钻测量系统及试验情况,试验最大孔深为609 m,此时地面接收信号高达200 mV。试验研究表明：该系统性能可靠,完全能够满足随钻测量近钻头处钻孔状态及环空压力、温度等参数的需求。  相似文献   

徐家围子断陷白垩纪火山活动与断裂组合关系     

印长海  董景海 《世界地质》2013,32(4):793-799

本文从断裂组合、火山机构和岩浆通道等方面分析,提出徐家围子断陷基底断裂及与之匹配的次级断裂控制白垩纪火山活动,形成受基底断裂控制的三个 NNW 向展布的火山岩发育带。由于基底断裂特征不同,各火山岩带分别具有中心式、裂隙式和复合式三种不同的喷发特征。徐家围子断陷安达地区精细解剖表明,其基底断裂上部发育 NWW 向雁列式断裂,向下沟通基底断裂,为西部火山岩浆上侵通道,反映了历史时期内火山活动西强东弱的特征,西部火山规模大,以爆发相为主,东部为大面积溢流相。火山岩的分布受基底断裂及沟通其的次级断裂控制,同时对断裂痕迹起到一定的改造作用。  相似文献   

基于年龄测试的黄庄—高丽营断裂活动性研究     

王海刚  贾三满  田芳 《城市地质》2013,8(1):32-34

黄庄—高丽营断裂是北京平原区一条重要的活动断裂,在庙城—高丽营段沿线发生地裂缝,造成大量房屋墙体开裂和道路破坏。在西王路村探槽揭示该断裂错断第四系地层,产生地表地裂缝。探糟断裂孢粉年龄测试,该断裂发生年龄大致在13～22ka,仍处于活动状态。  相似文献   

1997/1998年ENSO过程与热带大气季节内振荡   总被引：3，自引：1，他引：3  

翟盘茂  郭艳君  李晓燕 《热带气象学报》2001,17(1):1-9

根据珠江口气象站风速与潮汐站潮位资料,对1955～1998年12次El Nino过程的珠江口季风强度与海平面变化特点进行合成分析,结果表明,El Nino发生前一年冬季,珠江口冬季平均风速较常年值大0.4 m/s,El Nino发生当年,月平均风速也普遍大于常年,而月平均海平面则普遍较常年偏低,其中10与11月份负距平为6 cm左右。东亚地区的季风异常对珠江口海平面异常有着重大的影响。  相似文献   

Effect of ENSO events on sediment production in a large coastal basin in northern Peru     

Carolien Tote  Gerard Govers  Stijn Van Kerckhoven  Gert Verstraeten  Herman Eerens 《地球表面变化过程与地形》2011,36(13):1776-1788

Although the importance of ENSO on hydrological anomalies has been recognized, variations in sediment fluxes caused by these extreme events are poorly documented. The effect of ENSO is not limited to changes in sediment mobilization. Since ENSO events can affect terrestrial ecosystems, they may have important effects on sediment production and transport in river basins over time spans that are longer than the duration of the event itself. The Catamayo‐Chira basin is an interesting casestudy for investigating these geomorphic implications. The objectives were: (i) to study the effect of ENSO on stream flow and sediment yields in the basin, (ii) to investigate if ENSO events affect sediment yields in the post‐ENSO period and (iii) to understand which factors control the ENSO and post‐ENSO basin response. During strong negative ENSO periods, mean annual stream flow discharge at the inlet of the Poechos reservoir in the lower basin was 5.4 times higher than normal annual discharges, while average sediment fluxes exceeded those of normal years by a factor of about 11. In two heavily affected periods, 45.9% of the total sediment yield in the 29 years observation period was generated. Sediment fluxes in the post‐ENSO period are lower than expected, which proves post‐ENSO event dynamics are significantly different from pre‐event dynamics. Our analysis indicates the increase of vegetation growth in the lower basin is not the main reason explaining considerable sediment flux decrease in post‐ENSO periods. During strong ENSO events, sediment in alluvial stores in the lower part of the basin is removed due to enlarging and deepening of channels. In post‐ENSO periods, normal discharges and persisting sediment supplies from the middle/upper basin lead to river aggradation and storage of large amounts of sediment in alluvial plains. The decrease in sediment export will last for several years until the equilibrium is re‐established. Copyright © 2011 John Wiley & Sons, Ltd.  相似文献   

The peculiar case of the “double-humped” super-luminous supernova SN 2006oz     

Rachid Ouyed  Denis Leahy 《中国天文和天体物理学报》2013,(10):1202-1206

SN 2006oz is a super-luminous supernova with a mysterious bright precursor that has resisted explanation in standard models.However,such a precursor has been predicted in the dual-shock quark nova model of super-luminous supernovae–the precursor is the supernova event while the main light curve of the super-luminous supernova is powered by the Quark-Nova（explosive transition of the neutron star to a quark star）.As the supernova is fading,the Quark-Nova re-energizes the supernova ejecta,producing a＂double-humped＂light curve.We show that the quark nova model successfully reproduces the observed light curve of SN 2006oz.  相似文献   

The timing behavior of magnetar Swift J1822.3—1606： timing noise or a decreasing period derivative？     

Hao Tong  Ren-Xin Xu 《中国天文和天体物理学报》2013,(10):1207-1212

The different timing results of the magnetar Swift J1822.3—1606 are analyzed and understood theoretically.It is noted that different timing solutions are caused not only by timing noise,but also because the period derivative is decreasing after the outburst.Both the decreasing period derivative and the large timing noise may originate from wind braking associated with the magnetar.Future timing of Swift J1822.3—1606 will help clarify whether or not its period derivative is decreasing with time.  相似文献   

SN 2009ip and SN 2010mc as dual-shock Quark-Novae     

Rachid Ouyed  Nico Koning  Denis Leahy 《天体物理学报》2013,(12):1463-1470

In recent years a number of double-humped supernovae （SNe） have been discovered. This is a feature predicted by the dual-shock Quark-Nova （QN） model where an SN explosion is followed （a few days to a few weeks later） by a QN explo- sion. SN 2009ip and SN 2010mc are the best observed examples of double-humped SNe. Here, we show that the dual-shock QN model naturally explains their light curves including the late time emission, which we attribute to the interaction between the mixed SN and QN ejecta and the surrounding circumstellar matter. Our model applies to any star （O-stars, luminous blue variables, Wolf-Rayet stars, etc.） provided that the mass involved in the SN explosion is ~ 20 Mo which provides good conditions for forming a QN.  相似文献   

Geochronological Records of Oil-Gas Accumulations in the Permian Reservoirs of the Northeastern Ordos Basin     

CHEN Gang  YANG Fu  LI Shuheng  ZHANG Huiruo  HU Yanxu  LEI Panpan 《《地质学报》英文版》2013,87(6):1701-1711

Geochronology of oil-gas accumulation （OGA） is a challenging subject of petroleum geology in multi-cycle superimposed basins.By K-Ar dating of authigenic illite （AI） and fluid inclusion （FI） analysis combined with apatite fission track （AFT） thermal modeling,a case study of constraining the OGA times of the Permian reservoirs in northeast Ordos basin （NOB） has been conducted in this paper.AI dating of the Permian oil-gas-bearing sandstone core-samples shows a wide time domain of 178-108 Ma.The distribution of the AI ages presents 2-stage primary OGA processes in the Permian reservoirs,which developed in the time domains of 175-155 Ma and 145-115 Ma with 2-peak ages of 165 Ma and 130 Ma,respectively.The FI temperature peaks of the samples and their projected ages on the AFT thermal path not only present two groups with a low and a high peak temperatures in ranges of 90-78℃ and 125-118℃,respectively corresponding to 2-stage primary OGA processes of 162-153 Ma and 140-128 Ma in the Permian reservoirs,but also appear a medium temperature group with the peak of 98℃ in agreement with a secondary OGA process of c.～30 Ma in the Upper Permian reservoirs.The integrated analysis of the AI and FI ages and the tectono-thermal evolution reveals that the Permian reservoirs in the NOB experienced at least 2-stage primary OGA processes of 165-153 Ma and 140-128 Ma in agreement with the subsidence thermal process of the Mid-Early Jurassic and the tectono-thermal event of the Early Cretaceous.Then,the Upper Permian reservoirs further experienced at least 1-stage secondary OGA process of c.～30 Ma in coincidence with a critical tectonic conversion between the slow and the rapid uplift processes from the Late Cretaceous to Neogene.  相似文献   

蓝色翡翠的呈色机制探讨     

王铎  莫祖荣  李雪明  王洪权 《地质科学译丛》2013,(2):14-17

近期广东市场上出现了一种来自缅甸的蓝色翡翠样品,该样品目前未见相关报道。为了确定其定名,通过常规宝石学测试、红外光谱和X射线粉末衍射测试对样品进行分析,表明样品的主要矿物组成为硬玉,质量分数约97．1％,检测鉴定结论为翡翠。为了对蓝色翡翠呈色机制进行研究,通过紫外一可见吸收光谱测试,表明可见光区480nm以后逐渐增强的吸收带是其产生蓝色的原因;采用电子探针进行化学成分测试,表明蓝色的成因与钒离子有关。根据3d过渡金属离子的晶体场理论和翡翠晶体场理论的研究,可以推测：由于翡翠结构中M1位的Al3＋被过渡金属离子钒（V4＋）替代,目l起八面体结构畸变而导致蓝色的产生,因此,蓝色是过渡金属离子钒（v4＋）产生的原生色。  相似文献