重力方法研究河南区域构造及控煤作用     

管忠民 《中国煤田地质》2007,19(5):62-64

河南地区存在三个明显的重力异常区,与其区内三个次一级的构造分区相一致,其重力异常曲线的挤压扭曲特征、剪切平移特征、张性舒展特征分别对应构造挤压变形机制、平移剪切机制及变形拉张机制。这些变形受印支、燕山及喜马拉雅期三大构造运动控制,其中印支期剥蚀及沉降程度是构成现今煤层埋藏条件的重要因素,燕山期形成河南煤田的逆冲推覆型控煤构造,喜马拉雅期构造运动,最终确立了河南煤系的展布范围及赋存状态,这表明控煤模式是构造运动的结果。  相似文献   

天津滨海新区地面沉降预测方法研究   总被引：3，自引：2，他引：1  

张风霜  薄万举  陈聚忠  宋雯 《上海国土资源》2010,31(4):43-47,86

利用1985～2008年天津地面沉降监测资料,以水准监测点为基本研究对象,在分析其时间沉降的变化动态基础上,采用分段权函数线性模型提取沉降信息并进行外推预测,展示了天津滨海新区地面沉降现状,编绘了2008年天津滨海新区地面沉降年度沉降分布图和2008～2013年间地面沉降总量的预测分布图研究成果可供政府及有关部门制定和实施控沉管理决策参考,同时对存在类似问题的区域也有一定的参考价值。  相似文献   

3. Solar System Formation and Early Evolution: the First 100 Million Years     

Thierry Montmerle  Jean-Charles Augereau  Marc Chaussidon  Mathieu Gounelle  Bernard Marty  Alessandro Morbidelli 《Earth, Moon, and Planets》2006,98(1-4):39-95

The solar system, as we know it today, is about 4.5 billion years old. It is widely believed that it was essentially completed 100 million years after the formation of the Sun, which itself took less than 1 million years, although the exact chronology remains highly uncertain. For instance: which, of the giant planets or the terrestrial planets, formed first, and how? How did they acquire their mass? What was the early evolution of the “primitive solar nebula” (solar nebula for short)? What is its relation with the circumstellar disks that are ubiquitous around young low-mass stars today? Is it possible to define a “time zero” (t ₀), the epoch of the formation of the solar system? Is the solar system exceptional or common? This astronomical chapter focuses on the early stages, which determine in large part the subsequent evolution of the proto-solar system. This evolution is logarithmic, being very fast initially, then gradually slowing down. The chapter is thus divided in three parts: (1) The first million years: the stellar era. The dominant phase is the formation of the Sun in a stellar cluster, via accretion of material from a circumstellar disk, itself fed by a progressively vanishing circumstellar envelope. (2) The first 10 million years: the disk era. The dominant phase is the evolution and progressive disappearance of circumstellar disks around evolved young stars; planets will start to form at this stage. Important constraints on the solar nebula and on planet formation are drawn from the most primitive objects in the solar system, i.e., meteorites. (3) The first 100 million years: the “telluric” era. This phase is dominated by terrestrial (rocky) planet formation and differentiation, and the appearance of oceans and atmospheres.  相似文献   

Reflection effect in close binaries. II. Distribution of emergent radiation from the irradiated component along the line of sight     

A. Peraiah 《Journal of Astrophysics and Astronomy》1983,4(1):11-17

We have calculated the effects of irradiation from a point source observed at infinity. Plane-parallel approximation and spherically-symmetric approximations are employed in calculating the self-radiation field for the sake of comparison. It is found that there are considerable changes in the radiation received at infinity between the approximation of plane-parallel stratification and spherical symmetry.  相似文献   

Radiation-induced defects in quartz. III. Single-crystal EPR,ENDOR and ESEEM study of a peroxy radical     

Mark J. Nilges  Yuanming Pan  Rudolf I. Mashkovtsev 《Physics and Chemistry of Minerals》2009,36(2):61-73

The X- and W-band single-crystal electron paramagnetic resonance spectra of an electron-irradiated natural quartz permit quantitative analysis of a ²⁹Si hyperfine structure (A ~12.6 MHz) and an ²⁷Al hyperfine structure (A ≤ 0.8 MHz) for a previously reported hole-like center. The ²⁹Si hyperfine structure arises from interaction with two equivalent Si atoms and is characterized by the direction of the unique A axis close to a Si–O bond direction. The ²⁷Al hyperfine structure, confirmed by pulsed electron nuclear double resonance and electron spin echo envelope modulation spectra, is characterized by the unique A axis approximately along a twofold symmetry axis. These ²⁹Si and ²⁷Al hyperfine data, together with published theoretical results on peroxy radicals in SiO₂ as well as our own density functional theory (DFT) calculations on model peroxy centers, suggest this hole-like center to have the unpaired spin on a pair of oxygen atoms linked to two symmetrically equivalent Si atoms and a substitutional Al³⁺ ion across the c-axis channel, a first peroxy radical in quartz. The nuclear quadrupole matrix P also suggests that the Al³⁺ ion corresponds closely to the diamagnetic precursor to the [AlO₄]⁰ center. Electronic supplementary material  The online version of this article (doi:) contains supplementary material, which is available to authorized users.  相似文献   

含铁绿柱石的改色机制研究   总被引：7，自引：0，他引：7  

李湘祁  袁奎荣 《矿物岩石》1999,19(4):1-4

含铁绿柱石经γ射线辐照或特定温度热处理,可因铁价态的改变引起颜色发生相应变化。处理前后的吸收光谱和顺磁共振谱研究表明,辐作用使隧道位的Ｆｅ＾２＋氧化Ｆｅ％３＋,八一位上的Ｆｅ＾３＋还原为Ｆｅ＾２＋,热处理使隧道位及八面体位Ｆｅ＾３＋均还原为Ｆｅ＾２＋。  相似文献   

紫外线诱导太平洋牡蛎雄核发育的研究   总被引：2，自引：1，他引：1  

袁媛  李琪  于瑞海  于红 《中国海洋大学学报(自然科学版)》2005,35(1):29-32

为诱导太平洋牡蛎雄核发育单倍体 ,本文研究利用紫外线诱导太平洋牡蛎雄核发育的条件。结果表明 :在强度为2 .8mW·cm-2 ·s-1的紫外线 (2 5 4nm)下分别照射 0 ,10 ,15 ,2 0 ,2 5 ,3 0 ,3 5 ,40 ,5 0 ,60 ,70和 80s后 ,照射 3 0s的卵子能够保持较高的受精率 (73 .5 % ) ;该处理组的D形幼虫发生率为 0。染色体检查结果显示此时单倍体率最高 (4 7.8% )。证明在强度为2 .8mW·cm-2 ·s-1的紫外线下照射 3 0s是获得雄核发育单倍体的适宜条件。研究还表明受精率和D形幼虫发生率随照射时间的增加而下降 ,遗传失活的卵子与正常精子受精后其胚胎发育至D形幼虫前期停止。实验中各处理组均出现非整倍体。原因可能由于紫外线对卵子染色体遗传失活的作用程度不同以及光线对DNA的修复作用。  相似文献   

Photoinduced Reductive Decomposition of Perflurooctanoic Acid in Water: Effect of Temperature and Ionic Strength          下载免费PDF全文

Chaojie Zhang  Yan Qu  Xiaoyun Zhao  Qi Zhou 《洁净——土壤、空气、水》2015,43(2):223-228

  相似文献   

超声激励低渗煤层甲烷增透机理   总被引：3，自引：0，他引：3       下载免费PDF全文

肖晓春  潘一山  吕祥锋  杨新乐 《地球物理学报》2013,56(5):1726-1733

超声激励增透煤层是一种不受甲烷储层地质条件和气源特性限制,具有普遍应用价值的增采技术.但由于煤岩致密、裂隙发育,煤岩孔隙度存在多尺度效应,受储层介质尺度效应影响的增透促吸机理尚不明确.本文通过CT观测实验和渗透率测定实验,对超声波作用下煤样不同尺度裂隙发展规律进行了分析,对比测定超声作用煤样渗透率变化规律,建立了超声增透煤层甲烷渗透率的修正公式.研究结果表明:CT观测实验很好地证明了超声的机械震碎作用;在声场衰减范围内,煤体损伤和机械震碎作用明显;超声波作用后的煤层渗透率有平均135%～169%的提高.研究工作为超声激励增加煤层的渗透率提供了实验基础.  相似文献   

积水沉陷区水体的表观光学特性参数测量与分析     

朱继文  孟祥来  张贺 《地理空间信息》2011,9(3):6-8

通过实际测量试验区的积水沉陷区水深值,了解水体光学特性随水深不同而引起的衰减特征变化,建立水深与光谱特性响应间的关系表达式,确定获取水深信息的最佳波谱范围;揭示了叶绿素、悬浮物质、CDOM等水体组分与水体光谱特征变化的关系,探讨因水体各主要组分变化而引起的水体光谱吸收光谱、散射光谱的变化规律.  相似文献