辉绿岩裂缝对其磁组构的影响          下载免费PDF全文

石林权  沈忠悦  潘小青  李明月  张志亮 《高校地质学报》2015,21(2):223

磁组构是由岩石中磁性矿物定向分布而产生的组构特征,因此磁组构分析是研究岩石组构常用的技术手段,它具有 见效快、灵敏度高、无损样品等特点,近年来得到广泛应用。然而在磁组构研究工作中钻取定向样品或定向手标本时,常 常会遇到天然样品含有裂缝且裂缝中充填大量近地表沉积物和自生矿物。本文针对辉绿岩裂缝充填物对其磁组构结果的影 响程度做了详细研究,选用160个含裂缝的辉绿岩岩芯定向样品,通过对比去除裂缝充填物前后的磁组构变化,发现实验 前后所有样品磁化率大小变化率平均值<1%,磁组构方向变化平均值<1°,因此认为辉绿岩裂缝物质对其磁组构影响甚微。 矿物学和岩石磁学分析表明裂隙充填物主要为石英、长石,以及少量赤铁矿、黄铁矿和绿泥石等表生矿物。而辉绿岩的携 磁矿物主要是亚铁磁性的磁铁矿,其磁化率强度约为同等质量裂缝填充物的30倍,致使辉绿岩中的裂隙充填物对磁组构的 影响很小。  相似文献   

Excel 在坐标法测设曲线中的应用     

王政  杨波  李翼龙 《测绘与空间地理信息》2015,(8):198-201

利用Excel软件计算带有缓和曲线的圆曲线放样数据,可有效解决坐标的计算问题,提高内业工作效率,并提出坐标法测设曲线的方法,分析了在不同的情况下,如何选择合适的坐标放样方法保证曲线测设的精度。  相似文献   

极地海区等距离正圆柱投影平面上等角航线的展绘方法   总被引：1，自引：0，他引：1  

张志衡  彭认灿  董箭  褚永磊 《测绘科学技术学报》2015,(5)

墨卡托投影由于其纬度渐长的特性导致在极地海区投影存在严重的长度变形,无法在南北纬80°以外高纬度海区航海图中较好地应用。将长度变形程度明显低于墨卡托投影的等距离正圆柱投影作为极地海区的海图投影,研究了该投影平面中等角航线在极地海区的展绘方法。建立了等距离正圆柱投影平面上等角航线方程并对其曲率进行了分析,推导了绘制一般曲线形态的"以直代曲"公式;最后提出了一种可满足给定精度要求的等角航线展绘算法。实验结果表明:该算法简单易行,可在海图编绘规范规定的误差范围内,实现等角航线的精确展绘。  相似文献   

Kinematic classification of non-interacting spiral galaxies     

《New Astronomy》2014

  相似文献   

Radial velocity studies of HeII and Hβ emission from cataclysmic variables     

《New Astronomy》2014

  相似文献   

Getting SMARTS on Novae: Highlights of the Early Evolution of Nova V475 Sct     

Guy S. Stringfellow  Frederich M. Walter 《Astrophysics and Space Science》2006,304(1-4):401-403

There is a disconcerting global trend of retiring telescopes of modest aperture, supplanting them instead with fewer expensive telescopes of quite large aperture. As a consequence, the available time and feasibility of following transient objects in astrophysics is diminishing. We show the utility of having a suite of small to moderate aperture telescopes capable of conducting imaging and spectroscopic observations in a service queue mode. The example we provide is the high-cadence early observations of the classical nova V475 Scuti (2003) carried out with the SMARTS suite of telescopes located at CTIO.  相似文献   

Stability Regions and Quasi-Periodic Motion in the Vicinity of Triangular Equilibrium Points     

O. Ragos  K. E. Papadakis  C. G. Zagouras 《Celestial Mechanics and Dynamical Astronomy》1997,67(4):251-274

The regions of quasi-periodic motion around non-symmetric periodic orbits in the vicinity of the triangular equilibrium points are studied numerically. First, for a value of the mass parameter less than Routh's critical value, the stability regions determined by quasi-periodic motion are examined around the existing families of short (L^s ₄) and long (L^l ₄) period solutions. Then, for two values of μ greater than the Routh value, the unified family L^sl ₄, to which, in these cases, L^s ₄ and L^l ₄ merge, is considered. It is found that such regions surround in general the linearly stable segments of the corresponding families and become smaller as the mass ratio increases. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

球面线要素的多分辨率实时简化方法   总被引：1，自引：0，他引：1  

王志鹏  ZHAO Xue-sheng  胡婷婷 《地理信息世界》2008,6(2):65-69

在分析球面3维数据可视化特点的基础上,提出了视点相关的球面矢量数据LOD简化方法,基本原理是:以视点为基础在屏幕空间获取投影误差,反投影到模型空间得到动态简化阈值,并结合Douglas-Peucker算法,对矢量数据进行多分辨率实时简化表达.最后,开发实验系统并对相关方法进行了验证.结果表明:在不影响球面图形可视化效果下,数据量减少了约4～5倍,有效地提高了图形渲染速度和效率.  相似文献   

Invariant rotational curves in Sitnikov's Problem     

J. Martínez Alfaro  Cristina Chiralt 《Celestial Mechanics and Dynamical Astronomy》1993,55(4):351-367

The Sitnikov's Problem is a Restricted Three-Body Problem of Celestial Mechanics depending on a parameter, the eccentricity,e. The Hamiltonian,H(z, v, t, e), does not depend ont ife=0 and we have an integrable system; ife is small the KAM Theory proves the existence of invariant rotational curves, IRC. For larger eccentricities, we show that there exist two complementary sequences of intervals of values ofe that accumulate to the maximum admissible value of the eccentricity, 1, and such that, for one of the sequences IRC around a fixed point persist. Moreover, they shrink to the planez=0 ase tends to 1.  相似文献   

A study on the bio-hydro mechanical effects of the tree roots on the Agaclı coal reclaimed – forested land     

Dr.?Nuray?Tokg?zEmail author 《Geotechnical and Geological Engineering》2005,23(5):519-535

The research area that is in the north of Istanbul (Turkey) and it is a land of open pit coal mining residuals reclaimed and turned to forest in 1988–1989. The materials that are open pit mine spoils are formed by sandy loam, sandy clay loam, heavy loam and clay (noncalcareous Pliocene I sediments). Pseudoacacia (Robinia pseudoacacia), Maritima Pine (Pinus pinaster) and Stone Pine (Pinus pinea) are planted on these materials. The aims of this research were to determine the strength of the material provided by tree roots and evaluate the performance of the forestation practices at lands especially where open pit coal mining spoil (residual) materials piled up. The research has been performed at two stages. The first one was hydro-mechanical effect concerned about material moisture depletion as a result of transpiration and the second one was bio-mechanical effects due to strength parameters of the roots and their growth pattern within the material. All results were evaluated in relation to tensile strength and displacement curves due to pre and post failure behaviors of materials and root systems. The results showed the increase of the displacement of the material was the significant indicator of the bio-mechanics tensile strength of the material provided by the tree roots. The fast growing type of tree roots have stabilized the material up to a depth for 80–100 cm by covering the coal residual materials within 12 years.  相似文献