太原地震台短水准受水位影响分析及异常识别

水位是影响水准高差变化最为显著和普遍的因素,本文研究了晋7-1~#井水位变化对太原地震台水准高差的影响,分析了两者的相关性及年最大变化量的异同情况。结果显示,相关性、年最大变化量比值异常与山西地震带地震有较好对应。     

Models for the X‐ray spectra and variability of luminous accreting black holes

The X‐ray spectra of luminous Seyfert 1 galaxies often appear to be reflection dominated. In a number of Narrow Line Seyfert 1 (NLS1) galaxies and galactic black holes in the very high state, the variability of the continuum and of the iron line are decoupled, the reflected component being often much less variable than the continuum. These properties have been interpreted as effects of gravitational light bending. In this framework, we present detailed Monte‐Carlo simulations of the reflection continuum in the Kerr metric. These calculations confirm that the spectra and variability behaviour of these sources can be reproduced by the light bending model. As an alternative to the light bending model, we show that similar observational properties are expected from radiation pressure dominated discs subject to violent clumping instabilities and, as a result, have a highly inhomogeneous two‐phase structure. In this model, most of the observed spectral and variability features originate from the complex geometrical structure of the inner regions of near‐Eddington accretion flows and are therefore a signature of accretion physics rather than general relativity. (© 2006 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

青藏块体强震与祁连山地震带中强震相关性的初步探讨

对青藏块体强震与祁连山地震带中强震的相关性进行了初步分析。结果表明：青藏块体发生强地震后,祁连山地震带中强地震活动具有增强趋势。通过分析认为,祁连山地震带已进入新的地震活跃期,并有可能发生7级以上地震。     

相对论效应及其对GPS技术的影响

本文根据相对论基本原理,系统地阐述了GPS中必须仔细考虑的几项主要的相对论效应,包括运动时钟的时间膨胀、引力频移以及地球自转引起的Sagnac效应等,并对相对论效应在GPS中的实际应用进行了定量分析和讨论。     

工程化广播星历参数拟合算法与接口设计

对导航卫星广播星历参数拟合算法和接口设计问题进行了研究。通过条件数、参数相关性分析,指出小倾角问题是造成GPS开普勒轨道根数广播星历拟合算法不能适用于GEO卫星的最主要原因;通过分析定轨理论和拟合实例证明,GEO卫星星历参数Crc、Crs超限的主要原因是由于其轨道特性决定的;针对GEO卫星星历参数拟合法方程严重病态的问题,提出了动态加权的带参数约束条件平差算法。该方法能有效稳定星历拟合结果,解决Δn等星历参数超限的问题。     

时间、距离、速度、红移基本物理概念的演变简史

为了尝试回答“我们能否观测到退行速度超过光速的星系”这一问题,重新考察了在牛顿物理学、狭义相对论、广义相对论和宇宙学中的时伺、距离、速度和红移等概念．揭开了一些错误观念的实质,发现只要摆脱狭义相对论先入为主的束缚,上述问题即可迎刃而解．强调了宇宙学并不是纯粹的广义相对论,而是该理论在服从宇宙学原理的条件下的一个特例,其中一系列基本物理概念都因此得到新的内涵。     

渤海海域变质岩风化壳发育特征及其储层定量预测

随着渤海油田锦州25-1南、锦州20-2以及渤中26-2等风化壳型油气田的相继发现,以及近两年渤中19-6千亿方大气田的重大勘探突破,元古—太古宇变质岩逐步成为渤海海域潜山勘探层系的重点之一。为了研究渤海变质岩潜山风化壳的发育特征并建立其储层预测方法,通过对典型潜山取心、薄片、测井、常量元素以及物性资料分析,划分了变质岩潜山的风化壳纵向结构,明确了风化壳发育差异的控制因素,并以5项因素灰关联系数为介质,采用Q型聚类法对储层级别进行了优劣排序。研究结果表明：变质岩风化壳可以划分为5个纵向结构,其发育程度明显受岩性、构造和保存条件等因素的影响,其中,被前人忽视的上覆沉积环境作为风化壳的保存条件意义重大。对11口已钻井风化壳进行变量因子归类,由好到差划分了Ⅰ—Ⅳ 4个储层级别。利用该方法在渤中19-6风化壳预测中的应用效果较好。     

Resonance behaviour and partial averaging in a three-body system with gravitational radiation damping

In a previous investigation, a model of three-body motion was developed which included the effects of gravitational radiation reaction. The aim was to describe the motion of a relativistic binary pulsar that is perturbed by a third mass and look for resonances between the binary and third-mass orbits. Numerical integration of an equation of relative motion that approximates the binary gives evidence of such resonances. These ( m : n ) resonances are defined for the present purposes by the resonance condition,   m ω= 2 n Ω  , where m and n are relatively prime integers and ω and Ω are the angular frequencies of the binary orbit and third-mass orbit (around the centre of mass of the binary), respectively. The resonance condition consequently fixes a value for the semimajor axis a of the binary orbit for the duration of the resonance because of the Kepler relationship  ω= a ^−3/2  . This paper outlines a method of averaging developed by Chicone, Mashhoon and Retzloff, which renders a non-linear system that undergoes resonance capture into a mathematically amenable form. This method is applied to the present system and one arrives at an analytical solution that describes the average motion during resonance. Furthermore, prominent features of the full non-linear system, such as the frequency of oscillation and antidamping, accord with their analytically derived formulae.     

兰州市城市热岛效应评价与灰色预测

利用兰州市及其郊区（永登、榆中、皋兰3县）1958—2004年气象观测资料分析了兰州市热岛强度的年变化规律,结果表明,1975年以后,兰州市城市热岛效应呈上升趋势,但热岛强度整体保持在3.0 ℃以下;1981—1998年平均热岛强度为3.30 ℃,1990年以后城郊热岛强度增加到3.6 ℃以上;1996年达到最高为4.25 ℃;根据兰州市社会发展状况及前人的研究结果,分别分析了兰州市城市热岛强度在1971—1980年、1990—1995年和1997—2003年3个时段的季节变化规律,未来兰州夏季热岛效应将会排在第一位。运用灰色关联度分析法对影响兰州市城市热岛效应的因子群进行了贡献测度分析,结果表明,人为热释放是造成兰州市城市热岛效应的关键因素;风速、总云量是影响兰州市城市热岛效应的主要气象因子。最后通过改进GM(1,1)模型的拟合与预测,结果与实际情况具有良好一致性,表明兰州市城市热岛效应有进一步加重的趋势。