低电阻率油气层的测井系列研究

根据低电阻率油气层的成因,将低电阻率油气层分为四种主要不同的类型,这四种类型的低电阻率油气层除了需要进行常规测井系列外,不同成因的低电阻率油气层应采用不同的新技术测井项目,对于高不动水含量型低阻油气层,将核磁共振测井作为解决这种类型的针对对性测井项目,而MDT测井作为选择性项目;对于粘土附加导电型低阻油气层,将极化率测井作为解决该类低阻问题的针对性测井项目,核磁共振、双频介电、MDT测井作为选择性测井项目;对于砂泥岩间互型低阻油气层,高分辨率感应测井或者阵列侧向测井是解决此类低阻油气层的关键技术;对于盐水泥浆侵入型低阻油气层,可以有针对性的进行过套管电阻率测井,同时在储层物性条件较好时还可以选测C／O或PND测井替代过套管电阻率测井项目,或者根据地面及地下地质情况,选取随钻测井系列.     

支气管囊肿外科治疗36例临床分析

纵隔型支气管囊肿（MBC）是一种先天性支气管囊肿,多发生于中纵隔中上部,发生在后下纵隔相对少见。本文报道1例后下纵隔支气管囊肿患者,19岁,男性,体检发现纵隔占位。CT表现为后下纵隔脊柱旁不规则肿块,密度混杂,边缘及内部可见结节状钙化,增强后未见强化。MRI检查T1WI呈不均匀低信号,T2WI呈高信号,内见条索状、分隔样低信号,增强后延迟期病灶边缘及分隔轻度强化。术后病理诊断：支气管源性囊肿。本文回顾性分析该病例的CT和MRI影像特征,并复习国内外文献,总结后下纵隔不典型支气管囊肿的影像表现,以提高对该疾病的认识。

     

Multiple resonance in one problem of the stability of the motion of a satellite relative to the center of mass

We investigate the stability of the periodic motion of a satellite, a rigid body, relative to the center of mass in a central Newtonian gravitational field in an elliptical orbit. The orbital eccentricity is assumed to be low. In a circular orbit, this periodic motion transforms into the well-known motion called hyperboloidal precession (the symmetry axis of the satellite occupies a fixed position in the plane perpendicular to the radius vector of the center of mass relative to the attractive center and describes a hyperboloidal surface in absolute space, with the satellite rotating around the symmetry axis at a constant angular velocity). We consider the case where the parameters of the problem are close to their values at which a multiple parametric resonance takes place (the frequencies of the small oscillations of the satellite’s symmetry axis are related by several second-order resonance relations). We have found the instability and stability regions in the first (linear) approximation at low eccentricities.     

Secular resonances in the asteroid belt: Theoretical perturbation approach and the problem of their location

In this paper a theoretical perturbation approach to the problem of the dynamics in secular resonance is exposed. This approach avoids any expansion of the main term of the Hamiltonian (linear term in the masses) with respect to the eccentricity or the inclination of the asteroid, in order to achieve results valid for any value of these variables. Moreover suitable action-angle variables are introduced to take properly into account the dynamics related to the motion of the argument of perihelion of the asteroid, which is relevant at high inclination. A class of secular resonances wider than that usually considered is found. An explicit computation of the location of the main secular resonances, estimating also the contribution of the quadratic term in the masses by means of classical series expansion, is reported in the last sections. The accuracy of computations obtained by series expansion is discussed in the paper.     

On one special case of parametric resonance in problems of celestial mechanics

We consider a periodic (in time) linear Hamiltonian system that depends on a small parameter. At a zero value of this parameter, the matrix of the system is constant, has two identical pairs of purely imaginary roots, and is not reducible to diagonal form. Therefore, the unperturbed system is unstable. We propose an algorithm for determining the boundaries of the instability regions for the system at nonzero values of the small parameter. This algorithm was used to analyze the stability of triangular libration points in the elliptical restricted three-body problem and in the stability problem in one special case of stationary rotation of a satellite relative to the center of mass.     

A simple mapping for comets in resonance

The dynamical evolution of a low inclination, intermediate period comet in mean-motion resonance with a giant planet can be described by a simple mapping giving the comet's heliocentric energy and ecliptic longitude at successive aphelia. Provided that the energy oscillations produced by the resonance are not too large, this mapping is linear. When the amplitude of the oscillations is close to the maximum possible within the resonance, the mapping can be improved by adding non-linear terms.     

1950~2011年渤海地区海表风场的季节特征与多尺度变化分析

基于1950~2011年的NCEP/NCAR再分析资料,对渤海10 m风场的风速与风向变化进行多尺度分析。利用小波分析、交叉谱分析等方法对渤海海域的海表风速、风向的变化趋势以及周期进行研究。分析发现：渤海地区海表风的风向与风速除了存在显著的季节性变化特征外,在年际、年代际的变化尺度上也有明显的周期性。风向存在1 a、8.7 a、15.8 a的显著周期,风速存在1 a、6.3 a、15 a的显著周期。风向与风速在时间尺度分别为20 a、5.71 a、2.67 a时存在显著共振周期;共振周期受东亚季风、西太平副热带高压的年际、年代际变化的影响呈现出多尺度变化周期。     

血液流动对MR成像的影响

本文讨论了血液流动对ＭＲ成像的影响。它们是图像为影的来源，在血管造影中，它们用于显示血管和提供关于血液流动速度的信息。流动两个方面的影响敏感，第一质子群的流入和注出。第二流动产生的相位移。本文也介绍了流动补偿技术。     

Study of inorganic ligand-chromium(III)-surface ternary complexes by ESR spectroscopy

Cr(III) sorbed at the solid/water interface of latex and hectorite was studied by ESR spectroscopy in the presence of different inorganic ligands. The ESR spectra of the surface obtained in the presence of selenite, phosphate and fluoride can be explained in terms of ternary surface complex formation. This is contrasted by the behaviour of sulfate and selenate ions which were found to have no effect on the ligand field of Cr(III), either in the adsorbed state or in solution.     

Stability of the triangular libration points of the circular restricted problem in the presence of resonances

The stability of triangular libration points, when the bigger primary is a source of radiation and the smaller primary is an oblate spheroid. has been investigated in the resonance cases ₁ = 2₂ and ₁ = 3₂. The motion is unstable for all the values of parameters q and A when ₁ = 2₂ and the motion is unstable and stable depending upon the values of the parameters q and A when ₁ = 3₂. Here q is the radiation parameter and A is the oblateness parameter.