SS-Y型伸缩仪气压扰动影响的特征分析与数学改正

收集、整理淮北台数字化SS-Y型伸缩仪观测资料,根据SS-Y型伸缩仪工作原理,分析气压因素对其观测资料的影响。结果表明,气压变化对观测数据有明显的干扰,且二者呈正相关关系。最后通过量化分析,建立淮北台SS-Y型伸缩仪观测值的气压改正数学解析式,能够对该气压效应进行有效改正。     

主成分分析法在林甸Ms5．1地震回顾性预测中的应用

用2005年林甸Ms5．1级地震前后震中附近的地震资料,选择与地震强度有关的3级以上地震频次N、b值、Mf值、C值、和Ac值等6个参量进行主成分分析,实现对上述参量的有效约简。这6个参量之间有一定的相关性,各参量在不同时段的变化各有所异,预报效果并不理想。但是根据主成分分析可以得到反映地震强度的综合指标W,发现该指标在震源区附近出现明显的异常变化,震后异常恢复。表明综合指标W可以较好的反映地震活动的异常特征。     

Boltzmann方程的矩形式及旋转慢收缩中子星中心附近的温度特性

推出中子星在旋转慢塌缩情况下零质量粒子的Ｂｏｌｔｚｍａｎｎ方程及其矩形式,并研究了典型条件下的慢坍缩问题,而且在近热平衡及扩散近似下得到一个可直接研究中子星中心附近温度特性的有用方程：ａＴｃ＾４ｃ－ａＴ＾４＝ｒＨ３０（６Ｎ＾ΦＯ／Ｎｏｅ－ＮｏА＾－１３ｔｓｉｎθ。     

Effects of Kerr space–time on spectral features from X-ray illuminated accretion discs

We performed detailed calculations of the relativistic effects acting on both the reflection continuum and the iron line from accretion discs around rotating black holes. Fully relativistic transfer of both illuminating and reprocessed photons has been considered in Kerr space–time. We calculated overall spectra, line profiles and integral quantities, and present their dependences on the black hole angular momentum. We show that the observed EW of the lines is substantially enlarged when the black hole rotates rapidly and/or the source of illumination is near above the hole. Therefore, such calculations provide a way to distinguish between different models of the central source.     

Non-linear hydrodynamical evolution of rotating relativistic stars: numerical methods and code tests

We present numerical hydrodynamical evolutions of rapidly rotating relativistic stars, using an axisymmetric, non-linear relativistic hydrodynamics code. We use four different high-resolution shock-capturing (HRSC) finite-difference schemes (based on approximate Riemann solvers) and compare their accuracy in preserving uniformly rotating stationary initial configurations in long-term evolutions. Among these four schemes, we find that the third-order piecewise parabolic method scheme is superior in maintaining the initial rotation law in long-term evolutions, especially near the surface of the star. It is further shown that HRSC schemes are suitable for the evolution of perturbed neutron stars and for the accurate identification (via Fourier transforms) of normal modes of oscillation. This is demonstrated for radial and quadrupolar pulsations in the non-rotating limit, where we find good agreement with frequencies obtained with a linear perturbation code. The code can be used for studying small-amplitude or non-linear pulsations of differentially rotating neutron stars, while our present results serve as testbed computations for three-dimensional general-relativistic evolution codes.     

Radiating gravitational collapse with shear viscosity

A model is proposed of a collapsing radiating star consisting of an isotropic fluid with shear viscosity undergoing radial heat flow with outgoing radiation. The pressure of the star, at the beginning of the collapse, is isotropic but owing to the presence of the shear viscosity the pressure becomes more and more anisotropic. The behaviour of the density, pressure, mass, luminosity and the effective adiabatic index is analysed. Our work is compared to the case of a collapsing shearing fluid of a previous model, for a star with 6 M_⊙.     

云南强对流暴雨的闪电和雷达回波特征及相关性

利用闪电监测资料和多普勒天气雷达探测资料,对2007年汛期强对流暴雨的闪电和雷达回波特征及相关性进行分析,结果表明:云南大多数暴雨属于强对流性暴雨,而且以负闪电为主,负闪电占总闪电的90 %以上;暴雨日降水量与日闪电数相关小,强的降水不一定有强的闪电活动,但大的日闪频数一般对应的暴雨日降水量大;伴随有闪电活动的强对流暴...     

安达曼弧与缅甸、云南强震相关性研究

研究区包括安达曼弧、缅甸平原和云南地区三个部分。对安达曼弧7级以上地震与缅甸、云南7级和6.8级地震的群体与个体的相关特征进行了研究,发现安达曼弧、缅甸平原M≥7.0地震与云南M≥6.8地震在群体上有一定相关性,但并非一一相关。云南有4个地震活跃期,但安达曼弧与缅甸平原却只有3个,缺失第3活跃期。研究区强震活动从板缘向板内逐渐减弱,三个地区最大震级分别为8.7级、7.8级和7.7级。安达曼弧与缅甸、云南7级地震的个体相关概率分别为33%和27%,平均30%左右,缅甸与云南的个体相关概率为43%。最后对云南的地震趋势进行了预测。     

云南高原楚雄市热岛效应因子的灰色分析

采用云南高原楚雄市和其郊区南华气象观测站近30年的温度差值作为衡量热岛效应的标准,并合理选取楚雄市8项综合指标作为城市热岛效应因子,运用灰色关联度分析法对影响楚雄城市热岛效应的因子群进行了贡献关联度分析.结果表明:人口密度和耗电量是造成城市热岛效应的主要人为因子,风速和日照时数是影响城市热岛效应的主要气象因子.灰色系统协调预测模型的拟合和预测表明楚雄城市热岛效应今后5年有增强的趋势.     

苏北地区代表性森林土壤理化特性的比较研究

在苏北地区5种代表性森林植被下设置样地,进行植被因子调查及土壤理化特性分析。结果表明:不同植被类型林下土壤硬度的平均值变化范围在11.86(±3.59)~18.57(±10.26)kg/cm2、土壤有机质平均含量为1.89(±0.27)%~2.36(±0.08)%;常绿针叶林下土壤的平均容重、粘粒组成、田间持水量等指标均小于落叶阔叶林,并且该林下样地的土壤养分含量及pH值也低于落叶阔叶林下的土壤;常绿针叶林下土壤通透性及保肥能力较好,落叶阔叶林尤其是刺槐(Robinia pseudoacacia)林下土壤有机质、氮、磷等养分含量相对较高,供肥能力较强。