The pattern speed of the bar in NGC 4596

The pattern speed is a defining parameter of any barred galaxy. A large number of model-dependent techniques have therefore been developed to derive the pattern speed. However, the only model-independent technique for measuring this quantity – the Tremaine–Weinberg method – has hitherto been applied to just one case, the SB0 galaxy NGC 936. In this paper, we apply the technique to a second system, the SBa galaxy NGC 4596. The resulting estimate for the pattern speed is Ω_p=52±13 km s⁻¹ kpc⁻¹. This result is corroborated by a spectrum obtained along the major axis of the bar in this system. The corotation radius associated with this pattern speed lies just beyond the end of the bar indicating a fast bar. Combining the bar major-axis spectra with data obtained from a Hubble Space Telescope WFPC2 image, we also find strong evidence for a nuclear disc.     

Kalman滤波方法在黑河出山径流年平均流量预报中的应用

应用Kalman滤波方法,以流域平均降水量、气温、太阳黑子相对数及莺落峡站6年显著周期序列等为控制参数,对黑河出山径流年平均流量的预测问题进行了初步研究和探讨。     

A partial susceptibility approach to analysing the magnetic properties of environmental materials: a case study

An approach to expressing the magnetic properties of environmental materials in terms of the contributions of the magnetic susceptibilities of specific magnetic components is reported. The approach links the partial susceptibilities of discrete particles, domains or mineral fractions with the concentration-dependent parameters by means of multiple linear regression methods. The case study, using the Liverpool street dust data set, demonstrates that the technique is able to model the contributions of the main magnetic components satisfactorily. Several factors may have a significant impact on the regression results. These include the validity of the linear proportional relationships between partial susceptibilities and the relevant concentration-dependent parameters, the adequacy of the variable selection procedure and the regression model, and the suitability of certain magnetic parameters.     

区域降水分布定量测量及其在IMGRASS综合试验中的应用方案研究

在综合分析现有地基测量降水时空分布方法及设备条件的基础上,我们选择了雷达－雨量计联合测雨及雷达－辐射计联合遥感降水分布方法作为ＩＭＧＲＡＳＳ综合试验中的降水测量方案。除了介绍方法的原理、探测方案外,还讨论了误差来源及改进措施。     

中国南海东部海域气候特征及风浪流极值参数的研究——LAGFD数值模式群的应用

本文采用先进的ＬＡＧＦＤ风、浪数值模式和ＰＯＭ（ＰｒｉｎｃｅｔｏｎＯｃｅａｎＭｏｄｅｌ）三维海流模式对自１９４５～１９９５年间发生并影响南海东部海域的２９９个历史最强热带气旋过程进行数值后报,给出了南海东部部分海域（１９°～２３°Ｎ,１１３°～１１８°Ｅ）中１０００ｍ等深线内６０个点的多年一遇风、浪、流和水位极值,并简要分析了南海东部（１５°～２７°Ｎ,１０８°～１２２°Ｅ）的气候特征,为该海域区域性海洋环境研究与工程开发提供了基础参考数据。     

南京地区雨滴谱参数的详细统计分析及其在天气雷达探测中的应用

雨滴谱包含了降雨的丰富信息,不仅能反映雨滴群的微物理特性,也能反映降雨类型、降雨强度等宏观特性,并且在雷达气象领域也有重要的价值。论文对2015和2016年度南京地区32次降雨过程的雨滴谱资料进行了处理、并对多种雨滴参数进行了详细的统计和分析,拟合了层状云降雨、对流云降雨以及积层混合云降雨的雨滴谱Gamma分布参数。另外,还基于雨滴谱数据拟合了雷达反射率因子Z与降雨强度R的Z-R关系,计算了差分反射率Z_DR、相位常数K_DP以及衰减参数,并利用衰减参数进行了C波段雷达回波的衰减订正试验。结果表明:（1）层状云降雨的各微物理参数比较稳定,积雨云的变化剧烈;层云降雨和积层混合云降雨的中雨滴、积雨云降雨的大雨滴对雷达反射率因子的贡献最大。（2）积雨云降雨的滴谱最宽,层状云降雨的最窄。（3）利用依据雨滴谱数据拟合的三类降雨Z-R关系,可以一定程度地提高雷达估测降雨的精度。（4）利用基于雨滴谱数据拟合的衰减系数,有效地进行了C波段双偏振雷达回波强度的衰减订正,体现了统计参数和拟合参数准确性。     

A mass ratio limit for primordial black holes

We augment our scenario for the formation of astronomical objects from macroscopic superstrings by the assumption that the central matter keeps its identity in the fragmentation. From the condition that the angular momentum per mass squared of this matter should be less than the Kerr limit G/c, we obtain upper limits for the ratio of the mass of central black holes M(BH) to the mass M of the host object. This limit is M(BH)/M ≈ 0.001, and, expressed in observed quantities, approximately M(BH)/M ≈ σ²/(v · c) where σ is the r.m.s. velocity, v the rotational velocity and c the velocity of light. The valuesM(BH) agree with the observed behaviour both in order of magnitude and in the variation with velocity dispersion. (© 2003 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

用连续小波变换分析探地雷达回波信号

脉冲探地雷达回波信号是典型的非平稳、非线性信号.本文通过连续小波变换,对地下圆柱目标实测结果进行分析,得到了目标冲击响应的典型波形特征.分析结果证明,这种方法可以有效地用于目标检测,时延估计等脉冲探地雷达信号处理中的关键问题     

钻孔地质雷达工作原理及应用

阐述了钻孔雷达的工作原理,介绍了单孔反射和跨孔层析成像2 种工作方式,并将其用于深部岩层岩性评价和地质异常体探测,效果显着