Analysis on the stability of triangular points in the perturbed photogravitational restricted three-body problem with variable masses

This paper examines the effect of a constant κ of a particular integral of the Gylden-Meshcherskii problem on the stability of the triangular points in the restricted three-body problem under the influence of small perturbations in the Coriolis and centrifugal forces, together with the effects of radiation pressure of the bigger primary, when the masses of the primaries vary in accordance with the unified Meshcherskii law. The triangular points of the autonomized system are found to be conditionally stable due to κ. We observed further that the stabilizing or destabilizing tendency of the Coriolis and centrifugal forces is controlled by κ, while the destabilizing effects of the radiation pressure remain unchanged but can be made strong or weak due to κ. The condition that the region of stability is increasing, decreasing or does not exist depend on this constant. The motion around the triangular points L _4,5 varying with time is studied using the Lyapunov Characteristic Numbers, and are found to be generally unstable.     

On the supernova remnants with flat radio spectra

A considerable fraction of Galactic supernova remnants (SNRs) characterize flat spectral indices (α<0.5). There are several explanations of the flat radio spectra of SNRs in the present literature. The most of models involve a significant contribution of the second-order Fermi mechanism but some of them also discuss high compressions (>4), contribution of secondary electrons left over from the decay of charged pions, as well as the possibility of thermal contamination. In the case of expansion in high density environment, intrinsic thermal bremsstrahlung could theoretically shape the radio spectrum of an SNR and also account for observable curved—“concave up” radio spectra of some Galactic SNRs. This model could also shed a light on the question of flat spectral indices determined in some Galactic SNRs. On the other hand, present knowledge of the radio continuum spectra (integrated flux densities at different frequencies) of SNRs prevent definite conclusions about the significance of proposed models so the question on flat spectral indices still remains open. New observations, especially at high radio continuum frequencies, are expected to solve these questions in the near future. Finally, as there is a significant connection between the majority of Galactic SNRs with flat integrated radio spectrum and their detection in γ-rays as well as detection of radiative recombination continua in their X-ray spectra, the analysis of high energy properties of these SNRs is very important.     

单站地基GPS实时估计电波折射弯曲角

提出了利用单站地基GPS多普勒频移实时估计弯曲角的方法,该方法克服了探空法和模型法的局限,可以全天候观测,适合于实时应用。实验结果显示,GPS结果与探空结果具有较好的一致性,且在低仰角范围内优于模型结果。     

Inversion problem in regional electromagnetic induction studies

For completeness of the theory proposed by Oni (1972), the inversion problem is examined. It is shown that parameters which constrain distinct solutions of the inverse problem can be determined in the application of the theory. The fundamental basis of the inversion and the strategy to be adopted are discussed.     

Accuracy improvement of zenith tropospheric delay estimation based on GPS precise point positioning algorithm

In the precise point positioning(PPP),some impossible accurately simulated systematic errors still remained in the GPS observations and will inevitably degrade the precision of zenith tropospheric delay(ZTD) estimation.The stochastic models used in the GPS PPP mode are compared.In this paper,the research results show that the precision of PPP-derived ZTD can be obviously improved through selecting a suitable stochastic model for GPS measurements.Low-elevation observations can cover more troposphere informat...     

互相关干扰下微弱GPS信号的直接检测算法

微弱GPS信号的检测是当前的研究热点之一。基于GPS C/A码的互相关干扰理论模型,详细分析研究了强弱信号间的相对载波多普勒频移对互相关干扰的影响,在此基础上,研究了一种新的基于相对载波多普勒频移的微弱GPS信号直接检测算法,该算法不需要对互相干扰进行扣除,计算量小、便于工程实现,仿真结果表明:当干扰信号高出弱信号29dB时,该算法依然可以达到90%以上的检测成功概率。     

A mathematical structure for a theory of electromagnetic induction in the Earth in low latitude

Summary In low latitude the spatial distribution functions of the source field over the surface and the dimensions of the source, are important in any theory of electromagnetic induction developed for studying the conductivity structure of the Earth. The author has built up a mathematical structure for a theory of electromagnetic induction in anyn-layered earth model in low latitude. No simple solution is assumed for the horizontal distribution function of the source field and no assumption is made about the horizontal gradients of the source. The mathematical structure involves the concept of downward continuity of the field equations inside then-layered earth model. The resulting mathematical functions derived for anyn-layered earth model are complex. Hence a new matrix algebra of complex numbers is introduced by the author and this is built into the theory. From the upward continuity of the field equations, an inequality equation is derived in order to determine the heighth ₀ at which the induction field of the earth becomes negligible compared with the source field. The comparison of such heights at two or more stations under the same influence of the source field can be used for the resolution of the lateral distribution of the earch conductivity structure at these stations. The application of the theory will follow in a subsequent paper.     

中国东南沿海地区大气反常结构遥感初探

对流层大气作为电波传播的主要媒介,其大气剖面参数直接影响无线电系统的作用距离和导航、定位精度,因此,研究大气剖面的微波遥感技术,尤其是大气反常结构,对分析评估无线电信息系统在复杂大气环境条件下工作性能和提供电波折射修正精度等具有重要的应用价值。中国东南沿海地区一直是研究的热点区域,本文选取青岛、射阳、厦门、海口4个站的气象探空仪观测数据,统计了这些地区大气波导的平均高度和厚度,对采用地基多通道微波辐射计的天顶和扫角亮温遥感其参数的算法进行了初步探索,提出了改进的组合神经网络算法来判别并遥感大气波导。同时,使用多年的探空数据对该算法进行了仿真验证,并用青岛气象站的实测数据验证了该算法的精度。结果表明该算法可用于遥感大气反常结构,并且与以往的算法相比更加实用、有效,可为雷达、通信、导航等系统设备提供环境信息保障。