Effect of Interplanetary Transients on Cosmic Ray Anisotropic Variations

In the present work the cosmic ray intensity data recorded with ground-based neutron monitor at Deep River has investigated taking into account the associated interplanetary magnetic field and solar wind plasma data during 1981—1994.A large number of days having abnormally high/low amplitudes for successive number of five or more days as compared to annual average amplitude of diurnal anisotropy have been taken as high/low amplitude anisotropic wave train events(HAE/LAE).The amplitude of the diurnal anisotropy of these events is found to increase on the days of magnetic cloud as compared to the days prior to the event and it found to decrease during the later period of the event as the cloud passes the Earth.The High-Speed Solar Wind Streams(HSSWS)do not play any significant role in causing these types of events. The interplanetary disturbances(magnetic clouds)are also effective in producing cosmic ray decreases.Hαsolar flares have a good positive correlation with both amplitude and direction of the anisotropy for HAEs, whereas PMSs have a good positive correlation with both amplitude and direction of the anisotropy for LAEs. The source responsible for these unusual anisotropic wave trains in CR has been proposed.     

Ni-Mo电沉积层的组成和结构

利用Ｘ射线光电子谱（ＸＰＳ）研究了Ｎｉ－Ｍｏ沉积层的组成元素及其价态和深度分布,用扫描电子显微镜（ＳＥＭ）、Ｘ射线衍射技术（ＸＲＤ）和电子探针显微分析技术（ＥＰＭＡ）研究了电沉积Ｎｉ－Ｍｏ合金层的形貌、结晶状态、组成元素分布情况。结果表明,电沉积Ｎｉ－Ｍｏ合金层呈现亮色,表面比较均匀。电沉积层为非晶结构,２θ在４０°～５０°间有一弥散对称峰。沉积层中的Ｎｉ和Ｍｏ为零价态,它们的结合能分别为８５２．８ｅＶ和２２８．２ｅＶ。沉积层的真实组成（相对原子百分浓度）为：Ｎｉ５０．８６％,Ｍｏ２２．６３％,Ｏ２６．５１％。     

基于时域有限差分的微放电仿真算法

为克服传统微放电阈值预测方法建模粗糙、精度低的缺点,提高阀值预测精度和效率,研究了基于时域有限差分的精确微放电阀值预测算法。基于时域有限差分算法和粒子追踪算法,通过时空网格自洽互耦实现复杂结构微波器件微放电阈值准确计算。其中,共形和并行算法是提高微放电仿真精度和效率的关键。文章基于空间蛙跳策略实现了基于时域有限差分的微放电仿真算法,利用算法分析了典型微波器件的微放电阈值,仿真与实验结果吻合良好,误差小于0.3dB;同时,并行效率最高可达83%,验证了算法的准确性和高效性。     

基于Daubechies小波的X射线脉冲星信号降噪研究

针对X射线脉冲星弱信号埋没在强噪声中,在短时间内周期叠加的脉冲轮廓的信噪比低,影响脉冲到达时间的估计精度和效率,提出基于Daubechies小波的X射线脉冲星信号降噪的算法。在对RXTE观测数据预降噪处理和周期叠加的基础上,采用Daubechies小波算法做降噪处理,使得较短的时间内仍能获得高信噪比的脉冲轮廓。利用RXTE观测数据进行验证仿真,结果表明,该算法能有效滤除X射线脉冲星信号所包含的设备及空间环境的噪声,在保证脉冲到达时间精度的情况下,缩短了观测时间,提高X射线脉冲星导航的效率。      

基于射线模型的水声传播衰减特性

介绍了水声信号传播射线模型的理论基础,给出了水声传播衰减详细的理论推导和数学分析过程;在射线模型的基础上分析了水声信号传播的过程,并根据数学模型,实现了传播过程在matlab下的仿真。根据不同的仿真条件得到了相关的传播损失分布图,并对结果进行了分析。     

机舱内部超宽带确定性信道建模

将室内无线信道仿真中常用的几何光学和射线追踪技术,引入到对客机机舱内部的超宽带(Ultra-WideBand,UWB)信道研究当中。信道仿真的主要算法基于一种称为射线密度归一化(RayDensityNormalization,RDN)的方法。该方法使用射线密度的概念来计算每条射线对接收点处总信号强度的贡献。为了验证方法的有效性,实验构建了一个Boeing737-200客机机舱模型进行仿真。仿真将接收机设置在每个座位的顶部、扶手和底部,以研究不同水平高度信道的差别。仿真中对路径损耗和均方根(RMS)时延扩展两类大尺度信道参数进行了统计和分析,部分仿真结果与国外实测结果进行了对比。对比结果证明了仿真结果的保真度以及现有仿真工具的有效性。     

World grid of cosmic ray vertical cut-off rigidity for the last decade

Cosmic ray cut-off rigidity tables and maps over the world concerning the epochs 2010, 2015 and the current one 2020 have been constructed. These maps display the effective cut-off rigidity in every five degrees in latitude and in longitude at the altitude of 20 km above the surface of the international reference ellipsoid. The values of the geomagnetic cut-off rigidity were calculated in every 5° in latitude and in every 15° in longitude applying the well-known method of particle trajectory calculations resulted from the theory of the particle motion in the Earth's magnetic field. The applied software employed the 12th Generation of the International Geomagnetic Reference Field (IGRF 12) and trajectories were calculated at 0.01 GV intervals in order to determine the vertical cut-off rigidity for each location. Beyond the use of the calculated cut-off rigidity values as a basic reference of charged particle access to different geographical locations during quiet and/or more intense geomagnetic periods, these results can be used for a long- term forecasting of the geomagnetic conditions variations.     

Quasi-periodicities in cosmic rays recorded by the KACST muon detector during 2002–2012

In this study, daily cosmic ray data obtained with the KACST muon detector for the period 2002–2012 were analyzed for quasi-periodicities. Power-spectrum analysis was carried out and several periodicities were identified. The results reveal several periodicities at different frequency scales: 817 days (~2.19 years), 617 days (~1.7 years), 475 days (~1.3 years), 421 days (1.15 years), 290 days (~0.8 years), 227 days (~0.62 years), 185 days (~0.52 years), 153 days, 135 days, 120 days, 93 days, 84 days, 73 days, 65 days, 53–45 days, 38 days, 31 days, 25–27 days, 21 days and 13 days. The obtained periodicities are in an agreement with those previously reported by several investigators.The identified periodicities have strong relevance to solar activity parameters such as variations in the interplanetary magnetic field.In comparison, the data from two neutron monitors (NMs), Lomnický ?tít and Oulu NMs, for the same period were used and their power spectra were correspondingly obtained. Similarities and differences in the position of the cosmic-ray peaks measured by the KACST muon detector and by the two NMs have been presented and discussed. While most of the periodicities reported by the muon detector are also found in the NM data, the ~1.7-yr variation is not found. Instead, a shift of 1.6–1.8 years in the NM data is observed which may be due to the limited epoch considered in this study.     

USO-KBR测距系统建模与仿真

K频段微波测距(KBR)系统是低-低卫星跟踪卫星(SST-LL)重力测量卫星的关键载荷之一,其性能直接影响地球重力场空间变化率的测定结果,而KBR系统中超稳振荡器(USO)的稳定度对KBR系统整体测距精度有着重要影响。文章根据双向测量载波相位对比原理和USO幂率谱模型,对KBR系统进行了建模。首先,描述了测距系统的基本原理、系统功能组成及适用于KBR系统的数学模型;然后,利用Matlab软件对"重力恢复和气候实验"(GRACE)卫星的KBR系统进行了仿真。仿真结果表明,采用该模型和方法后获得的双向测距中误差(RMSE)为9.81μm,与公布的GRACE卫星KBR系统10μm的中误差相符。文章为KBR系统的工程设计提供了仿真分析工具,可为工程应用提供设计参考。     

角形结构的电磁散射和雷达截面分析

角形结构是飞行器及其它许多目标的强散射源之一。本文采用复射线展开法分析了双平面角形结构的雷达截面,所得计算结果与实验结果及其它方法的理论结果十分吻合。