三频BDS电离层延迟改正分析

针对电离层改正会引起观测噪声放大,尤其三频二阶改正致使观测噪声被过分放大的不足,该文分别推导了BDS电离层双频一阶改正、三频一阶改正和三频二阶改正模型及三频载波无电离层组合模型。改正电离层延迟的同时会不同程度地放大观测噪声,为此分析比较了各种方法改正后的观测值精度和观测噪声,并对不同方法的应用进行了分析。     

北斗三频数据线性组合优化分析

随着GPS现代化的实施和欧洲Galileo计划的实行,多频数据组合逐渐成为卫星导航定位的发展方向。针对关于北斗导航定位系统多频数据组合的研究较少这一现状,该文首先简要介绍了北斗导航定位系统,并在分析BDS三频数据线性组合的数学模型和确保模糊度参数整数特性的基础之上,给出了BDS三频数据线性组合的优化选取标准;然后从消除或减弱电离层延迟、对流层延迟和观测噪声三个方面系统地分析了BDS三频数据线性组合系数的优化选取问题;最后通过MATLAB模拟,给出了一些典型的组合,分析了它们可能的应用。     

中国地震预警延迟时间算法及其对预警盲区的影响研究

通过分析预警系统的预警步骤来探讨影响获得预警时间的因素,并与瑞士地震台网预警延迟各步骤进行对比,得出中国地震预警系统仪器延迟时间为7.6s。提出地震波到台站所需时间的算法,较震中假设在台站中间的传统算法更为准确,在此算法下采用双台法和四台法计算接收地震波所需时间,得到中国地震预警延迟时间。讨论双台法和四台法在不同震源深度和台站密度下对预警盲区大小的影响,在台间距小于20km时,2种方法预警盲区差异不大。通过理论计算得出,在台站到达一定密度时,预警系统仪器延迟时间缩短比台站加密对预警盲区的缩小更有效。     

1PN近似下脉冲星导航的观测方程及精度分析

完整推导1PN度规形式下脉冲到达时间方程与脉冲星导航的观测方程。分析导航观测中的相对论影响;给出观测方程的级数展开形式,在此基础上分析脉冲星历表参数对观测时间的影响;讨论行星星历误差对观测时间的影响;推导星体扁率引起的测量时延表达式,分析不同星体扁率引起的时延量级。     

全球定位系统的新进展(讲座四)——信号内部时延及其对钟差的影响

介绍了卫星信号内部时延的定义以及在GPS导航电文NAV和CNAV中所给出的各种时延差参数,推导了采用不同的卫星信号测距时应采用的各种卫星钟差模型。     

长三角区域对流层延迟简易模型的建立

在对流层经验模型Saastamoinen模型和EGNOS模型的基础上,通过对长三角地区近40年气象规律的研究,总结了温度、气压、相对湿度相对于年积日的函数关系,建立了适用于长三角区域的对流层天顶延迟的简易模型。通过实验验证了该模型的有效性,该模型输入参数是年积日,不仅方便快捷,还提高了经验模型的精度,为更精确的区域模型研究提供了参考。     

GPS定位与水汽反演中对流层干延迟的订正研究

根据美国Shreveport地区及中国徐州地区2006年的气象探空资料计算了GPS测量中的大气干延迟,将其作为真值与目前常用的普适模型计算的延迟值进行对比,结果表明,目前常用的几种普适模型在美国Shreveport地区的改正效果要明显好于中国徐州地区,直接反映出普适模型更适合北美地区.利用徐州地区2000-2006年的探空数据计算了大气干延迟值,在此基础上,根据地面气象要素建立了徐州地区大气干延迟的局地订正模型.分析表明,局地订正模型的改正效果好于普适模型.     

TEM中心回线中—远带响应特征

近20年来,中心回线观测已进入全域时段,然而有关中—远带响应特征的文章极为少见,致使用户困惑,比如晚延时响应值大于早延时响应值(ε-上凸)、在同一测点2种仪器系统观测结果相差太大等。对此笔者做了详细分析。结果表明,中—远带响应特征基本为4种,ε-上凸只是其中之一,导致所测响应出现差别的主要原因是接收线圈延时。因此,若工作于中—远带,必须确切测定线圈延时,合理选择发射回线边长。     

Comparison between real‐time dynamic substructuring and shake table testing techniques for nonlinear seismic applications

Results from real‐time dynamic substructuring (RTDS) tests are compared with results from shake table tests performed on a two‐storey steel building structure model. At each storey, the structural system consists of a cantilevered steel column resisting lateral loads in bending. In two tests, a slender diagonal tension‐only steel bracing member was added at the first floor to obtain an unsymmetrical system with highly variable stiffness. Only the first‐storey structural components were included in the RTDS test program and a Rosenbrock‐W linearly implicit integration scheme was adopted for the numerical solution. The tests were performed under seismic ground motions exhibiting various amplitude levels and frequency contents to develop first and second mode‐dominated responses as well as elastic and inelastic responses. A chirp signal was also used. Coherent results were obtained between the shake table and the RTDS testing techniques, indicating that RTDS testing methods can be used to successfully reproduce both the linear and nonlinear seismic responses of ductile structural steel seismic force resisting systems. The time delay introduced by actuator‐control systems was also studied and a novel adaptive compensation scheme is proposed. Copyright © 2010 John Wiley & Sons, Ltd.     

The influence of the interplanetary medium on SuperDARN radar scattering occurrence

The effects of the characteristics of the interplanetary medium on the radar scattering occurrence, related to the whole array of SuperDARN radars installed in the Northern Hemisphere, have been studied over a two-year period. Statistically significant correlations of the variation of the scattering occurrence are found with the merging electric field and with the negative B_z component of the interplanetary magnetic field, independent of the seasonal period considered. This result demonstrates that the merging rate (and in particular the reconnection process) between the interplanetary magnetic field and the magnetosphere is a relevant factor affecting the occurrence of scattering. For comparison, we note that no statistically significant correlations are obtained when the interplanetary ion density or the solar wind speed are considered, although also these variables affect to a small degree the scattering occurrence variation. The study of the latitudinal and magnetic local time dependence of the observations shows an association between the considered correlation and the location of the auroral oval and the cusp/cleft region.