RTK-GPS�����������񶯵Ķ�Ƶ�ʳɷַ���   总被引：2，自引：1，他引：1  

谷川  王丽华  万军 《大地测量与地球动力学》2008,28(2):120-122

???????RTK-GPS(????????λ??)???????????????????????????????????????????????????????RTK-GPS???????????????????????????????????????????????????????????е??  相似文献   

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陈兴权  王解先 《大地测量与地球动力学》2008,28(4):111-114

????????????????????????????Σ?????????????????????????????????趨???????????м???????е???????????????????ó?????????????????????????????????????????????????????????????????????????????淽??????????????????????????????????????????????????????????????????????????????淽???????????????????????????????????÷??????????Ч???  相似文献   

地下电短天线的输入特性分析     

孙建国  康国军  张辉 《吉林大学学报(地球科学版)》2004,34(1):128-133

地下电短天线的输入导纳是其几何尺寸、工作频率及地下和近地表物质(围岩及土层)电磁参数的函数.通过分析其变化规律得到下列结论:(1)短天线的输入导纳随频率的变化比较复杂.当频率较低时,短天线的输入电导随地下物质电磁参数的变化不明显,而输入电纳基本上随着频率的增高呈线性变化.(2)在频率比较低时,介电常数的变化对短天线的输入电导影响不明显,存在有一个电导曲线重合频段.对于低阻物质,这个重合频段的上限比较低;对于高阻物质,重合频段的上限升高.对于输入电纳,当电阻率和频率两者都较高时,其对介电常数的变化比较敏感.(3)输入导纳对低阻物质反应敏感,而对具有中等以上电阻率的物质基本上退化成为一条相同的频率变化曲线.(4)短天线的输入导纳值随其几何尺度的增加而增加.  相似文献   

二维圆柱坐标下FDTD法对多频电磁波测井的数值模拟   总被引：5，自引：2，他引：3  

刘四新 《吉林大学学报(地球科学版)》2004,34(2):283-286

在介质围绕Z轴旋转对称的情况下,三维直角坐标下的麦克斯韦方程可变成两组分别对应TM波和TE波的二维柱坐标下的偏微分方程.采用线圈作为电磁波测井的发射器和接收器的时候,可采用TE波对应的方程,这时相当于磁极子的情况.而采用电偶极子作为发射和接收器的时候,则对应TM波的方程.采用时间和空间均为二阶精确的有限差分方法,将偏微分方程进行差分化.这样,空间的电磁场可由时间域有限差分法(FDTD)来求解.  相似文献   

新一代天气雷达轴角盒故障的分析处理     

郭泽勇  曾广宇  吴少峰  胡伟峰  罗业永  叶宗毅 《气象科技》2014,42(5):777-781

CINRAD/SA天气雷达在PPI扫描过程中天线来回摆动,导致雷达无规律出现方位扇形范围无回波,雷达不能正常发挥其有效作用。为查找故障原因,从新一代天气雷达伺服系统信号流程入手,结合雷达基数据分析软件,分析雷达天线运行轨迹,通过信号流程中关键点参数的测量和比较,发现问题出现在轴角编码盒方位环节,导致轴角盒串行方位轴角数据输出不连续,造成雷达无规律出现方位扇形范围无回波。通过对此类故障分析思路与处理经验的总结,对台站级雷达技术保障提供借鉴。  相似文献   

不同天线组合对GPS姿态测量精度的影响分析          下载免费PDF全文

鲁洋为  王振杰  聂志喜  王毅 《海洋测绘》2014,34(6):43-45,48

GPS姿态确定的精度不仅与单历元基线解算精度有关,还受基线长度和天线布设结构的影响。探讨了GPS姿态测量系统中基线长度和天线布设结构与姿态测量精度的关系。仿真结果表明:增加航向基线长度,能够提高航向角和俯仰角的精度,增加横向基线长度,能提高横滚角的精度;当基线长度一定时,将两基线正交布设,横滚角的精度最高。  相似文献   

40m天线面板调试与精度分析     

金旺  汪敏  张巨勇  赵辉  张萍  宋俊峰  许春 《天文研究与技术》2006,3(4):401-407

总结了40m天线面板安装调试及检测的过程，分析了反映望远镜面板指标的吨性能检测结果。结果表明天线面板精度优于原设计要求。  相似文献   

RFI Test Observations at a Candidate Ska Site in China     

B. Peng  J. M. Sun  H. Y. Zhang  T. Y. Piao  J. Q. Li  L. Lei  T. Luo  D. H. Li  Y. J. Zheng  R. NAN 《Experimental Astronomy》2004,17(1-3):423-430

Radio frequency interference (RFI) test observations were carried out at one of the candidate Square Kilometre Array (SKA) sites in Guizhou province, following the “RFI Measurement Protocol for Candidate SKA Sites” (hereafter RFI protocol). All data (raw and calibrated) are preserved in some suitable format, such as that set by the international RFI working group of the Site Evaluation and Selection Committee (SESC). An RFI test in December 2003 was performed according to Mode 1 of the RFI Protocol, in order to identify technical difficulties which might arise during a co-ordinated RFI measurement campaign over a period of 1 year. In this paper we describe the current equipment, observational technique and data presentation. The preliminary results demonstrate that the RFI situation at Dawodang depression in Guizhou province makes it quite a promising location for the proposed SKA. Furthermore, the first session of the RFI monitoring program, which was made in May 2004, showed that a complete RFI measurement including both modes 1 and 2 of the RFI Protocol would take about 2 weeks. The possible ways to minimize some limitations of the current equipment are also discussed, which will enable us to meet the RFI protocol.  相似文献   

Array Configurations That Tile the Plane     

John D. Bunton 《Experimental Astronomy》2001,11(1):193-206

Future radiotelescopes need ever increasing sensitivity. With the limits of receiver sensitivity being reached this can only be achieved by increasing collecting area. The increase in antenna numbers and the multi-resolution capabilities of these telescopes, such as the SKA, means a significant departure from existing designs is needed. In this article, some fundamental designs for antenna arrays that uniformly sample the UV plane are presented. The SKA is used to provide target specifications. The designs presented allow asymmetric configurations providing more freedom for site selection. They also allow a direct tradeoff between field of view and correlator complexity. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

偏航姿态对北斗精密单点定位的影响分析     

叶世榕  夏凤雨  赵乐文  夏朋飞  陈德忠 《测绘学报》2017,46(8):971-977

当太阳相对于卫星轨道面的高度角较小时,北斗导航卫星将不会跟踪太阳位置,卫星姿态发生异常复杂的变化后一段时间内处于零偏模式。在此期间采用名义姿态将影响卫星天线相位中心偏差、相位缠绕等误差计算,进而使精密单点定位(PPP)参数估计和天顶对流层延迟估计出现偏差。研究表明,在北斗导航卫星处于零偏期间,采用名义姿态计算的相位缠绕、天线相位中心偏差中存在超过15cm的误差。在此期间的北斗卫星采用零偏姿态改正相位缠绕等误差,与采用名义姿态相比,动态PPP位置参数N、E、U的估计精度可以提高53.2%、54.2%、39.3%,静态PPP位置参数N、E、U的估计精度可以提高61.0%、72.3%、58.4%,天顶对流层延迟估计精度提高33.0%。  相似文献