共查询到17条相似文献，搜索用时 187 毫秒
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基于局域GNSS网络,以历元间、星间差分技术实时估计了GPS卫星相对钟差的历元间差值;针对所估计实时精密钟差的特征,推导了实时精密单点定位的估计模型.对所估计得到的相对钟差的历元间差值、实时定位结果分别进行了比较、分析.结果表明,相对钟差的历元间差值与IGS的最终星历相比其精度可以达到0.08 ns;每小时观测的实时静态定位结果在N、E、U三个方向的精度分别为1.47、3.62、4.09 cm.动态模式,实时结果在N、E、U三个方向的精度分别为2.63、3.82、5.20 cm.与采用IGS最终轨道和钟差解算的结果相比较,实时计算结果优于采用精密轨道和精密钟差计算结果. 相似文献
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从GPS基本观测模型出发,给出并推导了分离相位小数偏差求解非差整数模糊度的精密单点定位数学模型和算法.利用少量IGS跟踪站组成服务端观测网计算未检校的相位小数偏差改正信息,用于改正用户端接收机的相位观测值,实现了固定非差整数模糊度的快速精密单点定位与定轨.试验结果表明: 利用30 min的地面动态或静态观测数据进行精密单点定位,非差模糊度固定成整数后,其定位结果较PPP浮点解有明显改善,水平方向提高了近一个数量级,可达到1 cm甚至毫米级的精度;高程方向与对流层延迟解算精度也改善了20%~60%.与浮点解相比,固定解能显著改善PPP的定轨精度,仅用15 min的短弧段观测数据,切向与法向的定轨精度可达到1 cm左右;径向方向为3~5 cm左右,较浮点解定轨精度改善了50%~70%.因此,固定非差整数模糊度后的PPP能够满足毫米至厘米级的快速精密定位和定轨的要求,这在GPS(准)实时应用与服务中具有很好的应用前景. 相似文献
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讨论了实时精密单点定位的若干关键技术,着重研究了实时精密钟差估计算法;利用全球40个IGS跟踪站连续、实时的观测数据流进行实时精密卫星钟差估计,解算出的实时精密钟差与CODE事后精密钟差具有较好的一致性,二者互差的RMS优于0.2 ns.采用实时估计的卫星钟差和IGS发布的超快速精密卫星轨道进行实时精密单点定位模拟实验,结果表明：经过大约15~30 min初始化后,实时精密单点定位滤波收敛之后水平方向的定位精度优于5 cm,高程方向的精度优于10 cm,能满足在该精度级别的实时用户的定位需求.处理汶川地震期间震区的GPS观测数据,结果表明实时精密单点定位能够探测地震发生期间的地面同震位移. 相似文献
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《地震研究》2016,(4)
利用2014年6月福建省地震局进行的人工爆破实验的50 Hz超高频GPS观测数据,采用快速预报星历以及事后精密星历,对观测的数据分别进行准实时和事后精密处理。结果显示高频GPS在差分处理模式下,其水平向噪声大致为5 mm,垂直向大致为10 mm。高频GPS差分单历元解在采用快速预报星历与事后精密星历得到的结果基本一致,因此采用快速预报星历进行高频GPS实时解算的结果具有很高的可靠性。同时,通过比较并址的高频GPS和强震仪信号的波形和频率成分发现,差异主要是由于高频GPS和强震仪记录对于不同频率震动信号的响应不同,两者在重叠的频段上有较好的一致性,而这种差异本身体现了一种互补的特征。因此,高频GPS数据的实时处理结果具备监测地表震动的能力,可应用于地震烈度速报与地震预警,成为地表震动和地震研究的良好补充。 相似文献
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利用单频接收机实现大范围、高精度快速实时定位是卫星大地测量研究的热点和难点问题之一.本文提出了一套基于连续运行参考站系统(CORS)的误差实时建模数据处理方法,设计并实现了一种新的GPS单频接收机实时精密单点定位服务方法.然后,利用山西省CORS网内一组实测动态数据,以及从湖北省CORS网和武汉市CORS网选取的一组实测静态数据进行测试,验证分析了所提出方法用于实时定位服务的可行性.结果表明:对于站间平均距离小于71 km的参考网,网内单频用户按照实时处理模式,在经过数秒钟的初始化后即可获得厘米级的动态精密单点定位结果.这为GPS单频接收机用户实现快速实时精密单点定位提供了一种可行的新方法. 相似文献
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张宝成 Teunissen J G Peter Odijk Dennis 欧吉坤中国科学院测量与地球物理研究所 动力大地测量学重点实验室 蒋振伟 《地球物理学报》2012,55(7):2203-2211
提出利用GPS参考网估计电离层延迟、卫星相位偏差的算法,用于实现区域内精密单点定位(Precise Point Positioning, PPP)的整周模糊度快速固定.利用站间距约为100~200 km的参考网进行实验,结果表明:电离层延迟的内插和外推精度均优于1 dm,卫星相位偏差估值的日内变化不超过0.2周;此外,单天内不同时刻始,固定PPP整周模糊度所需时长最多不超过10 min,且当模糊度成功固定后,三维位置解较之相应浮点解的精度改善优于80%.新算法可望解决PPP普遍存在的收敛时间过长问题,增强了PPP技术的实用性. 相似文献
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基于星载GPS的HY-2卫星高精度精密定轨模拟研究(英文) 总被引：2，自引：0，他引：2
HY-2卫星是我国第一颗测高卫星,其径向定轨精度要求厘米量级,搭载了星载GPS接收机。目前HY-2还处于测试阶段,没有公布观测数据。为了确定基于星载GPS的HY-2精密定轨流程及其定轨精度,本文模拟了HY-2卫星星载GPS观测数据,结果表明HY-2星载GPS天线每个历元至少观测7颗GPS卫星。给出了基于星载GPS的精密定轨流程,分别采用简化动力学方法和动态几何法进行了精密定轨实验。对于相位1mm和3mm随机误差的相位观测数据,简化动力学法和动态几何法定轨都能够实现厘米量级的径向精密定轨,几何法定轨精度略低于简化动力定轨。地球重力场模型是影响HY-2卫星精密定轨的重要因素,本文对不同阶次的重力场模型EIGEN2、EGM96、TEG4和GEMT3进行了简化动力学定轨实验,高于50阶次的重力场模型都能够实现厘米级径向精密定轨,主要原因在于大量的高精度星载GPS观测数据和重力场模型精度的提高。 相似文献
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《中国科学:地球科学(英文版)》2015,(11)
In this study, we demonstrate an approach for inverting earthquake source parameters based on high-rate global positioning system(GPS) velocity seismograms. The velocity records obtained from single-station GPS velocity solutions with broadcast ephemeris are used directly for earthquake source parameter inversion using the Cut and Paste method, without requiring conversion of the velocity records into displacement records. Taking the El Mayor-Cucapah earthquake as an example, GPS velocity records from 10 stations with reasonable azimuthal coverage provide earthquake source parameters very close to those from the Global centroid moment tensor(Global CMT) solution. In sparse network tests, robust source parameters with acceptable bias can be achieved with as few as three stations. When the number of stations is reduced to two, the bias in rake angle becomes appreciable, but the magnitude and strike estimations are still robust. The results of this study demonstrate that rapid and reliable estimation of earthquake source parameters can be obtained from GPS velocity data. These parameters could be used for early earthquake warning and shake map construction, because such GPS velocity records can be obtained in real time. 相似文献
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对于GPS动态定位模式, 高频(≥1 Hz)GPS数据需要30 s或者更高采样率的卫星钟差, 而满足需要的IGS星历产品至少要延迟12～18 d才能获得。 显然, 常规的GPS数据处理方法无法满足地震应急的需要。 本文提出一种针对地震应急高频GPS数据处理方法, 利用陆态网络GPS高频数据解算获得中国大陆区域高精度卫星钟差, 进而解算获得测站地表瞬时形变位移, 突破常规处理方法的限制, 可在地震发生后仅数小时获得快速、 准确、 可靠的结果。 这种方法在2013年芦山MS7.0级地震得到了实际应用。 相似文献
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《Journal of Atmospheric and Solar》2007,69(12):1312-1330
The aim of this study is to assess the availability and quality of data from the International GNSS Service (IGS) Global Positioning System (GPS) network in Africa, especially for retrieving zenith tropospheric delay (ZTD), from which precipitable water vapour (PWV) can be derived, in view of application to the African Monsoon Multidisciplinary Analysis (AMMA) project. Three major error sources for the GPS data analysis evaluating PWV in Africa are the accuracy of the satellite orbits, the correction for the radio delay induced by the ionosphere and the vertical site displacements due to ocean loading. The first part of this study examines these error sources and the validity of GPS data for meteorological applications in Africa in dedicated analyses spanning the year 2001. These analyses were performed using the IGS precise orbits. Weak degradation of baseline precision with increasing baseline lengths suggests that the average orbital error is not limiting the GPS analysis in Africa. The impact of the ionosphere has been evaluated during a maximum of solar activity in 2001. The loss of L2 data has actually been observed. It amounts to 2% on average for 2001, with maxima of 8% during magnetic storm events. A slight decrease in formal accuracy of ZTD seems to be related to the loss of L2 data at the end of the day. This indicates that scintillation effects are present in the GPS observations but however are not a major limitation. The impact of ocean loading is found to be significant on ZTD estimates (up to ±2 mm in equivalent PWV). The use of a proper ocean loading model eliminates this effect.The second aspect of this study concerns the IGS analysis quality for the African stations. The accuracy has been assessed through position dispersion between individual solutions and the most recent version of the IGS combined solution IGb00, and residuals from the transformation of the IGS combined solution into the International Terrestrial Reference Frame 2005. The positioning performance of the IGS analysis is consistent with an accuracy in ZTD of ±6 mm (±1 mm in PWV), as requested for meteorological applications such as planned in AMMA. 相似文献
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提出了一种基于拟准检定的实时单站GPS载波相位观测数据历元间差分提取同震速度的改进算法.改进算法将实时高频历元差分数据质量控制作为同震速度准确提取的重要保障,对原始高频数据中的小周跳和粗差十分敏感,且能够有效地估计小周跳和粗差,从而抵抗它们对同震速度估计的不良影响;另外,改进算法还简化了数据处理流程,也使得利用广播星历单站提取同震速度、监测地震形变的算法更为稳健.选取了2011年3月11日日本大地震距离震中140 km的MIZU站1 Hz高频GPS观测数据和广播星历来测试改进算法.结果表明：拟准检定法具有更好的小周跳与粗差自动定位和估计性能,改进算法利用广播星历求得的同震速度与事后动态精密单点定位结果表现出很好的一致性. 相似文献
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自1995年起,国际南极研究科学委员会（SCAR,the Scientific Committee on Antarctic Research）组织实施全南极国际GPS（Global Positioning System）联测.本文运用GAMIT/GLOBK软件分析了从1997到2004年的SCAR GPS数据和在南极的一些GPS永久跟踪站数据.数据处理分为两步,第一步：运用GAMIT软件进行单天解算,估计站位置、轨道等参数,其数据源主要有以下三类：(1) SCAR GPS观测站;（2）南极的连续跟踪站;（3）南极及其周边的部分IGS站;第二步：运用GLOBK软件加入SOPAC（Scripps Orbit and Permanent Array Center）的全球GPS子网（IGS1、IGS2、IGS3）进行全球网平差解算测站位置和速度.然后,参照地质构造讨论网的形变,分析了南极板块的现今地壳运动.GPS结果显示南极板块的欧拉角速度是0.224(°)/Ma,旋转极的位置为（58.69°N,128.29°W）,这与NNR-NUVEL-1A预测的和一些前期GPS研究的成果有着较大的不同.相对于澳大利亚板块,本文结果同其他模型的旋转角速度相差约0.01(°)/Ma,旋转极的位置相差在4°以内,不同模型之间的差异相对较小.这为描述南极板块运动提供了一个更为精确的新的运动模型. 相似文献
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R. Orús M. Hernndez-Pajares J. M. Juan J. Sanz M. García-Fernndez 《Journal of Atmospheric and Solar》2002,64(18)
The existence of a worldwide international GPS service (IGS) permanent network of dual-frequency receivers makes the computation of global ionospheric maps (GIMs) of total electron content (TEC) feasible. The GIMs computed by the IGS Associate Analysis Centers on a daily basis and by other kinds of forecast GIMs, which can be computed from, for instance, the international reference ionosphere (IRI) model, and the GPS broadcast models in the navigation message, can be applied to a broad diversity of fields, for instance as, navigation and time transfer.In this context, the performance of different kinds of models are presented in order to determine the accuracy of the different GIM. This is carried out by comparison with the TOPEX data that provides an independent and precise (at the level of few TECU) vertical TEC determination over the oceans and seas. Thus, the obtained accuracies, in terms of global relative error, ranging from 54% corresponding to the GPS broadcast model, to about 41% corresponding to IRI climatological model, and to less than 30% corresponding to GPS data driven models. 相似文献
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Tidally induced sub-daily Earth Rotation Parameters (ERP) variations, when not properly accounted for, can cause apparent orbit and ERP rate errors, which can significantly exceed the IGS solution errors. All International GPS Service (IGS) Analysis Centers currently apply the conventional sub-daily ERP model in their transformations from ITRF (International Terrestrial Reference Frame) to ICRF (International Celestial Reference Frame), both of which are used for IGS global analyses. However, some IGS Analysis Centers did not apply the sub-daily ERP model when transforming ICRF orbit solutions to ITRF, which is used for IGS orbit/clock products. This transformation inconsistency can cause significant orbit RMS differences that could exceed the 5-cm level. Independent ERP rate solutions are sensitive even to small errors in the sub-daily ERP model, and can be used to verify the sub-daily ERP model at, or below 0.1 mas/day precision level.The Precise Point Positioning (PPP) via precise station position solutions with the IGS orbit/clock combined products, provides an ideal interface to access the IGS realization of ITRF. PPP also yields precise station clock and tropospheric zenith delays (TZD) solutions, all at the sub-cm precision level. However, when using IGS orbit/clock products it is important that the same convention be used with respect to sub-daily ERP. Otherwise, the solutions of station navigation positions, station clocks and TZD's will be affected by significant errors that could exceed the 1-cm level. 相似文献