共查询到18条相似文献，搜索用时 156 毫秒
1.
为提高区域电离层模型和导航定位服务的精度,利用河北省连续运行参考站系统（CORS） 6个基准站的GPS卫星观测数据进行区域电离层建模和接收机差分码偏差（DCB）估计,并引入中国科学院（CAS）发布的电离层产品内插得到的垂直总电子含量（VTEC）进行区域电离层模型精度验证。实验结果表明,估计的单日GPS卫星DCB与产品值精度相当,偏差控制在0.5 ns以内;河北省CORS站GPS系统接收机DCB稳定性较好,5 d的标准偏差均小于0.1 ns;利用河北省CORS建立的区域电离层TEC在地磁平静期与磁暴期均与CAS产品值具有较高的一致性,TEC偏差控制在2 TECU以内。河北省区域电离层模型能有效监测电离层TEC在不同地磁状态下的时空变化,提高区域导航定位服务水平。 相似文献
2.
《测绘科学》2020,(1):48-53
针对电离层延迟改正对单频接收机用户带来误差较大的问题,该文基于球谐函数借助山东区域CORS双频观测数据建立山东区域电离层模型,并对硬件延迟偏差(DCB)和电子含量进行可靠性、稳定性分析,进一步使用单频精密单点定位(PPP)验证山东区域电离层模型的有效性。实验结果表明:测站DCB解算精度稳定在0.4ns内,解算卫星DCB与欧洲定轨中心(CODE)的偏差总体稳定在0.5ns内,区域电离层模型与CODE解算VTEC差值的均方根为1.22TECU,STD为0.93TECU,对山东区域单频PPP而言,山东区域电离层模型比CODE发布全球电离层模型在N、E、U方向精度明显提高。同时,建立的山东区域电离层模型从时间分辨率、空间分辨率上均优于CODE中心发布全球电离层模型。 相似文献
3.
《武汉大学学报(信息科学版)》2020,(5)
卫星导航定位中,电离层延迟是影响用户实时定位精度的重要因素之一。利用全球电离层格网(global ionosphere maps,GIM)提供电离层延迟改正是较为常用的方法,而GIM格网的精度受限于地面GNSS(global navigation satellite system)跟踪站的分布密度。利用区域内少量或1个GNSS跟踪站建立实时区域电离层总电子含量(total electron content,TEC)模型,生成高精度的实时区域电离层格网,为用户提供区域电离层延迟改正显得尤为重要。基于CODE(Center for Orbit Determination in Europe)分析中心2016—2018年995 d的GIM格网数据,分析了相邻格网点TEC的变化范围以及不同时间间隔同一格网点TEC的变化范围。结果表明,GIM在经度方向上分辨率为5°变化的均值范围为0.2～1.0 TECU,在纬度方向上分辨率为2.5°变化的均值范围为0.4～1.4 TECU,在经度和纬度分辨率均小于1°时,电离层TEC的变化小于1.0 TECU;1 h内同一格网点电离层TEC的变化均值约为1.28 TECU,30 min内同一格网点电离层TEC的变化小于1.0 TECU。该研究为小范围内(半径小于100 km)实时区域电离层TEC模型的建立及电离层格网的时间适用范围提供了有效的数据支撑和理论验证,同时对区域电离层TEC时空变化的研究、电离层TEC预报、电离层异常监测和磁暴监测等具有一定的参考意义。 相似文献
4.
差分码偏差(DCB)作为电离层建模和导航定位中一项重要的误差源,对其进行估计求解至关重要. 为提高北斗卫星导航系统(BDS) DCB估计和电离层建模精度,提出了一种综合高度角、卫地距和测站纬度多因素的随机模型,并对比分析了不同随机模型对BDS DCB估计和电离层垂直总电子含量(VTEC)建模精度的影响. 结果表明:不同随机模型对卫星端DCB解算产生约0.2 ns差异. 相较于高度角随机模型,采用高度角、卫地距组合模型测站DCB估计精度平均提高0.13 ns,电离层建模精度提高了约0.2 TECU. 新提出的随机模型,在低纬度测站DCB解算精度上差于高度角模型和高度角、卫地距组合模型,但在高纬度测站DCB解算结果上更优,且对电离层VTEC建模精度提升效果明显,与前两种随机模型相比分别提升了0.88 TECU和0.68 TECU. 相似文献
5.
针对电离层电子总含量(total electron content,TEC)时间序列高噪声、非线性和非平稳的动态序列的特点，基于反向传播神经网络(back propagation neural network,BPNN)模型对欧洲定轨中心(Centre for Orbit Determination in Europe,CODE)提供的电离层格网(global ionosphere maps,GIM)数据产品中低纬度、中纬度、高经纬格网点TEC数据和对应的时间点、经纬度、太阳射电通量F10.7数据、赤道地磁活动指数Dst、全球地磁活动指数Kp数据进行样本训练并进行电离层预报.结果表明：基于BPNN模型能够较好地预报低纬度、中纬度和高纬度电离层TEC数值，平均相对精度分别到达了90.5%、88.7%、85.35%，残差均值分别为1.505 TECU、1.595 TECU、1.885 TECU，平均均方根误差(root mean square error,RMSE)值分别为1.94 TECU、2.13 TECU、3.08 TECU. 相似文献
6.
《武汉大学学报(信息科学版)》2016,(6)
电离层总电子含量TEC(total electron content)是影响卫星导航定位的主要误差源之一。为了构建精确的电离层TEC模型,基于Chapman函数建立了基于物理机制的电离层TEC同化模型背景场,并着重以IGS发布的2008年4个时段低纬度、中纬度和高纬度地区的电离层TEC数据为样本,同化稀疏点上的已知电离层TEC值,分析模型计算值的残差和相对精度分布,利用模型对电离层TEC进行了2h短期预报和1d预报,并将1d的预报值和IGS发布值进行对比。实验结果表明:(1)由同化模型计算得到的TEC残差值超过92%分布在±2TECU以内,并且除边缘区域外,同化模型TEC计算值的相对精度均在90%以上;(2)2h和1d预报残差小于±3TECU的比例分别为81.8%和81.5%。 相似文献
7.
利用球冠谐分析方法和GPS数据建立中国区域电离层TEC模型 总被引：1，自引：0，他引：1
利用GPS实测资料建立了中国区域电离层TEC球冠谐分析模型(spherical cap harmonic analysis,SCHA),评估了该模型的精度和有效性.结果表明,该模型有较高的拟合精度,其拟合残差约为±3 TECU,且精度在时间和空间上分布较均匀.根据IGS分析中心发布的IONEX全球电离层数据(GIM),内插得到了区域内相应时段的平均电离层电子含量,并利用它对CSHA模型的零阶项系数C0.0所表示的区域平均电离层电子含量进行了检核.结果表明,二者具有较高的一致性和相关性,其谱特征相关系数为0.993.由于SCHA模型较GIM模型利用了更多本区域的GPS观测数据,因此其拟舍精度更高,拟合结果与实测数据更一致.时SCHA模型参数的时间序列进行谱分析,结果表明,该模型的模型系数较好地描述了区域电离层TEC的周期性变化特征. 相似文献
8.
根据高精度卫星导航和电离层活动监测的需要,利用全球238个GPS基准站的双频实测数据,通过建立球谐函数模型的同时解算电离层电子含量以及GPS与GLONASS卫星DCB及其相应的接收机DCB;将其结果与CODE、IGS分析中心的结果进行比较分析,表明该方法建立的模型是可靠的,其GPS和GLONASS卫星DCB相对于CODE精度优于0.1ns,相对于IGS精度优于0.2ns,其GPS测站DCB和GLONASS测站DCB相对于CODE和IGS精度优于1ns,垂直总电子含量相对CODE和IGS精度优于3TECU,组合结果精度高于组合前。 相似文献
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为了分析与评估国际GNSS监测评估系统(iGMAS)全球电离层TEC格网产品精度,该文基于iGMAS及IGS各电离层分析中心发布的全球电离层TEC格网产品,进行了精度比较分析,结果表明:iGMAS与IGS、CODE、JPL、ESOC、UPC等IGS电离层工作组发布的全球电离层TEC格网产品,在全球、不同纬度带和欧洲等不同区域均表现出较高的一致性和强相关性,互差为0~2.0 TECU;JPL分析中心GIM的内符合精度约为2.5 TECU,iGMAS、IGS、CODE、ESOC和UPC等分析中心GIM的内符合精度均小于1.5 TECU;在2~8 TECU的精度范围内,iGMAS全球电离层TEC格网产品的精度总体与IGS、CODE、JPL、ESOC、UPC等IGS电离层工作组的精度相当。 相似文献
11.
An approach to modeling the regional ionospheric total electron content (TEC) based on spherical cap harmonic analysis is
presented. This approach not only provides a better regional TEC mapping accuracy, but also the capability for ionospheric
model prediction based on spectrum analysis and least squares collocation. Unlike conventional approaches, which predict the
immediate TEC with models using current observations, the spherical cap harmonic approach utilizes models using past observations
to predict a model which will provide future TEC values. A significant advantage in comparison with conventional approaches
is that the spherical cap harmonic approach can be used to predict the long-term TEC with reasonable accuracy. This study
processes a set of GPS data with an observation time span of 1 year from two GPS networks in China. The TEC mapping accuracy
of the spherical cap harmonic model is compared with the polynomial model and the global ionosphere model from IGS. The results
show that the spherical cap harmonic model has a better TEC mapping accuracy with smoother residual distributions in both
temporal and spatial domains. The TEC prediction with the spherical cap harmonic model has been investigated for both short-
and long-term intervals. For the short-term interval, the prediction accuracies for the latencies of 1-day, 2-days, and 3-days
are 2.5 TECU, 3.5 TECU, and 4.5 TECU, respectively. For the long-term interval, the prediction accuracy is 4.5 TECU for a
2-month latency. 相似文献
12.
为了分析单站区域电离层总电子含量(total electron content,TEC)模型的适用范围和精度,基于2～15阶次球谐函数,分别建立了欧洲区域16个单站区域电离层TEC模型,生成了区域格网TEC,并与欧洲定轨中心(Center for Orbit Determination in Europe,CODE)、... 相似文献
13.
Wenfeng Nie Tianhe Xu Adria Rovira-Garcia José Miguel Juan Zornoza Jaume Sanz Subirana Guillermo González-Casado Wu Chen Guochang Xu 《GPS Solutions》2018,22(3):85
The calibration errors on experimental slant total electron content (TEC) determined with global positioning system (GPS) observations is revisited. Instead of the analysis of the calibration errors on the carrier phase leveled to code ionospheric observable, we focus on the accuracy analysis of the undifferenced ambiguity-fixed carrier phase ionospheric observable determined from a global distribution of permanent receivers. The results achieved are: (1) using data from an entire month within the last solar cycle maximum, the undifferenced ambiguity-fixed carrier phase ionospheric observable is found to be over one order of magnitude more accurate than the carrier phase leveled to code ionospheric observable and the raw code ionospheric observable. The observation error of the undifferenced ambiguity-fixed carrier phase ionospheric observable ranges from 0.05 to 0.11 total electron content unit (TECU) while that of the carrier phase leveled to code and the raw code ionospheric observable is from 0.65 to 1.65 and 3.14 to 7.48 TECU, respectively. (2) The time-varying receiver differential code bias (DCB), which presents clear day boundary discontinuity and intra-day variability pattern, contributes the most part of the observation error. This contribution is assessed by the short-term stability of the between-receiver DCB, which ranges from 0.06 to 0.17 TECU in a single day. (3) The remaining part of the observation errors presents a sidereal time cycle pattern, indicating the effects of the multipath. Further, the magnitude of the remaining part implies that the code multipath effects are much reduced. (4) The intra-day variation of the between-receiver DCB of the collocated stations suggests that estimating DCBs as a daily constant can have a mis-modeling error of at least several tenths of 1 TECU. 相似文献
14.
Determining receiver biases in GPS-derived total electron content in the auroral oval and polar cap region using ionosonde measurements 总被引：2，自引：1，他引：1
David R. Themens P. T. Jayachandran R. B. Langley J. W. MacDougall M. J. Nicolls 《GPS Solutions》2013,17(3):357-369
Global Positioning System (GPS) total electron content (TEC) measurements, although highly precise, are often rendered inaccurate due to satellite and receiver differential code biases (DCBs). Calculated satellite DCB values are now available from a variety of sources, but receiver DCBs generally remain an undertaking of receiver operators and processing centers. A procedure for removing these receiver DCBs from GPS-derived ionospheric TEC at high latitudes, using Canadian Advanced Digital Ionosonde (CADI) measurements, is presented. Here, we will test the applicability of common numerical methods for estimating receiver DCBs in high-latitude regions and compare our CADI-calibrated GPS vertical TEC (vTEC) measurements to corresponding International GNSS Service IONEX-interpolated vTEC map data. We demonstrate that the bias values determined using the CADI method are largely independent of the topside model (exponential, Epstein, and α-Chapman) used. We further confirm our results via comparing bias-calibrated GPS vTEC with those derived from incoherent scatter radar (ISR) measurements. These CADI method results are found to be within 1.0 TEC units (TECU) of ISR measurements. The numerical methods tested demonstrate agreement varying from within 1.6 TECU to in excess of 6.0 TECU when compared to ISR measurements. 相似文献
15.
针对区域电离层变化情况较为复杂,所确定的电离层模型系数难以反映其短时间内的变化情况问题,该文提出了利用旋转地图内插结合曲面拟合模型实现区域电离层实时监测方法。采用旋转地图内插IGS提供的电离层数据,能够有效补偿电离程度与太阳位置的强相关性,提高总电子含量内插精度;基于曲面拟合模型对区域电离层进行实时监测,实现了模型系数的实时更新。利用JSCORS网的双频观测数据,采用曲面拟合模型建立了实时的区域电离层监测模型,数据计算结果表明,其网内外精度分别优于0.81TECU和0.96TECU。 相似文献
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The Global Positioning System (GPS) satellite differential code bias (DCB) should be precisely calibrated when obtaining ionospheric slant total electron content (TEC). So far, it is ground-based GPS observations that have been used to estimate GPS satellite DCB. With the increased Low Earth Orbit (LEO) missions in the near future, the real-time satellite DCB estimation is a crucial factor in real-time LEO GPS data applications. One alternative way is estimating GPS DCB based on the LEO observations themselves, instead of using ground observations. We propose an approach to estimate the satellite DCB based on Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) and Challenging Minisatellite Payload (CHAMP) GPS observations during the years 2002–2012. The results have been validated through comparisons with those issued by Center for Orbit Determination in Europe (CODE). The evaluations indicate that: The approach can estimate satellite DCB in a reasonable way; the DCB estimated based on CHAMP observations is much better than those on COSMIC observations; the accuracy and precision of DCB show a possible dependency on the ionospheric ionization level. This method is significance for the real-time processing of LEO-based GNSS TEC data from the perspective of real-time applications. 相似文献
18.
Compensation for differential code bias (DCB) is necessary because it is the major source of errors in total electron content (TEC) measurements. The DCB estimation performance is degraded when only the regional GPS network is used. Because DCB estimation is highly correlated with ionospheric modeling, this degradation is particularly evident for measurements concentrated in an area of high TEC concentration. This study proposes a DCB estimation method that uses the long-term stability of the DCB to improve the estimation performance of the regional GPS network. We estimate satellite DCBs by assuming their constancy over seven months. This extended period increases the number of measurements used in DCB estimation and changes the local time distribution of collected measurements. As a result, the unbalanced distribution of specific ionospheric conditions disappears. Tests are performed using both global and regional networks, and the estimation performance is evaluated based on the position error and pseudorange residuals. First, the difference between the global and regional networks when using the conventional method is analyzed. Second, proposed methods are applied to regional networks. The proposed method can improve the DCB estimation performance, and the results are similar to those obtained using one-day global network data. 相似文献