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电离层误差是影响单频用户机定位精度的主要误差源。卫星导航系统播发电离层模型改正参数供用户使用,模型改正精度会对定位结果产生直接影响。北斗卫星导航系统根据连续监测站实测数据,计算并发播地理坐标系下8参数Klobuchar电离层模型参数,且每2 h更新一次。为了科学评估北斗电离层模型改正效果,文中基于北斗最新观测数据,首先,以CODE提供的GIM模型作为比对基准,详细分析了不同纬度地区、不同时间段内的电离层模型改正精度;其次,分别按照以下定位模式进行计算:1)北斗单频不加电离层改正,2)北斗单频+北斗K8模型,3)北斗单频+GPS K8模型,并分析了电离层改正残差对定位结果影响大小。结果表明,北斗电离层模型改正精度在北半球优于南半球,中纬度地区改正效果最好,其改正残差RMS均值在0.6 m左右,往低纬和高纬度地区呈递减趋势;北京地区北斗单频+北斗K8模型定位精度优于GPS K8模型。 相似文献
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GEO卫星区域电离层监测分析 总被引：4，自引：1，他引：3
由于GEO卫星的静地特性,由双频观测数据获取的穿刺点垂直总电子含量(VTEC)可以充分反映电离层的时域变化,而根据地面监测站的分布,可以进一步获取VTEC的空域变化.分析根据区域卫星导航系统观测数据计算VTEC的精度,理论分析表明VTEC精度优于2 TECU.根据实测数据计算分析我国高、中、低纬度不同穿刺点电离层平时、磁暴期间的周日变化特性和2011年全年变化特性,并与IGS全球电离层图(GIM)的穿刺点插值结果进行分析比较.结果表明,两者在电离层周日和全年变化趋势上具有很好的一致性,但磁暴期间我国低纬度地区GIM误差的峰值可达29TECU,2011年全年评估结果GIM误差标准差为2～8 TECU.根据2011年的观测结果,电离层VTEC呈现出明显的半年异常现象.区域卫星导航系统为我国的电离层监测尤其是空间天气期间的电离层监测提供了新的支持. 相似文献
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冯磊 《测绘与空间地理信息》2021,44(1):134-140
随着PPP的发展与应用,对PPP误差源的研究更加精细、更加科学。电离层折射是高精度PPP的主要误差之一,国内外通用方法是用大气传播理论建立电离层修正模型。本文主要探讨了电离层对精密单点定位影响的基本理论,总结了目前常用方法;研究了Klobuchar模型的改正公式及计算方法;系统地研究了双频观测值建立消电离层延迟模型的理论和方法。使用相同时段的观测数据,将广播星历、Klobuchar模型和双频观测值改正消电离层模型的结果进行比较,发现用GPS双频观测值建立的消电离层模型的精度明显优于广播星历及Klobuchar模型。 相似文献
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GPS电离层延迟Klobuchar模型与双频数据解算值的比较与分析 总被引：10，自引：0，他引：10
电离层延迟是影响GPS绝对定位的最主要因素,但由于电离层本身的不稳定性,加上目前对其物理特性的了解还有一定的模糊性,还只能采用精度有限的经验模型对其进行描述.对于GPS实时绝对定位,GPS系统的广播星历提供了Klobuchr模型的8个系数,可以用于单频接收机的电离层延迟改正;对于双频接收机,可以利用L1,L2,C1,P2进行计算得到电离层延迟值,但应考虑到卫星发射信号时产生的两频率间的硬件延迟TGD的影响.本文采用双频伪距求得电离层延迟值,用广播星历中各颗卫星的TGD参数进行改正,再根据L1和L2双频相位值求得的历元间的电离层延迟的变化采用Hatch类滤波递推模型对其进行平滑,从而求得较准确的对应于各个历元的电离层延迟值,将其作为真值与Klobuchar模型计算值进行比较,从而研究Klobuchar模型的精度和特点,并与IGS的后处理Klobuchar模型系数求得的电离层结果进行对比分析.对双频数据计算电离层延迟的算法进行详细研究,给出Klobuchar模型的具体计算过程,用位于武汉、北京和上海的IGS跟踪站的观测数据进行实际验证和算例分析,最后给出结论. 相似文献
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不同Klobuchar模型参数的性能比较 总被引：3，自引：1，他引：2
对于GPS单频用户而言,电离层延迟是最重要的误差来源之一。GPS系统使用Klobuchar模型对电离层延迟进行改正,其改正数从370组常数中选取。目前全球分布的GPS测站可以获得高精度的全球电离层监测结果,GPS为什么不发播采用实测数据计算得到的Klobuchar模型参数呢？本文针对这一问题进行分析。首先对欧洲定轨中心CODE提供的全球电离层图GIM预报COPG电离层进行精度评估,然后根据COPG电离层进行Klobuchar模型参数拟合并利用IGS提供的事后高精度电离层图进行精度分析,最后将不同的电离层模型参数应用于单点定位以评估其对单频用户的影响。分析结果表明：受8参数的Klobuchar模型本身结构限制,采用全球实测数据计算的电离层模型参数与导航电文中发播的电离层模型精度相当,为55%左右。而仅采用地磁纬度45oS以北的数据拟合得到的模型参数,其电离层改正精度有明显提升,可达65%左右,但其对单频用户定位精度改善不明显。本文研究结果为我国全球电离层建模提供参考。 相似文献
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电离层延迟是影响导航定位精度的最主要因素。北斗卫星导航系统采用Klobuchar模型修正单频接收机用户的电离层延迟误差,对于双频接收机,可以利用不同频率信号的伪距观测数据解算得到电离层延迟值。为比较两种方法在天津地区的电离层延迟修正效果,利用NovAtel GPStation6接收机(GNSS电离层闪烁和TEC监测接收机)采集到的卫星实测数据进行计算。以国际全球导航卫星系统服务组织(IGS)发布的全球电离层格网数据为参考,对两种方法的修正效果进行比较分析。结果表明,在天津地区,利用双频观测值解算电离层延迟比Klobuchar模型计算结果更加精确,且平均每天的修正值达到IGS发布数据的82.11％,比Klobuchar模型计算值高948％ 相似文献
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The in situ measurements of electron contents from GRACE K-band (dual-frequency) ranging system and CHAMP planar Langmuir
probe were used to validate the international reference ionosphere (IRI) models. The comparison using measurements from year
2003 to 2007 shows a general agreement between data and the model outputs. The improvement in the newer IRI model (IRI-2007)
is evident with the measurements from the GRACE satellites orbiting at the higher altitude. We present the comparison between
the models and data comprehensively for various cases in solar activity, local time, season, and latitude. The IRI models
do not well predict the electron density in the years 2006 and later, when the solar activity is extremely low. The IRI models
generally overestimate the electron density during local winter while they underestimate during local summer. In the equatorial
region, the large difference at local sunrise lasts for all years and all seasons. The IRI models do not perform well in predicting
the anomaly in the polar region such as the Weddell Sea Anomaly. These discrepancies are likely due to smoothed (12-month
averaged) solar activity indices used in the IRI models and due to insufficient spherical harmonic representation not able
to capture small spatial scales. In near future, further improvement on the IRI models is expected by assimilating those in
situ satellite data by implementing higher resolution (spatial and temporal) parameterizations. 相似文献
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Combination of different space-geodetic observations for regional ionosphere modeling 总被引：2，自引：1，他引：1
Denise Dettmering Michael Schmidt Robert Heinkelmann Manuela Seitz 《Journal of Geodesy》2011,85(12):989-998
Most of the space-geodetic observation techniques can be used for modeling the distribution of free electrons in the Earth’s
ionosphere. By combining different techniques one can take advantage of their different spatial and temporal distributions
as well as their different observation characteristics and sensitivities concerning ionospheric parameter estimation. The
present publication introduces a procedure for multi-dimensional ionospheric modeling. The model consists of a given reference
part and an unknown correction part expanded in terms of B-spline functions. This approach is used to compute regional models
of Vertical Total Electron Content (VTEC) based on the International Reference Ionosphere (IRI 2007) and GPS observations
from terrestrial Global Navigation Satellite System (GNSS) reference stations, radio occultation data from Low Earth Orbiters
(LEOs), dual-frequency radar altimetry measurements, and data obtained by Very Long Baseline Interferometry (VLBI). The approach
overcomes deficiencies in the climatological IRI model and reaches the same level of accuracy than GNSS-based VTEC maps from
IGS. In areas without GNSS observations (e.g., over the oceans) radio occultations and altimetry provide valuable measurements
and further improve the VTEC maps. Moreover, the approach supplies information on the offsets between different observation
techniques as well as on their different sensitivity for ionosphere modeling. Altogether, the present procedure helps to derive
improved ionospheric corrections (e.g., for one-frequency radar altimeters) and at the same time it improves our knowledge
on the Earth’s ionosphere. 相似文献
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Ionospheric delay is a dominant error source in Global Navigation Satellite System (GNSS). Single-frequency GNSS applications require ionospheric correction of signal delay caused by the charged particles in the earth’s ionosphere. The Chinese Beidou system is developing its own ionospheric model for single-frequency users. The number of single-frequency GNSS users and applications is expected to grow fast in the next years in China. Thus, developing an appropriate ionospheric model is crucially important for the Chinese Beidou system and worldwide single-frequency Beidou users. We study the performance of five globally accessible ionospheric models Global Ionospheric Map (GIM), International Reference Ionosphere (IRI), Parameterized Ionospheric Model (PIM), Klobuchar and NeQuick in low- and mid-latitude regions of China under mid-solar activity condition. Generally, all ionospheric models can reproduce the trend of diurnal ionosphere variations. It is found that all the models have better performances in mid-latitude than in low-latitude regions. When all the models are compared to the observed total electron content (TEC) data derived from GIM model, the IRI model (2012 version) has the best agreement with GIM model and the NeQuick has the poorest agreement. The RMS errors of the IRI model using the GIM TEC as reference truth are about 3.0–10.0 TECU in low-latitude regions and 3.0–8.0 TECU in mid-latitude regions, as observed during a period of 1 year with medium level of solar activity. When all the ionospheric models are ingested into single-frequency precise point positioning (PPP) to correct the ionospheric delays in GPS observations, the PIM model performs the best in both low and mid-latitudes in China. In mid-latitude, the daily single-frequency PPP accuracy using PIM model is ~10 cm in horizontal and ~20 cm in up direction. At low-latitude regions, the PPP error using PIM model is 10–20 cm in north, 30–40 cm in east and ~60 cm in up component. The single-frequency PPP solutions indicate that NeQuick model has the lowest accuracy among all the models in both low- and mid-latitude regions of China. This study suggests that the PIM model may be considered for single-frequency GNSS users in China to achieve a good positioning accuracy in both low- and mid-latitude regions. 相似文献
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Global Ionosphere Maps of VTEC from GNSS,satellite altimetry,and formosat-3/COSMIC data 总被引：1，自引：1，他引：0
For space geodetic techniques, operating in microwave band, ionosphere is a dispersive medium; thus signals traveling through
this medium are in the first approximation affected proportional to inverse of the square of their frequencies. This effect
allows gaining information about the parameters of the ionosphere in terms of Total Electron Content (TEC) or the electron
density (N
e
). TEC or electron density can then be expressed by means of spherical harmonic base functions to provide a Global Ionosphere
Map (GIM). The classical input data for development of GIMs are obtained from dual-frequency observations carried out at Global
Navigation Satellite Systems (GNSS) stations. However, GNSS stations are in-homogeneously distributed around the world, with
large gaps particularly over the oceans; this fact reduces the precision of the GIM over these areas. On the other hand, dual-frequency
satellite altimetry missions such as Jason-1 provide information about the ionosphere precisely above the oceans; and furthermore
Low Earth Orbiting (LEO) satellites, such as Formosat-3/COSMIC (F/C) provide well-distributed information of ionosphere globally.
This study investigates on global modeling of TEC through combining GNSS and satellite altimetry data with global TEC data
derived from the occultation measurements of the F/C mission. The combined GIMs of vertical TEC (VTEC) show a maximum difference
of 1.3–1.7 TEC units (TECU) with respect to the GNSS-only GIMs in the whole day. The root mean square error (RMS) maps of
combined solution show a reduction of about 0.1 TECU in the whole day. This decrease of RMS can reach up to 0.5 TECU in areas
where no or few GNSS observations are available, but high number of F/C measurement is carried out. This proves that the combined
GIMs provide a more homogeneous global coverage and higher reliability than results of each single method. All comparisons
and validations made within this study provide vital information regarding combination and integration of various observation
techniques in the Global Geodetic Observing System of the International Association of Geodesy. 相似文献
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Application of the TaiWan Ionospheric Model to single-frequency ionospheric delay corrections for GPS positioning 总被引：2，自引：2，他引：0
The performance of a three-dimensional ionospheric electron density model derived from FormoSat3/COSMIC GPS Radio Occultation measurements, called the TaiWan Ionosphere Model (TWIM), in removing the ionospheric delays in single-frequency pseudorange observations is presented. Positioning results using TWIM have been compared with positioning results using other ionospheric models, such as the Klobuchar (KLOB) and the global ionospheric model (GIM). C/A code pseudoranges have been observed at three International GPS Service reference stations that are representative of mid-latitude (BOR1 and IRKJ) and low-latitude (TWTF) regions of the ionosphere. The observations took place during 27 geomagnetically quiet days from April 2010 to October 2011. We perform separate solutions using the TWIM, KLOB, GIM ionospheric models and carry out a solution applying no ionospheric correction at all. We compute the daily mean horizontal errors (DMEAN) and the daily RMS (DRMS) for these solutions with respect to the published reference station coordinates. It has demonstrated that TEC maps generate using the TWIM exhibit a detailed structure of the ionosphere, particularly at low-latitude region, whereas the Klobuchar and the GIM only provide the basic diurnal and geographic features of the ionosphere. Also, it is shown that even for lower satellite elevations, the TWIM provides better positioning than the Klobuchar and GIM models. Specifically, using TWIM, the difference of the uncorrected solution (no ionospheric correction), and the other solutions, relative to the uncorrected solution, is 45 % for the mean horizontal error (DMEAN) and 42 % for the horizontal root-mean-square error (DRMS). Using Klobuchar and GIM, the percent for DMEAN only reaches to about 12 % and 3 %, while the values for the DRMS are only 12 and 4 %, respectively. In the vertical direction, all models have a percentage of about 99 and 70 % for the mean vertical error (VMEAN) and vertical root-mean-square error (VRMS), respectively. These percentages show the greater impact of TWIM on the ionospheric correction compared to the other models. In at least 40 % of the observed days and across all stations, TWIM has the smallest DMEAN, VMEAN, DRMS, and VRMS daily values. These values reach 100 % at station TWTF. This shows the overall performance of TWIM is better than the Klobuchar and GIM. 相似文献
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The majority of navigation satellite receivers operate on a single frequency. They compensate for the ionospheric delay using
either an ionospheric model which typically only corrects for 50% of the delay or a thin-shell map of the ionosphere. A 4D
tomographic imaging technique is used to map the free electron density over the full-height of the ionosphere above North
America during autumn 2003. The navigation solutions computed using correction based upon the thin-shell and the full-height
maps are compared in this paper. The maps are used to calculate the excess propagation delay on the L1 frequency experienced
by GPS receivers at selected locations across North America. The excess delay is applied to correct the single-frequency pseudorange
observations at each location, and the improvements to the resulting positioning are calculated. It is shown that the thin-shell
and full-height maps perform almost as well as a dual-frequency carrier-smoothed benchmark and for most receivers better than
the unfiltered dual-frequency benchmark. The full-height corrections perform well and are considerably better than thin-shell
corrections under extreme storm conditions. 相似文献
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中国近海1992～1998海平面变化监测与分析 总被引：14，自引：1，他引：13
利用Topex/Poseidon和ERS-1卫星测高资料采用“共线”法计算出1992-10～1998-06中国近海海域海平面及其变化。在扣除T/P卫星测高仪的零点漂移影响后,发现与全球海平面上升率(+2.1±1.3)mm/a相比,不同海域的海平面变化趋势大不相同,黄、东、南海的海平面年变化率分别为：(+3.44±0.61)mm/a,(+3.12±0.47)mm/a,(-1.41±0.48)mm/a。从海平面变化异常中可以看出1993,1994,1997～1998年3次El Nino异常对中国近海海域海平面的影响是南海海域最大,东海次之,黄海最小。除了对海平面进行传统的频谱分析外,还进行了多分辨率的小波分析,还发现在上述3个海域中除了年周期变化较为稳定外,半年及季节(100 d)周期项存在着时间漂移。此外,在上述3个海域还存在着明显的两个月(62 d)周期的变化,其激发原因在此做了初步探讨。 相似文献
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Patricia Doherty joins the regular contributors of this column to discuss the correlation between measurements of solar 10.7
cm radio flux and ionospheric range delay effects on GPS. Mrs. Doherty has extensive experience in the analysis of ionospheric
range delays from worldwide systems and in the utilization and development of analytical and theoretical models of the Earth's
ionosphere.
Ionospheric range delay effects on GPS and other satellite ranging systems are directly proportional to the Total Electron
Content (TEC) encountered along slant paths from a satellite to a ground location. TEC is a highly variable and complex parameer
that is a function of geographic location, local time, season, geomagnetic activity, and solar activity. When insufficiently
accounted for, ionospheric TEC can seriously limit the performance of satellite ranging applications. Since the ionosphere
is a dispersive medium, dual-frequency Global Positoning System (GPS) users can make automatic corrections for ionospheric
range delay by computing the apparent difference in the time delays between the two signals. Single-frequency GPS users must
depend on alternate methods to account for the ionospheric range delay. Various models of the ionosphere have been used to
provide estimates of ionospheric range delay. These models range from the GPS system's simple eight-coefficient algorithm
designed to correct for approximately 50% rms of the TEC, to state-of-the-art models derived from physical first principles,
which can correct for up to 70 to 80% rms of the TEC but at a much greater computational cost.
In an effort to improve corrections for the day-to-day variability of the ionosphere, some attempts have been made to predict
the TEC by using the daily values of solar 10.7 cm radio flux (F10,7). The purpose of this article is to show that this type of prediction is not useful due to irregular, and sometimes very
poor, correlation between daily values of TEC and F10.7. Long-term measurements of solar radio flux, however, have been shown to be well correlated with monthly mean TEC, as well
as with the critical frequency of the inonospheric F2 region (foF2), which is proportional to the electron density at the
peak of the ionospheric F2 region. ? 2000 John Wiley & Sons, Inc. 相似文献
19.
Raul Orus Perez 《Journal of Geodesy》2017,91(4):397-407
For single-frequency users of the global satellite navigation system (GNSS), one of the main error contributors is the ionospheric delay, which impacts the received signals. As is well-known, GPS and Galileo transmit global models to correct the ionospheric delay, while the international GNSS service (IGS) computes precise post-process global ionospheric maps (GIM) that are considered reference ionospheres. Moreover, accurate ionospheric maps have been recently introduced, which allow for the fast convergence of the real-time precise point position (PPP) globally. Therefore, testing of the ionospheric models is a key issue for code-based single-frequency users, which constitute the main user segment. Therefore, the testing proposed in this paper is straightforward and uses the PPP modeling applied to single- and dual-frequency code observations worldwide for 2014. The usage of PPP modeling allows us to quantify—for dual-frequency users—the degradation of the navigation solutions caused by noise and multipath with respect to the different ionospheric modeling solutions, and allows us, in turn, to obtain an independent assessment of the ionospheric models. Compared to the dual-frequency solutions, the GPS and Galileo ionospheric models present worse global performance, with horizontal root mean square (RMS) differences of 1.04 and 0.49 m and vertical RMS differences of 0.83 and 0.40 m, respectively. While very precise global ionospheric models can improve the dual-frequency solution globally, resulting in a horizontal RMS difference of 0.60 m and a vertical RMS difference of 0.74 m, they exhibit a strong dependence on the geographical location and ionospheric activity. 相似文献
20.
从2017年1月开始，北斗系统在播发基本导航电文的同时，提供了包含实时轨道改正数、钟差改正数、电离层格网改正数和分区综合改正数四重广域差分参数，使得系统具备了基于系统广播的电文参数实现广域单站实时动态分米级定位的能力。实际应用表明，北斗系统播发的分区综合改正数存在中断的情况，使得实时定位存在因重新收敛而造成跳变的情况。本文分析了分区中断期间定位跳变产生的原因，提出一种适用于分区切换的广域差分分米级定位算法。采用中国境内7个北斗测站10 d的静态数据和车载动态数据对新算法进行评估验证。结果表明，在分区改正数中断的情况下，分区切换算法得到的坐标误差与使用连续分区综合改正数结果一致，双频动态定位水平和高程方向分别小于0.3 m和0.5 m，平均三维定位精度优于0.5 m；车载实时动态定位测试中，分区切换前后的单双频定位精度不受切换影响，与切换前保持一致。分区切换算法有效保证了分区改正数中断后北斗广域分米级实时动态定位的连续性。 相似文献