南极BDS/GNSS精密单点定位性能评估

Performance Evaluation of Antarctic BDS/GNSS Precise Point Positioning

  • 摘要: 当前我国极地科学考察对高精度全球导航卫星定位(global navigation satellite system,GNSS)服务需求日益迫切。基于南极国际GNSS服务组织测站,以及中国第41次南极科学考察期间昆仑站(KUNL)和泰山站(TAIS)的GNSS观测数据,从卫星可见数、定位精度、初始化时间及模糊度固定率等方面,系统评估了2024年3月1日—10日北斗卫星导航系统(BeiDou navigation satellite system,BDS)/GNSS在南极高纬度地区的精密单点定位(precise point positioning,PPP)性能,并对比了2024年3月24日磁暴事件对极区PPP定位性能的影响。结果表明,南极CAS1、DAV1、TAIS和KUNL测站上空可见卫星数达50~60颗,单频标准单点定位(standard point positioning,SPP)平均定位精度约为2.7~3.3 m,双频SPP平均定位精度提升至2.0 m左右。与SPP相比,各个测站在单BDS或单Galileo系统条件下,其静态和动态PPP固定解定位精度可达厘米级,而TAIS和KUNL站单GPS系统静态PPP固定解定位误差为分米级。多系统融合(GPS/BDS/Galileo)可明显改善PPP定位精度,缩短初始化时间,并提升模糊度固定率;其中CAS1和DAV1站GPS/BDS/Galileo多系统融合PPP固定解平均初始化时间可缩短至12 min左右。相比之下,动态PPP定位性能总体上不及静态PPP。此外,磁暴期间南极不同测站各系统的PPP固定解平均三维定位误差明显增大,初始化时间也显著变长,这与磁暴期间电离层扰动增强有关。

     

    Abstract:
    Objectives With the continuous expansion of China's polar scientific expeditions, the demand for reliable and high-precision global navigation satellite system (GNSS) positioning services in Antarctica has become increasingly prominent. However, the Antarctic inland region is characterized by extremely harsh environmental conditions, sparse infrastructure, and limited communication capability, making it difficult to establish dense continuous GNSS observation networks or ground-based augmentation systems. Under these conditions, precise point positioning (PPP), which enables high-precision positioning using a single receiver with precise satellite orbit and clock products, provides an important technical solution for Antarctic inland applications.
    Methods Based on GNSS observations from Antarctic international GNSS service (IGS) stations, including CAS1 and DAV1, as well as rare GNSS data collected at China's Kunlun station (KUNL) and Taishan station (TAIS) during the 41st Chinese national antarctic research expedition, this study systematically evaluates the positioning performance of BeiDou navigation satellite system(BDS)/GNSS in the Antarctic high-latitude region, with particular focus on China's inland Antarctic stations. Geomagnetically quiet days from March 1 to March 10, 2024, and the strong geomagnetic storm event on March 24, 2024, were selected for comparative analysis. Standard point positioning (SPP), undifferenced and uncombined PPP float solutions, and PPP ambiguity resolution (PPP-AR) solutions were assessed under both static and simulated kinematic modes for single-system GPS, BDS, Galileo, and multi-system combinations of GPS/BDS and GPS/BDS/Galileo. Positioning accuracy, initialization time, ambiguity fix rate, visible satellite number, geometric dilution of precision (GDOP), and the rate of total electron content index (ROTI) were comprehensively analyzed.
    Results The results indicate that multi-GNSS observations significantly enhance satellite availability in Antarctica, with approximately 50-60 visible satellites observed at Antarctic stations. The positioning accuracy of single-frequency SPP is approximately 2.7-3.3 m, while dual-frequency SPP improves the accuracy to about 2.0 m, highlighting the advantage of dual-frequency observations in polar environments. Compared with SPP, static PPP ambiguity resolution (PPP-AR) solutions achieve decimeter- to centimeter-level accuracy, demonstrating the feasibility of PPP for high-precision Antarctic positioning. BDS and Galileo outperform GPS in both positioning accuracy and ambiguity fixing capability. Multi-GNSS integration, especially the GPS/BDS/Galileo combination, further improves positioning stability and shortens initialization time, with the initialization time of the CAS1 and DAV1 reduced to about 12 min under favorable conditions. The average PPP-AR initialization times of high-latitude stations such as TAIS and KUNL are generally longer than those of the relatively lower-latitude CAS1 and DAV1 stations. This may be mainly attributed to the combined effects of satellite geometry, and observation noise in ice-snow environments in the high-latitude inland Antarctic region. Compared with static PPP, the overall performance in terms of average initialization time and average three-dimensional positioning error of simulated kinematic PPP-AR is degraded. For the four Antarctic stations, both kinematic and static PPP float resolution achieve centimeter-level average 3D positioning accuracy. The average convergence times of static and kinematic PPP float solutions at CAS1 and DAV1 are less than 15 minutes, whereas TAIS and KUNL exhibit longer average convergence time. During the geomagnetic storm, PPP positioning errors increased and ROTI values fluctuated markedly at Antarctic stations, suggesting that enhanced polar ionospheric disturbances adversely affect PPP performance.
    Conclusions Overall, this study demonstrates that BDS/GNSS PPP, particularly multi-GNSS PPP, is an effective and reliable approach for high-precision positioning in Antarctic inland scientific expeditions. Meanwhile, the influence of space weather should be carefully considered in practical GNSS applications in polar regions.

     

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