The impact of magnetic storms on GPS receiver performance

被引:0
|
作者
S. H. Skone
机构
[1] Department of Geomatics Engineering,
[2] University of Calgary,undefined
[3] 2500 University Drive NW,undefined
[4] Calgary,undefined
[5] Alberta,undefined
[6] Canada T2N 1N4 e-mail: sskone@ensu.ucalgary.ca; Tel.: +1-403-220-7589; Fax: +1-403-284-1980,undefined
来源
Journal of Geodesy | 2001年 / 75卷
关键词
Key words: Positioning – GPS – Ionosphere – Scintillations;
D O I
暂无
中图分类号
学科分类号
摘要
 During the past decade, geodetic measurements have been greatly improved through the use of space geodesy techniques based on the global positioning system (GPS). The GPS allows for precise surveys, where centimetre-level accuracies may be obtained through differential carrier phase-based positioning algorithms. GPS positioning techniques often rely on the availability of dual-frequency data for formation of ionosphere-free and widelane observables (in the case of ambiguity resolution). While GPS positioning results generally provide adequate accuracies for several precise positioning applications, users may experience degraded positioning accuracies over the next few years. Of particular concern are ionospheric phenomena called magnetic storms, which are characterized by an increased spatial decorrelation of ionosphere range delays and scintillation effects at low and high latitudes. During such events, degradations in differential positioning accuracies are observed, and availability of the L2 observations may be limited through loss of signal lock. The magnitude of such effects is estimated during a global magnetic storm event, and a performance comparison of two survey-grade receivers is conducted. This storm is representative of the activity at solar maximum and several years beyond.
引用
收藏
页码:457 / 468
页数:11
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