Abstract
In solar cycle 24, the strongest geomagnetic storm took place on 17 March 2015, when the geomagnetic activity index was as high as −223 nT. To verify the impact that the storm had on the Global Navigation Satellite System (GNSS)’s positioning accuracy and precision, we used 30-s observations from 15 reference stations located in Central Europe. For each of them, we applied kinematic precise point positioning (PPP) using gLAB software for the day of the storm and, for comparison, for a selected quiet day (13 March 2015). Based on the conducted analyses, we found out that the position root mean square (RMS) values on the day of the geomagnetic storm were significantly high and amounted to several dozen centimeters. The average RMS for the altitude coordinates was 0.58 m between 12:00 and 24:00 (GPS time), and 0.37 and 0.26 m for directions North and East, respectively. The compromised accuracy level was caused by a sudden decrease in the number of satellites used for calculations. This was due to a high number of cycle slips (CSs) detected during this period. The occurrence of these effects was strictly correlated with the appearance of traveling ionospheric disturbances (TIDs). This was proven by analyzing changes in the total electron content (TEC) estimated for each station–satellite pair.
Highlights
The ionosphere is a layer of the Earth’s atmosphere, wherein density distribution of free electrons is heterogeneous and is determined by the intensity of solar radiation, which stimulates ionization of atoms and gas particles
traveling ionospheric disturbances (TIDs) are sudden changes in plasma density in the ionosphere causing interference in a radio signal by changing the refraction index. They can cause sudden and notable changes in total electron content (TEC), which can result in the hindered acquisition of Global Navigation Satellite System (GNSS) signals and decrease positioning accuracy and precision [12]
Similar results were obtained by Jacobsen and Andalsvik who noticed the rapid increasing of vertical position errors together with increasing rate of TEC (ROT) index (ROTI) for both precise point positioning (PPP) and real-time kinematic (RTK) techniques [18]
Summary
The ionosphere is a layer of the Earth’s atmosphere, wherein density distribution of free electrons is heterogeneous and is determined by the intensity of solar radiation, which stimulates ionization of atoms and gas particles. They can cause sudden and notable changes in TEC, which can result in the hindered acquisition of GNSS signals and decrease positioning accuracy and precision [12]. Luo et al (2018) investigated the accuracy of PPP positioning during a selected geomagnetic storm in solar cycle 24.
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