Abstract

Medium-scale traveling ionospheric disturbances (MSTIDs) are fluctuations in the plasma density that propagate through the upper layer of the atmosphere at velocities of approximately 100 m/s and periods reaching some tens of minutes. Due to their wavelengths, MSTIDs can degrade the performance of differential positioning techniques, such as real-time kinematics (RTK) or network-RTK (NRTK). This paper defines a novel methodology as a tool for relating the errors in NRTK positioning based on an MSTIDs indicator using the second difference in time of the slant total electron content (STEC). The proposed methodology performs integer ambiguity resolution (IAR) on the undifferenced measurements instead of using double-differenced carrier-phase measurements, as it is usual in RTK and NRTK. Statistical tests are applied to evaluate the degradation in the position errors caused by the impacts of MSTIDs on RTK and NRTK positioning over a data set spanning one year gathered from the CATNET network; a dual-frequency network of fixed permanent GNSS receivers located at the mid-latitudes of northeastern Spain. With the development of the proposed methodology for measuring the position degradation, another results of the present research are the establishment of thresholds for the proposed MSTIDs index, which can be used to monitor the positioning solution and to warn users when the measurements are affected by MSTIDs events, relating the position error to MSTIDs that affect not only the user receivers but also of the reference receivers within the network.

Highlights

  • Traveling ionospheric disturbances (TIDs) are plasma density fluctuations that propagate through the ionosphere with a broad range of velocities and frequencies

  • Statistical tests are applied to evaluate the degradation in the position errors caused by the impacts of Medium-scale traveling ionospheric disturbances (MSTIDs) on real-time kinematics (RTK) and NRTK positioning over a data set spanning one year gathered from the CATNET network; a dual-frequency network of fixed permanent Global Navigation Satellite Systems (GNSS) receivers located at the mid-latitudes of northeastern Spain

  • The present contribution analyses the impacts of MSTIDs on a network of permanent geodetic receivers located at midlatitudes

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Summary

Introduction

Traveling ionospheric disturbances (TIDs) are plasma density fluctuations that propagate through the ionosphere with a broad range of velocities and frequencies. The sources of MSTIDs are not unique, MSTIDs are linked to meteorological phenomena such as neutral winds, eclipses and the solar terminator (ST), which produces atmospheric gravity waves (AGW) and manifests them as TIDs at ionospheric heights (HernándezPajares et al, 2006). Single-frequency receivers must apply ionospheric models to account for the ionospheric refraction (Rovira-Garcia et al, 2019). The effects of the frequency-dependent terms (including the ionospheric refraction) can be estimated using the geometry-free (GF) combination of code (PGF = P2 À P1) or carrier-phase measurements (LGF = L1 À L2), which cancels out the geometric part of the measurements

TECU represents an ionospheric delay of approximately
Data: the CATNET NRTK service
Methodology for obtaining unambiguous measurements in the CATNET service
Fixing carrier-phase ambiguities
Detecting MSTIDs and defining a MSTIDs activity index
Relationship of MSTIDIDX with the error in the ionospheric corrections
Relationship of MSTIDIDX with the degradation in positioning
Statistical analysis
Findings
Conclusions
Full Text
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