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LdT: An indicator of ionospheric activity based on statistical distributions in GNSS-derived TEC rates of change: An indicator of ionospheric activity based on statistical distributions in GNSS-derived TEC rates of change

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Abstract

Many aspects of our societies now depend upon satellite telecommunications, such as those requiring Global Navigation Satellite Systems (GNSS). GNSS is based on radio waves that propagate through the ionosphere and experience complicated propagation effects caused by inhomogeneities in its electron density. The Earth’s ionosphere forms part of the solar-terrestrial environment, and its state is determined by the spatial distribution and temporal evolution of its electron density. It varies in response to the “space weather” combination of solar activity and geomagnetic conditions. Notably, the radio waves used in satellite telecommunications suffer due to the dispersive nature of the ionospheric plasma.Scales and indices that summarise the state of the solar-terrestrial environment due to solar activity and geomagnetic conditions already exist. However, the response of the ionosphere to active geomagnetic conditions, its geoeffectiveness, and its likely impact on systems and services are not encapsulated by these. This is due to the ionosphere’s intrinsic day-to-day variability, persistent seasonal patterns, and because radio wave measurements of the ionosphere depend upon many factors. Here we develop a novel index ((Formula presented)) that describes the state of the ionosphere – as is relevant to GNSS – during specific space weather conditions. It is based on propagation disturbances in GNSS signals, and is able to characterise the spatio-temporal evolution of ionospheric disturbances. This new scale encapsulates day-to-day variability, seasonal patterns, and the geo-effective response of the ionosphere to disturbed space weather conditions; and can be applied to data from any GNSS network. It is intended that this new scale will be utilised by agencies providing space weather services, as well as by service operators to appreciate the current conditions in the ionosphere that affect GNSS, thus informing their operations.
Original languageEnglish
Number of pages16
JournalAdvances in Space Research
Early online date14 Jul 2026
DOIs
Publication statusE-pub ahead of print - 14 Jul 2026

Acknowledgements

The work at the University of Bath was supported by the UK Natural Environment Research Council (Grant No. NE/V002597/1 and Grant No. NE/X019004/1). The
KP index data were obtained from the GFZ International KP index Service (ftp://ftp.gfz-potsdam.de/pub/home/obs/); Dst data were obtained from the WDC for Geomagnetism service (https://wdc.kugi.kyoto-u.ac.jp); and RINEX data were accessed through the International GNSS Service (IGS) (https://cddis.nasa.gov/archive/gnss/products/)(Noll, 2010; Johnston et al., 2017).

Funding

The work at the University of Bath was supported by the UK Natural Environment Research Council (Grant No. NE/V002597/1 and Grant No. NE/X019004/1). The index data were obtained from the GFZ International index Service (ftp://ftp.gfz-potsdam.de/pub/home/obs/); Dst data were obtained from the WDC for Geomagnetism service (https://wdc.kugi.kyoto-u.ac.jp); and RINEX data were accessed through the International GNSS Service (IGS) (https://cddis.nasa.gov/archive/gnss/products/) (Noll, 2010, Johnston et al., 2017).

FundersFunder number
Natural Environment Research CouncilNE/X019004/1, NE/V002597/1

Keywords

  • GNSS
  • Radio propagation
  • Ionosphere

ASJC Scopus subject areas

  • Aerospace Engineering
  • Astronomy and Astrophysics
  • Geophysics
  • Atmospheric Science
  • Space and Planetary Science
  • General Earth and Planetary Sciences

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