An EISCAT UHF/ESR Experiment That Explains How Ionospheric Irregularities Induce GPS Phase Fluctuations at Auroral and Polar Latitudes

H. M. John, B. Forte, I. Astin, T. Allbrook, A. Arnold, B. C. Vani, I. Häggström, H. Sato

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4 Citations (SciVal)

Abstract

A limitation to the use of Global Navigation Satellite System (GNSS) for precise and real-time services is introduced by irregularities in the ionospheric plasma density. An EISCAT UHF/ESR experiment was conducted to characterize the effect of electron density irregularities on temporal fluctuations in TEC along directions transverse to GPS ray paths in the high latitudes ionosphere. Two representative case studies are described: Enhancements in temporal TEC fluctuations originating (a) in the auroral ionosphere following auroral particle precipitation and (b) in the polar ionosphere following the drift of a polar patch as well as particle precipitation. The results indicate that the origin of enhancements in TEC fluctuations is due to the propagation through large-to-medium scale irregularities (i.e., ranging from few kilometres in the E region to few tens of kilometres in the F region) and occurring over spatial distances of up to approximately (Formula presented.) in the E region and up to approximately (Formula presented.) in the F region with a patchy distribution. Furthermore, the results indicate that enhancements in TEC fluctuations produced by polar plasma patches and particle precipitation occur over similar temporal scales, thus explaining the overall observation of higher phase scintillation indices in the high-latitude ionosphere. The similarity in the temporal scales over which enhancements in TEC fluctuations occur in the presence of both particle precipitation and plasma patches suggests an intrinsic limitation in the monitoring and tracking of plasma patches through ground GNSS observations.

Original languageEnglish
Article numbere2020RS007236
JournalRadio Science
Volume56
Issue number9
Early online date26 Aug 2021
DOIs
Publication statusPublished - 10 Sept 2021

Bibliographical note

Funding Information:
H. M. John wishes to thank Petroleum Technology Development Fund (PTDF), Abuja, Nigeria for providing for the PhD research scholarship and Department of Electronic and Electrical Engineering, University of Abuja, Nigeria for allowing me on a study‐leave. The EISCAT campaigns were supported through the EISCAT UK time allocation (funded through UK Natural Environment Research Council). This work was also supported by Natural Environment Research Council (NERC) (grant number NE/R009082/1). EISCAT is an international association supported by research organizations in China (CRIRP), Finland (SA), Japan (NIPR and STEL), Norway (NFR), Sweden (VR), and the United Kingdom (NERC). The authors thank the institutes who maintain the IMAGE Magnetometer Array: Tromsø Geophysical Observatory of UiT the Arctic University of Norway (Norway), Finnish Meteorological Institute (Finland), Institute of Geophysics Polish Academy of Sciences (Poland), GFZ German Research Centre for Geosciences (Germany), Geological Survey of Sweden (Sweden), Swedish Institute of Space Physics (Sweden), Sodankylä Geophysical Observatory of the University of Oulu (Finland), and Polar Geophysical Institute (Russia) ( https://space.fmi.fi/image/www/index.php ).

Funding Information:
H. M. John wishes to thank Petroleum Technology Development Fund (PTDF), Abuja, Nigeria for providing for the PhD research scholarship and Department of Electronic and Electrical Engineering, University of Abuja, Nigeria for allowing me on a study-leave. The EISCAT campaigns were supported through the EISCAT UK time allocation (funded through UK Natural Environment Research Council). This work was also supported by Natural Environment Research Council (NERC) (grant number NE/R009082/1). EISCAT is an international association supported by research organizations in China (CRIRP), Finland (SA), Japan (NIPR and STEL), Norway (NFR), Sweden (VR), and the United Kingdom (NERC). The authors thank the institutes who maintain the IMAGE Magnetometer Array: Troms? Geophysical Observatory of UiT the Arctic University of Norway (Norway), Finnish Meteorological Institute (Finland), Institute of Geophysics Polish Academy of Sciences (Poland), GFZ German Research Centre for Geosciences (Germany), Geological Survey of Sweden (Sweden), Swedish Institute of Space Physics (Sweden), Sodankyl? Geophysical Observatory of the University of Oulu (Finland), and Polar Geophysical Institute (Russia) (https://space.fmi.fi/image/www/index.php).

Publisher Copyright:
© 2021. The Authors.

Keywords

  • Auroral and polar irregularities
  • EISCAT UHF/ESR
  • GNSS signals
  • particle precipitation and patches
  • TEC fluctuations

ASJC Scopus subject areas

  • Condensed Matter Physics
  • Earth and Planetary Sciences(all)
  • Electrical and Electronic Engineering

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