Influence of different types of ionospheric disturbances on GPS signals at polar latitudes
The comparative research of the influence of different types of auroral particle precipitation and polar cap patches (PCPs) on the global positioning system (GPS) signals disturbances in the polar ionosphere was done. For this purpose, we use the GPS scintillation receivers at Ny-Ålesund and Skibotn...
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2021
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ftdoajarticles:oai:doaj.org/article:e4d3f2f5fc0f4b9f9069605409423c8d 2023-05-15T16:04:39+02:00 Influence of different types of ionospheric disturbances on GPS signals at polar latitudes V. B. Belakhovsky Y. Jin W. J. Miloch 2021-07-01T00:00:00Z https://doi.org/10.5194/angeo-39-687-2021 https://doaj.org/article/e4d3f2f5fc0f4b9f9069605409423c8d EN eng Copernicus Publications https://angeo.copernicus.org/articles/39/687/2021/angeo-39-687-2021.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.5194/angeo-39-687-2021 0992-7689 1432-0576 https://doaj.org/article/e4d3f2f5fc0f4b9f9069605409423c8d Annales Geophysicae, Vol 39, Pp 687-700 (2021) Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 article 2021 ftdoajarticles https://doi.org/10.5194/angeo-39-687-2021 2022-12-31T05:56:59Z The comparative research of the influence of different types of auroral particle precipitation and polar cap patches (PCPs) on the global positioning system (GPS) signals disturbances in the polar ionosphere was done. For this purpose, we use the GPS scintillation receivers at Ny-Ålesund and Skibotn, operated by the University of Oslo. The presence of the auroral particle precipitation and polar cap patches was determined by using data from the EISCAT 42m radar on Svalbard. The optical aurora observations in 557.7 and 630.0 nm spectrum lines on Svalbard were used as well for the detection of ionospheric disturbances. The cusp identification was done with using SuperDARN (Hankasalmi) data. We consider events when the simultaneous EISCAT 42m and GPS data were available for the years 2010–2017, and in this paper we present, in detail, typical examples describing the overall picture, and we present the statistics for 120 events. We considered the dayside/cusp precipitation, substorm precipitation, daytime and nighttime PCPs, and precipitation associated with the interplanetary shock wave arrival. We demonstrate that substorm-associated precipitation (even without PCPs) can lead to a strong GPS phase ( σ ϕ ) scintillations up to ∼ 1.5–3 radians, which is much stronger than those usually produced by other types of considered ionosphere disturbances. The value of the substorm-phase scintillations in general correlate with the value of the geomagnetic field disturbance. But sometimes even a small geomagnetic substorm, when combined with the PCPs, produces quite strong phase scintillations. Cusp phase scintillations are lower than dayside PCPs scintillations. PCPs can lead to stronger ROT (rate of total electron content) variations than other types of ionosphere disturbances. So our observations suggest that the substorms and PCPs, being different types of the high-latitude disturbances, lead to the development of different types and scales of ionospheric irregularities. Article in Journal/Newspaper EISCAT Ny Ålesund Ny-Ålesund Skibotn Svalbard Directory of Open Access Journals: DOAJ Articles Svalbard Ny-Ålesund Annales Geophysicae 39 4 687 700 |
institution |
Open Polar |
collection |
Directory of Open Access Journals: DOAJ Articles |
op_collection_id |
ftdoajarticles |
language |
English |
topic |
Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 |
spellingShingle |
Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 V. B. Belakhovsky Y. Jin W. J. Miloch Influence of different types of ionospheric disturbances on GPS signals at polar latitudes |
topic_facet |
Science Q Physics QC1-999 Geophysics. Cosmic physics QC801-809 |
description |
The comparative research of the influence of different types of auroral particle precipitation and polar cap patches (PCPs) on the global positioning system (GPS) signals disturbances in the polar ionosphere was done. For this purpose, we use the GPS scintillation receivers at Ny-Ålesund and Skibotn, operated by the University of Oslo. The presence of the auroral particle precipitation and polar cap patches was determined by using data from the EISCAT 42m radar on Svalbard. The optical aurora observations in 557.7 and 630.0 nm spectrum lines on Svalbard were used as well for the detection of ionospheric disturbances. The cusp identification was done with using SuperDARN (Hankasalmi) data. We consider events when the simultaneous EISCAT 42m and GPS data were available for the years 2010–2017, and in this paper we present, in detail, typical examples describing the overall picture, and we present the statistics for 120 events. We considered the dayside/cusp precipitation, substorm precipitation, daytime and nighttime PCPs, and precipitation associated with the interplanetary shock wave arrival. We demonstrate that substorm-associated precipitation (even without PCPs) can lead to a strong GPS phase ( σ ϕ ) scintillations up to ∼ 1.5–3 radians, which is much stronger than those usually produced by other types of considered ionosphere disturbances. The value of the substorm-phase scintillations in general correlate with the value of the geomagnetic field disturbance. But sometimes even a small geomagnetic substorm, when combined with the PCPs, produces quite strong phase scintillations. Cusp phase scintillations are lower than dayside PCPs scintillations. PCPs can lead to stronger ROT (rate of total electron content) variations than other types of ionosphere disturbances. So our observations suggest that the substorms and PCPs, being different types of the high-latitude disturbances, lead to the development of different types and scales of ionospheric irregularities. |
format |
Article in Journal/Newspaper |
author |
V. B. Belakhovsky Y. Jin W. J. Miloch |
author_facet |
V. B. Belakhovsky Y. Jin W. J. Miloch |
author_sort |
V. B. Belakhovsky |
title |
Influence of different types of ionospheric disturbances on GPS signals at polar latitudes |
title_short |
Influence of different types of ionospheric disturbances on GPS signals at polar latitudes |
title_full |
Influence of different types of ionospheric disturbances on GPS signals at polar latitudes |
title_fullStr |
Influence of different types of ionospheric disturbances on GPS signals at polar latitudes |
title_full_unstemmed |
Influence of different types of ionospheric disturbances on GPS signals at polar latitudes |
title_sort |
influence of different types of ionospheric disturbances on gps signals at polar latitudes |
publisher |
Copernicus Publications |
publishDate |
2021 |
url |
https://doi.org/10.5194/angeo-39-687-2021 https://doaj.org/article/e4d3f2f5fc0f4b9f9069605409423c8d |
geographic |
Svalbard Ny-Ålesund |
geographic_facet |
Svalbard Ny-Ålesund |
genre |
EISCAT Ny Ålesund Ny-Ålesund Skibotn Svalbard |
genre_facet |
EISCAT Ny Ålesund Ny-Ålesund Skibotn Svalbard |
op_source |
Annales Geophysicae, Vol 39, Pp 687-700 (2021) |
op_relation |
https://angeo.copernicus.org/articles/39/687/2021/angeo-39-687-2021.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576 doi:10.5194/angeo-39-687-2021 0992-7689 1432-0576 https://doaj.org/article/e4d3f2f5fc0f4b9f9069605409423c8d |
op_doi |
https://doi.org/10.5194/angeo-39-687-2021 |
container_title |
Annales Geophysicae |
container_volume |
39 |
container_issue |
4 |
container_start_page |
687 |
op_container_end_page |
700 |
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1766400253465985024 |