Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment
Evolution of artificial field-aligned irregularities (FAIs) is studied by coordinated observations of GNSS satellite and EISCAT UHF radar during EISCAT HF experiments. We show that the electron density variation due to artificial FAIs can be characterized by GNSS scintillation and total electron con...
Main Authors: | , , , , |
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Format: | Conference Object |
Language: | unknown |
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2024
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Online Access: | https://elib.dlr.de/205753/ https://en.uit.no/tavla/artikkel/830164/21st_international_eiscat_symposium_2024 |
_version_ | 1835014015747620864 |
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author | Sato, Hiroatsu Yaroshenko, Victoriya Günzkofer, Florian Ludwig Varverg, Erik Rietveld, Michael |
author_facet | Sato, Hiroatsu Yaroshenko, Victoriya Günzkofer, Florian Ludwig Varverg, Erik Rietveld, Michael |
author_sort | Sato, Hiroatsu |
collection | Unknown |
description | Evolution of artificial field-aligned irregularities (FAIs) is studied by coordinated observations of GNSS satellite and EISCAT UHF radar during EISCAT HF experiments. We show that the electron density variation due to artificial FAIs can be characterized by GNSS scintillation and total electron content (TEC) parameters derived from high-rate GNSS receivers located at EISCAT and in Tromsø when the satellite-receiver links intersected the expected heating impact area around 250 km altitude. GNSS amplitude scintillation and TEC fluctuation data show that the largest density perturbation is found near the magnetic zenith direction. We find that during the existence of small-scale GNSS scintillation, the UHF radar detected an enhanced ion shoulder from a narrow range of altitudes that can lead to erroneous incoherent radar fitting results. In fact, a large deviation is found between the estimated electron densities derived from GNSS TEC and UHF data during this period. We discuss that the source of this particular GNSS scintillation are likely a type of FAIs caused by parametric instabilities. |
format | Conference Object |
genre | EISCAT Tromsø |
genre_facet | EISCAT Tromsø |
geographic | Tromsø |
geographic_facet | Tromsø |
id | ftdlr:oai:elib.dlr.de:205753 |
institution | Open Polar |
language | unknown |
op_collection_id | ftdlr |
op_relation | Sato, Hiroatsu und Yaroshenko, Victoriya und Günzkofer, Florian Ludwig und Varverg, Erik und Rietveld, Michael (2024) Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment. 21st International EISCAT Symposium 2024, 2024-07-29 - 2024-08-03, Tromsø, Norway. |
publishDate | 2024 |
record_format | openpolar |
spelling | ftdlr:oai:elib.dlr.de:205753 2025-06-15T14:26:13+00:00 Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment Sato, Hiroatsu Yaroshenko, Victoriya Günzkofer, Florian Ludwig Varverg, Erik Rietveld, Michael 2024 https://elib.dlr.de/205753/ https://en.uit.no/tavla/artikkel/830164/21st_international_eiscat_symposium_2024 unknown Sato, Hiroatsu und Yaroshenko, Victoriya und Günzkofer, Florian Ludwig und Varverg, Erik und Rietveld, Michael (2024) Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment. 21st International EISCAT Symposium 2024, 2024-07-29 - 2024-08-03, Tromsø, Norway. Solar-Terrestrische Kopplungsprozesse Institut für Solar-Terrestrische Physik Konferenzbeitrag NonPeerReviewed 2024 ftdlr 2025-06-04T04:58:05Z Evolution of artificial field-aligned irregularities (FAIs) is studied by coordinated observations of GNSS satellite and EISCAT UHF radar during EISCAT HF experiments. We show that the electron density variation due to artificial FAIs can be characterized by GNSS scintillation and total electron content (TEC) parameters derived from high-rate GNSS receivers located at EISCAT and in Tromsø when the satellite-receiver links intersected the expected heating impact area around 250 km altitude. GNSS amplitude scintillation and TEC fluctuation data show that the largest density perturbation is found near the magnetic zenith direction. We find that during the existence of small-scale GNSS scintillation, the UHF radar detected an enhanced ion shoulder from a narrow range of altitudes that can lead to erroneous incoherent radar fitting results. In fact, a large deviation is found between the estimated electron densities derived from GNSS TEC and UHF data during this period. We discuss that the source of this particular GNSS scintillation are likely a type of FAIs caused by parametric instabilities. Conference Object EISCAT Tromsø Unknown Tromsø |
spellingShingle | Solar-Terrestrische Kopplungsprozesse Institut für Solar-Terrestrische Physik Sato, Hiroatsu Yaroshenko, Victoriya Günzkofer, Florian Ludwig Varverg, Erik Rietveld, Michael Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment |
title | Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment |
title_full | Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment |
title_fullStr | Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment |
title_full_unstemmed | Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment |
title_short | Simultaneous observation of GNSS scintillation and UHF radar enhanced ion shoulder during EISCAT HF experiment |
title_sort | simultaneous observation of gnss scintillation and uhf radar enhanced ion shoulder during eiscat hf experiment |
topic | Solar-Terrestrische Kopplungsprozesse Institut für Solar-Terrestrische Physik |
topic_facet | Solar-Terrestrische Kopplungsprozesse Institut für Solar-Terrestrische Physik |
url | https://elib.dlr.de/205753/ https://en.uit.no/tavla/artikkel/830164/21st_international_eiscat_symposium_2024 |