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...

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Main Authors: Sato, Hiroatsu, Yaroshenko, Victoriya, Günzkofer, Florian Ludwig, Varverg, Erik, Rietveld, Michael
Format: Conference Object
Language:unknown
Published: 2024
Subjects:
Online Access:https://elib.dlr.de/205753/
https://en.uit.no/tavla/artikkel/830164/21st_international_eiscat_symposium_2024
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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