Ducting of incoherent scatter radar waves by field-aligned irregularities
We provide an explanation for a mysterious phenomenon that has been recognized in recent years in European Incoherent Scatter (EISCAT) UHF incoherent scatter radar (ISR) measurements during many high-power high-frequency (HF) ionospheric pumping experiments. The phenomenon is an apparent increase in...
Published in: | Annales Geophysicae |
---|---|
Main Authors: | , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
Copernicus Publications
2020
|
Subjects: | |
Online Access: | https://hdl.handle.net/10037/20536 https://doi.org/10.5194/angeo-38-1101-2020 |
_version_ | 1829307768098521088 |
---|---|
author | Rietveld, Michael T Senior, Andrew |
author_facet | Rietveld, Michael T Senior, Andrew |
author_sort | Rietveld, Michael T |
collection | University of Tromsø: Munin Open Research Archive |
container_issue | 5 |
container_start_page | 1101 |
container_title | Annales Geophysicae |
container_volume | 38 |
description | We provide an explanation for a mysterious phenomenon that has been recognized in recent years in European Incoherent Scatter (EISCAT) UHF incoherent scatter radar (ISR) measurements during many high-power high-frequency (HF) ionospheric pumping experiments. The phenomenon is an apparent increase in electron density observed above the HF reflection altitude, extending up to the observable limits usually in the range 400–650 km, as shown in several publications in recent years. It was shown by Senior et al. (2013) that several examples of these enhanced backscatter could not be explained by increases in electron density. A summary of characteristics of the backscatter enhancements is presented as well as the results of a survey of events. We propose that medium- to large-scale HF-induced field-aligned irregularities (tens to hundreds of metres scale) act to refract the radar signals along the magnetic field, thereby acting as a guide so that the free-space r−2 spreading of the signals no longer applies. The nature of the irregularities and the physical mechanism of their production by powerful HF waves is an exciting topic for future research since, surprisingly, they appear to be preferentially excited by X-mode waves. The explanation proposed here involving HF-induced irregularities may well apply to other ISR observations of the ionosphere in the presence of specific natural irregularities. |
format | Article in Journal/Newspaper |
genre | EISCAT |
genre_facet | EISCAT |
id | ftunivtroemsoe:oai:munin.uit.no:10037/20536 |
institution | Open Polar |
language | English |
op_collection_id | ftunivtroemsoe |
op_container_end_page | 1113 |
op_doi | https://doi.org/10.5194/angeo-38-1101-2020 |
op_relation | Annales Geophysicae FRIDAID 1848924 https://hdl.handle.net/10037/20536 |
op_rights | openAccess Copyright 2020 The Author(s) |
publishDate | 2020 |
publisher | Copernicus Publications |
record_format | openpolar |
spelling | ftunivtroemsoe:oai:munin.uit.no:10037/20536 2025-04-13T14:18:07+00:00 Ducting of incoherent scatter radar waves by field-aligned irregularities Rietveld, Michael T Senior, Andrew 2020-10-22 https://hdl.handle.net/10037/20536 https://doi.org/10.5194/angeo-38-1101-2020 eng eng Copernicus Publications Annales Geophysicae FRIDAID 1848924 https://hdl.handle.net/10037/20536 openAccess Copyright 2020 The Author(s) VDP::Mathematics and natural science: 400::Physics: 430::Astrophysics astronomy: 438 VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Astrofysikk astronomi: 438 Journal article Tidsskriftartikkel Peer reviewed publishedVersion 2020 ftunivtroemsoe https://doi.org/10.5194/angeo-38-1101-2020 2025-03-14T05:17:57Z We provide an explanation for a mysterious phenomenon that has been recognized in recent years in European Incoherent Scatter (EISCAT) UHF incoherent scatter radar (ISR) measurements during many high-power high-frequency (HF) ionospheric pumping experiments. The phenomenon is an apparent increase in electron density observed above the HF reflection altitude, extending up to the observable limits usually in the range 400–650 km, as shown in several publications in recent years. It was shown by Senior et al. (2013) that several examples of these enhanced backscatter could not be explained by increases in electron density. A summary of characteristics of the backscatter enhancements is presented as well as the results of a survey of events. We propose that medium- to large-scale HF-induced field-aligned irregularities (tens to hundreds of metres scale) act to refract the radar signals along the magnetic field, thereby acting as a guide so that the free-space r−2 spreading of the signals no longer applies. The nature of the irregularities and the physical mechanism of their production by powerful HF waves is an exciting topic for future research since, surprisingly, they appear to be preferentially excited by X-mode waves. The explanation proposed here involving HF-induced irregularities may well apply to other ISR observations of the ionosphere in the presence of specific natural irregularities. Article in Journal/Newspaper EISCAT University of Tromsø: Munin Open Research Archive Annales Geophysicae 38 5 1101 1113 |
spellingShingle | VDP::Mathematics and natural science: 400::Physics: 430::Astrophysics astronomy: 438 VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Astrofysikk astronomi: 438 Rietveld, Michael T Senior, Andrew Ducting of incoherent scatter radar waves by field-aligned irregularities |
title | Ducting of incoherent scatter radar waves by field-aligned irregularities |
title_full | Ducting of incoherent scatter radar waves by field-aligned irregularities |
title_fullStr | Ducting of incoherent scatter radar waves by field-aligned irregularities |
title_full_unstemmed | Ducting of incoherent scatter radar waves by field-aligned irregularities |
title_short | Ducting of incoherent scatter radar waves by field-aligned irregularities |
title_sort | ducting of incoherent scatter radar waves by field-aligned irregularities |
topic | VDP::Mathematics and natural science: 400::Physics: 430::Astrophysics astronomy: 438 VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Astrofysikk astronomi: 438 |
topic_facet | VDP::Mathematics and natural science: 400::Physics: 430::Astrophysics astronomy: 438 VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Astrofysikk astronomi: 438 |
url | https://hdl.handle.net/10037/20536 https://doi.org/10.5194/angeo-38-1101-2020 |