Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard

This study analyses the observations of a new type of small-scale aurora-like feature, which is further referred to as fragmented aurora-like emission(s) (FAEs). An all-sky camera captured these FAEs on three separate occasions in 2015 and 2017 at the Kjell Henriksen Observatory near the arctic town...

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Published in:Annales Geophysicae
Main Authors: Dreyer, Joshua, Partamies, Noora, Whiter, Daniel, Ellingsen, Pål Gunnar, Baddeley, Lisa, Buchert, Stephan C.
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2021
Subjects:
Online Access:https://hdl.handle.net/11250/2767703
https://doi.org/10.5194/angeo-39-277-2021
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spelling ftunivbergen:oai:bora.uib.no:11250/2767703 2023-05-15T15:09:36+02:00 Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard Dreyer, Joshua Partamies, Noora Whiter, Daniel Ellingsen, Pål Gunnar Baddeley, Lisa Buchert, Stephan C. 2021 application/pdf https://hdl.handle.net/11250/2767703 https://doi.org/10.5194/angeo-39-277-2021 eng eng Copernicus Publications urn:issn:0992-7689 https://hdl.handle.net/11250/2767703 https://doi.org/10.5194/angeo-39-277-2021 cristin:1917672 Annales Geophysicae. 2021, 39 (2), 277-288. Navngivelse 4.0 Internasjonal http://creativecommons.org/licenses/by/4.0/deed.no Copyright Author(s) 2021 Annales Geophysicae 277-288 39 2 Journal article Peer reviewed 2021 ftunivbergen https://doi.org/10.5194/angeo-39-277-2021 2023-03-14T17:40:47Z This study analyses the observations of a new type of small-scale aurora-like feature, which is further referred to as fragmented aurora-like emission(s) (FAEs). An all-sky camera captured these FAEs on three separate occasions in 2015 and 2017 at the Kjell Henriksen Observatory near the arctic town of Longyearbyen, Svalbard, Norway. A total of 305 FAE candidates were identified. They seem to appear in two categories – randomly occurring individual FAEs and wave-like structures with regular spacing between FAEs alongside auroral arcs. FAEs show horizontal sizes typically below 20 km, a lack of field-aligned emission extent, and short lifetimes of less than a minute. Emissions were observed at the 557.7 nm line of atomic oxygen and at 673.0 nm (N2; first positive band system) but not at the 427.8 nm emission of N+2 or the 777.4 nm line of atomic oxygen. This suggests an upper limit to the energy that can be produced by the generating mechanism. Their lack of field-aligned extent indicates a different generation mechanism than for aurorae, which are caused by particle precipitation. Instead, these FAEs could be the result of excitation by thermal ionospheric electrons. FAE observations are seemingly accompanied by elevated electron temperatures between 110–120 km and increased ion temperatures at F-region altitudes. One possible explanation for this is Farley–Buneman instabilities of strong local currents. In the present study, we provide an overview of the observations and discuss their characteristics and potential generation mechanisms. publishedVersion Article in Journal/Newspaper Arctic Longyearbyen Svalbard University of Bergen: Bergen Open Research Archive (BORA-UiB) Arctic Farley ENVELOPE(-152.500,-152.500,-86.583,-86.583) Longyearbyen Norway Svalbard Annales Geophysicae 39 2 277 288
institution Open Polar
collection University of Bergen: Bergen Open Research Archive (BORA-UiB)
op_collection_id ftunivbergen
language English
description This study analyses the observations of a new type of small-scale aurora-like feature, which is further referred to as fragmented aurora-like emission(s) (FAEs). An all-sky camera captured these FAEs on three separate occasions in 2015 and 2017 at the Kjell Henriksen Observatory near the arctic town of Longyearbyen, Svalbard, Norway. A total of 305 FAE candidates were identified. They seem to appear in two categories – randomly occurring individual FAEs and wave-like structures with regular spacing between FAEs alongside auroral arcs. FAEs show horizontal sizes typically below 20 km, a lack of field-aligned emission extent, and short lifetimes of less than a minute. Emissions were observed at the 557.7 nm line of atomic oxygen and at 673.0 nm (N2; first positive band system) but not at the 427.8 nm emission of N+2 or the 777.4 nm line of atomic oxygen. This suggests an upper limit to the energy that can be produced by the generating mechanism. Their lack of field-aligned extent indicates a different generation mechanism than for aurorae, which are caused by particle precipitation. Instead, these FAEs could be the result of excitation by thermal ionospheric electrons. FAE observations are seemingly accompanied by elevated electron temperatures between 110–120 km and increased ion temperatures at F-region altitudes. One possible explanation for this is Farley–Buneman instabilities of strong local currents. In the present study, we provide an overview of the observations and discuss their characteristics and potential generation mechanisms. publishedVersion
format Article in Journal/Newspaper
author Dreyer, Joshua
Partamies, Noora
Whiter, Daniel
Ellingsen, Pål Gunnar
Baddeley, Lisa
Buchert, Stephan C.
spellingShingle Dreyer, Joshua
Partamies, Noora
Whiter, Daniel
Ellingsen, Pål Gunnar
Baddeley, Lisa
Buchert, Stephan C.
Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard
author_facet Dreyer, Joshua
Partamies, Noora
Whiter, Daniel
Ellingsen, Pål Gunnar
Baddeley, Lisa
Buchert, Stephan C.
author_sort Dreyer, Joshua
title Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard
title_short Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard
title_full Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard
title_fullStr Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard
title_full_unstemmed Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard
title_sort characteristics of fragmented aurora-like emissions (faes) observed on svalbard
publisher Copernicus Publications
publishDate 2021
url https://hdl.handle.net/11250/2767703
https://doi.org/10.5194/angeo-39-277-2021
long_lat ENVELOPE(-152.500,-152.500,-86.583,-86.583)
geographic Arctic
Farley
Longyearbyen
Norway
Svalbard
geographic_facet Arctic
Farley
Longyearbyen
Norway
Svalbard
genre Arctic
Longyearbyen
Svalbard
genre_facet Arctic
Longyearbyen
Svalbard
op_source Annales Geophysicae
277-288
39
2
op_relation urn:issn:0992-7689
https://hdl.handle.net/11250/2767703
https://doi.org/10.5194/angeo-39-277-2021
cristin:1917672
Annales Geophysicae. 2021, 39 (2), 277-288.
op_rights Navngivelse 4.0 Internasjonal
http://creativecommons.org/licenses/by/4.0/deed.no
Copyright Author(s) 2021
op_doi https://doi.org/10.5194/angeo-39-277-2021
container_title Annales Geophysicae
container_volume 39
container_issue 2
container_start_page 277
op_container_end_page 288
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