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...

Full description

Bibliographic Details
Published in:Annales Geophysicae
Main Authors: Dreyer, Joshua, Partamies, Noora, Whiter, Daniel, Ellingsen, Pål, Baddeley, Lisa, Buchert, Stephan
Format: Article in Journal/Newspaper
Language:English
Published: 2021
Subjects:
Online Access:https://eprints.soton.ac.uk/447557/
https://eprints.soton.ac.uk/447557/1/Characteristicsoffragmentedaurora_like.pdf
id ftsouthampton:oai:eprints.soton.ac.uk:447557
record_format openpolar
spelling ftsouthampton:oai:eprints.soton.ac.uk:447557 2023-12-03T10:18:12+01:00 Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard Dreyer, Joshua Partamies, Noora Whiter, Daniel Ellingsen, Pål Baddeley, Lisa Buchert, Stephan 2021-03-04 text https://eprints.soton.ac.uk/447557/ https://eprints.soton.ac.uk/447557/1/Characteristicsoffragmentedaurora_like.pdf en English eng https://eprints.soton.ac.uk/447557/1/Characteristicsoffragmentedaurora_like.pdf Dreyer, Joshua, Partamies, Noora, Whiter, Daniel, Ellingsen, Pål, Baddeley, Lisa and Buchert, Stephan (2021) Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard. Annales Geophysicae, 39 (2), 277-288. (doi:10.5194/angeo-39-277-2021 <http://dx.doi.org/10.5194/angeo-39-277-2021>). cc_by_4 Article PeerReviewed 2021 ftsouthampton https://doi.org/10.5194/angeo-39-277-2021 2023-11-03T00:00:51Z 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 NC 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. Article in Journal/Newspaper Arctic Longyearbyen Svalbard University of Southampton: e-Prints Soton Arctic Svalbard Longyearbyen Norway Farley ENVELOPE(-152.500,-152.500,-86.583,-86.583) Annales Geophysicae 39 2 277 288
institution Open Polar
collection University of Southampton: e-Prints Soton
op_collection_id ftsouthampton
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 NC 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.
format Article in Journal/Newspaper
author Dreyer, Joshua
Partamies, Noora
Whiter, Daniel
Ellingsen, Pål
Baddeley, Lisa
Buchert, Stephan
spellingShingle Dreyer, Joshua
Partamies, Noora
Whiter, Daniel
Ellingsen, Pål
Baddeley, Lisa
Buchert, Stephan
Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard
author_facet Dreyer, Joshua
Partamies, Noora
Whiter, Daniel
Ellingsen, Pål
Baddeley, Lisa
Buchert, Stephan
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
publishDate 2021
url https://eprints.soton.ac.uk/447557/
https://eprints.soton.ac.uk/447557/1/Characteristicsoffragmentedaurora_like.pdf
long_lat ENVELOPE(-152.500,-152.500,-86.583,-86.583)
geographic Arctic
Svalbard
Longyearbyen
Norway
Farley
geographic_facet Arctic
Svalbard
Longyearbyen
Norway
Farley
genre Arctic
Longyearbyen
Svalbard
genre_facet Arctic
Longyearbyen
Svalbard
op_relation https://eprints.soton.ac.uk/447557/1/Characteristicsoffragmentedaurora_like.pdf
Dreyer, Joshua, Partamies, Noora, Whiter, Daniel, Ellingsen, Pål, Baddeley, Lisa and Buchert, Stephan (2021) Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard. Annales Geophysicae, 39 (2), 277-288. (doi:10.5194/angeo-39-277-2021 <http://dx.doi.org/10.5194/angeo-39-277-2021>).
op_rights cc_by_4
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
_version_ 1784265183550504960