Probing discrete auroral arcs by ionospheric tomography
Optical observations of 557.7 nm and 630.0 nm emissions from discrete auroral arcs in the post-noon sector have been related to localised field-aligned enhancements in the spatial distribution of E- and F-layer electron density respectively seen in images reconstructed by ionospheric tomography. Res...
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ftcopernicus:oai:publications.copernicus.org:angeo34156 2023-05-15T18:29:47+02:00 Probing discrete auroral arcs by ionospheric tomography Moen, J. Berry, S. T. Kersley, L. Lybekk, B. 2018-09-27 application/pdf https://doi.org/10.1007/s00585-998-0574-z https://angeo.copernicus.org/articles/16/574/1998/ eng eng doi:10.1007/s00585-998-0574-z https://angeo.copernicus.org/articles/16/574/1998/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.1007/s00585-998-0574-z 2020-07-20T16:28:06Z Optical observations of 557.7 nm and 630.0 nm emissions from discrete auroral arcs in the post-noon sector have been related to localised field-aligned enhancements in the spatial distribution of E- and F-layer electron density respectively seen in images reconstructed by ionospheric tomography. Results from two case studies are presented in which meridian scanning photometer and all-sky camera observations on Svalbard have been compared to electron-density structures found by tomographic inversion of measurements made by reception of radio signals at a chain of four stations at high latitude. The F-layer features are long-lived and show exact correspondence to the red-line emissions. Transient arcs in green-line intensity result in E-region structures that are resolved in one case, but not in another where the dynamic auroral forms are separated by less than one degree of latitude. The signature of an inverted-V precipitation event is clearly evident in one example. Key words. Ionosphere (Auroral ionosphere) · Magnetospheric physics (Auroral phenomena) · Radio science (Ionospheric physics) Text Svalbard Copernicus Publications: E-Journals Svalbard Annales Geophysicae 16 5 574 582 |
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Copernicus Publications: E-Journals |
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ftcopernicus |
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English |
description |
Optical observations of 557.7 nm and 630.0 nm emissions from discrete auroral arcs in the post-noon sector have been related to localised field-aligned enhancements in the spatial distribution of E- and F-layer electron density respectively seen in images reconstructed by ionospheric tomography. Results from two case studies are presented in which meridian scanning photometer and all-sky camera observations on Svalbard have been compared to electron-density structures found by tomographic inversion of measurements made by reception of radio signals at a chain of four stations at high latitude. The F-layer features are long-lived and show exact correspondence to the red-line emissions. Transient arcs in green-line intensity result in E-region structures that are resolved in one case, but not in another where the dynamic auroral forms are separated by less than one degree of latitude. The signature of an inverted-V precipitation event is clearly evident in one example. Key words. Ionosphere (Auroral ionosphere) · Magnetospheric physics (Auroral phenomena) · Radio science (Ionospheric physics) |
format |
Text |
author |
Moen, J. Berry, S. T. Kersley, L. Lybekk, B. |
spellingShingle |
Moen, J. Berry, S. T. Kersley, L. Lybekk, B. Probing discrete auroral arcs by ionospheric tomography |
author_facet |
Moen, J. Berry, S. T. Kersley, L. Lybekk, B. |
author_sort |
Moen, J. |
title |
Probing discrete auroral arcs by ionospheric tomography |
title_short |
Probing discrete auroral arcs by ionospheric tomography |
title_full |
Probing discrete auroral arcs by ionospheric tomography |
title_fullStr |
Probing discrete auroral arcs by ionospheric tomography |
title_full_unstemmed |
Probing discrete auroral arcs by ionospheric tomography |
title_sort |
probing discrete auroral arcs by ionospheric tomography |
publishDate |
2018 |
url |
https://doi.org/10.1007/s00585-998-0574-z https://angeo.copernicus.org/articles/16/574/1998/ |
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Svalbard |
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Svalbard |
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Svalbard |
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Svalbard |
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eISSN: 1432-0576 |
op_relation |
doi:10.1007/s00585-998-0574-z https://angeo.copernicus.org/articles/16/574/1998/ |
op_doi |
https://doi.org/10.1007/s00585-998-0574-z |
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Annales Geophysicae |
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16 |
container_issue |
5 |
container_start_page |
574 |
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582 |
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1766213171383631872 |