Reconfiguration of polar-cap plasma in the magnetic midnight sector

Radio tomography and the EISCAT and SuperDARN radars have been used to identify long-lived, high-altitude, cold plasma in the antisunward convective flow across the polar cap. The projection of the feature to later times suggests that it was reconfigured in the Harang discontinuity to form an enhanc...

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Published in:Annales Geophysicae
Main Authors: Pryse, S. E., Wood, A. G., Middleton, H. R., McCrea, I. W., Lester, M.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/angeo-24-2201-2006
https://angeo.copernicus.org/articles/24/2201/2006/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo35973 2023-05-15T16:04:39+02:00 Reconfiguration of polar-cap plasma in the magnetic midnight sector Pryse, S. E. Wood, A. G. Middleton, H. R. McCrea, I. W. Lester, M. 2018-09-27 application/pdf https://doi.org/10.5194/angeo-24-2201-2006 https://angeo.copernicus.org/articles/24/2201/2006/ eng eng doi:10.5194/angeo-24-2201-2006 https://angeo.copernicus.org/articles/24/2201/2006/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-24-2201-2006 2020-07-20T16:27:12Z Radio tomography and the EISCAT and SuperDARN radars have been used to identify long-lived, high-altitude, cold plasma in the antisunward convective flow across the polar cap. The projection of the feature to later times suggests that it was reconfigured in the Harang discontinuity to form an enhancement that was elongated in longitude in the sunward return flow of the high-latitude convection pattern. Comparison with a tomographic image at a later time supports the interpretation of a polar patch being reconfigured into a boundary blob. There is also evidence for a second plasma enhancement equatorward of the reconfigured blob, likely to have been produced by in situ precipitation. The observations indicate that the two mechanisms proposed in the literature for the production of boundary blobs are operating simultaneously to form two distinct density features separated slightly in latitude. Text EISCAT Copernicus Publications: E-Journals Annales Geophysicae 24 8 2201 2208
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Radio tomography and the EISCAT and SuperDARN radars have been used to identify long-lived, high-altitude, cold plasma in the antisunward convective flow across the polar cap. The projection of the feature to later times suggests that it was reconfigured in the Harang discontinuity to form an enhancement that was elongated in longitude in the sunward return flow of the high-latitude convection pattern. Comparison with a tomographic image at a later time supports the interpretation of a polar patch being reconfigured into a boundary blob. There is also evidence for a second plasma enhancement equatorward of the reconfigured blob, likely to have been produced by in situ precipitation. The observations indicate that the two mechanisms proposed in the literature for the production of boundary blobs are operating simultaneously to form two distinct density features separated slightly in latitude.
format Text
author Pryse, S. E.
Wood, A. G.
Middleton, H. R.
McCrea, I. W.
Lester, M.
spellingShingle Pryse, S. E.
Wood, A. G.
Middleton, H. R.
McCrea, I. W.
Lester, M.
Reconfiguration of polar-cap plasma in the magnetic midnight sector
author_facet Pryse, S. E.
Wood, A. G.
Middleton, H. R.
McCrea, I. W.
Lester, M.
author_sort Pryse, S. E.
title Reconfiguration of polar-cap plasma in the magnetic midnight sector
title_short Reconfiguration of polar-cap plasma in the magnetic midnight sector
title_full Reconfiguration of polar-cap plasma in the magnetic midnight sector
title_fullStr Reconfiguration of polar-cap plasma in the magnetic midnight sector
title_full_unstemmed Reconfiguration of polar-cap plasma in the magnetic midnight sector
title_sort reconfiguration of polar-cap plasma in the magnetic midnight sector
publishDate 2018
url https://doi.org/10.5194/angeo-24-2201-2006
https://angeo.copernicus.org/articles/24/2201/2006/
genre EISCAT
genre_facet EISCAT
op_source eISSN: 1432-0576
op_relation doi:10.5194/angeo-24-2201-2006
https://angeo.copernicus.org/articles/24/2201/2006/
op_doi https://doi.org/10.5194/angeo-24-2201-2006
container_title Annales Geophysicae
container_volume 24
container_issue 8
container_start_page 2201
op_container_end_page 2208
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