Observations of diverging field-aligned ion flow with the ESR

We report on observations of a diverging ion flow along the geomagnetic field that is often seen at the EISCAT Svalbard radar. The flow is upward above the peak of the electron density in the F-region and downward below the peak. We estimate that in such events mass transport along the field line is...

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Published in:Annales Geophysicae
Main Authors: Buchert, S. C., Ogawa, Y., Fujii, R., Eyken, A. P.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/angeo-22-889-2004
https://angeo.copernicus.org/articles/22/889/2004/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo35138 2023-05-15T16:04:40+02:00 Observations of diverging field-aligned ion flow with the ESR Buchert, S. C. Ogawa, Y. Fujii, R. Eyken, A. P. 2018-09-27 application/pdf https://doi.org/10.5194/angeo-22-889-2004 https://angeo.copernicus.org/articles/22/889/2004/ eng eng doi:10.5194/angeo-22-889-2004 https://angeo.copernicus.org/articles/22/889/2004/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-22-889-2004 2020-07-20T16:27:37Z We report on observations of a diverging ion flow along the geomagnetic field that is often seen at the EISCAT Svalbard radar. The flow is upward above the peak of the electron density in the F-region and downward below the peak. We estimate that in such events mass transport along the field line is important for the ionization balance, and that the shape of the F-layer and its ion composition should be strongly influenced by it. Diverging flow typically occurs when there are signatures of direct entry of sheath plasma to the ionosphere in the form of intense soft particle precipitation, and we suggest that it is caused by the ionization and ionospheric electron heating associated with this precipitation. On average, 30% of all events with ion upflow also show significant ion downflow below. Key words. Ionosphere (polar ionosphere; ionization mechanism; plasma temperature and density) Text EISCAT Svalbard Copernicus Publications: E-Journals Svalbard Annales Geophysicae 22 3 889 899
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description We report on observations of a diverging ion flow along the geomagnetic field that is often seen at the EISCAT Svalbard radar. The flow is upward above the peak of the electron density in the F-region and downward below the peak. We estimate that in such events mass transport along the field line is important for the ionization balance, and that the shape of the F-layer and its ion composition should be strongly influenced by it. Diverging flow typically occurs when there are signatures of direct entry of sheath plasma to the ionosphere in the form of intense soft particle precipitation, and we suggest that it is caused by the ionization and ionospheric electron heating associated with this precipitation. On average, 30% of all events with ion upflow also show significant ion downflow below. Key words. Ionosphere (polar ionosphere; ionization mechanism; plasma temperature and density)
format Text
author Buchert, S. C.
Ogawa, Y.
Fujii, R.
Eyken, A. P.
spellingShingle Buchert, S. C.
Ogawa, Y.
Fujii, R.
Eyken, A. P.
Observations of diverging field-aligned ion flow with the ESR
author_facet Buchert, S. C.
Ogawa, Y.
Fujii, R.
Eyken, A. P.
author_sort Buchert, S. C.
title Observations of diverging field-aligned ion flow with the ESR
title_short Observations of diverging field-aligned ion flow with the ESR
title_full Observations of diverging field-aligned ion flow with the ESR
title_fullStr Observations of diverging field-aligned ion flow with the ESR
title_full_unstemmed Observations of diverging field-aligned ion flow with the ESR
title_sort observations of diverging field-aligned ion flow with the esr
publishDate 2018
url https://doi.org/10.5194/angeo-22-889-2004
https://angeo.copernicus.org/articles/22/889/2004/
geographic Svalbard
geographic_facet Svalbard
genre EISCAT
Svalbard
genre_facet EISCAT
Svalbard
op_source eISSN: 1432-0576
op_relation doi:10.5194/angeo-22-889-2004
https://angeo.copernicus.org/articles/22/889/2004/
op_doi https://doi.org/10.5194/angeo-22-889-2004
container_title Annales Geophysicae
container_volume 22
container_issue 3
container_start_page 889
op_container_end_page 899
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