Polar cap influx

This study uses digital ionosonde data from a cusp latitude station (Cambridge Bay, 77° CGM lat.) to study the convection into the polar cap. Days when the IMF magnetic field was relatively steady were used. On many days it was possible to distinguish an interval near noon MLT when the ionosonde dat...

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Published in:Annales Geophysicae
Main Authors: MacDougall, J., Jayachandran, P. T.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/angeo-23-1755-2005
https://angeo.copernicus.org/articles/23/1755/2005/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo35622 2023-05-15T15:48:34+02:00 Polar cap influx MacDougall, J. Jayachandran, P. T. 2018-09-27 application/pdf https://doi.org/10.5194/angeo-23-1755-2005 https://angeo.copernicus.org/articles/23/1755/2005/ eng eng doi:10.5194/angeo-23-1755-2005 https://angeo.copernicus.org/articles/23/1755/2005/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-23-1755-2005 2020-07-20T16:27:24Z This study uses digital ionosonde data from a cusp latitude station (Cambridge Bay, 77° CGM lat.) to study the convection into the polar cap. Days when the IMF magnetic field was relatively steady were used. On many days it was possible to distinguish an interval near noon MLT when the ionosonde data had a different character from that at earlier and later times. Based on our data, and other published measurements, we used the interval 10:00-13:00MLT as the cusp interval and calculated the convection into the polar cap in this interval. The integrated convection accounted for only ~1/3 of the open polar cap flux. If the convection through the prenoon/postnoon regions on either side of the cusp was calculated the remaining 2/3 of the flux could be accounted for. The characteristics of the prenoon/postnoon regions were different from the cusp region, and we attribute this to transient flank merging versus more steady frontside merging for the cusp. Keywords. Ionosphere (Plasma convection) Magnetospheric physics (Polar cap phenomenon) Text Cambridge Bay Copernicus Publications: E-Journals Cambridge Bay ENVELOPE(-105.130,-105.130,69.037,69.037) Annales Geophysicae 23 5 1755 1761
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description This study uses digital ionosonde data from a cusp latitude station (Cambridge Bay, 77° CGM lat.) to study the convection into the polar cap. Days when the IMF magnetic field was relatively steady were used. On many days it was possible to distinguish an interval near noon MLT when the ionosonde data had a different character from that at earlier and later times. Based on our data, and other published measurements, we used the interval 10:00-13:00MLT as the cusp interval and calculated the convection into the polar cap in this interval. The integrated convection accounted for only ~1/3 of the open polar cap flux. If the convection through the prenoon/postnoon regions on either side of the cusp was calculated the remaining 2/3 of the flux could be accounted for. The characteristics of the prenoon/postnoon regions were different from the cusp region, and we attribute this to transient flank merging versus more steady frontside merging for the cusp. Keywords. Ionosphere (Plasma convection) Magnetospheric physics (Polar cap phenomenon)
format Text
author MacDougall, J.
Jayachandran, P. T.
spellingShingle MacDougall, J.
Jayachandran, P. T.
Polar cap influx
author_facet MacDougall, J.
Jayachandran, P. T.
author_sort MacDougall, J.
title Polar cap influx
title_short Polar cap influx
title_full Polar cap influx
title_fullStr Polar cap influx
title_full_unstemmed Polar cap influx
title_sort polar cap influx
publishDate 2018
url https://doi.org/10.5194/angeo-23-1755-2005
https://angeo.copernicus.org/articles/23/1755/2005/
long_lat ENVELOPE(-105.130,-105.130,69.037,69.037)
geographic Cambridge Bay
geographic_facet Cambridge Bay
genre Cambridge Bay
genre_facet Cambridge Bay
op_source eISSN: 1432-0576
op_relation doi:10.5194/angeo-23-1755-2005
https://angeo.copernicus.org/articles/23/1755/2005/
op_doi https://doi.org/10.5194/angeo-23-1755-2005
container_title Annales Geophysicae
container_volume 23
container_issue 5
container_start_page 1755
op_container_end_page 1761
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