Ion upflow and downflow at the topside ionosphere observed by the EISCAT VHF radar

We have determined the MLT distribution and KP dependence of the ion upflow and downflow of the thermal bulk oxygen ion population based on a data analysis using the EISCAT VHF radar CP-7 data obtained at Tromsø during the period between 1990 and 1996: (1) both ion upflow and downflow events can be...

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Published in:Annales Geophysicae
Main Authors: Endo, M., Fujii, R., Ogawa, Y., Buchert, S. C., Nozawa, S., Watanabe, S., Yoshida, N.
Format: Article in Journal/Newspaper
Language:English
Published: Springer Verlag 2000
Subjects:
Online Access:https://doi.org/10.1007/s00585-000-0170-3
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author Endo, M.
Fujii, R.
Ogawa, Y.
Buchert, S. C.
Nozawa, S.
Watanabe, S.
Yoshida, N.
author_facet Endo, M.
Fujii, R.
Ogawa, Y.
Buchert, S. C.
Nozawa, S.
Watanabe, S.
Yoshida, N.
author_sort Endo, M.
collection Niedersächsisches Online-Archiv NOA
container_issue 2
container_start_page 170
container_title Annales Geophysicae
container_volume 18
description We have determined the MLT distribution and KP dependence of the ion upflow and downflow of the thermal bulk oxygen ion population based on a data analysis using the EISCAT VHF radar CP-7 data obtained at Tromsø during the period between 1990 and 1996: (1) both ion upflow and downflow events can be observed at any local time (MLT), irrespective of dayside and nightside, and under any magnetic disturbance level, irrespective of quiet and disturbed levels; (2) these upflow and downflow events are more frequently observed in the nightside than in the dayside; (3) the upflow events are more frequently observed than the downflow events at any local time except midnight and at any KP level and the difference of the occurrence frequencies between the upflow and downflow events is smaller around midnight; and (4) the occurrence frequencies of both the ion upflow and downflow events appear to increase with increasing KP level, while the occurrence frequency of the downflow appears to stop increasing at some KP level. Key words: Ionosphere (particle acceleration; plasma waves and instabilities) - Space plasma physics (transport processes)
format Article in Journal/Newspaper
genre EISCAT
Tromsø
genre_facet EISCAT
Tromsø
geographic Tromsø
geographic_facet Tromsø
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op_doi https://doi.org/10.1007/s00585-000-0170-3
op_relation Annales Geophysicae -- http://www.bibliothek.uni-regensburg.de/ezeit/?1458425 -- https://www.ann-geophys.net/ -- https://www.ann-geophys.net/volumes.html -- http://link.springer.com/journal/585 -- 1432-0576
https://doi.org/10.1007/s00585-000-0170-3
https://noa.gwlb.de/receive/cop_mods_00036830
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spelling ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00036830 2025-01-16T21:42:01+00:00 Ion upflow and downflow at the topside ionosphere observed by the EISCAT VHF radar Endo, M. Fujii, R. Ogawa, Y. Buchert, S. C. Nozawa, S. Watanabe, S. Yoshida, N. 2000-02 electronic https://doi.org/10.1007/s00585-000-0170-3 https://noa.gwlb.de/receive/cop_mods_00036830 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00036784/angeo-18-170-2000.pdf https://angeo.copernicus.org/articles/18/170/2000/angeo-18-170-2000.pdf eng eng Springer Verlag Annales Geophysicae -- http://www.bibliothek.uni-regensburg.de/ezeit/?1458425 -- https://www.ann-geophys.net/ -- https://www.ann-geophys.net/volumes.html -- http://link.springer.com/journal/585 -- 1432-0576 https://doi.org/10.1007/s00585-000-0170-3 https://noa.gwlb.de/receive/cop_mods_00036830 https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00036784/angeo-18-170-2000.pdf https://angeo.copernicus.org/articles/18/170/2000/angeo-18-170-2000.pdf https://open-access.net/ uneingeschränkt info:eu-repo/semantics/openAccess article Verlagsveröffentlichung article Text doc-type:article 2000 ftnonlinearchiv https://doi.org/10.1007/s00585-000-0170-3 2022-02-08T22:43:48Z We have determined the MLT distribution and KP dependence of the ion upflow and downflow of the thermal bulk oxygen ion population based on a data analysis using the EISCAT VHF radar CP-7 data obtained at Tromsø during the period between 1990 and 1996: (1) both ion upflow and downflow events can be observed at any local time (MLT), irrespective of dayside and nightside, and under any magnetic disturbance level, irrespective of quiet and disturbed levels; (2) these upflow and downflow events are more frequently observed in the nightside than in the dayside; (3) the upflow events are more frequently observed than the downflow events at any local time except midnight and at any KP level and the difference of the occurrence frequencies between the upflow and downflow events is smaller around midnight; and (4) the occurrence frequencies of both the ion upflow and downflow events appear to increase with increasing KP level, while the occurrence frequency of the downflow appears to stop increasing at some KP level. Key words: Ionosphere (particle acceleration; plasma waves and instabilities) - Space plasma physics (transport processes) Article in Journal/Newspaper EISCAT Tromsø Niedersächsisches Online-Archiv NOA Tromsø Annales Geophysicae 18 2 170 181
spellingShingle article
Verlagsveröffentlichung
Endo, M.
Fujii, R.
Ogawa, Y.
Buchert, S. C.
Nozawa, S.
Watanabe, S.
Yoshida, N.
Ion upflow and downflow at the topside ionosphere observed by the EISCAT VHF radar
title Ion upflow and downflow at the topside ionosphere observed by the EISCAT VHF radar
title_full Ion upflow and downflow at the topside ionosphere observed by the EISCAT VHF radar
title_fullStr Ion upflow and downflow at the topside ionosphere observed by the EISCAT VHF radar
title_full_unstemmed Ion upflow and downflow at the topside ionosphere observed by the EISCAT VHF radar
title_short Ion upflow and downflow at the topside ionosphere observed by the EISCAT VHF radar
title_sort ion upflow and downflow at the topside ionosphere observed by the eiscat vhf radar
topic article
Verlagsveröffentlichung
topic_facet article
Verlagsveröffentlichung
url https://doi.org/10.1007/s00585-000-0170-3
https://noa.gwlb.de/receive/cop_mods_00036830
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00036784/angeo-18-170-2000.pdf
https://angeo.copernicus.org/articles/18/170/2000/angeo-18-170-2000.pdf