Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars

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This paper describes the ionospheric response to a geomagnetic storm beginning on 17 April 2002. We present the measurements of ionospheric parameters in the F-region obtained by the network of eight incoherent scatter radars. The main effects of this storm include a deep decrease in the electron de...

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Detalles Bibliográficos
Autores: Goncharenko, L. P., Salah, J. E., Van Eyken, A., Howells, V., Thayer, J. P., Taran, V. I., Shpynev, B., Zhou, Q., Chau Chong Shing, Jorge Luis
Formato: artículo
Fecha de Publicación:2005
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/1872
Enlace del recurso:http://hdl.handle.net/20.500.12816/1872
https://doi.org/10.5194/angeo-23-163-2005
Nivel de acceso:acceso abierto
Materia:Ionosphere
Auroral ionosphere
Mid-latitude ionosphere
Equatorial ionosphere
Magnetosphereic physics
http://purl.org/pe-repo/ocde/ford#1.05.01
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dc.title.none.fl_str_mv Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars
title Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars
spellingShingle Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars
Goncharenko, L. P.
Ionosphere
Auroral ionosphere
Mid-latitude ionosphere
Equatorial ionosphere
Magnetosphereic physics
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars
title_full Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars
title_fullStr Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars
title_full_unstemmed Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars
title_sort Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars
author Goncharenko, L. P.
author_facet Goncharenko, L. P.
Salah, J. E.
Van Eyken, A.
Howells, V.
Thayer, J. P.
Taran, V. I.
Shpynev, B.
Zhou, Q.
Chau Chong Shing, Jorge Luis
author_role author
author2 Salah, J. E.
Van Eyken, A.
Howells, V.
Thayer, J. P.
Taran, V. I.
Shpynev, B.
Zhou, Q.
Chau Chong Shing, Jorge Luis
author2_role author
author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Goncharenko, L. P.
Salah, J. E.
Van Eyken, A.
Howells, V.
Thayer, J. P.
Taran, V. I.
Shpynev, B.
Zhou, Q.
Chau Chong Shing, Jorge Luis
dc.subject.none.fl_str_mv Ionosphere
Auroral ionosphere
Mid-latitude ionosphere
Equatorial ionosphere
Magnetosphereic physics
topic Ionosphere
Auroral ionosphere
Mid-latitude ionosphere
Equatorial ionosphere
Magnetosphereic physics
http://purl.org/pe-repo/ocde/ford#1.05.01
dc.subject.ocde.none.fl_str_mv http://purl.org/pe-repo/ocde/ford#1.05.01
description This paper describes the ionospheric response to a geomagnetic storm beginning on 17 April 2002. We present the measurements of ionospheric parameters in the F-region obtained by the network of eight incoherent scatter radars. The main effects of this storm include a deep decrease in the electron density observed at high and middle latitudes in the pre-noon sector, and a minor enhancement in the density observed in the daytime sector at middle latitudes. Extreme plasma heating (>1000-3000 K) is observed at high latitudes, subsiding to 200-300K at subauroral latitudes. The western hemisphere radar chain observed the prompt penetration of the electric field from auroral to equatorial latitudes, as well as the daytime enhancement of plasma drift parallel to the magnetic field line, which is related to the enhancement in the equatorward winds. We suggest that in the first several hours after the storm onset, a negative phase above Millstone Hill (pre-noon sector) results from counteracting processes - penetration electric field, meridional wind, and electrodynamic heating, with electrodynamic heating being the dominant mechanism. At the lower latitude in the pre-noon sector (Arecibo and Jicamarca), the penetration electric field becomes more important, leading to a negative storm phase over Arecibo. In contrast, in the afternoon sector at mid-latitudes (Kharkov, Irkutsk), effects of penetration electric field and meridional wind do not counteract, but add up, leading to a small (~15%), positive storm phase over these locations. As the storm develops, Millstone Hill and Irkutsk mid-latitude radars observe further depletion of electron density due to the changes in the neutral composition.
publishDate 2005
dc.date.accessioned.none.fl_str_mv 2018-07-16T14:15:00Z
dc.date.available.none.fl_str_mv 2018-07-16T14:15:00Z
dc.date.issued.fl_str_mv 2005-01
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv Goncharenko, L. P., Salah, J. E., Van Eyken, A., Howells, V., Thayer, J. P., Taran, V. I., ... Chau, J. L. (2005). Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars.==$Annales Geophysicae, 23$==(1), 163–181. https://doi.org/10.5194/angeo-23-163-2005
dc.identifier.govdoc.none.fl_str_mv index-oti2018
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/1872
dc.identifier.journal.none.fl_str_mv Annales Geophysicae
dc.identifier.doi.none.fl_str_mv https://doi.org/10.5194/angeo-23-163-2005
identifier_str_mv Goncharenko, L. P., Salah, J. E., Van Eyken, A., Howells, V., Thayer, J. P., Taran, V. I., ... Chau, J. L. (2005). Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars.==$Annales Geophysicae, 23$==(1), 163–181. https://doi.org/10.5194/angeo-23-163-2005
index-oti2018
Annales Geophysicae
url http://hdl.handle.net/20.500.12816/1872
https://doi.org/10.5194/angeo-23-163-2005
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv urn:issn:0992-7689
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eu_rights_str_mv openAccess
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dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv European Geosciences Union (EGU)
publisher.none.fl_str_mv European Geosciences Union (EGU)
dc.source.none.fl_str_mv reponame:IGP-Institucional
instname:Instituto Geofísico del Perú
instacron:IGP
instname_str Instituto Geofísico del Perú
instacron_str IGP
institution IGP
reponame_str IGP-Institucional
collection IGP-Institucional
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spelling Goncharenko, L. P.Salah, J. E.Van Eyken, A.Howells, V.Thayer, J. P.Taran, V. I.Shpynev, B.Zhou, Q.Chau Chong Shing, Jorge Luis2018-07-16T14:15:00Z2018-07-16T14:15:00Z2005-01Goncharenko, L. P., Salah, J. E., Van Eyken, A., Howells, V., Thayer, J. P., Taran, V. I., ... Chau, J. L. (2005). Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars.==$Annales Geophysicae, 23$==(1), 163–181. https://doi.org/10.5194/angeo-23-163-2005index-oti2018http://hdl.handle.net/20.500.12816/1872Annales Geophysicaehttps://doi.org/10.5194/angeo-23-163-2005This paper describes the ionospheric response to a geomagnetic storm beginning on 17 April 2002. We present the measurements of ionospheric parameters in the F-region obtained by the network of eight incoherent scatter radars. The main effects of this storm include a deep decrease in the electron density observed at high and middle latitudes in the pre-noon sector, and a minor enhancement in the density observed in the daytime sector at middle latitudes. Extreme plasma heating (>1000-3000 K) is observed at high latitudes, subsiding to 200-300K at subauroral latitudes. The western hemisphere radar chain observed the prompt penetration of the electric field from auroral to equatorial latitudes, as well as the daytime enhancement of plasma drift parallel to the magnetic field line, which is related to the enhancement in the equatorward winds. We suggest that in the first several hours after the storm onset, a negative phase above Millstone Hill (pre-noon sector) results from counteracting processes - penetration electric field, meridional wind, and electrodynamic heating, with electrodynamic heating being the dominant mechanism. At the lower latitude in the pre-noon sector (Arecibo and Jicamarca), the penetration electric field becomes more important, leading to a negative storm phase over Arecibo. In contrast, in the afternoon sector at mid-latitudes (Kharkov, Irkutsk), effects of penetration electric field and meridional wind do not counteract, but add up, leading to a small (~15%), positive storm phase over these locations. 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