Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radars
Descripción del Articulo
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...
| Autores: | , , , , , , , , |
|---|---|
| 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 |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess |
| dc.rights.uri.none.fl_str_mv |
https://creativecommons.org/licences/by/4.0/ |
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openAccess |
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https://creativecommons.org/licences/by/4.0/ |
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application/pdf |
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European Geosciences Union (EGU) |
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European Geosciences Union (EGU) |
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reponame:IGP-Institucional instname:Instituto Geofísico del Perú instacron:IGP |
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Instituto Geofísico del Perú |
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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. 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.Por paresapplication/pdfengEuropean Geosciences Union (EGU)urn:issn:0992-7689info:eu-repo/semantics/openAccesshttps://creativecommons.org/licences/by/4.0/IonosphereAuroral ionosphereMid-latitude ionosphereEquatorial ionosphereMagnetosphereic physicshttp://purl.org/pe-repo/ocde/ford#1.05.01Observations of the April 2002 geomagnetic storm by the global network of incoherent scatter radarsinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALobs2005.pdfobs2005.pdfapplication/pdf2594856https://repositorio.igp.gob.pe/bitstreams/5d2ef735-9ea4-4cc6-b13a-94cc97f21768/download1fd93dd9565f1570dabe6fd911bfeb6dMD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/b452b167-1feb-43b5-bc29-0b48457ea6bc/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILobs2005.pdf.jpgobs2005.pdf.jpgIM Thumbnailimage/jpeg97808https://repositorio.igp.gob.pe/bitstreams/c99f5cec-09e7-47a7-b8ad-df50394c041a/download46726d859dbd8a0ab5893763ba54b456MD53TEXTobs2005.pdf.txtobs2005.pdf.txtExtracted texttext/plain71141https://repositorio.igp.gob.pe/bitstreams/16ddfd59-a16c-4d27-b2e5-a39f60661f57/download9eb811a70c6cde04978687fdf87300fbMD5420.500.12816/1872oai:repositorio.igp.gob.pe:20.500.12816/18722024-10-12 22:18:29.367https://creativecommons.org/licences/by/4.0/info:eu-repo/semantics/openAccessopen.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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 |
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La información contenida en este registro es de entera responsabilidad de la institución que gestiona el repositorio institucional donde esta contenido este documento o set de datos. El CONCYTEC no se hace responsable por los contenidos (publicaciones y/o datos) accesibles a través del Repositorio Nacional Digital de Ciencia, Tecnología e Innovación de Acceso Abierto (ALICIA).