A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003
Descripción del Articulo
Variations of nighttime F2 peak height (hmF2) over the American sector during the 28–29 October 2003 storm period were investigated using the National Center for Atmospheric Research Thermosphere‐Ionosphere Electrodynamics Global Circulation Model. The model was generally able to reproduce the ionos...
| Autores: | , , , , , |
|---|---|
| Formato: | artículo |
| Fecha de Publicación: | 2016 |
| Institución: | Instituto Geofísico del Perú |
| Repositorio: | IGP-Institucional |
| Lenguaje: | inglés |
| OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/3738 |
| Enlace del recurso: | http://hdl.handle.net/20.500.12816/3738 https://doi.org/10.1002/2016JA023091 |
| Nivel de acceso: | acceso abierto |
| Materia: | Peak height Northward Bz TADs Penetration electric field http://purl.org/pe-repo/ocde/ford#1.05.01 |
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Chen, XuetaoLei, JiuhouWang, WenbinBurns, Alan G.Luan, XiaoliDou, Xiankang2018-11-20T18:05:06Z2018-11-20T18:05:06Z2016-08-17Chen, X., Lei, J., Wang, W., Burns, A. G., Luan, X., & Dou, X. (2016). A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003.==$Journal of Geophysical Research: Space Physics, 121$==(9), 8985-8994. https://doi.org/10.1002/2016JA023091http://hdl.handle.net/20.500.12816/3738Journal of Geophysical Research: Space Physicshttps://doi.org/10.1002/2016JA023091Variations of nighttime F2 peak height (hmF2) over the American sector during the 28–29 October 2003 storm period were investigated using the National Center for Atmospheric Research Thermosphere‐Ionosphere Electrodynamics Global Circulation Model. The model was generally able to reproduce the ionospheric variations on 28–29 October 2003 observed by the ionosondes. A series of controlled model simulations were subsequently undertaken to examine the effects of electric fields and neutral winds on the ionosphere. The numerical experiments suggest that the dramatic nighttime increase of hmF2 on the storm day 29 October is mainly caused by traveling atmospheric disturbances (TADs) from the high latitudes of the Northern Hemisphere. However, the electric field plays an important role in causing the elevation of hmF2 in the equatorial region. The prompt penetration electric field (PPEF) associated with the southward component of the interplanetary magnetic field (Bz) is westward on the nightside, whereas when Bz reverses and becomes northward, the PPEF is westward in the premidnight and turns to eastward in the postmidnight. These PPEFs greatly affect the low‐latitude ionosphere during storm time. On 28 October, even though the Bz disturbance was weak with a short duration of southward Bz, the TADs from the Southern Hemisphere can propagate to the Northern Hemisphere and result in the corresponding oscillations in the nightside hmF2.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:2169-9380info:eu-repo/semantics/openAccessPeak heightNorthward BzTADsPenetration electric fieldhttp://purl.org/pe-repo/ocde/ford#1.05.01A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003info:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALIGP-1-1-1-1495126727.pdfIGP-1-1-1-1495126727.pdfapplication/pdf1276834https://repositorio.igp.gob.pe/bitstreams/62f4c957-a9a7-4963-b3ff-8ed29cd4de7b/download845755552fbf50cab8a109aa57769cf5MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-8391https://repositorio.igp.gob.pe/bitstreams/bbcf3d6f-0828-40d0-808f-af2832843a6b/downloadef941c35636116525aadeaab7bbf4ca3MD52THUMBNAILIGP-1-1-1-1495126727.pdf.jpgIGP-1-1-1-1495126727.pdf.jpgIM Thumbnailimage/jpeg109472https://repositorio.igp.gob.pe/bitstreams/b2fb512d-8045-4123-863f-33b6f76c3735/download491577b08df5342312aa6e0e833325e2MD53TEXTIGP-1-1-1-1495126727.pdf.txtIGP-1-1-1-1495126727.pdf.txtExtracted texttext/plain39300https://repositorio.igp.gob.pe/bitstreams/2cab4c0d-c11e-48ce-bdc2-047770abaa2e/downloadec358162b998bffe4aee255d6c297653MD5420.500.12816/3738oai:repositorio.igp.gob.pe:20.500.12816/37382025-08-13 09:59:13.457open.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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 |
| dc.title.none.fl_str_mv |
A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003 |
| title |
A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003 |
| spellingShingle |
A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003 Chen, Xuetao Peak height Northward Bz TADs Penetration electric field http://purl.org/pe-repo/ocde/ford#1.05.01 |
| title_short |
A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003 |
| title_full |
A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003 |
| title_fullStr |
A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003 |
| title_full_unstemmed |
A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003 |
| title_sort |
A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003 |
| author |
Chen, Xuetao |
| author_facet |
Chen, Xuetao Lei, Jiuhou Wang, Wenbin Burns, Alan G. Luan, Xiaoli Dou, Xiankang |
| author_role |
author |
| author2 |
Lei, Jiuhou Wang, Wenbin Burns, Alan G. Luan, Xiaoli Dou, Xiankang |
| author2_role |
author author author author author |
| dc.contributor.author.fl_str_mv |
Chen, Xuetao Lei, Jiuhou Wang, Wenbin Burns, Alan G. Luan, Xiaoli Dou, Xiankang |
| dc.subject.none.fl_str_mv |
Peak height Northward Bz TADs Penetration electric field |
| topic |
Peak height Northward Bz TADs Penetration electric field 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 |
Variations of nighttime F2 peak height (hmF2) over the American sector during the 28–29 October 2003 storm period were investigated using the National Center for Atmospheric Research Thermosphere‐Ionosphere Electrodynamics Global Circulation Model. The model was generally able to reproduce the ionospheric variations on 28–29 October 2003 observed by the ionosondes. A series of controlled model simulations were subsequently undertaken to examine the effects of electric fields and neutral winds on the ionosphere. The numerical experiments suggest that the dramatic nighttime increase of hmF2 on the storm day 29 October is mainly caused by traveling atmospheric disturbances (TADs) from the high latitudes of the Northern Hemisphere. However, the electric field plays an important role in causing the elevation of hmF2 in the equatorial region. The prompt penetration electric field (PPEF) associated with the southward component of the interplanetary magnetic field (Bz) is westward on the nightside, whereas when Bz reverses and becomes northward, the PPEF is westward in the premidnight and turns to eastward in the postmidnight. These PPEFs greatly affect the low‐latitude ionosphere during storm time. On 28 October, even though the Bz disturbance was weak with a short duration of southward Bz, the TADs from the Southern Hemisphere can propagate to the Northern Hemisphere and result in the corresponding oscillations in the nightside hmF2. |
| publishDate |
2016 |
| dc.date.accessioned.none.fl_str_mv |
2018-11-20T18:05:06Z |
| dc.date.available.none.fl_str_mv |
2018-11-20T18:05:06Z |
| dc.date.issued.fl_str_mv |
2016-08-17 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article |
| format |
article |
| dc.identifier.citation.none.fl_str_mv |
Chen, X., Lei, J., Wang, W., Burns, A. G., Luan, X., & Dou, X. (2016). A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003.==$Journal of Geophysical Research: Space Physics, 121$==(9), 8985-8994. https://doi.org/10.1002/2016JA023091 |
| dc.identifier.uri.none.fl_str_mv |
http://hdl.handle.net/20.500.12816/3738 |
| dc.identifier.journal.none.fl_str_mv |
Journal of Geophysical Research: Space Physics |
| dc.identifier.doi.none.fl_str_mv |
https://doi.org/10.1002/2016JA023091 |
| identifier_str_mv |
Chen, X., Lei, J., Wang, W., Burns, A. G., Luan, X., & Dou, X. (2016). A numerical study of nighttime ionospheric variations in the American sector during 28–29 October 2003.==$Journal of Geophysical Research: Space Physics, 121$==(9), 8985-8994. https://doi.org/10.1002/2016JA023091 Journal of Geophysical Research: Space Physics |
| url |
http://hdl.handle.net/20.500.12816/3738 https://doi.org/10.1002/2016JA023091 |
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eng |
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eng |
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urn:issn:2169-9380 |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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American Geophysical Union |
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American Geophysical Union |
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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).