Statistical analysis of radar observed F region irregularities from three longitudinal sectors
Descripción del Articulo
Equatorial Spread F (ESF) is a manifestation of ionospheric interchange instabilities in the nighttime equatorial F region. These instabilities generate plasma density irregularities with scale sizes ranging from centimetres to thousands of kilometres. The irregularities can be detected from a varie...
| Autores: | , , |
|---|---|
| Formato: | artículo |
| Fecha de Publicación: | 2013 |
| Institución: | Instituto Geofísico del Perú |
| Repositorio: | IGP-Institucional |
| Lenguaje: | inglés |
| OAI Identifier: | oai:repositorio.igp.gob.pe:20.500.12816/1569 |
| Enlace del recurso: | http://hdl.handle.net/20.500.12816/1569 https://doi.org/10.5194/angeo-31-2137-2013 |
| Nivel de acceso: | acceso abierto |
| Materia: | Ionosphere Equatorial ionosphere Ionospheric irregularities Ionospheric physics http://purl.org/pe-repo/ocde/ford#1.05.01 |
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| dc.title.none.fl_str_mv |
Statistical analysis of radar observed F region irregularities from three longitudinal sectors |
| title |
Statistical analysis of radar observed F region irregularities from three longitudinal sectors |
| spellingShingle |
Statistical analysis of radar observed F region irregularities from three longitudinal sectors Cueva, R. Y. C. Ionosphere Equatorial ionosphere Ionospheric irregularities Ionospheric physics http://purl.org/pe-repo/ocde/ford#1.05.01 |
| title_short |
Statistical analysis of radar observed F region irregularities from three longitudinal sectors |
| title_full |
Statistical analysis of radar observed F region irregularities from three longitudinal sectors |
| title_fullStr |
Statistical analysis of radar observed F region irregularities from three longitudinal sectors |
| title_full_unstemmed |
Statistical analysis of radar observed F region irregularities from three longitudinal sectors |
| title_sort |
Statistical analysis of radar observed F region irregularities from three longitudinal sectors |
| author |
Cueva, R. Y. C. |
| author_facet |
Cueva, R. Y. C. De Paula, E. R. Kherani, A. E. |
| author_role |
author |
| author2 |
De Paula, E. R. Kherani, A. E. |
| author2_role |
author author |
| dc.contributor.author.fl_str_mv |
Cueva, R. Y. C. De Paula, E. R. Kherani, A. E. |
| dc.subject.none.fl_str_mv |
Ionosphere Equatorial ionosphere Ionospheric irregularities Ionospheric physics |
| topic |
Ionosphere Equatorial ionosphere Ionospheric irregularities Ionospheric 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 |
Equatorial Spread F (ESF) is a manifestation of ionospheric interchange instabilities in the nighttime equatorial F region. These instabilities generate plasma density irregularities with scale sizes ranging from centimetres to thousands of kilometres. The irregularities can be detected from a variety of instruments such as digisonde, coherent and incoherent scatter radars, in situ space probes, and airglow photometers. In the present study, occurrence statistics of the ESF, based on various parameters are presented using data obtained from the VHF radars located at three longitudinally separated equatorial stations: Christmas Island (2◦ N, 202.6◦ E, 2.9◦ N dip latitude), São Luís (2.59◦ S, 315.8◦ E, 0.5◦ S dip latitude) and Jicamarca (12◦ S, 283.1◦ E, 0.6◦ N dip latitude). The ESF parameters presented here are the onset altitude, onset time (onset refers to first appearance of signal in the radar field of view) of the bottom-type and plume, and the peak altitude of the plume. Recent studies have used these parameters to classify the spread F occurrence characteristics. The present study reveals novel features namely, the dependence of ESF parameters on the seasonal, solar flux, declination angle and longitudinal dependence from the three radar sites. In addition, we also present an empirical model to determine the nature of these ESF parameters as a function of the solar flux which may enable us to forecast (with 30 min to 1 h tolerance) the plume occurrence at any longitude located in between São Luís and Christmas Island. |
| publishDate |
2013 |
| dc.date.accessioned.none.fl_str_mv |
2018-06-28T14:55:17Z |
| dc.date.available.none.fl_str_mv |
2018-06-28T14:55:17Z |
| dc.date.issued.fl_str_mv |
2013-12 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article |
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article |
| dc.identifier.citation.none.fl_str_mv |
Cueva, R. Y. C., De Paula, E. R., & Kherani, A. E. (2013). Statistical analysis of radar observed F region irregularities from three longitudinal sectors.==$Annales Geophysicae, 31$==(12), 2137–2146. https://doi.org/10.5194/angeo-31-2137-2013 |
| dc.identifier.uri.none.fl_str_mv |
http://hdl.handle.net/20.500.12816/1569 |
| dc.identifier.journal.none.fl_str_mv |
Annales Geophysicae |
| dc.identifier.doi.none.fl_str_mv |
https://doi.org/10.5194/angeo-31-2137-2013 |
| identifier_str_mv |
Cueva, R. Y. C., De Paula, E. R., & Kherani, A. E. (2013). Statistical analysis of radar observed F region irregularities from three longitudinal sectors.==$Annales Geophysicae, 31$==(12), 2137–2146. https://doi.org/10.5194/angeo-31-2137-2013 Annales Geophysicae |
| url |
http://hdl.handle.net/20.500.12816/1569 https://doi.org/10.5194/angeo-31-2137-2013 |
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eng |
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eng |
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urn:issn:0992-7689 |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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European Geosciences Union |
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European Geosciences Union |
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Cueva, R. Y. C.De Paula, E. R.Kherani, A. E.2018-06-28T14:55:17Z2018-06-28T14:55:17Z2013-12Cueva, R. Y. C., De Paula, E. R., & Kherani, A. E. (2013). Statistical analysis of radar observed F region irregularities from three longitudinal sectors.==$Annales Geophysicae, 31$==(12), 2137–2146. https://doi.org/10.5194/angeo-31-2137-2013http://hdl.handle.net/20.500.12816/1569Annales Geophysicaehttps://doi.org/10.5194/angeo-31-2137-2013Equatorial Spread F (ESF) is a manifestation of ionospheric interchange instabilities in the nighttime equatorial F region. These instabilities generate plasma density irregularities with scale sizes ranging from centimetres to thousands of kilometres. The irregularities can be detected from a variety of instruments such as digisonde, coherent and incoherent scatter radars, in situ space probes, and airglow photometers. In the present study, occurrence statistics of the ESF, based on various parameters are presented using data obtained from the VHF radars located at three longitudinally separated equatorial stations: Christmas Island (2◦ N, 202.6◦ E, 2.9◦ N dip latitude), São Luís (2.59◦ S, 315.8◦ E, 0.5◦ S dip latitude) and Jicamarca (12◦ S, 283.1◦ E, 0.6◦ N dip latitude). The ESF parameters presented here are the onset altitude, onset time (onset refers to first appearance of signal in the radar field of view) of the bottom-type and plume, and the peak altitude of the plume. Recent studies have used these parameters to classify the spread F occurrence characteristics. The present study reveals novel features namely, the dependence of ESF parameters on the seasonal, solar flux, declination angle and longitudinal dependence from the three radar sites. In addition, we also present an empirical model to determine the nature of these ESF parameters as a function of the solar flux which may enable us to forecast (with 30 min to 1 h tolerance) the plume occurrence at any longitude located in between São Luís and Christmas Island.Por paresapplication/pdfengEuropean Geosciences Unionurn:issn:0992-7689info:eu-repo/semantics/openAccessIonosphereEquatorial ionosphereIonospheric irregularitiesIonospheric physicshttp://purl.org/pe-repo/ocde/ford#1.05.01Statistical analysis of radar observed F region irregularities from three longitudinal sectorsinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALAAI0055.pdfAAI0055.pdfapplication/pdf4050671https://repositorio.igp.gob.pe/bitstreams/5de59ad5-82cc-4de5-ab5f-5f848b4b012c/download634bde785f6d39e2fb2e284e4c23c3f1MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-81748https://repositorio.igp.gob.pe/bitstreams/217fbe5f-181f-4f7d-b33a-8b259ab450d3/download8a4605be74aa9ea9d79846c1fba20a33MD52THUMBNAILAAI0055.pdf.jpgAAI0055.pdf.jpgIM Thumbnailimage/jpeg171171https://repositorio.igp.gob.pe/bitstreams/bdeb67f4-bdf5-42b6-8129-29d918a45311/downloade6c8f71e23a7724ac6d032b2273514ceMD53TEXTAAI0055.pdf.txtAAI0055.pdf.txtExtracted texttext/plain42363https://repositorio.igp.gob.pe/bitstreams/cd13193b-10ca-45b8-9a84-4cef60c2b98f/downloadd9453370759858014c4ef2e50e2efde0MD5420.500.12816/1569oai:repositorio.igp.gob.pe:20.500.12816/15692025-08-13 10:58:44.48open.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).