Statistical analysis of radar observed F region irregularities from three longitudinal sectors

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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...

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Detalles Bibliográficos
Autores: Cueva, R. Y. C., De Paula, E. R., Kherani, A. E.
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
format 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
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
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv European Geosciences Union
publisher.none.fl_str_mv European Geosciences Union
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
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collection IGP-Institucional
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spelling 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.peTk9URTogUExBQ0UgWU9VUiBPV04gTElDRU5TRSBIRVJFClRoaXMgc2FtcGxlIGxpY2Vuc2UgaXMgcHJvdmlkZWQgZm9yIGluZm9ybWF0aW9uYWwgcHVycG9zZXMgb25seS4KCk5PTi1FWENMVVNJVkUgRElTVFJJQlVUSU9OIExJQ0VOU0UKCkJ5IHNpZ25pbmcgYW5kIHN1Ym1pdHRpbmcgdGhpcyBsaWNlbnNlLCB5b3UgKHRoZSBhdXRob3Iocykgb3IgY29weXJpZ2h0Cm93bmVyKSBncmFudHMgdG8gRFNwYWNlIFVuaXZlcnNpdHkgKERTVSkgdGhlIG5vbi1leGNsdXNpdmUgcmlnaHQgdG8gcmVwcm9kdWNlLAp0cmFuc2xhdGUgKGFzIGRlZmluZWQgYmVsb3cpLCBhbmQvb3IgZGlzdHJpYnV0ZSB5b3VyIHN1Ym1pc3Npb24gKGluY2x1ZGluZwp0aGUgYWJzdHJhY3QpIHdvcmxkd2lkZSBpbiBwcmludCBhbmQgZWxlY3Ryb25pYyBmb3JtYXQgYW5kIGluIGFueSBtZWRpdW0sCmluY2x1ZGluZyBidXQgbm90IGxpbWl0ZWQgdG8gYXVkaW8gb3IgdmlkZW8uCgpZb3UgYWdyZWUgdGhhdCBEU1UgbWF5LCB3aXRob3V0IGNoYW5naW5nIHRoZSBjb250ZW50LCB0cmFuc2xhdGUgdGhlCnN1Ym1pc3Npb24gdG8gYW55IG1lZGl1bSBvciBmb3JtYXQgZm9yIHRoZSBwdXJwb3NlIG9mIHByZXNlcnZhdGlvbi4KCllvdSBhbHNvIGFncmVlIHRoYXQgRFNVIG1heSBrZWVwIG1vcmUgdGhhbiBvbmUgY29weSBvZiB0aGlzIHN1Ym1pc3Npb24gZm9yCnB1cnBvc2VzIG9mIHNlY3VyaXR5LCBiYWNrLXVwIGFuZCBwcmVzZXJ2YXRpb24uCgpZb3UgcmVwcmVzZW50IHRoYXQgdGhlIHN1Ym1pc3Npb24gaXMgeW91ciBvcmlnaW5hbCB3b3JrLCBhbmQgdGhhdCB5b3UgaGF2ZQp0aGUgcmlnaHQgdG8gZ3JhbnQgdGhlIHJpZ2h0cyBjb250YWluZWQgaW4gdGhpcyBsaWNlbnNlLiBZb3UgYWxzbyByZXByZXNlbnQKdGhhdCB5b3VyIHN1Ym1pc3Npb24gZG9lcyBub3QsIHRvIHRoZSBiZXN0IG9mIHlvdXIga25vd2xlZGdlLCBpbmZyaW5nZSB1cG9uCmFueW9uZSdzIGNvcHlyaWdodC4KCklmIHRoZSBzdWJtaXNzaW9uIGNvbnRhaW5zIG1hdGVyaWFsIGZvciB3aGljaCB5b3UgZG8gbm90IGhvbGQgY29weXJpZ2h0LAp5b3UgcmVwcmVzZW50IHRoYXQgeW91IGhhdmUgb2J0YWluZWQgdGhlIHVucmVzdHJpY3RlZCBwZXJtaXNzaW9uIG9mIHRoZQpjb3B5cmlnaHQgb3duZXIgdG8gZ3JhbnQgRFNVIHRoZSByaWdodHMgcmVxdWlyZWQgYnkgdGhpcyBsaWNlbnNlLCBhbmQgdGhhdApzdWNoIHRoaXJkLXBhcnR5IG93bmVkIG1hdGVyaWFsIGlzIGNsZWFybHkgaWRlbnRpZmllZCBhbmQgYWNrbm93bGVkZ2VkCndpdGhpbiB0aGUgdGV4dCBvciBjb250ZW50IG9mIHRoZSBzdWJtaXNzaW9uLgoKSUYgVEhFIFNVQk1JU1NJT04gSVMgQkFTRUQgVVBPTiBXT1JLIFRIQVQgSEFTIEJFRU4gU1BPTlNPUkVEIE9SIFNVUFBPUlRFRApCWSBBTiBBR0VOQ1kgT1IgT1JHQU5JWkFUSU9OIE9USEVSIFRIQU4gRFNVLCBZT1UgUkVQUkVTRU5UIFRIQVQgWU9VIEhBVkUKRlVMRklMTEVEIEFOWSBSSUdIVCBPRiBSRVZJRVcgT1IgT1RIRVIgT0JMSUdBVElPTlMgUkVRVUlSRUQgQlkgU1VDSApDT05UUkFDVCBPUiBBR1JFRU1FTlQuCgpEU1Ugd2lsbCBjbGVhcmx5IGlkZW50aWZ5IHlvdXIgbmFtZShzKSBhcyB0aGUgYXV0aG9yKHMpIG9yIG93bmVyKHMpIG9mIHRoZQpzdWJtaXNzaW9uLCBhbmQgd2lsbCBub3QgbWFrZSBhbnkgYWx0ZXJhdGlvbiwgb3RoZXIgdGhhbiBhcyBhbGxvd2VkIGJ5IHRoaXMKbGljZW5zZSwgdG8geW91ciBzdWJtaXNzaW9uLgo=
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