Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms

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Since their discovery in the 1970s, equatorial plasma bubbles (EPBs) have been invoked to explain the propagation of VHF signals on trans‐equatorial circuits at night, and blamed for highly detrimental scintillation of VHF and GHz trans‐ionospheric communications signals in equatorial regions. Over...

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Detalles Bibliográficos
Autores: McNamara, L. F., Caton, R. G., Parris, R. T., Pedersen, T. R., Thompson, D. C., Wiens, K. C., Groves, K. M.
Formato: artículo
Fecha de Publicación:2013
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/3543
Enlace del recurso:http://hdl.handle.net/20.500.12816/3543
https://doi.org/10.1002/rds.20025
Nivel de acceso:acceso abierto
Materia:Equatorial ionosphere
Equatorial plasma bubbles
Plasma
http://purl.org/pe-repo/ocde/ford#1.05.01
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spelling McNamara, L. F.Caton, R. G.Parris, R. T.Pedersen, T. R.Thompson, D. C.Wiens, K. C.Groves, K. M.2018-11-13T11:46:25Z2018-11-13T11:46:25Z2013-02-22McNamara, L. F., Caton, R. G., Parris, R. T., Pedersen, T. R., Thompson, D. C., Wiens, K. C., & Groves, K. M. (2013). Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms.==$Radio science, 48$==(2), 89-101. https://doi.org/10.1002/rds.20025http://hdl.handle.net/20.500.12816/3543Radio sciencehttps://doi.org/10.1002/rds.20025Since their discovery in the 1970s, equatorial plasma bubbles (EPBs) have been invoked to explain the propagation of VHF signals on trans‐equatorial circuits at night, and blamed for highly detrimental scintillation of VHF and GHz trans‐ionospheric communications signals in equatorial regions. Over the last four decades, the properties of EPBs have been deduced by multiple techniques such as incoherent scatter radar, 630 nm airglow, depletions in GPS total electron content observations, VHF and GHz scintillations, and HF observations by ionosondes. The initiation and evolution of EPBs have by now been successfully modeled and a good understanding developed of the underlying physics. However, different communities tend to concentrate on a single observing technique, without regard to whether the different techniques provide a consistent physical picture. In contrast, this paper discusses two very different types of observations made on a night‐by‐night basis during the COPEX campaign of late 2002 in Brazil, namely, VHF scintillations and ionograms, and shows that the two methods of observation can provide a consistent interpretation of the properties of EPBs. For example, an EPB seen as an eastward drifting scintillation event can also be seen as an extra ionogram reflection trace that moves closer to and then away from the ionosonde site. The scintillations are attributed to strong gradients across the walls of an EPB, whereas the extra ionogram traces are attributed to oblique reflection of the ionosonde signals from the walls of the EPB.Por paresapplication/pdfengAmerican Geophysical Unionurn:issn:0048-6604info:eu-repo/semantics/openAccessEquatorial ionosphereEquatorial plasma bubblesPlasmahttp://purl.org/pe-repo/ocde/ford#1.05.01Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionogramsinfo:eu-repo/semantics/articlereponame:IGP-Institucionalinstname:Instituto Geofísico del Perúinstacron:IGPORIGINALIGP-1-1-1-1495145285.pdfIGP-1-1-1-1495145285.pdfapplication/pdf1699061https://repositorio.igp.gob.pe/bitstreams/9b81a887-4b55-4eae-85fe-9c67a5131d13/downloadedc3fc28052fcf44a4f89c7494173207MD51LICENSElicense.txtlicense.txttext/plain; charset=utf-8391https://repositorio.igp.gob.pe/bitstreams/3c85a5bf-2462-487c-90e5-bb61db60d44e/downloadef941c35636116525aadeaab7bbf4ca3MD52THUMBNAILIGP-1-1-1-1495145285.pdf.jpgIGP-1-1-1-1495145285.pdf.jpgIM Thumbnailimage/jpeg94823https://repositorio.igp.gob.pe/bitstreams/52f5f52e-b1b3-475a-b58b-8e3869f90e18/downloadede4bbd4883fe4b5f27399aa57db18c6MD53TEXTIGP-1-1-1-1495145285.pdf.txtIGP-1-1-1-1495145285.pdf.txtExtracted texttext/plain57937https://repositorio.igp.gob.pe/bitstreams/9c8788ff-6e48-4aab-8ff1-baca9383a09e/download7f14f2279afcff7c035f9c35eee68e7eMD5420.500.12816/3543oai:repositorio.igp.gob.pe:20.500.12816/35432025-08-14 10:52:59.119open.accesshttps://repositorio.igp.gob.peRepositorio Geofísico Nacionalbiblio@igp.gob.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
dc.title.none.fl_str_mv Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms
title Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms
spellingShingle Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms
McNamara, L. F.
Equatorial ionosphere
Equatorial plasma bubbles
Plasma
http://purl.org/pe-repo/ocde/ford#1.05.01
title_short Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms
title_full Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms
title_fullStr Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms
title_full_unstemmed Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms
title_sort Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms
author McNamara, L. F.
author_facet McNamara, L. F.
Caton, R. G.
Parris, R. T.
Pedersen, T. R.
Thompson, D. C.
Wiens, K. C.
Groves, K. M.
author_role author
author2 Caton, R. G.
Parris, R. T.
Pedersen, T. R.
Thompson, D. C.
Wiens, K. C.
Groves, K. M.
author2_role author
author
author
author
author
author
dc.contributor.author.fl_str_mv McNamara, L. F.
Caton, R. G.
Parris, R. T.
Pedersen, T. R.
Thompson, D. C.
Wiens, K. C.
Groves, K. M.
dc.subject.none.fl_str_mv Equatorial ionosphere
Equatorial plasma bubbles
Plasma
topic Equatorial ionosphere
Equatorial plasma bubbles
Plasma
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 Since their discovery in the 1970s, equatorial plasma bubbles (EPBs) have been invoked to explain the propagation of VHF signals on trans‐equatorial circuits at night, and blamed for highly detrimental scintillation of VHF and GHz trans‐ionospheric communications signals in equatorial regions. Over the last four decades, the properties of EPBs have been deduced by multiple techniques such as incoherent scatter radar, 630 nm airglow, depletions in GPS total electron content observations, VHF and GHz scintillations, and HF observations by ionosondes. The initiation and evolution of EPBs have by now been successfully modeled and a good understanding developed of the underlying physics. However, different communities tend to concentrate on a single observing technique, without regard to whether the different techniques provide a consistent physical picture. In contrast, this paper discusses two very different types of observations made on a night‐by‐night basis during the COPEX campaign of late 2002 in Brazil, namely, VHF scintillations and ionograms, and shows that the two methods of observation can provide a consistent interpretation of the properties of EPBs. For example, an EPB seen as an eastward drifting scintillation event can also be seen as an extra ionogram reflection trace that moves closer to and then away from the ionosonde site. The scintillations are attributed to strong gradients across the walls of an EPB, whereas the extra ionogram traces are attributed to oblique reflection of the ionosonde signals from the walls of the EPB.
publishDate 2013
dc.date.accessioned.none.fl_str_mv 2018-11-13T11:46:25Z
dc.date.available.none.fl_str_mv 2018-11-13T11:46:25Z
dc.date.issued.fl_str_mv 2013-02-22
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.citation.none.fl_str_mv McNamara, L. F., Caton, R. G., Parris, R. T., Pedersen, T. R., Thompson, D. C., Wiens, K. C., & Groves, K. M. (2013). Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms.==$Radio science, 48$==(2), 89-101. https://doi.org/10.1002/rds.20025
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/20.500.12816/3543
dc.identifier.journal.none.fl_str_mv Radio science
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1002/rds.20025
identifier_str_mv McNamara, L. F., Caton, R. G., Parris, R. T., Pedersen, T. R., Thompson, D. C., Wiens, K. C., & Groves, K. M. (2013). Signatures of equatorial plasma bubbles in VHF satellite scintillations and equatorial ionograms.==$Radio science, 48$==(2), 89-101. https://doi.org/10.1002/rds.20025
Radio science
url http://hdl.handle.net/20.500.12816/3543
https://doi.org/10.1002/rds.20025
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv urn:issn:0048-6604
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
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dc.publisher.none.fl_str_mv American Geophysical Union
publisher.none.fl_str_mv American Geophysical Union
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