Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability
- Autores
- Perin Bertoni, Fernando Celso; Raulin, Jean Pierre; Rivero Gavilán, Hernán; Kaufmann, Pierre; Rodriguez, Rodolfo; Clilverd, Mark; Samanes Cárdenas, Jorge; Fernandez, German Enzo Leonel
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Daily profiles of phase measurements as observed on fixed VLF paths generally show a transient phase advance, followed by a phase delay, for about 90 min after sunrise hours. This is indicative of a reflecting ionospheric C region developing along the terminator line at an altitude below the normal D region. The suggested occurrence of a C region is consistent with rocket measurements made in the 1960s, showing a maximum of the electron density between 64 and 68 km, and by radio sounding in the 1980s. In order to correctly describe the properties of the phase effect associated with the presence of a C region, it is important to understand the subionospheric propagation characteristics of the VLF paths. In this paper, we analyze the variations presented by the temporal properties of the VLF narrowband phase effect and determined a parameter associated with the appearance of the C region at sunrise hours observed by receivers from the South America VLF Network. Periodic patterns emerge from the parameter curves. Two distinct temporal behavior regimes can be identified: one exhibiting slow variations between March and October, and another one exhibiting faster variations between October and March. Solar illumination conditions and the geometrical configuration of the VLF paths relative to the sunrise terminator partly explain the slow variation regime. During periods of faster variations, we have observed good association with atmospheric temperature variability found in the measurements of the Thermosphere Ionosphere Mesosphere Energetics and Dynamics and Sounding of the Atmosphere using Broadband Emission Radiometry satellite instrument, which we assume to be related to the winter anomaly atmospheric phenomenon. However, when comparing the parameter time series with temperature curves, no direct one-to-one correspondence was found for transient events.
Fil: Perin Bertoni, Fernando Celso. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil
Fil: Raulin, Jean Pierre. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil
Fil: Rivero Gavilán, Hernán. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil. Ministério da Ciência e Tecnologia. Instituto Nacional de Pesquisas Espaciais; Brasil
Fil: Kaufmann, Pierre. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil
Fil: Rodriguez, Rodolfo. Universidad de Piura; Perú
Fil: Clilverd, Mark. University Of Cambridge; Reino Unido
Fil: Samanes Cárdenas, Jorge. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil
Fil: Fernandez, German Enzo Leonel. Consejo Nacional de Investigaciones Cientíâficas y Técnicas. Centro Cientíâfico Tecnológico San Juan. Complejo Astronómico "el Leoncito"; Argentina - Materia
-
IONOSPHERE
VLF TECHNIQUE
SOLAR MONITORING
UPPER AND LOWER ATMOSPHERE INTERACTION - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/8922
Ver los metadatos del registro completo
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Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variabilityPerin Bertoni, Fernando CelsoRaulin, Jean PierreRivero Gavilán, HernánKaufmann, PierreRodriguez, RodolfoClilverd, MarkSamanes Cárdenas, JorgeFernandez, German Enzo LeonelIONOSPHEREVLF TECHNIQUESOLAR MONITORINGUPPER AND LOWER ATMOSPHERE INTERACTIONhttps://purl.org/becyt/ford/1.5https://purl.org/becyt/ford/1https://purl.org/becyt/ford/2.2https://purl.org/becyt/ford/2Daily profiles of phase measurements as observed on fixed VLF paths generally show a transient phase advance, followed by a phase delay, for about 90 min after sunrise hours. This is indicative of a reflecting ionospheric C region developing along the terminator line at an altitude below the normal D region. The suggested occurrence of a C region is consistent with rocket measurements made in the 1960s, showing a maximum of the electron density between 64 and 68 km, and by radio sounding in the 1980s. In order to correctly describe the properties of the phase effect associated with the presence of a C region, it is important to understand the subionospheric propagation characteristics of the VLF paths. In this paper, we analyze the variations presented by the temporal properties of the VLF narrowband phase effect and determined a parameter associated with the appearance of the C region at sunrise hours observed by receivers from the South America VLF Network. Periodic patterns emerge from the parameter curves. Two distinct temporal behavior regimes can be identified: one exhibiting slow variations between March and October, and another one exhibiting faster variations between October and March. Solar illumination conditions and the geometrical configuration of the VLF paths relative to the sunrise terminator partly explain the slow variation regime. During periods of faster variations, we have observed good association with atmospheric temperature variability found in the measurements of the Thermosphere Ionosphere Mesosphere Energetics and Dynamics and Sounding of the Atmosphere using Broadband Emission Radiometry satellite instrument, which we assume to be related to the winter anomaly atmospheric phenomenon. However, when comparing the parameter time series with temperature curves, no direct one-to-one correspondence was found for transient events.Fil: Perin Bertoni, Fernando Celso. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; BrasilFil: Raulin, Jean Pierre. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; BrasilFil: Rivero Gavilán, Hernán. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil. Ministério da Ciência e Tecnologia. Instituto Nacional de Pesquisas Espaciais; BrasilFil: Kaufmann, Pierre. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; BrasilFil: Rodriguez, Rodolfo. Universidad de Piura; PerúFil: Clilverd, Mark. University Of Cambridge; Reino UnidoFil: Samanes Cárdenas, Jorge. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; BrasilFil: Fernandez, German Enzo Leonel. Consejo Nacional de Investigaciones Cientíâficas y Técnicas. Centro Cientíâfico Tecnológico San Juan. Complejo Astronómico "el Leoncito"; ArgentinaAmerican Geophysical Union2013-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/8922Perin Bertoni, Fernando Celso; Raulin, Jean Pierre; Rivero Gavilán, Hernán; Kaufmann, Pierre; Rodriguez, Rodolfo; et al.; Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability; American Geophysical Union; Journal Of Geophysical Research; 118; 10; 10-2013; 6686-66930148-0227enginfo:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1002/jgra.50559/fullinfo:eu-repo/semantics/altIdentifier/doi/10.1002/jgra.50559info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:35:10Zoai:ri.conicet.gov.ar:11336/8922instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:35:10.348CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability |
title |
Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability |
spellingShingle |
Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability Perin Bertoni, Fernando Celso IONOSPHERE VLF TECHNIQUE SOLAR MONITORING UPPER AND LOWER ATMOSPHERE INTERACTION |
title_short |
Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability |
title_full |
Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability |
title_fullStr |
Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability |
title_full_unstemmed |
Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability |
title_sort |
Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability |
dc.creator.none.fl_str_mv |
Perin Bertoni, Fernando Celso Raulin, Jean Pierre Rivero Gavilán, Hernán Kaufmann, Pierre Rodriguez, Rodolfo Clilverd, Mark Samanes Cárdenas, Jorge Fernandez, German Enzo Leonel |
author |
Perin Bertoni, Fernando Celso |
author_facet |
Perin Bertoni, Fernando Celso Raulin, Jean Pierre Rivero Gavilán, Hernán Kaufmann, Pierre Rodriguez, Rodolfo Clilverd, Mark Samanes Cárdenas, Jorge Fernandez, German Enzo Leonel |
author_role |
author |
author2 |
Raulin, Jean Pierre Rivero Gavilán, Hernán Kaufmann, Pierre Rodriguez, Rodolfo Clilverd, Mark Samanes Cárdenas, Jorge Fernandez, German Enzo Leonel |
author2_role |
author author author author author author author |
dc.subject.none.fl_str_mv |
IONOSPHERE VLF TECHNIQUE SOLAR MONITORING UPPER AND LOWER ATMOSPHERE INTERACTION |
topic |
IONOSPHERE VLF TECHNIQUE SOLAR MONITORING UPPER AND LOWER ATMOSPHERE INTERACTION |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.5 https://purl.org/becyt/ford/1 https://purl.org/becyt/ford/2.2 https://purl.org/becyt/ford/2 |
dc.description.none.fl_txt_mv |
Daily profiles of phase measurements as observed on fixed VLF paths generally show a transient phase advance, followed by a phase delay, for about 90 min after sunrise hours. This is indicative of a reflecting ionospheric C region developing along the terminator line at an altitude below the normal D region. The suggested occurrence of a C region is consistent with rocket measurements made in the 1960s, showing a maximum of the electron density between 64 and 68 km, and by radio sounding in the 1980s. In order to correctly describe the properties of the phase effect associated with the presence of a C region, it is important to understand the subionospheric propagation characteristics of the VLF paths. In this paper, we analyze the variations presented by the temporal properties of the VLF narrowband phase effect and determined a parameter associated with the appearance of the C region at sunrise hours observed by receivers from the South America VLF Network. Periodic patterns emerge from the parameter curves. Two distinct temporal behavior regimes can be identified: one exhibiting slow variations between March and October, and another one exhibiting faster variations between October and March. Solar illumination conditions and the geometrical configuration of the VLF paths relative to the sunrise terminator partly explain the slow variation regime. During periods of faster variations, we have observed good association with atmospheric temperature variability found in the measurements of the Thermosphere Ionosphere Mesosphere Energetics and Dynamics and Sounding of the Atmosphere using Broadband Emission Radiometry satellite instrument, which we assume to be related to the winter anomaly atmospheric phenomenon. However, when comparing the parameter time series with temperature curves, no direct one-to-one correspondence was found for transient events. Fil: Perin Bertoni, Fernando Celso. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil Fil: Raulin, Jean Pierre. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil Fil: Rivero Gavilán, Hernán. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil. Ministério da Ciência e Tecnologia. Instituto Nacional de Pesquisas Espaciais; Brasil Fil: Kaufmann, Pierre. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil Fil: Rodriguez, Rodolfo. Universidad de Piura; Perú Fil: Clilverd, Mark. University Of Cambridge; Reino Unido Fil: Samanes Cárdenas, Jorge. Universidade Presbiteriana Mackenzie. Escola de Engenharia. Centro de Radio Astronomia E Astrofisica; Brasil Fil: Fernandez, German Enzo Leonel. Consejo Nacional de Investigaciones Cientíâficas y Técnicas. Centro Cientíâfico Tecnológico San Juan. Complejo Astronómico "el Leoncito"; Argentina |
description |
Daily profiles of phase measurements as observed on fixed VLF paths generally show a transient phase advance, followed by a phase delay, for about 90 min after sunrise hours. This is indicative of a reflecting ionospheric C region developing along the terminator line at an altitude below the normal D region. The suggested occurrence of a C region is consistent with rocket measurements made in the 1960s, showing a maximum of the electron density between 64 and 68 km, and by radio sounding in the 1980s. In order to correctly describe the properties of the phase effect associated with the presence of a C region, it is important to understand the subionospheric propagation characteristics of the VLF paths. In this paper, we analyze the variations presented by the temporal properties of the VLF narrowband phase effect and determined a parameter associated with the appearance of the C region at sunrise hours observed by receivers from the South America VLF Network. Periodic patterns emerge from the parameter curves. Two distinct temporal behavior regimes can be identified: one exhibiting slow variations between March and October, and another one exhibiting faster variations between October and March. Solar illumination conditions and the geometrical configuration of the VLF paths relative to the sunrise terminator partly explain the slow variation regime. During periods of faster variations, we have observed good association with atmospheric temperature variability found in the measurements of the Thermosphere Ionosphere Mesosphere Energetics and Dynamics and Sounding of the Atmosphere using Broadband Emission Radiometry satellite instrument, which we assume to be related to the winter anomaly atmospheric phenomenon. However, when comparing the parameter time series with temperature curves, no direct one-to-one correspondence was found for transient events. |
publishDate |
2013 |
dc.date.none.fl_str_mv |
2013-10 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/8922 Perin Bertoni, Fernando Celso; Raulin, Jean Pierre; Rivero Gavilán, Hernán; Kaufmann, Pierre; Rodriguez, Rodolfo; et al.; Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability; American Geophysical Union; Journal Of Geophysical Research; 118; 10; 10-2013; 6686-6693 0148-0227 |
url |
http://hdl.handle.net/11336/8922 |
identifier_str_mv |
Perin Bertoni, Fernando Celso; Raulin, Jean Pierre; Rivero Gavilán, Hernán; Kaufmann, Pierre; Rodriguez, Rodolfo; et al.; Lower ionosphere monitoring by the South America VLF Network (SAVNET): C region occurrence and atmospheric temperature variability; American Geophysical Union; Journal Of Geophysical Research; 118; 10; 10-2013; 6686-6693 0148-0227 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1002/jgra.50559/full info:eu-repo/semantics/altIdentifier/doi/10.1002/jgra.50559 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
American Geophysical Union |
publisher.none.fl_str_mv |
American Geophysical Union |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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