Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies
- Autores
- Yiğit, Erdal; Kilcik, Ali; Elias, Ana Georgina; Dönmez, Burçin; Ozguc, Atila; Yurchshyn, Vasyl; Rozelot, Jean Pierre
- Año de publicación
- 2018
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The long term solar activity dependencies of ionospheric F1 and F2 regions’ critical frequencies (f0F1 and f0F2) are analyzed for the last four solar cycles (1976–2015). We show that the ionospheric F1 and F2 regions have different solar activity dependencies in terms of the sunspot group (SG) numbers: F1 region critical frequency (f0F1) peaks at the same time with the small SG numbers, while the f0F2 reaches its maximum at the same time with the large SG numbers, especially during the solar cycle 23. The observed differences in the sensitivity of ionospheric critical frequencies to sunspot group (SG) numbers provide a new insight into the solar activity effects on the ionosphere and space weather. While the F1 layer is influenced by the slow solar wind, which is largely associated with small SGs, the ionospheric F2 layer is more sensitive to Coronal Mass Ejections (CMEs) and fast solar winds, which are mainly produced by large SGs and coronal holes. The SG numbers maximize during of peak of the solar cycle and the number of coronal holes peaks during the sunspot declining phase. During solar minimum there are relatively less large SGs, hence reduced CME and flare activity. These results provide a new perspective for assessing how the different regions of the ionosphere respond to space weather effects.
Fil: Yiğit, Erdal. George Mason University; Estados Unidos
Fil: Kilcik, Ali. Akdeniz University; Turquía
Fil: Elias, Ana Georgina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina
Fil: Dönmez, Burçin. Akdeniz University; Turquía
Fil: Ozguc, Atila. Bogazici University; Turquía
Fil: Yurchshyn, Vasyl. Big Bear Solar Observatory; Estados Unidos. Korea Astronomy and Space Science Institute; Corea del Sur
Fil: Rozelot, Jean Pierre. Observatoire de la Cote D'Azur; Francia - Materia
-
IONOSPHERE
IONOSPHERIC CRITICAL FREQUENCIES
SOLAR CYCLE
SUNSPOTS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/90431
Ver los metadatos del registro completo
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Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependenciesYiğit, ErdalKilcik, AliElias, Ana GeorginaDönmez, BurçinOzguc, AtilaYurchshyn, VasylRozelot, Jean PierreIONOSPHEREIONOSPHERIC CRITICAL FREQUENCIESSOLAR CYCLESUNSPOTShttps://purl.org/becyt/ford/1.5https://purl.org/becyt/ford/1The long term solar activity dependencies of ionospheric F1 and F2 regions’ critical frequencies (f0F1 and f0F2) are analyzed for the last four solar cycles (1976–2015). We show that the ionospheric F1 and F2 regions have different solar activity dependencies in terms of the sunspot group (SG) numbers: F1 region critical frequency (f0F1) peaks at the same time with the small SG numbers, while the f0F2 reaches its maximum at the same time with the large SG numbers, especially during the solar cycle 23. The observed differences in the sensitivity of ionospheric critical frequencies to sunspot group (SG) numbers provide a new insight into the solar activity effects on the ionosphere and space weather. While the F1 layer is influenced by the slow solar wind, which is largely associated with small SGs, the ionospheric F2 layer is more sensitive to Coronal Mass Ejections (CMEs) and fast solar winds, which are mainly produced by large SGs and coronal holes. The SG numbers maximize during of peak of the solar cycle and the number of coronal holes peaks during the sunspot declining phase. During solar minimum there are relatively less large SGs, hence reduced CME and flare activity. These results provide a new perspective for assessing how the different regions of the ionosphere respond to space weather effects.Fil: Yiğit, Erdal. George Mason University; Estados UnidosFil: Kilcik, Ali. Akdeniz University; TurquíaFil: Elias, Ana Georgina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; ArgentinaFil: Dönmez, Burçin. Akdeniz University; TurquíaFil: Ozguc, Atila. Bogazici University; TurquíaFil: Yurchshyn, Vasyl. Big Bear Solar Observatory; Estados Unidos. Korea Astronomy and Space Science Institute; Corea del SurFil: Rozelot, Jean Pierre. Observatoire de la Cote D'Azur; FranciaElsevier2018-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/90431Yiğit, Erdal; Kilcik, Ali; Elias, Ana Georgina; Dönmez, Burçin; Ozguc, Atila; et al.; Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies; Elsevier; Journal of Atmospheric and Solar-Terrestrial Physics; 171; 6-2018; 157-1631364-6826CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S1364682617301384info:eu-repo/semantics/altIdentifier/doi/10.1016/j.jastp.2017.11.018info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1711.11126info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:43:40Zoai:ri.conicet.gov.ar:11336/90431instacron: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 09:43:40.783CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies |
title |
Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies |
spellingShingle |
Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies Yiğit, Erdal IONOSPHERE IONOSPHERIC CRITICAL FREQUENCIES SOLAR CYCLE SUNSPOTS |
title_short |
Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies |
title_full |
Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies |
title_fullStr |
Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies |
title_full_unstemmed |
Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies |
title_sort |
Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies |
dc.creator.none.fl_str_mv |
Yiğit, Erdal Kilcik, Ali Elias, Ana Georgina Dönmez, Burçin Ozguc, Atila Yurchshyn, Vasyl Rozelot, Jean Pierre |
author |
Yiğit, Erdal |
author_facet |
Yiğit, Erdal Kilcik, Ali Elias, Ana Georgina Dönmez, Burçin Ozguc, Atila Yurchshyn, Vasyl Rozelot, Jean Pierre |
author_role |
author |
author2 |
Kilcik, Ali Elias, Ana Georgina Dönmez, Burçin Ozguc, Atila Yurchshyn, Vasyl Rozelot, Jean Pierre |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
IONOSPHERE IONOSPHERIC CRITICAL FREQUENCIES SOLAR CYCLE SUNSPOTS |
topic |
IONOSPHERE IONOSPHERIC CRITICAL FREQUENCIES SOLAR CYCLE SUNSPOTS |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.5 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The long term solar activity dependencies of ionospheric F1 and F2 regions’ critical frequencies (f0F1 and f0F2) are analyzed for the last four solar cycles (1976–2015). We show that the ionospheric F1 and F2 regions have different solar activity dependencies in terms of the sunspot group (SG) numbers: F1 region critical frequency (f0F1) peaks at the same time with the small SG numbers, while the f0F2 reaches its maximum at the same time with the large SG numbers, especially during the solar cycle 23. The observed differences in the sensitivity of ionospheric critical frequencies to sunspot group (SG) numbers provide a new insight into the solar activity effects on the ionosphere and space weather. While the F1 layer is influenced by the slow solar wind, which is largely associated with small SGs, the ionospheric F2 layer is more sensitive to Coronal Mass Ejections (CMEs) and fast solar winds, which are mainly produced by large SGs and coronal holes. The SG numbers maximize during of peak of the solar cycle and the number of coronal holes peaks during the sunspot declining phase. During solar minimum there are relatively less large SGs, hence reduced CME and flare activity. These results provide a new perspective for assessing how the different regions of the ionosphere respond to space weather effects. Fil: Yiğit, Erdal. George Mason University; Estados Unidos Fil: Kilcik, Ali. Akdeniz University; Turquía Fil: Elias, Ana Georgina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina. Universidad Nacional de Tucumán. Facultad de Ciencias Exactas y Tecnología; Argentina Fil: Dönmez, Burçin. Akdeniz University; Turquía Fil: Ozguc, Atila. Bogazici University; Turquía Fil: Yurchshyn, Vasyl. Big Bear Solar Observatory; Estados Unidos. Korea Astronomy and Space Science Institute; Corea del Sur Fil: Rozelot, Jean Pierre. Observatoire de la Cote D'Azur; Francia |
description |
The long term solar activity dependencies of ionospheric F1 and F2 regions’ critical frequencies (f0F1 and f0F2) are analyzed for the last four solar cycles (1976–2015). We show that the ionospheric F1 and F2 regions have different solar activity dependencies in terms of the sunspot group (SG) numbers: F1 region critical frequency (f0F1) peaks at the same time with the small SG numbers, while the f0F2 reaches its maximum at the same time with the large SG numbers, especially during the solar cycle 23. The observed differences in the sensitivity of ionospheric critical frequencies to sunspot group (SG) numbers provide a new insight into the solar activity effects on the ionosphere and space weather. While the F1 layer is influenced by the slow solar wind, which is largely associated with small SGs, the ionospheric F2 layer is more sensitive to Coronal Mass Ejections (CMEs) and fast solar winds, which are mainly produced by large SGs and coronal holes. The SG numbers maximize during of peak of the solar cycle and the number of coronal holes peaks during the sunspot declining phase. During solar minimum there are relatively less large SGs, hence reduced CME and flare activity. These results provide a new perspective for assessing how the different regions of the ionosphere respond to space weather effects. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018-06 |
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/11336/90431 Yiğit, Erdal; Kilcik, Ali; Elias, Ana Georgina; Dönmez, Burçin; Ozguc, Atila; et al.; Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies; Elsevier; Journal of Atmospheric and Solar-Terrestrial Physics; 171; 6-2018; 157-163 1364-6826 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/90431 |
identifier_str_mv |
Yiğit, Erdal; Kilcik, Ali; Elias, Ana Georgina; Dönmez, Burçin; Ozguc, Atila; et al.; Critical frequencies of the ionospheric F1 and F2 layers during the last four solar cycles: Sunspot group type dependencies; Elsevier; Journal of Atmospheric and Solar-Terrestrial Physics; 171; 6-2018; 157-163 1364-6826 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S1364682617301384 info:eu-repo/semantics/altIdentifier/doi/10.1016/j.jastp.2017.11.018 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1711.11126 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-nd/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-nd/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Elsevier |
publisher.none.fl_str_mv |
Elsevier |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
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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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1844613374448500736 |
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13.070432 |