Climatology of atmospheric solar tidal mode effects on ionospheric F2 parameters over the American sector during solar minimum between cycles #23 and #24

This work presents the contribution of solar atmospheric tides (diurnal, semidiurnal, and terdiurnal modes) to the variability of the parameters critical frequency (foF2) and peak height of the F2-layer (hmF2) in the American sector during the transition of solar cycles #23 and #24, a period conside...

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Main Authors: A. M. Santos, G. Yang, A. A. Pimenta, C. G. M. Brum, I. S. Batista, J. H. A. Sobral, V. F. Andrioli, P. P. Batista, M. A. Abdu, J. R. Souza, P. K. Manoharan, C. Wang, H. Li, Z. Liu
Format: Article
Language:English
Published: Frontiers Media S.A. 2024-01-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2024.1325218/full
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author A. M. Santos
A. M. Santos
A. M. Santos
G. Yang
A. A. Pimenta
C. G. M. Brum
I. S. Batista
J. H. A. Sobral
V. F. Andrioli
V. F. Andrioli
V. F. Andrioli
P. P. Batista
M. A. Abdu
J. R. Souza
P. K. Manoharan
C. Wang
H. Li
Z. Liu
author_facet A. M. Santos
A. M. Santos
A. M. Santos
G. Yang
A. A. Pimenta
C. G. M. Brum
I. S. Batista
J. H. A. Sobral
V. F. Andrioli
V. F. Andrioli
V. F. Andrioli
P. P. Batista
M. A. Abdu
J. R. Souza
P. K. Manoharan
C. Wang
H. Li
Z. Liu
author_sort A. M. Santos
collection DOAJ
description This work presents the contribution of solar atmospheric tides (diurnal, semidiurnal, and terdiurnal modes) to the variability of the parameters critical frequency (foF2) and peak height of the F2-layer (hmF2) in the American sector during the transition of solar cycles #23 and #24, a period considered one of the lowest solar activities of the modern era. The Digisonde data available in the GIRO data center were analyzed (12 stations), and the solar tide modes were evaluated regarding their amplitude, latitude, and seasonal dependence. The results showed that the hmF2 and foF2 strongly depend on latitude and seasonality, being more intense in the stations located in the south hemisphere. The same behavior is seen for the tidal amplitude fitted in these parameters, except for hmF2 diurnal tide, which is more intense at latitudes farther from the equator. Moreover, the seasonal variability of the amplitude of hmF2 in most cases presented an annual and semiannual component. A terannual component was also observed in 8 h tide mode in the height and frequency parameters. Likewise, what was observed in foF2, the variability in the mean amplitude and different modes of tides of hmF2 are higher over the sectors located in the southern hemisphere.
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spelling doaj.art-143648537da249ea93bef0491ebdc1ef2024-01-25T04:29:04ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2024-01-011110.3389/fspas.2024.13252181325218Climatology of atmospheric solar tidal mode effects on ionospheric F2 parameters over the American sector during solar minimum between cycles #23 and #24A. M. Santos0A. M. Santos1A. M. Santos2G. Yang3A. A. Pimenta4C. G. M. Brum5I. S. Batista6J. H. A. Sobral7V. F. Andrioli8V. F. Andrioli9V. F. Andrioli10P. P. Batista11M. A. Abdu12J. R. Souza13P. K. Manoharan14C. Wang15H. Li16Z. Liu17State Key Laboratory of Space Weather, National Space Science Center/Chinese Academy of Sciences, Beijing, ChinaChina-Brazil Joint Laboratory for Space Weather, National Space Science Center, São José dos Campos, BrazilNational Institute for Space Research, Heliophysics, Planetary Sciences and Aeronomy Division, São José dos Campos, São Paulo, BrazilState Key Laboratory of Space Weather, National Space Science Center/Chinese Academy of Sciences, Beijing, ChinaNational Institute for Space Research, Heliophysics, Planetary Sciences and Aeronomy Division, São José dos Campos, São Paulo, BrazilFlorida Space Institute, University of Central Florida, Orlando, FL, United StatesNational Institute for Space Research, Heliophysics, Planetary Sciences and Aeronomy Division, São José dos Campos, São Paulo, BrazilNational Institute for Space Research, Heliophysics, Planetary Sciences and Aeronomy Division, São José dos Campos, São Paulo, BrazilState Key Laboratory of Space Weather, National Space Science Center/Chinese Academy of Sciences, Beijing, ChinaChina-Brazil Joint Laboratory for Space Weather, National Space Science Center, São José dos Campos, BrazilNational Institute for Space Research, Heliophysics, Planetary Sciences and Aeronomy Division, São José dos Campos, São Paulo, BrazilNational Institute for Space Research, Heliophysics, Planetary Sciences and Aeronomy Division, São José dos Campos, São Paulo, BrazilNational Institute for Space Research, Heliophysics, Planetary Sciences and Aeronomy Division, São José dos Campos, São Paulo, BrazilNational Institute for Space Research, Heliophysics, Planetary Sciences and Aeronomy Division, São José dos Campos, São Paulo, BrazilFlorida Space Institute, University of Central Florida, Orlando, FL, United StatesState Key Laboratory of Space Weather, National Space Science Center/Chinese Academy of Sciences, Beijing, ChinaState Key Laboratory of Space Weather, National Space Science Center/Chinese Academy of Sciences, Beijing, ChinaState Key Laboratory of Space Weather, National Space Science Center/Chinese Academy of Sciences, Beijing, ChinaThis work presents the contribution of solar atmospheric tides (diurnal, semidiurnal, and terdiurnal modes) to the variability of the parameters critical frequency (foF2) and peak height of the F2-layer (hmF2) in the American sector during the transition of solar cycles #23 and #24, a period considered one of the lowest solar activities of the modern era. The Digisonde data available in the GIRO data center were analyzed (12 stations), and the solar tide modes were evaluated regarding their amplitude, latitude, and seasonal dependence. The results showed that the hmF2 and foF2 strongly depend on latitude and seasonality, being more intense in the stations located in the south hemisphere. The same behavior is seen for the tidal amplitude fitted in these parameters, except for hmF2 diurnal tide, which is more intense at latitudes farther from the equator. Moreover, the seasonal variability of the amplitude of hmF2 in most cases presented an annual and semiannual component. A terannual component was also observed in 8 h tide mode in the height and frequency parameters. Likewise, what was observed in foF2, the variability in the mean amplitude and different modes of tides of hmF2 are higher over the sectors located in the southern hemisphere.https://www.frontiersin.org/articles/10.3389/fspas.2024.1325218/fullionosphereF-region peaksolar atmospheric tidessolar minimumlatitudinal dependence
spellingShingle A. M. Santos
A. M. Santos
A. M. Santos
G. Yang
A. A. Pimenta
C. G. M. Brum
I. S. Batista
J. H. A. Sobral
V. F. Andrioli
V. F. Andrioli
V. F. Andrioli
P. P. Batista
M. A. Abdu
J. R. Souza
P. K. Manoharan
C. Wang
H. Li
Z. Liu
Climatology of atmospheric solar tidal mode effects on ionospheric F2 parameters over the American sector during solar minimum between cycles #23 and #24
Frontiers in Astronomy and Space Sciences
ionosphere
F-region peak
solar atmospheric tides
solar minimum
latitudinal dependence
title Climatology of atmospheric solar tidal mode effects on ionospheric F2 parameters over the American sector during solar minimum between cycles #23 and #24
title_full Climatology of atmospheric solar tidal mode effects on ionospheric F2 parameters over the American sector during solar minimum between cycles #23 and #24
title_fullStr Climatology of atmospheric solar tidal mode effects on ionospheric F2 parameters over the American sector during solar minimum between cycles #23 and #24
title_full_unstemmed Climatology of atmospheric solar tidal mode effects on ionospheric F2 parameters over the American sector during solar minimum between cycles #23 and #24
title_short Climatology of atmospheric solar tidal mode effects on ionospheric F2 parameters over the American sector during solar minimum between cycles #23 and #24
title_sort climatology of atmospheric solar tidal mode effects on ionospheric f2 parameters over the american sector during solar minimum between cycles 23 and 24
topic ionosphere
F-region peak
solar atmospheric tides
solar minimum
latitudinal dependence
url https://www.frontiersin.org/articles/10.3389/fspas.2024.1325218/full
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