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

被引:0
|
作者
Santos, A. M. [1 ,2 ,3 ]
Yang, G. [1 ]
Pimenta, A. A. [3 ]
Brum, C. G. M. [4 ]
Batista, I. S. [3 ]
Sobral, J. H. A. [3 ]
Andrioli, V. F. [1 ,2 ,3 ]
Batista, P. P. [3 ]
Abdu, M. A. [3 ]
Souza, J. R. [3 ]
Manoharan, P. K. [4 ]
Wang, C. [1 ]
Li, H. [1 ]
Liu, Z. [1 ]
机构
[1] Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing, Peoples R China
[2] Natl Space Sci Ctr, China Brazil Joint Lab Space Weather, Sao Jose Dos Campos, Brazil
[3] Natl Inst Space Res, Heliophys Planetary Sci & Aeron Div, Sao Jose Dos Campos, SP, Brazil
[4] Univ Cent Florida, Florida Space Inst, Orlando, FL USA
基金
巴西圣保罗研究基金会;
关键词
ionosphere; F-region peak; solar atmospheric tides; solar minimum; latitudinal dependence; ELECTRIC-FIELD; TIDES; VARIABILITY; LATITUDES; LAYER; ENHANCEMENT; MESOSPHERE;
D O I
10.3389/fspas.2024.1325218
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This work presents the contribution of solar atmospheric tides (diurnal, semidiurnal, and terdiurnal modes) to the variability of the parameters critical frequency (foF 2 ) and peak height of the F 2 -layer (hmF 2 ) 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 hmF 2 diurnal tide, which is more intense at latitudes farther from the equator. Moreover, the seasonal variability of the amplitude of hmF 2 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 foF 2 , the variability in the mean amplitude and different modes of tides of hmF 2 are higher over the sectors located in the southern hemisphere.
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页数:13
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