@Article{SantosYPBBSABASMWLL:2024:ClAtSo,
author = "Santos, Angela Machado dos and Yang, A. and Pimenta, Alexandre
Alvares and Brum, C. G. M. and Batista, Inez Staciarini and
Sobral, Jos{\'e} Humberto Andrade and Andrioli, Vania F{\'a}tima
and Batista, Paulo Prado and Abdu, Mangalathayil Ali and Souza,
Jonas Rodrigues de and Manoharan, P. K. and Wang, C. and Li, H.
and Liu, Z.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Chinese
Academy of Sciences} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {University of Central Florida} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{University of Central Florida} and {Chinese Academy of Sciences}
and {Chinese Academy of Sciences} and {Chinese Academy of
Sciences}",
title = "Climatology of atmospheric solar tidal mode effects on ionospheric
F2 parameters over the American sector during solar minimum
between cycles #23 and #24",
journal = "Frontiers in Astronomy and Space Sciences",
year = "2024",
volume = "11",
pages = "e1325218",
keywords = "F-region peak, ionosphere, latitudinal dependence, solar
atmospheric tides, solar minimum.",
abstract = "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.",
doi = "10.3389/fspas.2024.1325218",
url = "http://dx.doi.org/10.3389/fspas.2024.1325218",
issn = "2296-987X",
language = "en",
targetfile = "fspas-11-1325218_compressed.pdf",
urlaccessdate = "27 abr. 2024"
}