@Article{SantosBBSASJMT:2023:CoObDa,
author = "Santos, Angela Machado dos and Brum, Christiano G. M. and Batista,
Inez Staciarini and Sobral, Jos{\'e} Humberto Andrade and Abdu,
Mangalathayil Ali and Souza, Jonas Rodrigues de and Jesus, Rodolfo
de and Manoharan, Periasamy K. and Terra, Pedrina",
affiliation = "{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 {University of Central Florida}
and {University of Central Florida}",
title = "Ionospheric Variability over the Brazilian Equatorial Region
during the Minima Solar Cycles 1996 and 2009: Comparison between
Observational Data and the IRI Model",
journal = "Atmosphere",
year = "2023",
volume = "14",
number = "1",
pages = "e87",
month = "Jan.",
keywords = "atmospheric tides, deep solar minimum, F layer parameters, IRI
model, PRE.",
abstract = "The behavior of the Brazilian equatorial ionosphere during the
solar minimum periods, 1996 and 2009, which cover the solar cycles
22/23 and 23/24, respectively, is investigated. For this, the F2
layer critical frequency (foF2) and peak height (hmF2) registered
by a Digisonde operated at S{\~a}o Luis (2.33° S; 44° W) are
carefully analyzed. The results show that the seasonal mean values
of the foF2 and the hmF2 in the equinoxes and winter during 2009
were lower than in 1996. In the summer, an anomalous response to
solar variability was observed. In this case, the hmF2 in 2009 is
higher than in 1996 during a specific daytime interval. Besides
that, it was verified that the prereversal enhancement of the
zonal electric field (PRE) during the equinoxes in 2009 occurred a
few minutes earlier than in 1996. Additionally, a Fast Fourier
Transform (FFT) analysis was used to investigate the impacts of
solar atmospheric tides (amplitude, diurnal, semidiurnal, and
terdiurnal modes) on foF2 and hmF2 parameters with respect to its
seasonality. Significant differences were observed between their
values during the two minima, mainly in the amplitude of hmF2,
which was higher in 1996 than in 2009 for all days analyzed.
Moreover, the seasonality in the diurnal and semidiurnal modes for
both periods presented an annual variability, while the terdiurnal
mode exhibited annual and semiannual components. The results are
compared with the International Reference Ionosphere (IRI) model,
and the main differences between the observation and the model
results are discussed in this work.",
doi = "10.3390/atmos14010087",
url = "http://dx.doi.org/10.3390/atmos14010087",
issn = "2073-4433",
label = "self-archiving-INPE-MCTIC-GOV-BR",
language = "en",
targetfile = "atmosphere-14-00087.pdf",
urlaccessdate = "12 maio 2024"
}