@Article{NogueiraAbSoBaBaSaTa:2013:CoObMo,
author = "Nogueira, Paulo Alexandre Bronzato and Abdu, M. A. and Souza, J.
R. and Batista, Inez Staciarini and Bailey, G. J. and Santos, A.
M. and Takahashi, Hisao",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and
Divis{\~a}o de Aeronomia, Instituto Nacional de Pesquisas
Espaciais, S{\~a}o Jos{\'e} dos Campos, 12227-010 S{\~a}o
Paulo, Brazil and Divis{\~a}o de Aeronomia, Instituto Nacional de
Pesquisas Espaciais, S{\~a}o Jos{\'e} dos Campos, 12227-010
S{\~a}o Paulo, Brazil and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and University of Sheffield, Sheffield, England,
United Kingdom and Divis{\~a}o de Aeronomia, Instituto Nacional
de Pesquisas Espaciais, S{\~a}o Jos{\'e} dos Campos, 12227-010
S{\~a}o Paulo, Brazil and {Instituto Nacional de Pesquisas
Espaciais (INPE)}",
title = "Equatorial ionization anomaly development as studied by GPS TEC
and foF2 over Brazil: A comparison of observations with model
results from SUPIM and IRI-2012",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
year = "2013",
volume = "104",
pages = "45--54",
month = "Nov.",
keywords = "equatorial anomaly, equatorial ionization anomalies (EIA),
equatorial ionization anomaly, FoF2, international reference
ionospheres, ionospheric model, TEC, total electron content,
ionization, ionosphere, ionospheric measurement, magnetosphere,
global positioning system.",
abstract = "The equatorial ionization anomaly (EIA) development is studied
using the total electron content (TEC) observed by the Global
Positioning System (GPS) satellites, the F2-layer critical
frequency (foF2) as measured by digisondes operated in the
Brazilian sector, and by model simulation using the SUPIM
(Sheffield University Plasmasphere Ionosphere Model). We have used
two indices based on foF2 and TEC to represent the strength of the
EIA Southern Anomaly Crest (SAC), which are denoted, respectively,
by SAC(foF2) and SAC(TEC). Significant differences in the local
time variations of the EIA intensity, as represented by these two
indices, are investigated. The observed SAC indices are compared
with their values modeled by the SUPIM and also by the
International Reference Ionosphere (IRI)-2012. The SUPIM
simulations that use the standard E×. B plasma drift and neutral
air wind models are found to provide acceptable representations of
the observed foF2 and TEC, and hence the indices SAC(foF2) and
SAC(TEC) during daytime, whereas the IRI-2012 model is not, except
during the post-midnight/sunrise hours. It is found that the
differences in the local time variations between the SAC(foF2) and
SAC(TEC) can be reduced by limiting the TEC integrations in height
up to an altitude of 630. km in the SUPIM calculations. It is also
found that when the EIA intensity is calculated for an
intermediate dip latitude (12°S) the difference between the local
time variation patterns of the two corresponding indices in the
experimental data and in the SUPIM results is reduced. For the
IRI-2012 values, the subequatorial station modification does not
appear to have any effect.",
doi = "10.1016/j.jastp.2013.08.013",
url = "http://dx.doi.org/10.1016/j.jastp.2013.08.013",
issn = "1364-6826",
label = "scopus 2013-11",
language = "en",
targetfile = "1-s2.0-S1364682613002253-main.pdf",
url = "http://dx.doi.org/10.1016/j.jastp.2013.08.013",
urlaccessdate = "05 maio 2024"
}