@Article{SilvaDRMSCCBPCBS:2023:CaSt,
author = "Silva, R{\'e}gia Pereira da and Denardini, Clezio Marcos and
Resende, Laysa Cristina Ara{\'u}jo and Moro, Juliano and
Sousasantos, Jonas and Carmo, Carolina de Sousa do and Chen, Sony
Su and Barbosa Neto, Paulo Fran{\c{c}}a and Pican{\c{c}}o,
Giorgio Arlan da Silva and Campelo, Jaziel Felipe Braga and Borba,
Gilvan Luiz and Santos, Marcos Aur{\'e}lio Ferreira dos",
affiliation = "{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 Texas at Dallas (UTD)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Universidade
Salesiana de S{\~a}o Paulo (UNISAL)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Universidade Federal do Rio
Grande do Norte (UFRN)} and {Universidade Federal do Rio Grande do
Norte (UFRN)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)}",
title = "Latitudinal responses of the ionosphere over South America during
HILDCAA intervals: Case studies",
journal = "Advances in Space Research",
year = "2023",
volume = "71",
number = "12",
pages = "5185--5195",
note = "{Setores de Atividade: Pesquisa e desenvolvimento
cient{\'{\i}}fico.}",
keywords = "Space Weather, HILDCAA, Low Latitude Aeronomy.",
abstract = "Aspects regarding the influence of High-Intensity Long-Duration
Continuous Auroral Electrojet Activity (HILDCAA) intervals on
ionospheric dynamics have been objecting to increasing interest in
the last years. Notwithstanding, some key interconnections between
the HILDCAA intervals impacts on the ionosphere over distinct
latitudes, according to the solar cycle phase, remain to require
further investigation. In this work, the F2 layer peak height and
its critical frequency (hmF2 and foF2, respectively) from
Digisonde data obtained over Sao Lu\ıīs (2.60 S; 44.21 W),
Cachoeira Paulista (22.70 S; 44.98 W), and Port Stanley (51.60 S,
57.9 W), were evaluated to unravel more details of the ionospheric
responses to four HILDCAA intervals as case studies. Those are
equatorial, low, and midlatitude stations, respectively, and the
main results over them presented a similar trend in terms of solar
cycle dependence, with the greater impact on the ionospheric
density along with solar maximum conditions, despite the higher
frequency of HILDCAA occurrences in the descending and minimum
phases. The variation of hmF2 due to HILDCAA effects in comparison
to quiet time is about 20% in equatorial and mid-latitudes, while
over the low latitude station the hmF2 ranges positively up to
40%. These results enhance our understanding of the HILDCAAs
magnitude degree both regarding its solar cycle occurrence, and
its effects in different ionospheric latitudinal sections.",
doi = "10.1016/j.asr.2023.02.020",
url = "http://dx.doi.org/10.1016/j.asr.2023.02.020",
issn = "0273-1177 and 1879-1948",
label = "lattes: 8030262077949409 2 SilvaNRMSCSFPCBS:2023:CaSt",
language = "en",
targetfile = "1-s2.0-S0273117723001394-main.pdf",
urlaccessdate = "11 maio 2024"
}