@Article{BarbosaFaKaFePiDeMu:2018:PaDaSt,
author = "Barbosa, F. R. E. and Fagundes, Paulo Roberto and Kavutarapu,
Venkatesh and Fejer, B. G. and Pillat, V. G. and Denardin, Clezio
Marcos and Muella, M. T. A. H.",
affiliation = "{Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and
{Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and
{Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and {Utah
State University} and {Universidade do Vale do Para{\'{\i}}ba
(UNIVAP)} and {Instituto Nacional de Pesquisas Espaciais (INPE)}
and {Universidade do Vale do Para{\'{\i}}ba (UNIVAP)}",
title = "Multi-scale ionospheric irregularities occurrence over South
America during the St. Patrick's day storm on March 17, 2015",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
year = "2018",
volume = "174",
pages = "32--45",
note = "{Setores de Atividade: Pesquisa e desenvolvimento
cient{\'{\i}}fico.}",
keywords = "Aeronomy, Total Electron Content, Plasma Irregularities, Space
Weather.",
abstract = "During the solar cycle 24 there was a very intense geomagnetic
storm due to the St. Patrick's day storm and the effects of this
storm on ionosphere has become a topic of extensive space weather
investigation. Up to now several aspects of the St. Patrick's
ionospheric storm have been study such as the prompt penetration
electric fields (PPEFs), TEC changes, electron density
disturbances, plasma drift, O+ concentration modification,
hemispherical asymmetry developments, equatorial ionization
anomaly (EIA) modification, and ionospheric irregularities.
Besides all these important studies, there are some essential
aspects, which have not been addressed yet, related to the
occurrence of multi-scale ionospheric irregularities. In this
paper, we present and discuss the generation and suppression of
multi-scale ionospheric irregularities, using the observations
conducted in the Latin American Sector from 4 ionosondes, 20 dual
frequency GPS stations, and JULIA radar observations during the
month of March 2015, which includes the St. Patrick's day
geomagnetic storm period. Suppression of large-small scales
ionospheric irregularities has occurred during the main and second
night of the recovery phases. However, during the first night of
recovery phase there was post-midnight ionospheric
irregularities.",
doi = "10.1016/j.jastp.2018.05.001",
url = "http://dx.doi.org/10.1016/j.jastp.2018.05.001",
issn = "1364-6826",
label = "lattes: 8030262077949409 6 BarbosaFaKaFePiNaMu:2018:PaDaSt",
language = "en",
targetfile = "barbosa_multi.pdf",
urlaccessdate = "27 abr. 2024"
}