@Article{AbreuSaFaJeBiPi:2011:InIoRe,
author = "Abreu, A. J. and Sahai, Y. and Fagundes, P. R. and Jesus, R. and
Bittencourt, J. A. and Pillat, Valdir Gil",
affiliation = "{} and Departamento de F{\'{\i}}sica e Astronomia, Universidade
do Vale do Para{\'{\i}}ba (UNIVAP), Av. Shishima Hifumi, 2911,
S{\~a}o Jos{\'e} dos Campos, S{\~a}o Paulo, Brazil and
Departamento de F{\'{\i}}sica e Astronomia, Universidade do Vale
do Para{\'{\i}}ba (UNIVAP), Av. Shishima Hifumi, 2911, S{\~a}o
Jos{\'e} dos Campos, S{\~a}o Paulo, Brazil and Departamento de
F{\'{\i}}sica e Astronomia, Universidade do Vale do
Para{\'{\i}}ba (UNIVAP), Av. Shishima Hifumi, 2911, S{\~a}o
Jos{\'e} dos Campos, S{\~a}o Paulo, Brazil and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and Departamento de
F{\'{\i}}sica e Astronomia, Universidade do Vale do
Para{\'{\i}}ba (UNIVAP), Av. Shishima Hifumi, 2911, S{\~a}o
Jos{\'e} dos Campos, S{\~a}o Paulo, Brazil",
title = "An investigation of ionospheric F region response in the Brazilian
sector to the super geomagnetic storm of May 2005",
journal = "Advances in Space Research",
year = "2011",
volume = "48",
number = "7",
pages = "1211--1220",
month = "Oct",
keywords = "Geomagnetic storm, Ionosphere, Equatorial ionospheric
irregularities.",
abstract = "In this paper, we have investigated the responses of the
ionospheric F region at equatorial and low latitude regions in the
Brazilian sector during the super geomagnetic storm on 15-16 May
2005. The geomagnetic storm reached a minimum Dst of -263 nT at
0900 UT on 15 May. In this paper, we present vertical total
electron content (vTEC) and phase fluctuations (in TECU/min) from
Global Positioning System (GPS) observations obtained at Belem,
Brasilia, Presidente Prudente, and Porto Alegre, Brazil, during
the period 14-17 May 2005. Also, we present ionospheric parameters
h'F, hpF2, and foF2, using the Canadian Advanced Digital Ionosonde
(CADI) obtained at Palmas and Sao Jose dos Campos, Brazil, for the
same period. The super geomagnetic storm has fast decrease in the
Dst index soon after SSC at 0239 UT on 15 May. It is a good
possibility of prompt penetration of electric field of
magnetospheric origin resulting in uplifting of the F region. The
vTEC observations show a trough at BELE and a crest above UEPP,
soon after SSC, indicating strengthening of nighttime equatorial
anomaly. During the daytime on 15 and 16 May, in the recovery
phase, the variations in foF2 at SJC and the vTEC observations,
particularly at BRAZ, UEPP, and POAL, show large positive
ionospheric storm. There is ESF on the all nights at PAL, in the
post-midnight (UT) sector, and phase fluctuations only on the
night of 14-15 May at BRAZ, after the SSC. No phase fluctuations
are observed at the equatorial station BELE and low latitude
stations (BRAZ, UEPP, and POAL) at all other times. This indicates
that the plasma bubbles are generated and confined on this
magnetically disturbed night only up to the low magnetic latitude
and drifted possibly to west.",
doi = "10.1016/j.asr.2011.05.036",
url = "http://dx.doi.org/10.1016/j.asr.2011.05.036",
issn = "0273-1177",
label = "lattes: 1106857072073407 6 AbreuSaFaJeBiPi:2011:AnInOf",
language = "en",
targetfile = "Abreu-AdvSpaceRes-v48-n7-p1211-1220-science[1].pdf",
urlaccessdate = "01 maio 2024"
}