@Article{SahaiBFLOHEPABAPB:2007:ReNiEq,
author = "Sahai, Y. and Becker-Guedes, F. and Fagundes, P. R. and Lima, W.
L. C. and Otsuka, Y. and Huang, C. S. and Espinoza, E. S. and Pi,
X. and Abreu, A. J. and Bolzan, M. J. A. and Abalde, J. R. and
Pimenta, Alexandre Alvares and Bittencourt, Jos{\'e} Augusto",
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 {Centro
Universit{\'a}rio Luterano de Palmas} and STELAB and Haystack
Observatory, Massachusetts Institute of Technology and Radio
Observatorio de Jicamarca, Instituto Geofisico del Peru and {Jet
Propulsion Laboratory} and {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 {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)}",
title = "Response of nighttime equatorial and low latitude F-region to the
geomagnetic storm of August 18, 2003, in the Brazilian sector",
journal = "Advances in Space Research",
year = "2007",
volume = "39",
number = "8",
pages = "1325--1334",
keywords = "Equatorial and low latitude F-region, Geomagnetic storm,
Spread-F.",
abstract = "This paper presents an investigation of geomagnetic storm effects
in the equatorial and low latitude F-region in the Brazilian
sector during the intense geomagnetic storm on 18 August, 2003
(SSC 14:21 UT on 17/08; {\'O}Kp = 52+; Ap = 108; Dstmax = 168 at
1600 UT on 18/08). Simultaneous ionospheric sounding measurements
from two stations, viz., Palmas (10.2°S, 48.2°W; dip latitude
5.7°S) and Sao Jose dos Campos (23.2°S, 45.9°W; dip latitude
17.6°S), Brazil, are presented for the nights of 1617, 1718 and
1819 August, 2003 (quiet, disturbed and recovery phases). Both
stations are equipped with the Canadian Advanced Digital Ionosonde
(CADI). Quiet and disturbed conditions of the F-region ionosphere
are compared using data collected from the two stations. The
relationship between magnetospheric disturbance and low-latitude
ionospheric dynamics, and generation of ionospheric irregularities
are discussed. On the disturbed nights (1718 and 1819 August), the
low latitude station S. J. Campos showed strong enhancements in
the F-region critical frequency (foF2), whereas the near
equatorial station Palmas showed strong uplifting of the F-layer
about 1 h earlier. Normally during the June solstice months
(MayAugust) in the Brazilian sector, large-scale ionospheric
irregularities in form of plasma bubbles are rarely observed. On
the night of 1718 August, ionsospheric sounding observations at
Palmas showed the presence of bottomside spread-F, whereas on the
night of 1819 August, the observations at Palmas and S. J. Campos
showed the presence of plasma bubbles when the storm recovery
phase had just started. The complementary GPS data available from
several stations in the Rede Brasileira de Monitoramento Continuo
de GPS (Brazilian Network for Continuous GPS Monitoring) are used
to obtain the vertical total electron content (VTEC) and the rate
of change of TEC per minute on UT days 18 and 19 August, 2003 and
presented. Also, several global ionospheric TEC maps from the
worldwide network of GPS receivers are presented, showing
widespread latitudinal and longitudinal TEC changes during the
different phases of the storm. All the observations (local
ionospheric sounding and GPS network measurements, and global GPS
measurements) presented in this investigation related to the
geomagnetic storm on 18 August indicate that the equatorial and
low latitude region in the Brazilian sector had much stronger
effect during the recovery phase compared with the main phase. A
comparison of the observed disturbance drifts with the
FejerScherliess storm-time model drifts indicate that the modeled
drifts are not consistent with the present observations.",
copyholder = "SID/SCD",
issn = "0273-1177",
language = "en",
targetfile = "response of nightime.pdf",
urlaccessdate = "09 maio 2024"
}