@Article{PautetTaChTaMeSãFr:2009:SiObEq,
author = "Pautet, P. -D. and Taylor, M. J. and Chapagain, N. P. and
Takahashi, H. and Medeiros, A. F. and S{\~a}o Sabbas, F. T. and
Fritts, D. C.",
affiliation = "{Utah State University} and {Utah State University} and {Utah
State University} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Universidade Federal de Campina Grande} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {NW Res
Associates Inc}",
title = "Simultaneous observations of equatorial F-region plasma depletions
over Brazil during the Spread-F Experiment (SpreadFEx)",
journal = "Annales Geophysicae",
year = "2009",
volume = "27",
number = "6",
pages = "2371--2381",
keywords = "Atmospheric composition and structure, Airglow and aurora,
Ionosphere, Equatorial ionosphere, Ionospheric irregularities,
mesospheric gravity-waves, all-sky images, airglow observations,
zonal drift, ionosphere, bubbles, campaign, irregularities, winds,
scintillations.",
abstract = "From September to November 2005, the NASA Living with a Star
program supported the Spread-F Experiment campaign (SpreadFEx) in
Brazil to study the effects of convectively generated gravity
waves on the ionosphere and their role in seeding Rayleigh-Taylor
instabilities, and associated equatorial plasma bubbles. Several
US and Brazilian institutes deployed a broad range of instruments
(all-sky imagers, digisondes, photometers, meteor/VHF radars, GPS
receivers) covering a large area of Brazil. The campaign was
divided in two observational phases centered on the September and
October new moon periods. During these periods, an Utah State
University (USU) all-sky CCD imager operated at Sao Joao d'Alianca
(14.8 degrees S, 47.6 degrees W), near Brasilia, and a Brazilian
all-sky CCD imager located at Cariri (7.4 degrees S, 36 degrees
W), observed simultaneously the evolution of the ionospheric
bubbles in the OI (630 nm) emission and the mesospheric gravity
wave field. The two sites had approximately the same magnetic
latitude (9-10 degrees S) but were separated in longitude by
similar to 1500 km. Plasma bubbles were observed on every clear
night (17 from Brasilia and 19 from Cariri, with 8 coincident
nights). These joint datasets provided important information for
characterizing the ionospheric depletions during the campaign and
to perform a novel longitudinal investigation of their
variability. Measurements of the drift velocities at both sites
are in good agreement with previous studies, however, the
overlapping fields of view revealed significant differences in the
occurrence and structure of the plasma bubbles, providing new
evidence for localized generation. This paper summarizes the
observed bubble characteristics important for related
investigations of their seeding mechanisms associated with gravity
wave activity.",
issn = "0992-7689",
language = "en",
targetfile = "Simu{\c{c}}ataneous observation of equatorial.pdf",
urlaccessdate = "01 maio 2024"
}