@Article{ResendeBaDeCaAnMoBa:2016:CoWiEl,
author = "Resende, Laysa Cristina Ara{\'u}jo and Batista, Inez Staciarini
and Denardini, Clezio Marcos and Carrasco, Alexander Jos{\'e} and
Andrioli, V{\^a}nia de F{\'a}tima and Moro, Juliano and Batista,
Paulo Prado",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)}",
title = "Competition between winds and electric fields in the formation of
blanketing sporadic E layers at equatorial regions",
journal = "Earth, Planets and Space",
year = "2016",
volume = "68",
number = "201",
pages = "1--14",
note = "{Setores de Atividade: Pesquisa e desenvolvimento
cient{\'{\i}}fico.}",
keywords = "Equatorial Aeronomy, Sporadic E Layer, Electric Field, Neutral
Winds, Ionospheric Model.",
abstract = "In the present work, we analyze the competition between tidal
winds and electric fields in the formation of blanketing sporadic
E layers (Esb) over S{\~a}o Lu{\'{\i}}s, Brazil (2° 31\′
S, 44° 16\′ W), a quasi-equatorial station. To investigate
this competition, we have used an ionospheric E region model
(MIRE) that is able to model the Esb layers taking into account
the E region winds and electric fields. The model calculates the
densities for the main molecular and metallic ions by solving the
continuity and momentum equations for each of the species. Thus,
the main purpose of this analysis is to verify the electric fields
role in the occurrence or disruption of Esb layers through
simulations. The first results of the simulations show that the
Esb layer is usually present when only the tidal winds were
considered. In addition, when the zonal component of the electric
field is introduced in the simulation, the Esb layers do not show
significant changes. However, the simulations show the disruption
of the Esb layers when the vertical electric field is included. In
this study, we present two specific cases in which Esb layers
appear during some hours over S{\~a}o Lu{\'{\i}}s. We can see
that these layers appear when the vertical electric field was
weak, which means that the tidal components were more effective
during these hours. Therefore, the vertical component of the
electric field is the main agent responsible for the Esb layer
disruption.",
doi = "10.1186/s40623-016-0577-z",
url = "http://dx.doi.org/10.1186/s40623-016-0577-z",
issn = "1343-8832",
label = "lattes: 8030262077949409 3 ResendeBaNaCaAnMoCh:2016:CoWiEl",
language = "en",
targetfile = "resende_competition.pdf",
url = "http://earth-planets-space.springeropen.com/articles/10.1186/s40623-016-0577-z",
urlaccessdate = "20 maio 2024"
}