@Article{EgitoBatTakBatBur:2020:VaEqIo,
author = "Egito, F{\'a}bio and Batista, Inez Staciarini and Takahashi,
Hisao and Batista, Paulo Prado and Buriti, R. A.",
affiliation = "{Universidade Federal do Rec{\^o}ncavo da Bahia (UFRB)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Universidade Federal de Campina
Grande (UFCG)}",
title = "Variability of the equatorial ionosphere induced by nonlinear
interaction between an ultrafast Kelvin wave and the diurnal
tide",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
year = "2020",
volume = "208",
pages = "e105397",
month = "Oct.",
keywords = "Ultrafast Kelvin wave and tides, Nonlinear interaction, Secondary
waves, Ionosphere.",
abstract = "The wave forcing from below allows the neutral atmosphere to drive
short-term variability in the ionosphere. Recent modeling studies
have shown that secondary waves originated from the nonlinear
interaction of the atmospheric tides with planetary scale waves
can contribute significantly to day-to-day variability of the
ionosphere. In this study we used MLT neutral wind measured at S~
ao Jo~ ao do Cariri (7.4\�S, 36.5\�W) and
ionospheric soundings performed by a digisonde installed at
Fortaleza (3.9\�S, 38.4\�W) to investigate the
presence and the induced variability by a secondary wave in the
mesosphere-ionosphere system over the Brazilian equatorial region.
We found evidences of the nonlinear interaction between a 3.5-day
ultrafast Kelvin wave and the diurnal tide. The interaction
produced a 1.3-day secondary wave that was found to propagate
upward with maximum amplitude of 15 m/s and relatively long
vertical wavelength (~44 km) in the MLT, which may allow it to
penetrate into the ionosphere. In the ionosphere, we observed a
common 1.3-day periodic variation in the virtual height (hF) and
critical frequency (foF2), which may be connected to the secondary
wave observed in the MLT via modulation of the wind system in the
E region dynamo. These findings suggest that secondary waves may
impose additional variability to ionosphere.",
doi = "10.1016/j.jastp.2020.105397",
url = "http://dx.doi.org/10.1016/j.jastp.2020.105397",
issn = "1364-6826",
language = "en",
targetfile = "egito_variability.pdf",
urlaccessdate = "18 abr. 2024"
}