@Article{PaulinoLABBPTW:2017:LuTiTo,
author = "Paulino, A. R. and Lima, L. M. and Almeida, S. L. and Batista,
Paulo Prado and Batista, Inez Staciarini and Paulino, I. and
Takahashi, Hisao and Wrasse, Cristiano Max",
affiliation = "{Universidade Estadual da Para{\'{\i}}ba (UEPB)} and
{Universidade Estadual da Para{\'{\i}}ba (UEPB)} and
{Universidade Estadual da Para{\'{\i}}ba (UEPB)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Universidade Federal de Campina
Grande (UFCG)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Lunar tides in total electron content over Brazil",
journal = "Journal of Geophysical Research: Space Physics",
year = "2017",
volume = "122",
number = "7",
pages = "7519--7529",
month = "July",
keywords = "lunar tides, ionosphere, TEC.",
abstract = "Using data from Global Navigation Satellite Systems dual frequency
receivers, the lunar tides were studied in the ionospheric total
electron content (TEC) over Brazil from 2011 to 2014. In order to
calculate the amplitudes and phases of the lunar tides, quiet
magnetic days within a 27 day (window) have been used to remove
the solar rotation effects. Relative residuals TEC were calculated
by performing a spectral analysis by removing the solar tide
contributions. Lastly, a lunar month size window was used to
calculate the amplitude and phase of the lunar components. Lunar
diurnal tide amplitudes showed a semiannual variation with maximum
in the equinox months for almost all latitudes, while lunar
semidiurnal amplitudes were larger in December and January and may
be related to sudden stratospheric warming events. Both components
did not display significant longitudinal variation what could be
due to the short range of longitude (30 degrees). Lunar diurnal
amplitudes were basically uniform over Brazil, while lunar
semidiurnal amplitudes showed some peaks over the equatorial
ionization anomaly crest and minimum values near the magnetic
equator.",
doi = "10.1002/2017JA024052",
url = "http://dx.doi.org/10.1002/2017JA024052",
issn = "2169-9402",
language = "en",
targetfile = "paulino_lunar.pdf",
urlaccessdate = "27 abr. 2024"
}