@Article{TakahashiEFWBAOSL:2021:MuStLo,
author = "Takahashi, Hisao and Essien, Patrick and Figueiredo, Cosme
Alexandre Oliveira Barros and Wrasse, Cristiano Max and Barros,
Diego and Abdu, Mangalathayil Ali and Otsuka, Y. and Shiokawa, K.
and Li, Gouzhu",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Nagoya University} and {Nagoya University} and {Chinese Academy
of Sciences}",
title = "Multi-instrument study of longitudinal wave structures for plasma
bubble seeding in the equatorial ionosphere",
journal = "Earth and Planetary Physics",
year = "2021",
volume = "5",
number = "5",
pages = "368--377",
month = "Sept.",
keywords = "Multi-instrument study of longitudinal wave structures for plasma
bubble seeding in the equatorial ionosphere.",
abstract = "Large Scale Wave Structures (LSWS) in the equatorial ionospheric
F-region were observed by measuring spatial and temporal
variations within detrended total electron content (dTEC) data
obtained by ground-based GNSS receivers over the South American
continent. By using dTEC-maps, we have been able to produce, for
the first-time, two-dimensional representations of LSWS. During
the period from September to December, the LSWS frequently
occurred starting a few hours prior to Equatorial Plasma Bubble
(EPB) development. From 17 events of LSWS observed in 2014 and
2015, wave characteristics were obtained: the observed
wavelengths, periods, and the phase speeds are respectively,
similar to 900 km, similar to 41 min and similar to 399 m/s; the
waves propagated from the northeast to southeast. In some cases
the front of the oscillation was meridionally aligned, extending
to more than 1600 km, the first time such large extension of the
wavefront has been reported. From F-layer bottom height
oscillation data, measured by ionosonde, LSWS exhibit two
different vertical phase propagation modes, in-phase and downward
phase. The former mode indicates the presence of a polarization
electric field in the F-layer bottom side; the latter suggests
propagation of atmospheric gravity waves. The presence of LSWS
near the solar terminator, followed by the development of EPBs,
suggests that the upwelling of the F-layer bottom height produces
a condition favorable to the development of Rayleigh-Taylor
instability.",
doi = "10.26464/epp2021047",
url = "http://dx.doi.org/10.26464/epp2021047",
issn = "2096-3955",
language = "en",
targetfile = "takashi_multi.pdf",
urlaccessdate = "16 jun. 2024"
}