@Article{TakahashiWFPABLBCSSGMR:2007:SiUlFa,
author = "Takahashi, Hisao and Wrasse, Cristiano Max and Fechine, J. and
Pancheva, D. and Abdu, Mangalathayil Ali and Batista, Inez
Staciarini and Lima, L. M. and Batista, Paulo Prado and Clemesha,
Barclay Robert and Schuch, Nelson Jorge and Shiokawa, K. and
Gobbi, Delano and Mlynczak, M. G. and Russell, J. M.",
affiliation = "National Institute of Space Research (INPE), Brazil and National
Institute of Space Research (INPE), Brazil and National Institute
of Space Research (INPE), Brazil and Department of Electronic \&
Electrical Engineering, University of Bath, Bath, UK and National
Institute of Space Research (INPE), Brazil and National Institute
of Space Research (INPE), Brazil and Department of Physics,
University of State of Para{\'{\i}}ba, Campina Grande, PB,
Brazil and National Institute of Space Research (INPE), Brazil and
National Institute of Space Research (INPE), Brazil and National
Institute of Space Research (INPE), Brazil and Solar Terrestrial
Environmental Laboratory, Nagoya University, Toyokawa, Japan and
National Institute of Space Research (INPE), Brazil and
Atmospheric Sciences Division, NASA Langley Research Center,
Hampton, Virginia, USA and Center for Atmospheric Sciences,
Hampton University, Hampton, Virginia, USA",
title = "Signatures of ultra fast Kelvin waves in the equatorial middle
atmosphere and ionosphere",
journal = "Geophysical Research Letters",
year = "2007",
volume = "34",
number = "11",
pages = "L11108",
month = "June",
keywords = "equatorial ionosphere, mesosphere-ionosphere coupling, atmospheric
Kelvin waves.",
abstract = "In the equatorial atmosphere, oscillations with periods of 3 to 4
days have been observed in the meteor radar zonal wind at Cariri
(7.4°S, 36.5°W), in the ionospheric minimum virtual height h'F and
the maximum critical frequency foF2 at Fortaleza (3.9°S, 38.4°W),
and in the TIMED/SABER satellite temperature data in the
stratosphere-mesosphere. Wavelet analyses of these time series
reveal that the 34-day oscillation was observed for all of these
data during the period from March 1 to 11, 2005. From the
characteristics of the downward phase propagation (wavelength of
\∼40 km), longitudinal and latitudinal extension, we
conclude that this oscillation must be a 3.5day Ultra Fast Kelvin
(UFK) wave. This is the first report of clear evidence of
propagation of a UFK wave from the stratosphere to the ionosphere.
The UFK wave could have an important role in the day-to-day
variability of the equatorial ionosphere evening uplift.",
doi = "10.1029/2007GL029612",
url = "http://dx.doi.org/10.1029/2007GL029612",
issn = "0094-8276",
language = "en",
targetfile = "grl23031.pdf",
url = "http://www.agu.org/pubs/crossref/2007/2007GL029612.shtml",
urlaccessdate = "30 abr. 2024"
}