@Article{EgitoAndrBati:2016:VeWiMo,
author = "Egito, F{\'a}bio and Andrioli, V{\^a}nia de F{\'a}tima and
Batista, Paulo Prado",
affiliation = "{Universidade Federal do Oeste da Bahia (UFOB)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Vertical winds and momentum fluxes due to equatorial planetary
scale waves using all-sky meteor radar over Brazilian region",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
year = "2016",
volume = "149",
pages = "108--119",
month = "Nov.",
keywords = "Meteor radar, Planetary scale waves, Vertical wind.",
abstract = "In the equatorial region planetary scale waves play an important
role transporting significant amount of energy and momentum
through atmosphere. Quantifying the momentum transported by these
waves and its effects on the mean flow is rather important. Direct
estimates of the momentum flux transported by waves require
horizontal and vertical wind measurements. Ground-based meteor
radars have provided continuous and reliable measurements of the
horizontal wind components in the Mesosphere and Lower
Thermosphere (MLT) region and have contributed to improve our
knowledge of the dynamics of this region. However, instrumental
limitations hinder its use for measuring vertical winds and
momentum fluxes. On the other hand, according to Babu et al
(2012), all- sky meteor radars are able to infer tridimensional
winds when using a large number of meteor echoes centered at the
meteor ablation peak. Following this approach, we have used
measurements performed by a Meteor Radar installed at S{\~a}o
Jo{\~a}o do Cariri, Brazil (7.4°S; 36.5°W) in order to measure
vertical winds and calculate the momentum flux transported by
equatorial planetary scale waves. In order to evaluate the
accuracy of vertical wind values we have performed several tests
based on a simple model considering real meteor distributions and
theoretical equations for the MLT winds motion. From our tests, we
inferred that Brazilian meteor radar data can be used for this
purpose with an accuracy of ~ 1.8 m/s. The results show that the
vertical wind presents magnitudes of a few meters per second and
occasionally reaches magnitudes around 10 m/s. Below 92 km the
vertical wind is predominantly upward during the whole year and
above exhibits a semi-annual oscillation with downward phase
during the equinoxes. Variations associated to planetary scale
waves in the vertical wind are also observed and some of them
appear simultaneously in the zonal and meridional wind as well.
Largest wave induced amplitudes in the vertical wind are found in
the 34 d band, reaching up to 4 m/s. From the vertical and zonal
wind measurements, we calculated the vertical transport of zonal
momentum in the 34 d band and found it to be maximum near autumn
equinox, when its value reaches almost 20 m2/s2, while minimum
momentum flux is observed after the winter solstice.",
doi = "10.1016/j.jastp.2016.10.005",
url = "http://dx.doi.org/10.1016/j.jastp.2016.10.005",
issn = "1364-6826",
language = "en",
targetfile = "egito_vertical.pdf",
urlaccessdate = "27 abr. 2024"
}