@Article{NyassorWPGYTBNBPSF:2022:InCoGr,
author = "Nyassor, Prosper Kwamla and Wrasse, Cristiano Max and Paulino, Igo
and Gobbi, Delano and Yigit, E. and Takahashi, Hisao and Batista,
Paulo Prado and Naccarato, Kleber Pinheiro and Buriti, R. A. and
Paulino, A. R. and Silva, Diego Barros and Figueiredo, Cosme
Alexandre Oliveira Barros",
affiliation = "{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 {George Mason University} 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)} and {Universidade Estadual da Para{\'{\i}}ba (UEPB)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Investigations on Concentric Gravity Wave Sources Over the
Brazilian Equatorial Region",
journal = "Journal of Geophysical Research: Atmospheres",
year = "2022",
volume = "127",
number = "17",
pages = "e2021JD035149",
month = "Sept.",
keywords = "concentric gravity waves, convective source, ray tracing.",
abstract = "Observations of concentric gravity waves (CGWs) in the OH airglow
emission over the Brazilian equatorial region are presented. An
all-sky imager installed at Sao Joao do Cariri [7.4 degrees S,
36.5 degrees W] was used to acquire near-infrared OH images. Using
over 19 years of observational data from 2000 to 2019, more than
1,052 clear sky nights of airglow data were acquired with a total
of 25 observed CGW cases. Three CGW events were selected for this
study. These waves had small-scale characteristics and
well-defined concentric structures. The selected CGW events showed
horizontal wavelengths lambda(H) similar to 31.9, 42.5, and 30.9
km, horizontal phase speeds c(H) similar to 49.2, 57.6, and 74.1
m/s, and periods tau similar to 10.8, 12.3, and 7.0 min,
respectively. The CGW structures were well defined, with coherent
wave patterns expanding concentrically from the source point, with
the observed events having semi-circle or arc-like and
semi-elliptical shapes. We found the occurrence of the CGWs to
coincide with the seasons of intense tropospheric convective
activity and low background winds. This suggests little or no wave
breaking, critical level absorption, and filtering or reflection,
thereby allowing the CGWs to propagate up to the mesosphere and
lower thermosphere region. Using backward ray tracing, we also
found the positions and times where and when the ray paths reached
the tropopause. The tropopause positions and times of two of the
CGW events coincide with active convective systems with cold cloud
top temperatures. However, the tropopause position of one of the 3
CGW events did not coincide with any active convective system,
suggesting that this CGW was most likely generated in-situ.",
doi = "10.1029/2021JD035149",
url = "http://dx.doi.org/10.1029/2021JD035149",
issn = "2169-8996 and 2169-897X",
language = "en",
targetfile = "JGR Atmospheres - 2022 - Nyassor - Investigations on Concentric
Gravity Wave Sources Over the Brazilian Equatorial Region.pdf",
urlaccessdate = "15 jun. 2024"
}