Observations of equatorial mesospheric winds over Cariri (7.4° S) by a meteor radar and comparison with existing models

Mesospheric winds observed with a meteor radar at Cariri (7.4° S, 36.5° W), Brazil, during the period of July 2004 to June 2005, show a clear semiannual oscillation known as the Mesospheric Semiannual Oscillation (MSAO), which maximizes in the zonal mean wind mainly at 82 km, with...

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Main Authors: R. A. Buriti, W. K. Hocking, P. P. Batista, A. F. Medeiros, B. R. Clemesha
Format: Article
Language:English
Published: Copernicus Publications 2008-03-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/26/485/2008/angeo-26-485-2008.pdf
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spelling doaj-742de5187a6b450db2a24ba6753f46262020-11-24T23:23:55ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762008-03-012648549710.5194/angeo-26-485-2008Observations of equatorial mesospheric winds over Cariri (7.4° S) by a meteor radar and comparison with existing modelsR. A. Buriti0R. A. Buriti1W. K. Hocking2P. P. Batista3A. F. Medeiros4B. R. Clemesha5Departamento de Fisica, Universidade Federal de Campina Grande, Campina Grande, PB, 58109-970, Brazilnow at: Department of Physics and Astronomy, UWO, London, CanadaDepartment of Physics and Astronomy, University of Western Ontario, London, Ontario, CanadaInstituto Nacional de Pesquisas Espaciais (INPE), Sao Jose dos Campos, SP, BrazilDepartamento de Fisica, Universidade Federal de Campina Grande, Campina Grande, PB, 58109-970, BrazilInstituto Nacional de Pesquisas Espaciais (INPE), Sao Jose dos Campos, SP, BrazilMesospheric winds observed with a meteor radar at Cariri (7.4° S, 36.5° W), Brazil, during the period of July 2004 to June 2005, show a clear semiannual oscillation known as the Mesospheric Semiannual Oscillation (MSAO), which maximizes in the zonal mean wind mainly at 82 km, with amplitude decreasing with height. Maximum westward winds for the MSAO occurred in March and September. The meridional wind, on the other hand, presented a clear annual variation maximizing in December. On average, the amplitude of the meridional MSAO was smaller than the zonal MSAO component. Comparison with models shows on occasions that there are significant differences between the observed winds and the CIRA (Cospar International Reference Atmosphere) and HWM93 (Horizontal Wind Model) models. In addition, diurnal and semidiurnal parameters were calculated and compared to the GSWM model. Other results observed during one year of data are presented in this work.https://www.ann-geophys.net/26/485/2008/angeo-26-485-2008.pdf
collection DOAJ
language English
format Article
sources DOAJ
author R. A. Buriti
R. A. Buriti
W. K. Hocking
P. P. Batista
A. F. Medeiros
B. R. Clemesha
spellingShingle R. A. Buriti
R. A. Buriti
W. K. Hocking
P. P. Batista
A. F. Medeiros
B. R. Clemesha
Observations of equatorial mesospheric winds over Cariri (7.4° S) by a meteor radar and comparison with existing models
Annales Geophysicae
author_facet R. A. Buriti
R. A. Buriti
W. K. Hocking
P. P. Batista
A. F. Medeiros
B. R. Clemesha
author_sort R. A. Buriti
title Observations of equatorial mesospheric winds over Cariri (7.4° S) by a meteor radar and comparison with existing models
title_short Observations of equatorial mesospheric winds over Cariri (7.4° S) by a meteor radar and comparison with existing models
title_full Observations of equatorial mesospheric winds over Cariri (7.4° S) by a meteor radar and comparison with existing models
title_fullStr Observations of equatorial mesospheric winds over Cariri (7.4° S) by a meteor radar and comparison with existing models
title_full_unstemmed Observations of equatorial mesospheric winds over Cariri (7.4° S) by a meteor radar and comparison with existing models
title_sort observations of equatorial mesospheric winds over cariri (7.4° s) by a meteor radar and comparison with existing models
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2008-03-01
description Mesospheric winds observed with a meteor radar at Cariri (7.4° S, 36.5° W), Brazil, during the period of July 2004 to June 2005, show a clear semiannual oscillation known as the Mesospheric Semiannual Oscillation (MSAO), which maximizes in the zonal mean wind mainly at 82 km, with amplitude decreasing with height. Maximum westward winds for the MSAO occurred in March and September. The meridional wind, on the other hand, presented a clear annual variation maximizing in December. On average, the amplitude of the meridional MSAO was smaller than the zonal MSAO component. Comparison with models shows on occasions that there are significant differences between the observed winds and the CIRA (Cospar International Reference Atmosphere) and HWM93 (Horizontal Wind Model) models. In addition, diurnal and semidiurnal parameters were calculated and compared to the GSWM model. Other results observed during one year of data are presented in this work.
url https://www.ann-geophys.net/26/485/2008/angeo-26-485-2008.pdf
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