Case study of a mesospheric wall event over Ferraz station, Antarctica (62° S)

On 16–17 July 2007 during an observational campaign at Comandante Ferraz Antarctic Station (62° S, 58° W), a mesospheric wall was observed with an airglow all-sky imager. The wave appeared like an extensive dark region in the all-sky airglow images, with a large depletion in the OH emission. Simulta...

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Published in:Annales Geophysicae
Main Authors: Bageston, J. V., Wrasse, C. M., Hibbins, R. E., Batista, P. P., Gobbi, D., Takahashi, H., Andrioli, V. F., Fechine, J., Denardini, C. M.
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Language:English
Published: 2018
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Online Access:https://doi.org/10.5194/angeo-29-209-2011
https://angeo.copernicus.org/articles/29/209/2011/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo8209 2023-05-15T13:36:36+02:00 Case study of a mesospheric wall event over Ferraz station, Antarctica (62° S) Bageston, J. V. Wrasse, C. M. Hibbins, R. E. Batista, P. P. Gobbi, D. Takahashi, H. Andrioli, V. F. Fechine, J. Denardini, C. M. 2018-09-27 application/pdf https://doi.org/10.5194/angeo-29-209-2011 https://angeo.copernicus.org/articles/29/209/2011/ eng eng doi:10.5194/angeo-29-209-2011 https://angeo.copernicus.org/articles/29/209/2011/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-29-209-2011 2020-07-20T16:26:14Z On 16–17 July 2007 during an observational campaign at Comandante Ferraz Antarctic Station (62° S, 58° W), a mesospheric wall was observed with an airglow all-sky imager. The wave appeared like an extensive dark region in the all-sky airglow images, with a large depletion in the OH emission. Simultaneous mesospheric winds measured with a MF radar at Rothera station and temperature profiles from SABER instrument, on board of TIMED satellite, were used to obtain the propagation condition of the wave. Wind measurements during four days, around the time of observation of the wave, are presented in order to discuss the type and consistence of the duct in which this wave was propagating. By using wavelet analysis and tidal amplitude components we found that 12 and 8 h components were the most important periodicities around the time interval of the wave observation. A collocated imaging spectrometer, for mesospheric temperature measurements, has been operated simultaneously with the all-sky imager. Direct effects of the mesospheric front have been seen in the spectrometric measurements, showing an abrupt decrease in both OH intensity and rotational temperature when the wave front passes overhead. The main contribution of the present work is the investigation of the type of duct in which the wall event was propagating. We found evidences for a thermal duct structure to support the mesospheric wall propagation. This result was obtained by two types of analysis: (a) the tidal components analysis and winds filtering (harmonic analysis), and (b) comparison between the terms of the m 2 dispersion relation. Text Antarc* Antarctic Antarctica Copernicus Publications: E-Journals Antarctic Ferraz ENVELOPE(-64.117,-64.117,-65.117,-65.117) Rothera ENVELOPE(-68.130,-68.130,-67.568,-67.568) Rothera Station ENVELOPE(-68.120,-68.120,-67.569,-67.569) Annales Geophysicae 29 1 209 219
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description On 16–17 July 2007 during an observational campaign at Comandante Ferraz Antarctic Station (62° S, 58° W), a mesospheric wall was observed with an airglow all-sky imager. The wave appeared like an extensive dark region in the all-sky airglow images, with a large depletion in the OH emission. Simultaneous mesospheric winds measured with a MF radar at Rothera station and temperature profiles from SABER instrument, on board of TIMED satellite, were used to obtain the propagation condition of the wave. Wind measurements during four days, around the time of observation of the wave, are presented in order to discuss the type and consistence of the duct in which this wave was propagating. By using wavelet analysis and tidal amplitude components we found that 12 and 8 h components were the most important periodicities around the time interval of the wave observation. A collocated imaging spectrometer, for mesospheric temperature measurements, has been operated simultaneously with the all-sky imager. Direct effects of the mesospheric front have been seen in the spectrometric measurements, showing an abrupt decrease in both OH intensity and rotational temperature when the wave front passes overhead. The main contribution of the present work is the investigation of the type of duct in which the wall event was propagating. We found evidences for a thermal duct structure to support the mesospheric wall propagation. This result was obtained by two types of analysis: (a) the tidal components analysis and winds filtering (harmonic analysis), and (b) comparison between the terms of the m 2 dispersion relation.
format Text
author Bageston, J. V.
Wrasse, C. M.
Hibbins, R. E.
Batista, P. P.
Gobbi, D.
Takahashi, H.
Andrioli, V. F.
Fechine, J.
Denardini, C. M.
spellingShingle Bageston, J. V.
Wrasse, C. M.
Hibbins, R. E.
Batista, P. P.
Gobbi, D.
Takahashi, H.
Andrioli, V. F.
Fechine, J.
Denardini, C. M.
Case study of a mesospheric wall event over Ferraz station, Antarctica (62° S)
author_facet Bageston, J. V.
Wrasse, C. M.
Hibbins, R. E.
Batista, P. P.
Gobbi, D.
Takahashi, H.
Andrioli, V. F.
Fechine, J.
Denardini, C. M.
author_sort Bageston, J. V.
title Case study of a mesospheric wall event over Ferraz station, Antarctica (62° S)
title_short Case study of a mesospheric wall event over Ferraz station, Antarctica (62° S)
title_full Case study of a mesospheric wall event over Ferraz station, Antarctica (62° S)
title_fullStr Case study of a mesospheric wall event over Ferraz station, Antarctica (62° S)
title_full_unstemmed Case study of a mesospheric wall event over Ferraz station, Antarctica (62° S)
title_sort case study of a mesospheric wall event over ferraz station, antarctica (62° s)
publishDate 2018
url https://doi.org/10.5194/angeo-29-209-2011
https://angeo.copernicus.org/articles/29/209/2011/
long_lat ENVELOPE(-64.117,-64.117,-65.117,-65.117)
ENVELOPE(-68.130,-68.130,-67.568,-67.568)
ENVELOPE(-68.120,-68.120,-67.569,-67.569)
geographic Antarctic
Ferraz
Rothera
Rothera Station
geographic_facet Antarctic
Ferraz
Rothera
Rothera Station
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_source eISSN: 1432-0576
op_relation doi:10.5194/angeo-29-209-2011
https://angeo.copernicus.org/articles/29/209/2011/
op_doi https://doi.org/10.5194/angeo-29-209-2011
container_title Annales Geophysicae
container_volume 29
container_issue 1
container_start_page 209
op_container_end_page 219
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