Case study of a mesospheric wall event over Ferraz station, Antarctica (62 degrees 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, JV, Wrasse, CM, Hibbins, Robert, Batista, PP, Gobbi, D, Takahashi, H, Fritts, DC, Andrioli, VF, Fechine, J, Denardini, CM
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2011
Subjects:
Online Access:http://hdl.handle.net/11250/2611488
https://doi.org/10.5194/angeo-29-209-2011
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spelling ftntnutrondheimi:oai:ntnuopen.ntnu.no:11250/2611488 2023-05-15T13:58:49+02:00 Case study of a mesospheric wall event over Ferraz station, Antarctica (62 degrees S) Bageston, JV Wrasse, CM Hibbins, Robert Batista, PP Gobbi, D Takahashi, H Fritts, DC Andrioli, VF Fechine, J Denardini, CM 2011 http://hdl.handle.net/11250/2611488 https://doi.org/10.5194/angeo-29-209-2011 eng eng Copernicus Publications Annales Geophysicae. 2011, 29 (1), 209-219. urn:issn:0992-7689 http://hdl.handle.net/11250/2611488 https://doi.org/10.5194/angeo-29-209-2011 cristin:827657 Navngivelse 4.0 Internasjonal http://creativecommons.org/licenses/by/4.0/deed.no CC-BY 209-219 29 Annales Geophysicae 1 Journal article Peer reviewed 2011 ftntnutrondheimi https://doi.org/10.5194/angeo-29-209-2011 2019-09-17T06:55:23Z 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 m2 dispersion relation. publishedVersion © Author(s) 2011. This work is distributed under the Creative Commons Attribution 3.0 License. Article in Journal/Newspaper Antarc* Antarctic Antarctica NTNU Open Archive (Norwegian University of Science and Technology) Antarctic Rothera ENVELOPE(-68.130,-68.130,-67.568,-67.568) Ferraz ENVELOPE(-64.117,-64.117,-65.117,-65.117) Rothera Station ENVELOPE(-68.120,-68.120,-67.569,-67.569) Annales Geophysicae 29 1 209 219
institution Open Polar
collection NTNU Open Archive (Norwegian University of Science and Technology)
op_collection_id ftntnutrondheimi
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 m2 dispersion relation. publishedVersion © Author(s) 2011. This work is distributed under the Creative Commons Attribution 3.0 License.
format Article in Journal/Newspaper
author Bageston, JV
Wrasse, CM
Hibbins, Robert
Batista, PP
Gobbi, D
Takahashi, H
Fritts, DC
Andrioli, VF
Fechine, J
Denardini, CM
spellingShingle Bageston, JV
Wrasse, CM
Hibbins, Robert
Batista, PP
Gobbi, D
Takahashi, H
Fritts, DC
Andrioli, VF
Fechine, J
Denardini, CM
Case study of a mesospheric wall event over Ferraz station, Antarctica (62 degrees S)
author_facet Bageston, JV
Wrasse, CM
Hibbins, Robert
Batista, PP
Gobbi, D
Takahashi, H
Fritts, DC
Andrioli, VF
Fechine, J
Denardini, CM
author_sort Bageston, JV
title Case study of a mesospheric wall event over Ferraz station, Antarctica (62 degrees S)
title_short Case study of a mesospheric wall event over Ferraz station, Antarctica (62 degrees S)
title_full Case study of a mesospheric wall event over Ferraz station, Antarctica (62 degrees S)
title_fullStr Case study of a mesospheric wall event over Ferraz station, Antarctica (62 degrees S)
title_full_unstemmed Case study of a mesospheric wall event over Ferraz station, Antarctica (62 degrees S)
title_sort case study of a mesospheric wall event over ferraz station, antarctica (62 degrees s)
publisher Copernicus Publications
publishDate 2011
url http://hdl.handle.net/11250/2611488
https://doi.org/10.5194/angeo-29-209-2011
long_lat ENVELOPE(-68.130,-68.130,-67.568,-67.568)
ENVELOPE(-64.117,-64.117,-65.117,-65.117)
ENVELOPE(-68.120,-68.120,-67.569,-67.569)
geographic Antarctic
Rothera
Ferraz
Rothera Station
geographic_facet Antarctic
Rothera
Ferraz
Rothera Station
genre Antarc*
Antarctic
Antarctica
genre_facet Antarc*
Antarctic
Antarctica
op_source 209-219
29
Annales Geophysicae
1
op_relation Annales Geophysicae. 2011, 29 (1), 209-219.
urn:issn:0992-7689
http://hdl.handle.net/11250/2611488
https://doi.org/10.5194/angeo-29-209-2011
cristin:827657
op_rights Navngivelse 4.0 Internasjonal
http://creativecommons.org/licenses/by/4.0/deed.no
op_rightsnorm CC-BY
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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