Mesosphere and lower thermosphere temperature anomalies during the 2002 Antarctic stratospheric warming event

We present kinetic temperatures at ~87 km and ~94 km altitudes inferred from OH (6,2) and O 2 At(0,1) airglow observations, respectively, at South Pole (90° S), Antarctica in the austral winter of 2002. These OH and O 2 rotational temperatures measurements show mesosphere and lower thermosphere (MLT...

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Published in:Annales Geophysicae
Main Authors: Azeem, S. M. I., Talaat, E. R., Sivjee, G. G., Yee, J.-H.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/angeo-28-267-2010
https://angeo.copernicus.org/articles/28/267/2010/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo2295 2023-05-15T13:36:36+02:00 Mesosphere and lower thermosphere temperature anomalies during the 2002 Antarctic stratospheric warming event Azeem, S. M. I. Talaat, E. R. Sivjee, G. G. Yee, J.-H. 2018-09-27 application/pdf https://doi.org/10.5194/angeo-28-267-2010 https://angeo.copernicus.org/articles/28/267/2010/ eng eng doi:10.5194/angeo-28-267-2010 https://angeo.copernicus.org/articles/28/267/2010/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-28-267-2010 2020-07-20T16:26:29Z We present kinetic temperatures at ~87 km and ~94 km altitudes inferred from OH (6,2) and O 2 At(0,1) airglow observations, respectively, at South Pole (90° S), Antarctica in the austral winter of 2002. These OH and O 2 rotational temperatures measurements show mesosphere and lower thermosphere (MLT) temperature anomalies prior to the 2002 Southern Hemisphere Sudden Stratospheric Warming (SSW) . In this paper we focus on the first of the three minor stratospheric warmings which preceded the major SSW event. Temperature anomalies observed in the MLT region show sudden cooling (Δ T =~30 K) in OH temperatures accompanied by warming (Δ T =~15 K) in O 2 temperatures preceding the onset of SSW event by about three to four weeks. This shallow vertical extent of mesospheric cooling is in agreement with the numerical simulation of Coy et al. (2005), however, the model cooling was centered well below the mesopause level. The other observed feature of the South Pole MLT temperature dataset is the intensification of planetary wave activity prior to the onset of SSW event. Fourier analyses of both OH and O 2 temperatures show amplification of planetary wave activity in the 5–10 day range prior to the onset of SSW. The timing of wave amplification seen in the wave spectra coincides with the peak in OH and O 2 temperature anomalies. Text Antarc* Antarctic Antarctica South pole South pole Copernicus Publications: E-Journals Antarctic Austral South Pole Annales Geophysicae 28 1 267 276
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description We present kinetic temperatures at ~87 km and ~94 km altitudes inferred from OH (6,2) and O 2 At(0,1) airglow observations, respectively, at South Pole (90° S), Antarctica in the austral winter of 2002. These OH and O 2 rotational temperatures measurements show mesosphere and lower thermosphere (MLT) temperature anomalies prior to the 2002 Southern Hemisphere Sudden Stratospheric Warming (SSW) . In this paper we focus on the first of the three minor stratospheric warmings which preceded the major SSW event. Temperature anomalies observed in the MLT region show sudden cooling (Δ T =~30 K) in OH temperatures accompanied by warming (Δ T =~15 K) in O 2 temperatures preceding the onset of SSW event by about three to four weeks. This shallow vertical extent of mesospheric cooling is in agreement with the numerical simulation of Coy et al. (2005), however, the model cooling was centered well below the mesopause level. The other observed feature of the South Pole MLT temperature dataset is the intensification of planetary wave activity prior to the onset of SSW event. Fourier analyses of both OH and O 2 temperatures show amplification of planetary wave activity in the 5–10 day range prior to the onset of SSW. The timing of wave amplification seen in the wave spectra coincides with the peak in OH and O 2 temperature anomalies.
format Text
author Azeem, S. M. I.
Talaat, E. R.
Sivjee, G. G.
Yee, J.-H.
spellingShingle Azeem, S. M. I.
Talaat, E. R.
Sivjee, G. G.
Yee, J.-H.
Mesosphere and lower thermosphere temperature anomalies during the 2002 Antarctic stratospheric warming event
author_facet Azeem, S. M. I.
Talaat, E. R.
Sivjee, G. G.
Yee, J.-H.
author_sort Azeem, S. M. I.
title Mesosphere and lower thermosphere temperature anomalies during the 2002 Antarctic stratospheric warming event
title_short Mesosphere and lower thermosphere temperature anomalies during the 2002 Antarctic stratospheric warming event
title_full Mesosphere and lower thermosphere temperature anomalies during the 2002 Antarctic stratospheric warming event
title_fullStr Mesosphere and lower thermosphere temperature anomalies during the 2002 Antarctic stratospheric warming event
title_full_unstemmed Mesosphere and lower thermosphere temperature anomalies during the 2002 Antarctic stratospheric warming event
title_sort mesosphere and lower thermosphere temperature anomalies during the 2002 antarctic stratospheric warming event
publishDate 2018
url https://doi.org/10.5194/angeo-28-267-2010
https://angeo.copernicus.org/articles/28/267/2010/
geographic Antarctic
Austral
South Pole
geographic_facet Antarctic
Austral
South Pole
genre Antarc*
Antarctic
Antarctica
South pole
South pole
genre_facet Antarc*
Antarctic
Antarctica
South pole
South pole
op_source eISSN: 1432-0576
op_relation doi:10.5194/angeo-28-267-2010
https://angeo.copernicus.org/articles/28/267/2010/
op_doi https://doi.org/10.5194/angeo-28-267-2010
container_title Annales Geophysicae
container_volume 28
container_issue 1
container_start_page 267
op_container_end_page 276
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