The association of polar mesosphere summer echo layers with tial modes

The occurrence of PMSEs with time of day shows a semi-diurnal variation with minima at 8 and 20 h LT. PMSE layers observed for more than 30 min show an average rate of descent of 2 km h –1 . These characteristics suggest the influence of tidal winds. When the observed steady wind and diurnal and sem...

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Published in:Annales Geophysicae
Main Authors: Williams, P. J. S., Jones, G. O. L., Palmer, J. R., Rishbeth, H.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.1007/s00585-995-0454-8
https://angeo.copernicus.org/articles/13/454/1995/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo33671 2023-05-15T16:04:39+02:00 The association of polar mesosphere summer echo layers with tial modes Williams, P. J. S. Jones, G. O. L. Palmer, J. R. Rishbeth, H. 2018-09-27 application/pdf https://doi.org/10.1007/s00585-995-0454-8 https://angeo.copernicus.org/articles/13/454/1995/ eng eng doi:10.1007/s00585-995-0454-8 https://angeo.copernicus.org/articles/13/454/1995/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.1007/s00585-995-0454-8 2020-07-20T16:28:15Z The occurrence of PMSEs with time of day shows a semi-diurnal variation with minima at 8 and 20 h LT. PMSE layers observed for more than 30 min show an average rate of descent of 2 km h –1 . These characteristics suggest the influence of tidal winds. When the observed steady wind and diurnal and semi-diurnal tides at EISCAT are added, the overall magnitude shows a time-variation which matches the occurrence of PMSEs, and the observed rate of descent, approximately 2 km h –1 . Atmospheric gravity waves also contribute to the velocity of the neutral wind. When the wave reinforces the background wind, the PMSEs are stronger and descend more rapidly, but when the wave-related velocity opposes the background wind the PMSE is weaker and it descends more slowly. Text EISCAT Copernicus Publications: E-Journals Annales Geophysicae 13 4 454 457
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description The occurrence of PMSEs with time of day shows a semi-diurnal variation with minima at 8 and 20 h LT. PMSE layers observed for more than 30 min show an average rate of descent of 2 km h –1 . These characteristics suggest the influence of tidal winds. When the observed steady wind and diurnal and semi-diurnal tides at EISCAT are added, the overall magnitude shows a time-variation which matches the occurrence of PMSEs, and the observed rate of descent, approximately 2 km h –1 . Atmospheric gravity waves also contribute to the velocity of the neutral wind. When the wave reinforces the background wind, the PMSEs are stronger and descend more rapidly, but when the wave-related velocity opposes the background wind the PMSE is weaker and it descends more slowly.
format Text
author Williams, P. J. S.
Jones, G. O. L.
Palmer, J. R.
Rishbeth, H.
spellingShingle Williams, P. J. S.
Jones, G. O. L.
Palmer, J. R.
Rishbeth, H.
The association of polar mesosphere summer echo layers with tial modes
author_facet Williams, P. J. S.
Jones, G. O. L.
Palmer, J. R.
Rishbeth, H.
author_sort Williams, P. J. S.
title The association of polar mesosphere summer echo layers with tial modes
title_short The association of polar mesosphere summer echo layers with tial modes
title_full The association of polar mesosphere summer echo layers with tial modes
title_fullStr The association of polar mesosphere summer echo layers with tial modes
title_full_unstemmed The association of polar mesosphere summer echo layers with tial modes
title_sort association of polar mesosphere summer echo layers with tial modes
publishDate 2018
url https://doi.org/10.1007/s00585-995-0454-8
https://angeo.copernicus.org/articles/13/454/1995/
genre EISCAT
genre_facet EISCAT
op_source eISSN: 1432-0576
op_relation doi:10.1007/s00585-995-0454-8
https://angeo.copernicus.org/articles/13/454/1995/
op_doi https://doi.org/10.1007/s00585-995-0454-8
container_title Annales Geophysicae
container_volume 13
container_issue 4
container_start_page 454
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