Atmospheric stability at 90 km, 78°N, 16°E

Abstract We employ observations obtained from a meteor wind radar to derive ambipolar diffusion coefficients, neutral temperatures, temperature gradients and, subsequently, Brunt-Väisälä frequencies at an altitude of 90 km over Svalbard (78°N, 16°E). The derived values showed a good agreement with i...

Full description

Bibliographic Details
Published in:Earth, Planets and Space
Main Authors: Hall, C. M., Aso, T., Tsutsumi, M.
Format: Article in Journal/Newspaper
Language:English
Published: Springer Science and Business Media LLC 2007
Subjects:
Online Access:http://dx.doi.org/10.1186/bf03352689
https://link.springer.com/content/pdf/10.1186/BF03352689.pdf
https://link.springer.com/article/10.1186/BF03352689/fulltext.html
http://link.springer.com/content/pdf/10.1186/BF03352689
id crspringernat:10.1186/bf03352689
record_format openpolar
spelling crspringernat:10.1186/bf03352689 2023-05-15T18:29:50+02:00 Atmospheric stability at 90 km, 78°N, 16°E Hall, C. M. Aso, T. Tsutsumi, M. 2007 http://dx.doi.org/10.1186/bf03352689 https://link.springer.com/content/pdf/10.1186/BF03352689.pdf https://link.springer.com/article/10.1186/BF03352689/fulltext.html http://link.springer.com/content/pdf/10.1186/BF03352689 en eng Springer Science and Business Media LLC https://creativecommons.org/licenses/by/4.0/ https://creativecommons.org/licenses/by/4.0/ CC-BY Earth, Planets and Space volume 59, issue 3, page 157-164 ISSN 1880-5981 Space and Planetary Science Geology journal-article 2007 crspringernat https://doi.org/10.1186/bf03352689 2022-01-04T11:39:37Z Abstract We employ observations obtained from a meteor wind radar to derive ambipolar diffusion coefficients, neutral temperatures, temperature gradients and, subsequently, Brunt-Väisälä frequencies at an altitude of 90 km over Svalbard (78°N, 16°E). The derived values showed a good agreement with independent measurements at each step of the analysis. Current atmospheric models are based on sparse data obtained at such high latitude, so these results represent a viable alternative for incorporating in subsequent studies of atmospheric dynamics, particularly if the derived monthly variabilities are included. The Brunt-Väisälä frequencies are then combined with wind shear measurements to estimate horizontally averaged gradient Richardson Numbers (Ri). We find Ri to be consistently larger in summer than winter due to wind shears being similarly larger in winter and augmented by the inverse seasonal variation in Brunt-Väisälä frequency. These seasonal variations result in Ri indicative of dynamic stability in summer and instability in winter. The variabilities in wind shear and Brunt-Väisälä frequency are then included to—albeit more qualitatively—illustrate the distribution between stability and static and dynamic instabilities as a function of season, using a novel portrayal pioneered by Zink and Vincent ( J. Geophys. Res. , 109 , doi:10.1029/2003JD003992, 2004). The resulting picture is discussed in the framework of current conceptions of distribution of turbulent energy dissipation with height and season and of current opinion of the mesopause structure at 78°N. Article in Journal/Newspaper Svalbard Springer Nature (via Crossref) Svalbard Earth, Planets and Space 59 3 157 164
institution Open Polar
collection Springer Nature (via Crossref)
op_collection_id crspringernat
language English
topic Space and Planetary Science
Geology
spellingShingle Space and Planetary Science
Geology
Hall, C. M.
Aso, T.
Tsutsumi, M.
Atmospheric stability at 90 km, 78°N, 16°E
topic_facet Space and Planetary Science
Geology
description Abstract We employ observations obtained from a meteor wind radar to derive ambipolar diffusion coefficients, neutral temperatures, temperature gradients and, subsequently, Brunt-Väisälä frequencies at an altitude of 90 km over Svalbard (78°N, 16°E). The derived values showed a good agreement with independent measurements at each step of the analysis. Current atmospheric models are based on sparse data obtained at such high latitude, so these results represent a viable alternative for incorporating in subsequent studies of atmospheric dynamics, particularly if the derived monthly variabilities are included. The Brunt-Väisälä frequencies are then combined with wind shear measurements to estimate horizontally averaged gradient Richardson Numbers (Ri). We find Ri to be consistently larger in summer than winter due to wind shears being similarly larger in winter and augmented by the inverse seasonal variation in Brunt-Väisälä frequency. These seasonal variations result in Ri indicative of dynamic stability in summer and instability in winter. The variabilities in wind shear and Brunt-Väisälä frequency are then included to—albeit more qualitatively—illustrate the distribution between stability and static and dynamic instabilities as a function of season, using a novel portrayal pioneered by Zink and Vincent ( J. Geophys. Res. , 109 , doi:10.1029/2003JD003992, 2004). The resulting picture is discussed in the framework of current conceptions of distribution of turbulent energy dissipation with height and season and of current opinion of the mesopause structure at 78°N.
format Article in Journal/Newspaper
author Hall, C. M.
Aso, T.
Tsutsumi, M.
author_facet Hall, C. M.
Aso, T.
Tsutsumi, M.
author_sort Hall, C. M.
title Atmospheric stability at 90 km, 78°N, 16°E
title_short Atmospheric stability at 90 km, 78°N, 16°E
title_full Atmospheric stability at 90 km, 78°N, 16°E
title_fullStr Atmospheric stability at 90 km, 78°N, 16°E
title_full_unstemmed Atmospheric stability at 90 km, 78°N, 16°E
title_sort atmospheric stability at 90 km, 78°n, 16°e
publisher Springer Science and Business Media LLC
publishDate 2007
url http://dx.doi.org/10.1186/bf03352689
https://link.springer.com/content/pdf/10.1186/BF03352689.pdf
https://link.springer.com/article/10.1186/BF03352689/fulltext.html
http://link.springer.com/content/pdf/10.1186/BF03352689
geographic Svalbard
geographic_facet Svalbard
genre Svalbard
genre_facet Svalbard
op_source Earth, Planets and Space
volume 59, issue 3, page 157-164
ISSN 1880-5981
op_rights https://creativecommons.org/licenses/by/4.0/
https://creativecommons.org/licenses/by/4.0/
op_rightsnorm CC-BY
op_doi https://doi.org/10.1186/bf03352689
container_title Earth, Planets and Space
container_volume 59
container_issue 3
container_start_page 157
op_container_end_page 164
_version_ 1766213247152685056