Fast meridional transport in the lower thermosphere by planetary-scale waves

Observations showed that the main engine water exhaust plumes from space shuttles released at not, vert, similar110 km altitude from Florida could be transported over thousands of kilometers northward or southward, reaching the Arctic after a day or so, and in one case Antarctica after three days ([...

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Published in:Journal of Atmospheric and Solar-Terrestrial Physics
Other Authors: Yue, Jia (author), Liu, Han-Li (author)
Format: Article in Journal/Newspaper
Language:English
Published: Elsevier Ltd. 2010
Subjects:
Online Access:http://nldr.library.ucar.edu/repository/collections/OSGC-000-000-000-261
https://doi.org/10.1016/j.jastp.2010.10.001
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spelling ftncar:oai:drupal-site.org:articles_17094 2023-09-05T13:13:43+02:00 Fast meridional transport in the lower thermosphere by planetary-scale waves Yue, Jia (author) Liu, Han-Li (author) 2010-12-01 http://nldr.library.ucar.edu/repository/collections/OSGC-000-000-000-261 https://doi.org/10.1016/j.jastp.2010.10.001 en eng Elsevier Ltd. Journal of Atmospheric and Solar-Terrestrial Physics http://nldr.library.ucar.edu/repository/collections/OSGC-000-000-000-261 doi:10.1016/j.jastp.2010.10.001 ark:/85065/d7sf2xfh Copyright 2010 Elsevier. This is the author's version of a work accepted for publication by Elsevier. Changes resulting from the publishing process, including peer review, editing, corrections, structural formatting and other quality control mechanisms, may not be reflected in this document. Changes may have been made to this work since it was submitted for publication. Text article 2010 ftncar https://doi.org/10.1016/j.jastp.2010.10.001 2023-08-14T18:42:28Z Observations showed that the main engine water exhaust plumes from space shuttles released at not, vert, similar110 km altitude from Florida could be transported over thousands of kilometers northward or southward, reaching the Arctic after a day or so, and in one case Antarctica after three days ([Stevens et al., 2003] and [Stevens et al., 2005]). In this work, we study the meridional transport associated with the quasi-two-day wave (QTDW) and migrating tides. Diagnostic calculations are performed to trace the particle trajectories using winds from the Thermosphere-Ionosphere-Mesosphere-Electrodynamics General Circulation Model (TIME-GCM) simulations for January, when the amplitude of the QTDW usually peaks. The calculations demonstrate that the mean meridional circulation, a QTDW or a migrating tide cannot individually sustain planetary-scale meridional transport for one to three days, but the combined effects of a QTDW and a tide can. In particular, when the QTDW and the tides are scaled according to the observed amplitudes, particles released at not, vert, similar110 km and appropriate longitudes/local times can undergo transport fast enough to reach Antarctica within three days as observed. The magnitude and direction of the transport depend on the amplitudes and phases of the tides and the QTDW. These simulations thus suggest that the observed rapid planetary-scale meridional transport of the shuttle main engine plume can be driven by planetary waves and tides. Article in Journal/Newspaper Antarc* Antarctica Arctic OpenSky (NCAR/UCAR - National Center for Atmospheric Research/University Corporation for Atmospheric Research) Arctic Journal of Atmospheric and Solar-Terrestrial Physics 72 18 1372 1378
institution Open Polar
collection OpenSky (NCAR/UCAR - National Center for Atmospheric Research/University Corporation for Atmospheric Research)
op_collection_id ftncar
language English
description Observations showed that the main engine water exhaust plumes from space shuttles released at not, vert, similar110 km altitude from Florida could be transported over thousands of kilometers northward or southward, reaching the Arctic after a day or so, and in one case Antarctica after three days ([Stevens et al., 2003] and [Stevens et al., 2005]). In this work, we study the meridional transport associated with the quasi-two-day wave (QTDW) and migrating tides. Diagnostic calculations are performed to trace the particle trajectories using winds from the Thermosphere-Ionosphere-Mesosphere-Electrodynamics General Circulation Model (TIME-GCM) simulations for January, when the amplitude of the QTDW usually peaks. The calculations demonstrate that the mean meridional circulation, a QTDW or a migrating tide cannot individually sustain planetary-scale meridional transport for one to three days, but the combined effects of a QTDW and a tide can. In particular, when the QTDW and the tides are scaled according to the observed amplitudes, particles released at not, vert, similar110 km and appropriate longitudes/local times can undergo transport fast enough to reach Antarctica within three days as observed. The magnitude and direction of the transport depend on the amplitudes and phases of the tides and the QTDW. These simulations thus suggest that the observed rapid planetary-scale meridional transport of the shuttle main engine plume can be driven by planetary waves and tides.
author2 Yue, Jia (author)
Liu, Han-Li (author)
format Article in Journal/Newspaper
title Fast meridional transport in the lower thermosphere by planetary-scale waves
spellingShingle Fast meridional transport in the lower thermosphere by planetary-scale waves
title_short Fast meridional transport in the lower thermosphere by planetary-scale waves
title_full Fast meridional transport in the lower thermosphere by planetary-scale waves
title_fullStr Fast meridional transport in the lower thermosphere by planetary-scale waves
title_full_unstemmed Fast meridional transport in the lower thermosphere by planetary-scale waves
title_sort fast meridional transport in the lower thermosphere by planetary-scale waves
publisher Elsevier Ltd.
publishDate 2010
url http://nldr.library.ucar.edu/repository/collections/OSGC-000-000-000-261
https://doi.org/10.1016/j.jastp.2010.10.001
geographic Arctic
geographic_facet Arctic
genre Antarc*
Antarctica
Arctic
genre_facet Antarc*
Antarctica
Arctic
op_relation Journal of Atmospheric and Solar-Terrestrial Physics
http://nldr.library.ucar.edu/repository/collections/OSGC-000-000-000-261
doi:10.1016/j.jastp.2010.10.001
ark:/85065/d7sf2xfh
op_rights Copyright 2010 Elsevier. This is the author's version of a work accepted for publication by Elsevier. Changes resulting from the publishing process, including peer review, editing, corrections, structural formatting and other quality control mechanisms, may not be reflected in this document. Changes may have been made to this work since it was submitted for publication.
op_doi https://doi.org/10.1016/j.jastp.2010.10.001
container_title Journal of Atmospheric and Solar-Terrestrial Physics
container_volume 72
container_issue 18
container_start_page 1372
op_container_end_page 1378
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