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 ([...
Published in: | Journal of Atmospheric and Solar-Terrestrial Physics |
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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 |
_version_ |
1776204898171355136 |