Show simple item record

dc.creatorHu, Yongyun
dc.date.accessioned2012-06-07T22:44:59Z
dc.date.available2012-06-07T22:44:59Z
dc.date.created1996
dc.date.issued1996
dc.identifier.urihttps://hdl.handle.net/1969.1/ETD-TAMU-1996-THESIS-H834
dc.descriptionDue to the character of the original source materials and the nature of batch digitization, quality control issues may be present in this document. Please report any quality issues you encounter to digital@library.tamu.edu, referencing the URI of the item.en
dc.descriptionIncludes bibliographical references: p. 94-101.en
dc.descriptionIssued also on microfiche from Lange Micrographics.en
dc.description.abstractThe high-resolution SKYHI general circulation model is used to simulate tropical mixing behavior and to investigate mixing barriers in the tropical lower stratosphere. Results show that during the solstitial seasons a tropical weak-mixing zone is present in the SKYHI simulations. The weak-mixing zone is relatively isolated from the surf zones in the middle latitudes by two mixing barriers, one weak and one strong. Lagrangian trajectory calculations show that the tropical mixing barriers are quasi-penetrable, and the weak mixing zone allows more tropical air to mix into the winter hemisphere than into the summer hemisphere. The tropical mixing barriers have seasonal variations in location and strength. The variations are closely coincident with the annual cycle of the tropical easterly zonal flow and subtropical wave spectra. Wave spectrum analysis indicates that during the solstitial seasons there exists a zone in the tropics, which exactly matches the weak mixing zone, where there is relatively absence of westward-moving waves. Calculations of meridional diffusion coefficients with filtered and anti-filtered winds suggest that mixing in the tropical easterlies occurs near the critical layers for the large-scale westward-moving waves, where the waves would be expected to break. The presence of the tropical mixing barriers is a result of the absence of such waves. Experiments with wave phase-speed filters indicate that stationary and quasi-stationary waves have significant effects on tropical mixing. The Rossby-gravity waves are less important for tropical mixing, and the Kelvin waves make no contribution to tropical mixing. Analysis indicates that equatorward propagation of the extratropical waves has important influences on tropical mixing. An experiment with a modified zonal flow shows a tropical mixing configuration of the westerly QBO phase. Finally, the SKYHI simulation results are compared with the observations and other simulations.en
dc.format.mediumelectronicen
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherTexas A&M University
dc.rightsThis thesis was part of a retrospective digitization project authorized by the Texas A&M University Libraries in 2008. Copyright remains vested with the author(s). It is the user's responsibility to secure permission from the copyright holder(s) for re-use of the work beyond the provision of Fair Use.en
dc.subjectmeteorology.en
dc.subjectMajor meteorology.en
dc.titleGCM simulation of the tropical mixing barriers in the lower stratosphereen
dc.typeThesisen
thesis.degree.disciplinemeteorologyen
thesis.degree.nameM.S.en
thesis.degree.levelMastersen
dc.type.genrethesisen
dc.type.materialtexten
dc.format.digitalOriginreformatted digitalen


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record

This item and its contents are restricted. If this is your thesis or dissertation, you can make it open-access. This will allow all visitors to view the contents of the thesis.

Request Open Access