Turbulence in the middle atmosphere: A review

dc.contributor.authorWoodman Pollitt, Ronald Francisco
dc.date.accessioned2016-11-08T00:06:19Z
dc.date.accessioned2017-12-21T19:41:47Z
dc.date.available2016-11-08T00:06:19Z
dc.date.available2017-12-21T19:41:47Z
dc.date.issued1980
dc.description.abstractThe stratosphere is characterized for being highly statically stable. lt takes considerable energy to interchange parcels of air from different altitudes; thus, turbulence is normally inhibited, Wind shears of the order of 40 m/sec per kilometer are necessary to overcome the stabilizing effect of negative buoyancy if turbulence is to occur. Shears close to these values do exist in narrow but horizontally exten­sive layers as a consequence of internal gravity waves and the two­dimensional (horizontal) turbulent character of mesoscale stratospheric winds. Shorter wavelength waves, superimposed on these shears, make the local shear exceed the threshold (Richardson number < 0.25) for Kelvin­Helmholtz instabilities to occur and in turn, to break into turbulence. In addition, the shear of these waves may be enhanced by a nonlinear unstable amplification of those gravity waves whose phase velocity matches the local wind velocity. As a consequence, turbulence in the stratosphere occurs intermittently, in extensive layers from ten to a few hundred kilometers in extent, and only a few ten to a few hundred meters in thickness.es_ES
dc.formatapplication/pdfes_ES
dc.identifier.citationWoodman, R. F. (1980). Turbulence in the middle atmosphere: A review.es_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/579
dc.language.isoenges_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttps://creativecommons.org/licences/by/4.0/es_ES
dc.subjectStratospherees_ES
dc.subjectTurbulencees_ES
dc.subjectStratospheric windses_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.05.01es_ES
dc.titleTurbulence in the middle atmosphere: A reviewes_ES
dc.typeinfo:eu-repo/semantics/workingPaperes_ES

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