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Perturbations of the Richardson number field by gravity wavesAn analytic solution is presented for a stratified fluid of arbitrary constant Richardson number. By computer aided analysis the perturbation fields, including that of the Richardson number can be calculated. The results of the linear analytic model were compared with nonlinear simulations, leading to the following conclusions: (1) the perturbations in the Richardson number field, when small, are produced primarily by the perturbations of the shear; (2) perturbations of in the Richardson number field, even when small, are not symmetric, the increase being significantly larger than the decrease (the linear analytic solution and the nonlinear simulations both confirm this result); (3) as the perturbations grow, this asymmetry increases, but more so in the nonlinear simulations than in the linear analysis; (4) for large perturbations of the shear flow, the static stability, as represented by N2, is the dominating mechanism, becoming zero or negative, and producing convective overturning; and (5) the convectional measure of linearity in lee wave theory, NH/U, is no longer the critical parameter (it is suggested that (H/u sub 0) (du sub 0/dz) takes on this role in a shearing flow).
Document ID
19860020801
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Wurtele, M. G.
(California Univ. Los Angeles, CA, United States)
Sharman, R. D.
(California Univ. Los Angeles, CA, United States)
Date Acquired
September 5, 2013
Publication Date
July 1, 1985
Subject Category
Geophysics
Report/Patent Number
NASA-CR-176910
NAS 1.26:176910
Report Number: NASA-CR-176910
Report Number: NAS 1.26:176910
Accession Number
86N30273
Funding Number(s)
CONTRACT_GRANT: NSG-4024
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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