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Theoretical and experimental studies of baroclinic processesAn experimental study in a baroclinic annulus with heating and cooling on the upper and lower horizontal surfaces was completed. Four basic regimes of flow were observed: (1) axisymmetric flow, (2) cellular (deep) convection, (3) convective rolls (boundary layer), and (4) baroclinic instability. There was no symmetric (or nearly symmetric) baroclinic instability observed, although it was determined by numerical calculations that we transversed regions in parameter space where the symmetric instability was present. The non-symmetric baroclinic instability (Eady type) was observed instead. Although the vertical depth was rather small and hence viscous damping was strong, large-amplitude baroclinic waves were made possible by imposing a very weak static stability.
Document ID
19870003611
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Miller, T.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Leslie, F.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Fitzjarrald, D.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Reynolds, N.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 13, 2013
Publication Date
October 1, 1985
Publication Information
Publication: NASA(MSFC FY-85 Atmospheric Processes Research Review
Subject Category
Meteorology And Climatology
Accession Number
87N13044
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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