UMD AOSC-CSCAMM Seminar
Turbulent Fluid Dynamics at the Margins of Rotational and Stratified Control:
Submesoscale Fluid Dynamics in the Ocean
Dr. James C. McWilliams
Louis B. Slichter Professor of Earth Sciences
University of California, Los Angeles
Institute of Geophysics and Planetary Physics and
Department of Atmospheric and Oceanic Sciences
Geophysical fluid dynamicists have developed a mature perspective on
the dynamical influence of Earth's rotation, while most other areas of
fluid dynamics can safely disregard rotation. Similarly, geophysical
problems usually arise under the influence of stable density
stratification at least as importantly as velocity shear. In this talk
the dominant turbulence and wave behaviors in the rotating and
non-rotating, stratified and non-stratified fluid-dynamical realms are
described, and particular attention is given to their borderlands,
where rotational and stratified influences are significant but not
dominant. Contrary to the inverse energy cascade of geostrophic
turbulence toward larger scales, a forward energy cascade develops
within the borderlands from the breakdown of diagnostic force
balances, frontogenesis and frontal instabilities, and
filamentogenesis with strong surface convergences. Then the cascade
continues further through the small-scale, non-rotating, unstratified
(a.k.a. universal) realm until it dissipates at the microscale. In
particular, this submesoscale cascade behavior is of interest as a
global route to kinetic and available-potential energy dissipations in
the oceanic general circulation, as well as an energy source for
microscale material mixing across stably-stratified density surfaces
and a penetration route for potential vorticity across stably
stratified density surfaces.
April 16, 2009, Thurday
Seminar: 3:30-4:30pm
***Special Reception: 3:00pm (Everyone Welcome)***
Computer and Space Sciences (CSS) Building, Auditorium (Room 2400)
[Contact: Kayo Ide]
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