Dynamics of turbulent jets in the atmosphere and ocean
By: by Joseph Jinmoon Bernstein
Published: 2009
Language: eng
Number of pages: 116
Subjects: Fluid dynamics
Description: Quasi-zonal jets exist in both the mid-latitude atmosphere and ocean. These jets support a high eddy variance constituting a state of geostrophic turbulence. In addition to the turbulence, there is low frequency variability (LFV) which is not periodic. In the ocean it manifests as the zonal growth and collapse of the jet with a decadal timescale. In the atmosphere large meridional velocities occur producing blocking patterns which frequently persist for weeks. This work advances the idea that the mechanism for the origin of the LFV in both the atmosphere and ocean is eddy/mean flow interactions. In order to analyze these interactions the method of Stochastic Structural Stability Theory (SSST) is used. In the implementation of SSST used in this work the flow equations are split into separate sets governing the fast and slow timescale and a stochastic turbulence model is used to parameterize the nonlinear eddy-eddy interactions in the fast variable equation set.

The slow equation is then forced by turbulent fluxes coupling the two together. SSST results in a set of nonlinear deterministic equations describing the interaction between the eddies and mean flow. In the oceanic literature there are two opposing theories concerning the origin of LFV. One claims that turbulent eddy/mean flow interactions cause LFV while the other claims a homoclinic bifurcation of the laminar flow is the origin. Our calculations show that the LFV is produced by a homoclinic bifurcation arising from eddy mean flow interactions providing a framework in which both theories have a role. In the mid-latitude atmosphere the spatial structure of LFV is explained by SSST, but temporally irregular behavior is not found for realistic parameter ranges. However, if assumptions used in the derivation of SSST are relaxed then stochastic fluctuations arise. It is shown that these fluctuations are capable of reproducing the temporal variability of blocking seen in the atmosphere.
Notes: "May 2009."

Thesis (Ph.D., Dept. of Earth and Planetary Sciences)--Harvard University, 2009.

Includes bibliographical references.