NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
MHD Instability and Turbulence in the TachoclineThe focus of this project was to study the physical processes that govern tachocline dynamics and structure. Specific features explored included stratification, shear, waves, and toroidal and poloidal background fields. In order to address recent theoretical work on anisotropic mixing and dynamics in the tachocline, we were particularly interested in such anisotropic mixing for the specific tachocline processes studied. Transition to turbulence often shapes the largest-scale features that appear spontaneously in a flow during the development of turbulence. The resulting large-scale straining field can control the subsequent dynamics; therefore, anticipation of the large-scale straining field that results for individual realizations of the transition to turbulence can be important for subsequent dynamics, flow morphology, and transport characteristics. As a result, we paid particular attention to the development of turbulence in the stratified and sheared environment of the tachocline. This is complicated by the fact that the linearly stability of sheared MHD flows is non-self-adjoint, implying that normal asymptotic linear stability theory may not be relevant.
Document ID
20030020759
Acquisition Source
Headquarters
Document Type
Contractor or Grantee Report
Authors
Werne, Joe
(NorthWest Research Associates, Inc. Bellevue, WA, United States)
Wagner, William J.
(NASA Headquarters Washington, DC United States)
Date Acquired
August 21, 2013
Publication Date
March 25, 2003
Subject Category
Fluid Mechanics And Thermodynamics
Report/Patent Number
NWRA-CoRA-03-P258
NASA-9026-Final
Funding Number(s)
CONTRACT_GRANT: NASW-99026
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Document Inquiry

Available Downloads

There are no available downloads for this record.
No Preview Available