University of Minnesota
Aerospace Engineering and Mechanics
Spring 2002 Seminar Series



The Statistical and Structural Character of Acceleration in Wall Turbulence


Prof. Ken Christensen

Dept. of Mechanical Engineering, The University of New Mexico


Abstract

Robust large eddy simulation (LES) of turbulence requires accurate modeling of the small-scale features of the flow, including their interactions with the larger scales. Formulations based upon optimal estimation of the evolution of the filtered field minimize the mean-square error associated with estimating the short-term dynamics of the resolved scales. Optimal formulations show great promise (Langford and Moser, 1999), since this evolution term embodies the stochastic nature of the small scales. However, in order for optimal formulations to be extended to higher Reynolds numbers, the statistical and structural nature of the acceleration must be documented.

To this end, time-resolved particle-image velocimetry measurements are made in the streamwise-wall-normal plane of turbulent channel flow at Re?=550 and 1734. Temporal and convective derivatives of velocity are computed from this data in order to evaluate the small-scale behavior of these quantities as well as of the velocity itself. Instantaneous velocity fields indicate that the flow is dominated by small-scale vortex cores believed to be associated with hairpin/hairpin-like vortices. These vortices have been observed in realizations of the random velocity in other wall turbulence studies. In the present work, a deterministic "vortex signature" is determined by conditional averaging techniques. This average signature is consistent with the hairpin vortex signature defined by Adrian and co-workers. In addition, the spatial extent of these small-scale vortices appears to remain relatively constant within the Reynolds-number range studied herein.

Instantaneous time-derivative fields are spatially intermittent and are dominated by strong events that are spatially coincident with the small-scale vortex cores seen in the associated velocity fields. Stochastic estimation of the temporal derivative signature associated with the presence of a vortex core, coupled with Taylor's hypothesis considerations, shows that the small-scale vortices remain relatively frozen in time, implying that advective effects dominate the smaller spatial scales of the temporal derivative of velocity. The bulk convective derivative of velocity (i.e., the temporal derivative computed in a reference frame traveling at the bulk velocity) is found to be nearly an order of magnitude smaller than the temporal derivative of velocity and is mostly associated with the growth of the vortices away from the wall. Based upon the trends noted in the instantaneous data, scaling of the temporal and convective derivative statistics is considered to uncover a consistent Reynolds-number scaling of the statistics involved in optimal LES subgrid-scale models.

Friday, March 8, 2002
209 Akerman Hall
2:30-3:30 p.m.


Refreshments served after the seminar in 227 Akerman Hall.
Disability accomodations provided upon request.
Contact Kristal Belisle, Senior Secretary, 625-8000.