Skip to main content Accessibility help
×
Hostname: page-component-848d4c4894-xfwgj Total loading time: 0 Render date: 2024-06-15T18:14:15.926Z Has data issue: false hasContentIssue false

8 - Spectral Element and Lattice Gas Methods for Incompressible Fluid Dynamics

Published online by Cambridge University Press:  12 January 2010

Max D. Gunzburger
Affiliation:
Virginia Polytechnic Institute and State University
Roy A. Nicolaides
Affiliation:
Carnegie Mellon University, Pennsylvania
Get access

Summary

Introduction

The rapid development and introduction of new supercomputer systems over the last decade has opened new opportunities for numerical studies of incompressible fluid flows. A new awareness has also developed that the emerging hardware technologies influence both the nature and implementation of effective algorithms to solve these problems. Specific software implementation issues concern such varied questions as code dependencies, locality, round-off errors, storage access and capacity, input-output, workstation interfaces, cache utilization, . . . and are affected significantly by such computer hardware characteristics as the graininess of parallel systems, vector length, instruction conflicts, instruction set design, network access, distribution and paging of memory, to mention but a few. One significant result of this complex environment has been the stimulation of new ideas to make optimal use of the new supercomputer architectures and to achieve both high accuracy and high computational efficiency in the fluid simulations.

In this paper, we shall review some novel methods that are especially well suited for various aspects of incompressible fluid flow simulation studies. The key dynamical feature of these flows is the absence of shock waves, so many of the results to be stated for incompressible flows should also carry over to shock-free flows at moderate Mach numbers. Even within the context of incompressible flows, there is a wealth of dynamical phenomena to be studied, including laminar flows, transition to turbulence, turbulence, free surface flows, heat transfer, particle transport, fluid-structural interactions, and multiphase flows, among other phenomena.

Type
Chapter
Information
Incompressible Computational Fluid Dynamics
Trends and Advances
, pp. 203 - 266
Publisher: Cambridge University Press
Print publication year: 1993

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×