Skip to main content Accessibility help
×
Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-03T00:37:01.784Z Has data issue: false hasContentIssue false

4 - Inviscid Boundary Conditions

Published online by Cambridge University Press:  21 September 2009

Georges-Henri Cottet
Affiliation:
Université Joseph Fourier, Grenoble
Petros D. Koumoutsakos
Affiliation:
ETH-Zurich and CTR, NASA
Get access

Summary

Vortex methods were initially conceived as a tool to simulate the inviscid dynamics of vortical flows. The vorticity carried by the fluid elements is conserved in inviscid flows and simulating the flow amounts to the computation of the velocity field. In bounded domains the velocity field is constrained by the conditions imposed by the type and the motions of the boundaries. For an inviscid flow, it is not possible to enforce boundary conditions for all three velocity components as we have lost the highest-order viscous term from the set of governing Navier–Stokes equations. Usually for inviscid flows past solid bodies we impose conditions on the velocity component locally normal to the boundary.

The description of an inviscid flow can be facilitated when the velocity field is decomposed into two components that have a kinematic significance. In this decomposition, a rotational component accounts for the velocity field due to the vorticity in the flow whereas a potential component is used in order to enforce the boundary conditions and to ensure the compatibility of the velocity and the vorticity field in the presence of boundaries. This is the well-known Helmholtz decomposition.

Alternatively the evolution of the inviscid flow can be described in terms of an extended vorticity field. The enforcement of a boundary condition for the velocity components normal to the boundary does not constrain the wall-parallel velocity components. This allows for velocity discontinuities across the interface that may be viewed as velocity gradients over an infinitesimal region across the boundary.

Type
Chapter
Information
Vortex Methods
Theory and Practice
, pp. 90 - 120
Publisher: Cambridge University Press
Print publication year: 2000

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 [email protected] 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
×