Skip to content

Revisiting Wall Heating

Authors

Rider, William J.
RefereedArticle

Abstract

The results of computing a shock reflection are found to strongly depend on the chosen coordinate system, Lagrangian or Eulerian. This is seen by comparing the amount of “wall heating” associated with the solutions to Noh's shock reflection problem computed in each reference frame. Here, an explanation is offered that places a greater burden on the role of phase error or effective wave speed in producing this effect. The reason for the greater difficulties in the Lagrangian frame are the non- uniformity of the mass coordinates in a converging geometry. This produces a non-steady-state discrete shock profile.

Details

© The SAO Astrophysics Data System

help[at]scixplorer.org

SciX is a project created by the Astrophysics Data System (ADS), which is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement 80NSSC21M0056.

Version: v0.26.0

*The material contained in this document is based upon work supported by a National Aeronautics and Space Administration (NASA) grant or cooperative agreement. Any opinions, findings, conclusions or recommendations expressed in this material are those of the author and do not necessarily reflect the views of NASA.

RESOURCES

About SciXGive FeedbackSciX HelpSystem StatusCareers@SciXAccessibility Conformance ReportWeb Accessibility PolicyNASA Science Discovery Engine