Abstract
The propagation of waves governed by hyperbolic systems at a surface is in general reflective. The numerical solution of many problems in mechanics necessitates the truncation of an open space to a finite domain. The reflectivity of the boundary of a truncated domain can be effectively characterized by a few parameters and implemented as a time-domain impedance boundary condition. It is shown that the concept of a time-domain impedance boundary condition affords a simple and effective treatment of waves, allowing them to exit the surfaces of a truncated domain as a causal, local, space-time continuation rather than a global boundary confinement. We present and discuss the open-space impedances of radiative and convective fields, their modeling, analytic structures, implementation, and solution effectiveness as an open-space impedance boundary condition. We further propose a general methodology for numerical definition of open-space impedance and its application within existing schemes to reduce truncated domains and computational resources.
| Original language | English |
|---|---|
| Pages (from-to) | 1432-1441 |
| Number of pages | 10 |
| Journal | AIAA Journal |
| Volume | 46 |
| Issue number | 6 |
| DOIs | |
| State | Published - Jun 2008 |
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