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3 - The finite difference time domain method in two and three dimensions

Published online by Cambridge University Press:  05 July 2014

David B. Davidson
Affiliation:
University of Stellenbosch, South Africa
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Summary

Introduction

In the previous chapter, the basic concepts of the finite difference time domain method were introduced via a one-dimensional example. We will briefly reprise the issues one must attend to when doing an FDTD simulation, as follows:

  • An FDTD mesh (or grid) must be created for the problem. (This is trivial in 1D, requires a little thought in 2D, and becomes quite a major problem in 3D.)

  • This mesh must be fine enough – i.e. Δs must be no more than perhaps one-tenth of the minimum wavelength (i.e. maximum frequency) of interest (Δs represents the spatial step size; quite often, Δx, Δy and Δz are chosen equal and Δs is used as shorthand for this).

  • The time step Δt must satisfy the Courant limit (but be as close to this as possible to minimize dispersion).

  • Boundary conditions (the source and load resistors in our 1D example) must be specified.

  • An appropriate signal shape (e.g. differentiated Gaussian) with suitable time duration for the desired spectral content must be chosen. Also, in general, its spatial position must be specified. (In the transmission line example, it was fixed as the source voltage generator.)

In this chapter, we will study the FDTD method in two and three dimensions. Firstly, we will develop a 2D simulator for a problem of scattering in free space. Following this, a very important development, the perfectly matched layer absorbing boundary condition, will be discussed and implemented.

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Publisher: Cambridge University Press
Print publication year: 2010

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