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Radial basis functions for simulating PDEsOverviewFinite differences remain useful because they are simple, direct, Main limitation is restriction to (logically) rectangular grids. Radial basis functions offer the possibility of a difference-based 1. Background Interpolation (1D)In one dimension, data can be interpolated smoothly using splines.
Doesn't matter if nodes are scattered rather than equispaced.
Interpolation (2D)On a regular 2-D grid, data can be interpolated smoothly by splines.
On scattered nodes, smooth splines are diffcult.
Radial basis functionsA radial basis function interpolant can be smooth and accurate on
DefinitionGiven nodes xi and data fi, i = 1, . . . ,N, define
Use 2-norm for
In matrix terms,
Basis functions
Piecewise smooth
Infinitely smooth
Basic properties
•For many smooth choices of
Cubic splinesConsider 1-D,
can be used for analysis. For instance, Gibbs' phenomenon.
Overshoot is 10.78% (compared to 14.11% in trig interpolation). Cubic RBFs from cubic splinesA cubic spline is determined by interpolation plus two boundary Suppose x ∈[−1, 1]. To recreate a cubic RBF interpolant, use
Conclude. Boundaries are coupled together in RBF interpolation. Cubic splines from cubic RBFsNatural spline. s''(−1) = s''(1) = 0.
RBF interpolant with linear asymptotic growth. Not-a-knot spline. s''' continuous at x^2 and xN−1.
Improves convergence at ends. In nitely smooth RBFsMost important in practice is
Use
Introduce scaling parameter
Decreasing tends to flatten the basis functions.
Fourier analysisDiscretize
Spectral di erentiation is
Comparison on Fourier data
The flat-RBF societyAs
Limit resultTheorem (Driscoll and Fornberg). Expand a smooth
Define symmetric matrices by
If
SpinIn the flat limit, RBFs give something familiar and useful. In 2-D,
Work is underway on stable means of computing in the limit, RBF difference methodsUse RBF interpolant to compute spatial derivatives for a PDE at Already successful for elliptic and diffusive evolution equations. Issues condition of RBF matrix Strategies preconditioners, multigrid Nondissipative propagationFor example, Maxwell's equations with interfaces.
New challenge. Time stability at boundaries BoundariesFrom 1-D theory.
SuggestionsWithout dissipation, instability is deadly. 1. Change the basisReproduce polynomials exactly, or limit asymptotic growth.
V is Vandermonde m = −1 gives standard RBF. Effect of polynomial terms
Benefits for small m, but diminishing returns as degree increases. 2. Change the methodNot-a-knot. Separate two RBF centers from interpolation nodes.
Independent of the changed center locations. Improves cubic "Super" not-a-knot. Do it again.
Independent of altered locations. Improves accuracy to h4 even Not-a-knot example
May be special only for 1-D cubics. 3. Change the nodesFor 1-D polynomials, Chebyshev density
is optimal for stability.
for
Effects of node density
Most improvement for intermediate
Comparison in 2-DNode/center distributions on the unit disk.
Observations1. Adding polynomials to the basis 2. Not-a-Knot/SNaK 3. Boundary clustering These approaches may be combined freely. Promise and problemsRadial basis functions offer the promise of difference
methods that Significant problems remain to be fully resolved.
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