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Tight Frame


A tight frame in a Hilbert space is a collection {f_i}_(i in I) for which there is a constant A>0 such that

 sum_(i in I)|<x,f_i>|^2=A||x||^2

for every vector x in the space. Unlike an orthonormal basis, a tight frame may be redundant. Nevertheless, every vector has the reconstruction

 x=1/Asum_(i in I)<x,f_i>f_i.

A tight frame with A=1 is called a Parseval frame. Tight frames are used in signal processing because redundancy can provide robustness while retaining a simple reconstruction formula (Duffin and Schaeffer 1952, Christensen 2016).


See also

Hilbert Space, Orthonormal Basis, Seislet Transform

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References

Christensen, O. An Introduction to Frames and Riesz Bases, 2nd ed. Cham, Switzerland: Birkhäuser, 2016.Duffin, R. J. and Schaeffer, A. C. "A Class of Nonharmonic Fourier Series." Trans. Amer. Math. Soc. 72, 341-366, 1952.

Cite this as:

Weisstein, Eric W. "Tight Frame." From MathWorld--A Wolfram Resource. https://mathworld.wolfram.com/TightFrame.html

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