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Adapted from Benoit B Mandelbrot and R Pastor-Satorras, Antipodal Correlations and the Texture (Fractal Lacunarity) in Critical Ising Clusters; figure by Erik Rauch click for Postscript

Lacunarity

The properties and characteristics of a fractal set are not completely determined by its fractal dimension D. Indeed, it is easy to construct a family of fractals that share the same D but differ sharply. As an example of such a construction, the above depicts a stack of Cantor sets made up by a generator of intervals and a reduction factor . By construction, all have the same fractal dimension . Starting from the upper middle set, the index k varies from 1 to 6 when moving up and 1 to 5 when moving down. Below the middle, the segments are uniformly distributed; above, they are closely packed at the ends of the set. The extremes do not look ``like fractals'': the one in the bottom ( uniformly distributed segments) begins to resemble a filled interval, while the one on the top ( packed segments) looks like two isolated points at the ends of the set. Only the central Cantor set looks like a true fractal.

These sets have different ``texture'', more specifically, different lacunarity. Lacunarity is a notion distinct and independent from D; it is not related with the topology of the fractal and needs more than one numerical variable to be fully determined. Lacunarity is strongly related with the size distribution of the holes on the fractal and with its deviation from translational invariance; roughly speaking, a fractal is very lacunar if its holes tend to be large, in the sense that they include large regions of space.

See also

Mandelbrot B B 1982 The Fractal Geometry of Nature (New York: Freeman)

Mandelbrot B B 1993 Fractal in Medicine and Biology eds F Nonnenmacher (Basel: Birkhauser)
An expanded version more appropriate for physicist will appear in
Mandelbrot B B 1995 Fractal Geometry and Stochastics eds C Bandt, S Graf, and M Zäle (Basel and Boston: Birkhauser)


Erik Rauch
Mon Jan 22 20:24:28 MST 1996

http://starbase.jpl.nasa.gov/cdroms/igarss94/papers/p940101/p940167/p940167.htm