Large-scale fractal structure in laboratory turbulence, astrophysics, and the ocean

It is demonstrated that large-scale fractal structure in laboratory turbulence, the ocean, and the clustering of galaxies may have a common percolation nature. The fractal dimensionality of all these structures is shown to be approximately 4/3 (much smaller than 3, the dimensionality of spatial motion). The author compares laboratory measurements and natural observations of various scientists.

PACS: 47.53.+n, 92.10.Lq, 47.27.−i, 95.30.Lz, 05.45.Df (all)
DOI: 10.1070/PU1990v033n12ABEH002669
URL: https://ufn.ru/en/articles/1990/12/f/
Citation: Bershadskii A G "Large-scale fractal structure in laboratory turbulence, astrophysics, and the ocean" Sov. Phys. Usp. 33 (12) 1073–1075 (1990)

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%0 Journal Article
%T Large-scale fractal structure in laboratory turbulence, astrophysics, and the ocean
%A A. G. Bershadskii
%I Physics-Uspekhi
%D 1990
%J Phys. Usp.
%V 33
%N 12
%P 1073-1075
%U https://ufn.ru/en/articles/1990/12/f/
%U https://doi.org/10.1070/PU1990v033n12ABEH002669

Оригинал: Бершадский А Г «Крупномасштабные фрактальные структуры в лабораторной турбулентности, океане и астрофизике» УФН 160 (12) 189–194 (1990); DOI: 10.3367/UFNr.0160.199012i.0189