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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PT Journal Article
TI Large-scale fractal structure in laboratory turbulence, astrophysics, and the ocean
AU Bershadskii A G
FAU Bershadskii AG
DP 10 Dec, 1990
TA Phys. Usp.
VI 33
IP 12
PG 1073-1075
RX 10.1070/PU1990v033n12ABEH002669
URL https://ufn.ru/en/articles/1990/12/f/
SO Phys. Usp. 1990 Dec 10;33(12):1073-1075

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