Fractal properties of the interplanetary magnetic field fluctuations: indications of chaotic dynamics

Details Fractal properties of the interplanetary magnetic field fluctuations: indications of chaotic dynamics Fractal properties of the interplanetary magnetic field fluctuations: indications of chaotic dynamics

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...283..990p&link_type=abstract

Astronomy and Astrophysics, Vol. 283, p. 990 (1994)

Astronomy and Astrophysics

Astrophysics

6

Magnetic Fields - Solar Wind - Interplabetary Medium

Scientific paper

The fractal nature of the magnetic field fluctuations is verified using HEOS 2 (at 1 AU), Pioneer 10 (at 4.8 AU), Pioneer 11 (at 20 AU) interplanetary and ICE (Giacobini-Zinner) cometary environment high resolution measurements. The fractal dimension of the time series profiles is estimated and the self-affinity property is tested. The results show significant diversions from the powerlaw model. Certain properties of the field scaling, exhibited in most of the cases, indicate that deterministic, chaotic dynamics may exist in the solar wind turbulence.

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