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Fractal properties of the IMF and the Earth’s magnetotail field

Earth, Planets and Space volume 50, pages 87–90 (1998)Cite this article

Abstract

The time series of the interplanetary and Earth’s magnetotail magnetic fields are analyzed. The data subsets taken by the IMP 8 spacecraft outside and inside of the Earth’s magnetosphere show clearly the fractal properties: their “box dimensions” are found to be close to 1.7 and 1.5 respectively. It is shown that data gaps have a little effect on the results. The magnetic field increment distributions are found to be non-Gaussian, but self-affine.

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Authors and Affiliations

  1. Space Physics Research Laboratory, Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, 2455 Hayward St., Ann Arbor, MI, 48109-2143, USA

    K. Kabin & V. O. Papitashvili

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  1. K. Kabin
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  2. V. O. Papitashvili
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Correspondence to K. Kabin.

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Kabin, K., Papitashvili, V.O. Fractal properties of the IMF and the Earth’s magnetotail field. Earth Planet Sp 50, 87–90 (1998). https://doi.org/10.1186/BF03352089

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  • DOI: https://doi.org/10.1186/BF03352089

Keywords

  • Solar Wind
  • Fractal Property
  • Interplanetary Magnetic Field
  • Fractional Brownian Motion
  • Solar Wind Turbulence