On the fractal nature of the magnetic field energy density in the solar wind
Author:
Affiliation:
1. Centre for Fusion, Space and Astrophysics; University of Warwick; Coventry UK
2. Natural Complexity Programme; British Antarctic Survey; Cambridge UK
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Reference22 articles.
1. The solar wind as a turbulence laboratory;Bruno;Living Rev. Solar,2005
2. Lognormal and multifractal distributions of the heliospheric magnetic field;Burlaga;J. Geophys. Res.,2001
3. Scaling collapse and structure functions: Identifying self-affinity in finite length time series;Chapman;Nonlinear Processes Geophys.,2005
4. Turbulence
5. Magnetohydrodynamic turbulence in the solar wind;Goldstein;Phys. Plasmas,1999
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