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A study of magnetic fluctuations and their anomalous scaling in the solar wind: the Ulysses fast-latitude scan

Balogh, A.; Pagel, C.

The solar wind is a highly turbulent and intermittent medium at frequencies between 10^-4 and 10^-1 Hz. Power spectra are used to look at fluctuations in the components of the magnetic field at high frequencies over a wide range of latitudes. Results show steady turbulence in the polar regions of the Sun and a more varied envir…