Long slow solar wind intervals exhibit a 1/f magnetic spectrum at low frequencies while velocity spectra remain Kolmogorov-like, extending the fast-wind observation to slow wind when intervals exceed 7 days.
H., Dasso, S, Weygand, J
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The low-frequency break observed in the slow solar wind magnetic spectra
Long slow solar wind intervals exhibit a 1/f magnetic spectrum at low frequencies while velocity spectra remain Kolmogorov-like, extending the fast-wind observation to slow wind when intervals exceed 7 days.