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Three-dimensional spatial structures of solar wind turbulence from 10 000-km to 100-km scales

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Figure

Fig. 2. Frequency spectra of magnetic field fluctuations in the threeanalyzed intervals: the upper curve in thin color is the spectrum forthe interval 1, the lower curve the interval 2, and the middle curve inblack the interval 3
Fig. 3. Stereographic representation of the three-dimensional wave-vector spectra of fluctuating magnetic field in the solar wind for themagnetic field (in the z-axis orthree time intervals shown in Fig
Fig. 4. Values of the anisotropy index as a function of the tetrahe-the panel denote the analyzed time interval

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