Solar Orbiter observations of the Kelvin-Helmholtz waves in the solar wind

Solar Orbiter First Results (Cruise Phase)

Open Access

Fig. 11.

Magnetic spectra of all regions marked in Fig. 10. The Kolmogorov power law k^−5/3 and the dissipation range scalings k^−2.8 are plotted for reference as black dashed straight lines. The vortex size is noted by an arrow (top left). The ion gyroradius scale (ρ_p) and the ion inertial length (d_p) are marked by vertical black solid and dashed lines, respectively.

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