Frame Dependence of the Electric Field Spectrum of Solar Wind Turbulence

Abstract

We present the first survey of electric field data using the ARTEMIS spacecraft in the solar wind to study inertial range turbulence. It was found that the average perpendicular spectral index of the electric field depends on the frame of measurement. In the spacecraft frame it is -5/3, which matches the magnetic field due to the large solar wind speed in Lorentz transformation. In the mean solar wind frame, the electric field is primarily due to the perpendicular velocity fluctuations and has a spectral index slightly shallower than -3/2, which is close to the scaling of the velocity. These results are an independent confirmation of the difference in scaling between the velocity and magnetic field, which is not currently well understood. The spectral index of the compressive fluctuations was also measured and found to be close to -5/3, suggesting that they are not only passive to the velocity but may also interact nonlinearly with the magnetic field.

References in corpus (6)

• Anisotropic scaling of magnetohydrodynamic turbulence
• Imbalanced Strong MHD Turbulence
• Role of cross helicity in magnetohydrodynamic turbulence
• Strong Imbalanced Turbulence
• Strong Anisotropic MHD Turbulence with Cross Helicity
• Kolmogorov and Irosnikov-Kraichnan scaling in the anisotropic turbulent solar wind

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