Articles | Volume 37, issue 5
Ann. Geophys., 37, 825–834, 2019
Ann. Geophys., 37, 825–834, 2019

Regular paper 19 Sep 2019

Regular paper | 19 Sep 2019

Scaling laws in Hall inertial-range turbulence

Yasuhito Narita et al.

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Cited articles

Alexandrova, O., Carbone, V., Veltri, P., and Sorriso-Valvo, L.: Small-scale energy cascade of the solar wind turbulence, Astrophys. J., 674, 1153–1157,, 2008. a, b
Alexandrova, O., Saur, J., Lacombe, C., Mangeney, A., Mitchell, J., Schwartz, S. J., and Robert, P.: Universality of solar-wind turbulent spectrum from MHD to electron scales, Phys. Rev. Lett., 103, 165003,, 2009. a
Angelopoulos, V.: The THEMIS Mission, Space Sci. Rev., 141, 5–34,, 2008. a
Bale, S. D., Kellogg, P. J., Mozer, F. S., Horbury, T. S., and Reme, H.: Measurement of the electric fluctuation spectrum of magnetohydrodynamic turbulence, Phys. Rev. Lett., 94, 215002,, 2005. a, b
Biskamp, D., Schwarz, E., and Drake, J. F.: Two-dimensional electron magnetohydrodynamic turbulence, Phys. Rev. Lett., 76, 1264–1267, 1996. a
Short summary
Scaling laws and energy spectra for the electric field, magnetic field, flow velocity, and density are theoretically derived for small-scale turbulence in space plasma on which the electrons behave as a fluid but the ions more as individual particles due to the difference in the mass (the Hall effect). Our theoretical model offers an explanation for the small-scale turbulence spectra measured in near-Earth space.