Violation of the Taylor hypothesis at electron scales in the solar wind and its effects on the energy spectra measured onboard spacecraft
Résumé
The solar wind is a natural laboratory for the study of turbulent plasma. In-situ observations from different spacecraft such as STEREO, Wind, ACE or Cluster allow us to investigate turbulence from magnetohydrodynamic (MHD) to kinetic scales (sub-ion and electron scales) of solar wind turbulence. With single spacecraft observations the Taylor frozen-in-flow assumption (Vf<
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Soumis le : mardi 9 juin 2020-10:23:36
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- HAL Id : hal-02861681 , version 1
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S. Y. Huang, Fouad Sahraoui. Violation of the Taylor hypothesis at electron scales in the solar wind and its effects on the energy spectra measured onboard spacecraft. American Geophysical Union, Fall Meeting, Dec 2014, San Francisco, California, United States. 51, pp.SH51D-4189, 2014. ⟨hal-02861681⟩
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