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Communication Dans Un Congrès Année : 2015

Violation of the Taylor hypothesis at electron scales in the solar wind and its effects on the energy spectra measured onboard spacecraft

S. Y. Huang
  • Fonction : Auteur
Fouad Sahraoui

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 (Vphi
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Dates et versions

hal-02800186 , version 1 (05-06-2020)

Identifiants

  • HAL Id : hal-02800186 , version 1

Citer

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. EGU General Assembly, Apr 2015, Vienna, Austria. pp.7814. ⟨hal-02800186⟩
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