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  • Victor Montagud-CampsEmail author
Chapter
Part of the Springer Theses book series (Springer Theses)

Abstract

In the following, we show how the initial energy spectrum, cross helicity and expansion affect spectral anisotropy. We have checked that after an initial phase, the spectra don’t depend on the choice of these initial parameters. In the zero cross-helicity case, spectral anisotropy bas been analyzed by VG16. Our results will be compared with those of VG16 in the discussion.

Reference

  1. 1.
    Dong Y, Verdini A, Grappin R (2014) Evolution of turbulence in the expanding solar wind, a numerical study. Astrophys J 793(2):118.  https://doi.org/10.1088/0004-637X/793/2/118

Copyright information

© Springer Nature Switzerland AG 2019

Authors and Affiliations

  1. 1.Department of Surface and Plasma ScienceCharles UniversityPragueCzech Republic

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