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1D Turbulent Heating

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

Abstract

We consider here the evolution of a 1D spectrum in the expanding (radial) wind, that is, with wavevectors all aligned in a given direction. We consider two cases: wavevectors in the radial direction, and wavevectors in a transverse direction (perpendicular to the radial). Based on these assumptions, we present a model of turbulent heating that is then compared to direct numerical simulations of Hydrodynamic turbulence in 1D.

References

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    Grappin R, Velli M, Mangeney A (1993) Nonlinear wave evolution in the expanding solar wind. Phys Rev Lett 70(14):2190–2193Google Scholar

Copyright information

© Springer Nature Switzerland AG 2019

Authors and Affiliations

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

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