1D Turbulent Heating

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


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.


  1. 1.
    Belmont G, Grappin R, Mottez F, Pantellini F, Pelletier G (2014) Collisionless plasmas in astrophysics. Wiley, New York. Scholar
  2. 2.
    Burgers JM (1948) A mathematical model illustrating the theory of turbulence. In: A mathematical model illustrating the theory of turbulence, advances in applied mechanics, vol 1, Elsevier, pp 171–199.
  3. 3.
    Grappin R, Velli M, Mangeney A (1993) Nonlinear wave evolution in the expanding solar wind. Phys Rev Lett 70(14):2190–2193Google Scholar

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© Springer Nature Switzerland AG 2019

Authors and Affiliations

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

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