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Heating of Slow Winds

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Turbulent Heating and Anisotropy in the Solar Wind

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Abstract

The 1D hydrodynamic description of turbulence presented in the previous chapter has proven to be useful as a first approach to understand the development of turbulence in the expanding box simulations. However the 3D MHD model introduced in Sect. 2.2, the EBM equations, is clearly more realistic. In this chapter, we detail the initial properties of the plasma selected in our slow wind simulations. Then, we give the methods used to evaluate turbulent heating in our numerical simulations. Finally, we present the numerical results and the conclusions.

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References

  1. Grappin R, Velli M (1996) Waves and streams in the expanding solar wind. J Geophys Res 101:425–444

    Article  ADS  Google Scholar 

  2. Grappin R, Velli M, Mangeney A (1991) ’Alfvenic’ versus ’standard’ turbulence in the solar wind. Ann Geophys 9:416–426

    ADS  Google Scholar 

  3. Montagud-Camps V, Grappin R, Verdini A (2018) Turbulent Heating between 0.2 and 1 au: a numerical study. Astrophys J 853(2):153. https://doi.org/10.3847/1538-4357/aaa1ea

  4. Totten TL, Freeman JW, Arya S (1995) An empirical determination of the polytropic index for the free-streaming solar wind using Helios 1 data. J Geophys Res 100(A1):13–17

    Article  ADS  Google Scholar 

  5. Vasquez BJ, Smith CW, Hamilton K, MacBride BT, Leamon RJ (2007) Evaluation of the turbulent energy cascade rates from the upper inertial range in the solar wind at 1 AU. J Geophys Res 112(A7). https://doi.org/10.1029/2007JA012305

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Correspondence to Victor Montagud-Camps .

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Montagud-Camps, V. (2019). Heating of Slow Winds. In: Turbulent Heating and Anisotropy in the Solar Wind. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-030-30383-9_10

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