Introduction.- Solar Wind.- Plasma description.- Turbulence.- Solar Wind turbulence.- Plan of this thesis.- The Maltese Cross revisited.- Parameters and initial conditions.- Defining spectral properties in EBM simulations.- Results.- Discussion.- Can the Maltese Cross heat?.- Paper ApJ 2018: "Turbulent Heating between 0.2 and 1 au: A Numerical Study".- Heating fast winds.- Conclusions and future work.- Conclusions.- Future work: Anisotropy temperature description.- Appendix.
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