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Comparing Turbulent Cascades and Heating versus Spectral Anisotropy in Solar Wind via Direct Simulations
Abstract In a previous work (MGV18), we showed numerically that the turbulent cascade generated by quasi-2D structures (with wavevectors mostly perpendicular to the mean magnetic field) is able to generate a temperature profile close to the one observed in solar wind (≃1/ R ) in the range 0.2 ≤ R …