The Turbulent Cascade for High Cross-helicity States at 1 au. II. Minor Energy

The application of third moments to turbulence can determine the rate of the energy cascade. This approach is most readily done for statistically homogeneous turbulence in a uniform incompressible medium. Solar wind conditions near 1 au appear to fulfill these requirements sufficiently well to demon...

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Veröffentlicht in:	The Astrophysical journal 2018-11, Vol.867 (2), p.156
Hauptverfasser:	Vasquez, Bernard J., Forman, M. A., Coburn, J. T., Smith, C. W., Stawarz, J. E.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Correlation Energy Fluid dynamics Heating Helicity Homogeneous turbulence Intervals plasmas Protons Solar wind Turbulence Variation Wind speed
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