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Building up Solar-wind-like 3D Uniform-intensity Magnetic Fields
ArticleAbstract: A numerical model representing a 3D turbulent constant-magnitude magnetic field B is described. AssuPalabras claves:Magnetic fields, solar wind, TurbulenceAutores:Bruno R., Luca Sorriso-Valvo, Malara F., Primavera L., Valentini F.Fuentes:scopusThe low-frequency break observed in the slow solar wind magnetic spectra
ArticleAbstract: Fluctuations of solar wind magnetic field and plasma parameters exhibit a typical turbulence power sPalabras claves:Magnetic fields, plasmas, solar wind, Sun: heliosphere, Turbulence, WavesAutores:Bruno R., De Marco R., D’Amicis R., Luca Sorriso-Valvo, Raffaele Marino, Telloni D.Fuentes:scopus